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Thursday, October 2, 2008

Ten Politically Incorrect Truths About Human Nature


Very interesting and thought provoking ...

http://psychologytoday.com/articles/index.php?term=pto-4359.html


Ten Politically Incorrect Truths About Human Nature

Why most suicide bombers are Muslim, beautiful people have more daughters, humans are naturally polygamous, sexual harassment isn't sexist, and blonds are more attractive.



Human nature is one of those things that everybody talks about but no one can define precisely. Every time we fall in love, fight with our spouse, get upset about the influx of immigrants into our country, or go to church, we are, in part, behaving as a human animal with our own unique evolved nature—human nature.

This means two things. First, our thoughts, feelings, and behavior are produced not only by our individual experiences and environment in our own lifetime but also by what happened to our ancestors millions of years ago. Second, our thoughts, feelings, and behavior are shared, to a large extent, by all men or women, despite seemingly large cultural differences.

Human behavior is a product both of our innate human nature and of our individual experience and environment. In this article, however, we emphasize biological influences on human behavior, because most social scientists explain human behavior as if evolution stops at the neck and as if our behavior is a product almost entirely of environment and socialization. In contrast, evolutionary psychologists see human nature as a collection of psychological adaptations that often operate beneath conscious thinking to solve problems of survival and reproduction by predisposing us to think or feel in certain ways. Our preference for sweets and fats is an evolved psychological mechanism. We do not consciously choose to like sweets and fats; they just taste good to us.

The implications of some of the ideas in this article may seem immoral, contrary to our ideals, or offensive. We state them because they are true, supported by documented scientific evidence. Like it or not, human nature is simply not politically correct.

Adapted from Why Beautiful People Have More Daughters, by Alan S. Miller and Satoshi Kanazawa, to be published by Perigee in September 2007.


  1. Men like blond bombshells (and women want to look like them)

    Long before TV—in 15th- and 16th- century Italy, and possibly two millennia ago—women were dying their hair blond. A recent study shows that in Iran, where exposure to Western media and culture is limited, women are actually more concerned with their body image, and want to lose more weight, than their American counterparts. It is difficult to ascribe the preferences and desires of women in 15th-century Italy and 21st-century Iran to socialization by media.

    Women's desire to look like Barbie—young with small waist, large breasts, long blond hair, and blue eyes—is a direct, realistic, and sensible response to the desire of men to mate with women who look like her. There is evolutionary logic behind each of these features.

    Men prefer young women in part because they tend to be healthier than older women. One accurate indicator of health is physical attractiveness; another is hair. Healthy women have lustrous, shiny hair, whereas the hair of sickly people loses its luster. Because hair grows slowly, shoulder-length hair reveals several years of a woman's health status.

    Men also have a universal preference for women with a low waist-to-hip ratio. They are healthier and more fertile than other women; they have an easier time conceiving a child and do so at earlier ages because they have larger amounts of essential reproductive hormones. Thus men are unconsciously seeking healthier and more fertile women when they seek women with small waists.

    Until very recently, it was a mystery to evolutionary psychology why men prefer women with large breasts, since the size of a woman's breasts has no relationship to her ability to lactate. But Harvard anthropologist Frank Marlowe contends that larger, and hence heavier, breasts sag more conspicuously with age than do smaller breasts. Thus they make it easier for men to judge a woman's age (and her reproductive value) by sight—suggesting why men find women with large breasts more attractive.

    Alternatively, men may prefer women with large breasts for the same reason they prefer women with small waists. A new study of Polish women shows that women with large breasts and tight waists have the greatest fecundity, indicated by their levels of two reproductive hormones (estradiol and progesterone).

    Blond hair is unique in that it changes dramatically with age. Typically, young girls with light blond hair become women with brown hair. Thus, men who prefer to mate with blond women are unconsciously attempting to mate with younger (and hence, on average, healthier and more fecund) women. It is no coincidence that blond hair evolved in Scandinavia and northern Europe, probably as an alternative means for women to advertise their youth, as their bodies were concealed under heavy clothing.

    Women with blue eyes should not be any different from those with green or brown eyes. Yet preference for blue eyes seems both universal and undeniable—in males as well as females. One explanation is that the human pupil dilates when an individual is exposed to something that she likes. For instance, the pupils of women and infants (but not men) spontaneously dilate when they see babies. Pupil dilation is an honest indicator of interest and attraction. And the size of the pupil is easiest to determine in blue eyes. Blue-eyed people are considered attractive as potential mates because it is easiest to determine whether they are interested in us or not.

    The irony is that none of the above is true any longer. Through face-lifts, wigs, liposuction, surgical breast augmentation, hair dye, and color contact lenses, any woman, regardless of age, can have many of the key features that define ideal female beauty. And men fall for them. Men can cognitively understand that many blond women with firm, large breasts are not actually 15 years old, but they still find them attractive because their evolved psychological mechanisms are fooled by modern inventions that did not exist in the ancestral environment.

  2. Humans are naturally polygamous

    The history of western civilization aside, humans are naturally polygamous. Polyandry (a marriage of one woman to many men) is very rare, but polygyny (the marriage of one man to many women) is widely practiced in human societies, even though Judeo-Christian traditions hold that monogamy is the only natural form of marriage. We know that humans have been polygynous throughout most of history because men are taller than women.

    Among primate and nonprimate species, the degree of polygyny highly correlates with the degree to which males of a species are larger than females. The more polygynous the species, the greater the size disparity between the sexes. Typically, human males are 10 percent taller and 20 percent heavier than females. This suggests that, throughout history, humans have been mildly polygynous.

    Relative to monogamy, polygyny creates greater fitness variance (the distance between the "winners" and the "losers" in the reproductive game) among males than among females because it allows a few males to monopolize all the females in the group. The greater fitness variance among males creates greater pressure for men to compete with each other for mates. Only big and tall males can win mating opportunities. Among pair-bonding species like humans, in which males and females stay together to raise their children, females also prefer to mate with big and tall males because they can provide better physical protection against predators and other males.

    In societies where rich men are much richer than poor men, women (and their children) are better off sharing the few wealthy men; one-half, one-quarter, or even one-tenth of a wealthy man is still better than an entire poor man. As George Bernard Shaw puts it, "The maternal instinct leads a woman to prefer a tenth share in a first-rate man to the exclusive possession of a third-rate one." Despite the fact that humans are naturally polygynous, most industrial societies are monogamous because men tend to be more or less equal in their resources compared with their ancestors in medieval times. (Inequality tends to increase as society advances in complexity from hunter-gatherer to advanced agrarian societies. Industrialization tends to decrease the level of inequality.)

  3. Most women benefit from polygyny, while most men benefit from monogamy

    When there is resource inequality among men—the case in every human society—most women benefit from polygyny: women can share a wealthy man. Under monogamy, they are stuck with marrying a poorer man.

    The only exceptions are extremely desirable women. Under monogamy, they can monopolize the wealthiest men; under polygyny, they must share the men with other, less desirable women. However, the situation is exactly opposite for men. Monogamy guarantees that every man can find a wife. True, less desirable men can marry only less desirable women, but that's much better than not marrying anyone at all.

    Men in monogamous societies imagine they would be better off under polygyny. What they don't realize is that, for most men who are not extremely desirable, polygyny means no wife at all, or, if they are lucky, a wife who is much less desirable than one they could get under monogamy.

  4. Most suicide bombers are Muslim

    According to the Oxford University sociologist Diego Gambetta, editor of Making Sense of Suicide Missions, a comprehensive history of this troubling yet topical phenomenon, while suicide missions are not always religiously motivated, when religion is involved, it is always Muslim. Why is this? Why is Islam the only religion that motivates its followers to commit suicide missions?

    The surprising answer from the evolutionary psychological perspective is that Muslim suicide bombing may have nothing to do with Islam or the Koran (except for two lines in it). It may have nothing to do with the religion, politics, the culture, the race, the ethnicity, the language, or the region. As with everything else from this perspective, it may have a lot to do with sex, or, in this case, the absence of sex.

    What distinguishes Islam from other major religions is that it tolerates polygyny. By allowing some men to monopolize all women and altogether excluding many men from reproductive opportunities, polygyny creates shortages of available women. If 50 percent of men have two wives each, then the other 50 percent don't get any wives at all.

    So polygyny increases competitive pressure on men, especially young men of low status. It therefore increases the likelihood that young men resort to violent means to gain access to mates. By doing so, they have little to lose and much to gain compared with men who already have wives. Across all societies, polygyny makes men violent, increasing crimes such as murder and rape, even after controlling for such obvious factors as economic development, economic inequality, population density, the level of democracy, and political factors in the region.

    However, polygyny itself is not a sufficient cause of suicide bombing. Societies in sub-Saharan Africa and the Caribbean are much more polygynous than the Muslim nations in the Middle East and North Africa. And they do have very high levels of violence. Sub-Saharan Africa suffers from a long history of continuous civil wars—but not suicide bombings.

    The other key ingredient is the promise of 72 virgins waiting in heaven for any martyr in Islam. The prospect of exclusive access to virgins may not be so appealing to anyone who has even one mate on earth, which strict monogamy virtually guarantees. However, the prospect is quite appealing to anyone who faces the bleak reality on earth of being a complete reproductive loser.

    It is the combination of polygyny and the promise of a large harem of virgins in heaven that motivates many young Muslim men to commit suicide bombings. Consistent with this explanation, all studies of suicide bombers indicate that they are significantly younger than not only the Muslim population in general but other (nonsuicidal) members of their own extreme political organizations like Hamas and Hezbollah. And nearly all suicide bombers are single.

  5. Having sons reduces the likelihood of divorce

    Sociologists and demographers have discovered that couples who have at least one son face significantly less risk of divorce than couples who have only daughters. Why is this?

    Since a man's mate value is largely determined by his wealth, status, and power—whereas a woman's is largely determined by her youth and physical attractiveness—the father has to make sure that his son will inherit his wealth, status, and power, regardless of how much or how little of these resources he has. In contrast, there is relatively little that a father (or mother) can do to keep a daughter youthful or make her more physically attractive.

    The continued presence of (and investment by) the father is therefore important for the son, but not as crucial for the daughter. The presence of sons thus deters divorce and departure of the father from the family more than the presence of daughters, and this effect tends to be stronger among wealthy families.

  6. Beautiful people have more daughters

    It is commonly believed that whether parents conceive a boy or a girl is up to random chance. Close, but not quite; it is largely up to chance. The normal sex ratio at birth is 105 boys for every 100 girls. But the sex ratio varies slightly in different circumstances and for different families. There are factors that subtly influence the sex of an offspring.

    One of the most celebrated principles in evolutionary biology, the Trivers-Willard hypothesis, states that wealthy parents of high status have more sons, while poor parents of low status have more daughters. This is because children generally inherit the wealth and social status of their parents. Throughout history, sons from wealthy families who would themselves become wealthy could expect to have a large number of wives, mistresses and concubines, and produce dozens or hundreds of children, whereas their equally wealthy sisters can have only so many children. So natural selection designs parents to have biased sex ratio at birth depending upon their economic circumstances—more boys if they are wealthy, more girls if they are poor. (The biological mechanism by which this occurs is not yet understood.)

    This hypothesis has been documented around the globe. American presidents, vice presidents, and cabinet secretaries have more sons than daughters. Poor Mukogodo herders in East Africa have more daughters than sons. Church parish records from the 17th and 18th centuries show that wealthy landowners in Leezen, Germany, had more sons than daughters, while farm laborers and tradesmen without property had more daughters than sons. In a survey of respondents from 46 nations, wealthy individuals are more likely to indicate a preference for sons if they could only have one child, whereas less wealthy individuals are more likely to indicate a preference for daughters.

    The generalized Trivers-Willard hypothesis goes beyond a family's wealth and status: If parents have any traits that they can pass on to their children and that are better for sons than for daughters, then they will have more boys. Conversely, if parents have any traits that they can pass on to their children and that are better for daughters, they will have more girls.

    Physical attractiveness, while a universally positive quality, contributes even more to women's reproductive success than to men's. The generalized hypothesis would therefore predict that physically attractive parents should have more daughters than sons. Once again, this is the case. Americans who are rated "very attractive" have a 56 percent chance of having a daughter for their first child, compared with 48 percent for everyone else.

  7. What Bill Gates and Paul McCartney have in common with criminals

    For nearly a quarter of a century, criminologists have known about the "age-crime curve." In every society at all historical times, the tendency to commit crimes and other risk-taking behavior rapidly increases in early adolescence, peaks in late adolescence and early adulthood, rapidly decreases throughout the 20s and 30s, and levels off in middle age.

    This curve is not limited to crime. The same age profile characterizes every quantifiable human behavior that is public (i.e., perceived by many potential mates) and costly (i.e., not affordable by all sexual competitors). The relationship between age and productivity among male jazz musicians, male painters, male writers, and male scientists—which might be called the "age-genius curve"—is essentially the same as the age-crime curve. Their productivity—the expressions of their genius—quickly peaks in early adulthood, and then equally quickly declines throughout adulthood. The age-genius curve among their female counterparts is much less pronounced; it does not peak or vary as much as a function of age.

    Paul McCartney has not written a hit song in years, and now spends much of his time painting. Bill Gates is now a respectable businessman and philanthropist, and is no longer a computer whiz kid. J.D. Salinger now lives as a total recluse and has not published anything in more than three decades. Orson Welles was a mere 26 when he wrote, produced, directed, and starred in Citizen Kane.

    A single theory can explain the productivity of both creative geniuses and criminals over the life course: Both crime and genius are expressions of young men's competitive desires, whose ultimate function in the ancestral environment would have been to increase reproductive success.

    In the physical competition for mates, those who are competitive may act violently toward their male rivals. Men who are less inclined toward crime and violence may express their competitiveness through their creative activities.

    The cost of competition, however, rises dramatically when a man has children, when his energies and resources are put to better use protecting and investing in them. The birth of the first child usually occurs several years after puberty because men need some time to accumulate sufficient resources and attain sufficient status to attract their first mate. There is therefore a gap of several years between the rapid rise in the benefits of competition and similarly rapid rise in its costs. Productivity rapidly declines in late adulthood as the costs of competition rise and cancel its benefits.

    These calculations have been performed by natural and sexual selection, so to speak, which then equips male brains with a psychological mechanism to incline them to be increasingly competitive immediately after puberty and make them less competitive right after the birth of their first child. Men simply do not feel like acting violently, stealing, or conducting additional scientific experiments, or they just want to settle down after the birth of their child but they do not know exactly why.

    The similarity between Bill Gates, Paul McCartney, and criminals—in fact, among all men throughout evolutionary history—points to an important concept in evolutionary biology: female choice.

    Women often say no to men. Men have had to conquer foreign lands, win battles and wars, compose symphonies, author books, write sonnets, paint cathedral ceilings, make scientific discoveries, play in rock bands, and write new computer software in order to impress women so that they will agree to have sex with them. Men have built (and destroyed) civilization in order to impress women, so that they might say yes.

  8. The midlife crisis is a myth—sort of

    Many believe that men go through a midlife crisis when they are in middle age. Not quite. Many middle-aged men do go through midlife crises, but it's not because they are middle-aged. It's because their wives are. From the evolutionary psychological perspective, a man's midlife crisis is precipitated by his wife's imminent menopause and end of her reproductive career, and thus his renewed need to attract younger women. Accordingly, a 50-year-old man married to a 25-year-old woman would not go through a midlife crisis, while a 25-year-old man married to a 50-year-old woman would, just like a more typical 50-year-old man married to a 50-year-old woman. It's not his midlife that matters; it's hers. When he buys a shiny-red sports car, he's not trying to regain his youth; he's trying to attract young women to replace his menopausal wife by trumpeting his flash and cash.

  9. It's natural for politicians to risk everything for an affair (but only if they're male)

    On the morning of January 21, 1998, as Americans woke up to the stunning allegation that President Bill Clinton had had an affair with a 24-year-old White House intern, Darwinian historian Laura L. Betzig thought, "I told you so." Betzig points out that while powerful men throughout Western history have married monogamously (only one legal wife at a time), they have always mated polygynously (they had lovers, concubines, and female slaves). With their wives, they produced legitimate heirs; with the others, they produced bastards. Genes make no distinction between the two categories of children.

    As a result, powerful men of high status throughout human history attained very high reproductive success, leaving a large number of offspring (legitimate and otherwise), while countless poor men died mateless and childless. Moulay Ismail the Bloodthirsty, the last Sharifian emperor of Morocco, stands out quantitatively, having left more offspring—1,042—than anyone else on record, but he was by no means qualitatively different from other powerful men, like Bill Clinton.

    The question many asked in 1998—"Why on earth would the most powerful man in the world jeopardize his job for an affair with a young woman?"—is, from a Darwinian perspective, a silly one. Betzig's answer would be: "Why not?" Men strive to attain political power, consciously or unconsciously, in order to have reproductive access to a larger number of women. Reproductive access to women is the goal, political office but one means. To ask why the President of the United States would have a sexual encounter with a young woman is like asking why someone who worked very hard to earn a large sum of money would then spend it.

    What distinguishes Bill Clinton is not that he had extramarital affairs while in office—others have, more will; it would be a Darwinian puzzle if they did not—what distinguishes him is the fact that he got caught.

  10. Men sexually harass women because they are not sexist

    An unfortunate consequence of the ever-growing number of women joining the labor force and working side by side with men is the increasing number of sexual harassment cases. Why must sexual harassment be a necessary consequence of the sexual integration of the workplace?

    Psychologist Kingsley R. Browne identifies two types of sexual harassment cases: the quid pro quo ("You must sleep with me if you want to keep your job or be promoted") and the "hostile environment" (the workplace is deemed too sexualized for workers to feel safe and comfortable). While feminists and social scientists tend to explain sexual harassment in terms of "patriarchy" and other ideologies, Browne locates the ultimate cause of both types of sexual harassment in sex differences in mating strategies.

    Studies demonstrate unequivocally that men are far more interested in short-term casual sex than women. In one now-classic study, 75 percent of undergraduate men approached by an attractive female stranger agreed to have sex with her; none of the women approached by an attractive male stranger did. Many men who would not date the stranger nonetheless agreed to have sex with her.

    The quid pro quo types of harassment are manifestations of men's greater desire for short-term casual sex and their willingness to use any available means to achieve that goal. Feminists often claim that sexual harassment is "not about sex but about power;" Browne contends it is both—men using power to get sex. "To say that it is only about power makes no more sense than saying that bank robbery is only about guns, not about money."

    Sexual harassment cases of the hostile-environment variety result from sex differences in what men and women perceive as "overly sexual" or "hostile" behavior. Many women legitimately complain that they have been subjected to abusive, intimidating, and degrading treatment by their male coworkers. Browne points out that long before women entered the labor force, men subjected each other to such abusive, intimidating, and degrading treatment.

    Abuse, intimidation, and degradation are all part of men's repertoire of tactics employed in competitive situations. In other words, men are not treating women differently from men—the definition of discrimination, under which sexual harassment legally falls—but the opposite: Men harass women precisely because they are not discriminating between men and women.

Psychology Today Magazine, Jul/Aug 2007
Last Reviewed 20 Sep 2007
Article ID: 4359

Wednesday, October 1, 2008

Net neutrality: An American problem?

No estoy de acuerdo con la idea ésta de 'racionar' el bandwith, y querer cobrarle a los usuarios $ adicional por lo que bajen del web. Los ISPs no están perdiendo dinero, lo que quieren es aprovecharse de que los usuarios consumen más multimedia para chuparles más dinero.



September 28, 2008 11:42 AM PDT

Net neutrality: An American problem?

This story was written by Brett Winterford and Julian Hill.

The leaders of three of Australia's largest ISP's have declared the Net neutrality debate as solely a U.S. problem--and further, that the nation that pioneered the Internet might want to study the Australian market for clues as to how to solve the dilemma.

Net neutrality is a term coined by Internet users who oppose the increasing tendency among network owners (telecommunications companies) to tier or prioritize certain content on the network.

The debate was sparked after several American and British service providers offered to charge a premium to prioritize traffic connecting with some sites over others. These service providers claim the Internet is "running out of capacity" due to excessive use of rich content like video and file-sharing traffic. The only model with which capacity can be expanded, they argue, is to charge large media companies to prioritize traffic to and from their sites.

But Simon Hackett, the managing director of Adelaide-based ISP Internode, argues that it is ridiculous to suggest bandwidth is "running out."

"I don't subscribe to the view that network capacity is finite at all... Optical fiber basically doesn't run out of capacity, it's just a question of how fast you blink the bits at each end," he said in a recent interview with ZDNet.com.au.

"The (Net neutrality) problem isn't about running out of capacity. It's a business model that's about to explode due to stress. The problem, in my opinion, is the U.S. business model," said Hackett.

"The U.S. have got a problem," weighed in Justin Milne, group managing director for Telstra Media and former chief of Australia's largest ISP, BigPond. "Their problem is that unlike Australia, they (offer) truly unlimited plans."

The problem with an unlimited-access plan, explains Hackett, is that it "devalues what a megabyte is worth." American customers have never been able to put much of a dollar value on traffic, as historically, U.S. ISPs have "had it very easy" in terms of bandwidth costs. The United States invented the Internet and developed the first content for it, and the rest of the world essentially subsidized the U.S. to connect to that content.

"It was quite rational to charge (users) a fixed amount of money for access (in the U.S) because the actual downloads per month were trivial," said Hackett.

Today, there is as much local traffic floating around the rest of the world as there is in the United States, and America is as much a consumer of the world's content as it is a distributor of content to the world. In addition, the traffic being carried is far richer in terms of content, so the cost of feeding capacity to the YouTube generation is considerably higher.

"Now everybody file-shares and sends video all around the place," said Milne, "and the problem for the telcos in the U.S. is they are having to expand their networks as they go, but they are not getting paid any more money."

Who pays?
American ISPs are thus faced with a choice as to whom to charge in order to build out their networks to accommodate the increased traffic.

The first choice is to absorb the costs themselves, the status quo to date, which is less than desirable as a business model. The second choice is to cease to offer unlimited plans, which passes the cost of excessive bandwidth use onto those users that consume the most.

The final choice, says Michael Malone, CEO of ASX-listed ISP iiNet, is to charge content providers, the model that has stirred up controversy.

"The attempt is being made certainly in the U.K. but also in the U.S. to push that cost onto the content owner by saying, you pay, and we'll prioritize your traffic," he said. "(And) if you don't pay, your traffic will be really crap."

American ISPs are hesitant to take the option of charging customers for excessive use, Milne says, because they will "probably all knick off and go to my competitors who are not charging them." Instead, they plan to "charge the guys who are putting big gobs of video traffic into my network--which would be people like Microsoft and YouTube and Google etc."

"Those guys say, you're kidding, what about Net neutrality? The Net is supposed to be free, man! You can't charge us for putting traffic in there because that's denying the natural rights of Americans! I think the argument is thin but nevertheless Congress seems to be picking it up."

Lessons from Down Under
The right choice, all three Australian ISP leaders agree, is to put the onus on the user, a model that has worked well in Australia.

As an Australian ISP, around 60 percent to 70 percent of traffic comes from overseas. "You've got to haul the traffic," explains Milne. "All of that traffic is volumetrically charged--the more traffic you haul from overseas, the more you pay.

"So all ISPs in Australia, because of our unique geography, have got used to pay-as-you-go and have handed those pay-as-you-go principles on to their customers."

Malone says that when users are offered truly unlimited access to download as much as they want, 3 percent of customers use over 50 percent of all the downloads. Download quotas can eradicate that problem if they are set at such a level that it affects this 3 percent, while having zero affect on the majority.

Quotas, Malone says, aren't designed to be punitive.

"Quotas are meant to be able to say that for 95 percent of customers, this (much data) is enough...This is an effectively unlimited connection for most people.

"From my point of view, (Net neutrality is) an artificial problem created out of fear of modifying the business model," says Hackett. "The idea that the entire population can subsidize a minority with an extremely high download quantity actually isn't necessarily the only way to live," said Malone.

The Australian model gives ISPs predictability about income and network costs, explains Hackett.

"If a user uses much more stuff, they wind up on higher plans, so we can actually afford to bring in more (network equipment and capacity)," he said. "So it's kind of self-correcting. In the U.S., an ISP is visibly afraid of the idea of customers pulling video 24/7. (Whereas) if our users use more traffic, it doesn't actually scare us. You get the sense that it actually does scare (U.S. ISP) Comcast."

Milne says a number of U.S. cable companies have taken the hint and started charging "volumetrically."

"I think that's actually where things will finish up," he says. "Be it electricity, travel, petrol, we as humans have got used to the idea that the more you use the more you pay, albeit with a discount. The Net in the U.S. just magically decided to avoid that, and now I think they'll have to come back to reality."

"You can't just keep on building these networks forever for free. You can build them bigger and bigger and bigger, but somebody has to pay for it. There has to be a business model by which the network is paid for," added Milne.

Brett Winterford and Julian Hill of ZDNet Australia reported from London.

The 10 Most Mysterious Cyber Crimes / Los 10 Ciber-Crímenes más Misteriosos

http://www.pcmag.com/article2/0,2817,2331225,00.asp



The 10 Most Mysterious Cyber Crimes

When a major cyber crime remains unsolved, though, it probably also means that those of us outside the world of tech crime solving may never even know the crime occurred.

These are some of the top headline-worthy highlights in the world of unsolved computing crime—cases in which the only information available is the ruin left in their wake.

The WANK Worm (October 1989)
Possibly the first "hacktivist" (hacking activist) attack, the WANK worm hit NASA offices in Greenbelt, Maryland. WANK (Worms Against Nuclear Killers) ran a banner (pictured) across system computers as part of a protest to stop the launch of the plutonium-fueled, Jupiter-bound Galileo probe. Cleaning up after the crack has been said to have cost NASA up to a half of a million dollars in time and resources. To this day, no one is quite sure where the attack originated, though many fingers have pointed to Melbourne, Australia-based hackers.

Ministry of Defense Satellite Hacked (February 1999)
A small group of hackers traced to southern England gained control of a MoD Skynet military satellite and signaled a security intrusion characterized by officials as "information warfare," in which an enemy attacks by disrupting military communications. In the end, the hackers managed to reprogram the control system before being discovered. Though Scotland Yard's Computer Crimes Unit and the U.S. Air Force worked together to investigate the case, no arrests have been made.

CD Universe Credit Card Breach (January 2000)
A blackmail scheme gone wrong, the posting of over 300,000 credit card numbers by hacker Maxim on a Web site entitled "The Maxus Credit Card Pipeline" has remained unsolved since early 2000. Maxim stole the credit card information by breaching CDUniverse.com; he or she then demanded $100,000 from the Web site in exchange for destroying the data. While Maxim is believed to be from Eastern Europe, the case remains as of yet unsolved.

Military Source Code Stolen (December 2000)
If there's one thing you don't want in the wrong hands, it's the source code that can control missile-guidance systems. In winter of 2000, a hacker broke into government-contracted Exigent Software Technology and nabbed two-thirds of the code for Exigent's OS/COMET software, which is responsible for both missile and satellite guidance, from the Naval Research Lab in Washington, D.C. Officials were able to follow the trail of the intruder "Leaf" to the University of Kaiserslautern in Germany, but that's where the trail appears to end.

Anti-DRM Hack (October 2001)
In our eyes, not all hackers are bad guys (as evidenced by our list of the Ten Greatest Hacks of All Time); often they're just trying to right a wrong or make life generally easier for the tech-consuming public. Such is the case of the hacker known as Beale Screamer, whose FreeMe program allowed Windows Media users to strip digital-rights-management security from music and video files. While Microsoft tried to hunt down Beale, other anti-DRM activists heralded him as a crusader.

Next: Crimes 6 - 10 >

Dennis Kucinich on CBSNews.com (October 2003)
As Representative Kucinich's presidential campaign struggled in the fall of 2003, a hacker did what he could to give it a boost. Early one Friday morning the CBSNews.com homepage was replaced by the campaign's logo. The page then automatically redirected to a 30-minute video called "This is the Moment," in which the candidate laid out his political philosophy. The Kucinich campaign denied any involvement with the hack, and whoever was responsible was not identified.

Hacking Your MBA App (March 2006)
Waiting on a college or graduate school decision is a nail-biting experience, so when one hacker found out how to break into the automated ApplyYourself application system in 2006, it was only natural that he wanted to share the wealth. Dozens of top business schools, including Harvard and Stanford, saw applicants exploiting the hack in order to track their application statuses. The still-unknown hacker posted the ApplyYourself login process on Business Week's online forums; the information was promptly removed and those who used it were warned by schools that they should expect rejection letters in the mail.

The 26,000 Site Hack Attack (Winter 2008)
MSNBC.com was among the largest of the thousands of sites used by a group of unknown hackers earlier this year to redirect traffic to their own JavaScript code hosted by servers known for malware. The malicious code was embedded in areas of the sites where users could not see it, but where hackers could activate it.

Supermarket Security Breach (February 2008)
Overshadowed only by a T.J Maxx breach in 2005, the theft of at least 1,800 credit and debit card numbers (and the exposure of about 4.2 million others) at supermarket chains Hannaford and Sweetbay (both owned by the Belgium-based Delhaize Group) in the Northeast United States and Florida remains unsolved more than six months later. Chain reps and security experts are still unclear as to how the criminals gained access to the system; the 2005 T.J.Maxx breach took advantage of a vulnerability in the chain's wireless credit transfer system, but Hannaford and Sweetbay do not use wireless transfers of any sort. Without more information, the difficulty in tracking down those responsible grows exponentially.

Comcast.net Gets a Redirect (May 2008)
A devious hack doesn't always mean finding a back door or particularly crafty way into a secure network or server; sometimes it just means that account information was compromised. Such was the case earlier this year when a member of the hacker group Kryogeniks gained unauthorized access to Comcast.net's registrar, Network Solutions. The domain name system (DNS) hack altered Comcast.net's homepage to redirect those attempting to access webmail to the hackers' own page (pictured). Spokespeople for Comcast and Network Solutions are still unclear as to how the hackers got the username and password.

Copyright (c) 2008Ziff Davis Media Inc. All Rights Reserved.

Tuesday, September 30, 2008

Nova: Einstein's Big Idea / Nova : La Gran Idea de Einstein

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The Legacy of E = mc2
by Peter Tyson

Inquiry

Einstein's Big Idea homepage

What hasn't Einstein's equation touched in our world?

It's difficult to separate the enormous legacy of E = mc2 from Einstein's legacy as a whole. After all, the equation grew directly out of Einstein's work on special relativity, which is a subset of what most consider his greatest achievement, the theory of general relativity. But I'm going to give it a try nevertheless.

The equation explained

First, though, a capsule explanation of "energy equals mass times the speed of light squared" might be helpful. On the most basic level, the equation says that energy and mass (matter) are interchangeable; they are different forms of the same thing. Under the right conditions, energy can become mass, and vice versa. We humans don't see them that way-how can a beam of light and a walnut, say, be different forms of the same thing?-but Nature does.

So why would you have to multiply the mass of that walnut by the speed of light to determine how much energy is bound up inside it? The reason is that whenever you convert part of a walnut or any other piece of matter to pure energy, the resulting energy is by definition moving at the speed of light. Pure energy is electromagnetic radiation-whether light or X-rays or whatever-and electromagnetic radiation travels at a constant speed of roughly 670,000,000 miles per hour.

Why, then, do you have to square the speed of light? It has to do with the nature of energy. When something is moving four times as fast as something else, it doesn't have four times the energy but rather 16 times the energy-in other words, that figure is squared. So the speed of light squared is the conversion factor that decides just how much energy lies captured within a walnut or any other chunk of matter. And because the speed of light squared is a huge number-448,900,000,000,000,000 in units of mph-the amount of energy bound up into even the smallest mass is truly mind-boggling (see The Power of Tiny Things.)

Of course, intuitively understanding that energy and matter are essentially one, as well as why and how so much energy can be wrapped up in even minute bits of matter, is another thing. And E = mc2, which focuses on matter at rest, is a simplified version of a more elaborate equation that Einstein devised, which also takes into account matter in motion (more on that in a moment). But I hope that you, like I, now have a basic comprehension with which to appreciate the equation's prodigious influence.

E = mc2 in miniature

Perhaps the equation's most far-reaching legacy is that it provides the key to understanding the most basic natural processes of the universe, from microscopic radioactivity to the big bang itself.

Radioactivity is E = mc2 in miniature. Einstein himself suspected this even as he devised the equation. In the 1905 paper in which he introduced E = mc2 to the world, he suggested that it might be possible to test his theory about the equation using radium, an ounce of which, as Marie Curie had discovered not long before, continuously emits 4,000 calories of heat per hour. Einstein believed that radium was constantly converting part of its mass to energy exactly as his equation specified. He was eventually proved right.

Today we know radioactivity to be a property possessed by some unstable elements, such as uranium, or isotopes, such as carbon 14, of spontaneously emitting energetic particles as their atomic nuclei disintegrate. They are metamorphosing mass into energy in direct accordance with Einstein's equation.

We take advantage of that realization today in many technologies. PET scans and similar diagnostics used in hospitals, for example, make use of E = mc2. "Whenever you use a radioactive substance to illuminate processes in the human body, you're paying direct homage to Einstein's insight," says Sylvester James Gates, a physicist at the University of Maryland. Many everyday devices, from smoke detectors to exit signs, also host an ongoing, invisible fireworks of E = mc2 transformations. Radiocarbon dating, which archeologists use to date ancient material, is yet another application of the formula. "The decay products that we see in carbon dating-that energy is directly obtained from the missing mass that you see in E = mc2," Gates says.

Heavenly applications

Space technologies owe much to the equation. Unceasing E = mc2 disintegrations from radioactive elements such as plutonium provide everything from power for telecommunications satellites to the heat needed to keep the Mars rovers functioning during the frigid martian winter. Space travel in the distant future may also rely on such radiation-derived power. Photons streaming out from the sun and other stars hold energy that in the vacuum of space can theoretically be harnessed to propel a spaceship. "In the far future," says David Hogg, a cosmologist at New York University, "if you imagine that we're sailing to distant stars with spaceships that are driven by radiation pressure-if that ever happens, that will be a really big legacy of Einstein's kinematics."

Kinematics is the study of motion without reference to mass or force, and it figures in a more elaborate form of Einstein's equation that-unlike plain old E = mc2, which concerns mass at rest-also takes into account mass in motion. (If you must know, it's E2 = m2c4 + p2c2, where p equals momentum.) "His bigger equation plays an enormous part in our understanding of how light works, and how energy and light can be transferred and transformed from one place to another, and that sort of thing," Gates says. "So if you consider the larger context, the part of the equation that's not in the public eye, it has an even larger legacy in science."

One application that draws on this larger equation, Gates says, is the giant neutrino detector now being built in Antarctica. Sunk deep in the ice, it will detect the eerie blue light, known as Cherenkov radiation, that is given off by neutrinos. Neutrinos are subatomic particles so lacking in mass that they pass straight through the Earth unscathed. Studying their light helps cosmologists better understand these mysterious particles and their distant sources, which may include black holes. Thus, says Gates, "as part of the equation's legacy, we'll be using the ice of Antarctica to look at neutrinos and other objects coming from outer space. And without knowing the relationship between the energy, momentum, and mass, that would be inconceivable to do. In fact, it was the use of this equation that led to the realization that neutrinos must exist."

A nuclear world

Einstein's equation also perfectly describes what's happening when we produce nuclear energy. As Arlin Crotts, a professor of astronomy at Columbia University, puts it, "our entire understanding of nuclear processes would be sort of lost without it." Fission reactors in nuclear power plants generate electricity by unlocking the energy tied up in fissionable materials. Fusion also furnishes energy from mass just as the equation posits. When two hydrogen atoms fuse to form a helium atom, the mass of the resulting helium is less than the two hydrogens, with the missing mass manifesting itself as fusion energy. Nuclear weapons, too, operate on the principle defined by the equation. Indeed, the mushroom cloud of an atomic bomb explosion is E = mc2 made visible.

"One of its legacies is very sociological: it just captures the imagination of everyone."

The equation spawned a whole new branch of science-high-energy particle physics. Labs that work in this field thrive on E = mc2 conversions. In fact, proper design of particle accelerators, as well as analysis of the high-speed collisions within them, would be impossible without a thorough comprehension of the equation. Within accelerators, colliding particles are constantly vanishing, leaving only energy, and dollops of energy are constantly transmuting into newly fashioned particles. "Our species has repeatedly used an understanding of the equation to convert E into new forms of m that had never previously been seen," Gates says. "One of the outposts of science for the next century may well be whether the E includes super-E, and m includes super-m-new forms of energy and matter called 'super-partners.'"

A grasp of the equivalence of mass and energy also comes in handy when studying antimatter. When a particle meets its antiparticle, they annihilate eachother, leaving only a pulse of energy; by the same token, a high-energy photon can suddenly become a particle-antiparticle pair. Altogether, says Hogg, "E = mc2 has been very important in diagnosing and understanding properties of antimatter."

Einstein's formula also accounts for the heat in our planet's crust, which is kept warm by a steady barrage of E = mc2 conversions occurring within unstable radioactive elements such as uranium and thorium. "When they decay, some of the mass is lost and a little energy is created, and that keeps the crust warm," says John Rigden, a physicist at Washington University in St. Louis and author of Einstein 1905: The Standard of Greatness (Harvard, 2005). "So the temperature of the outer Earth, the crustal matter, is directly related to E = mc2."

A cosmological constant

A similar process happens far beyond Earth, inside stars. The warmth we feel from the sun, for example, is the result of the energy generated as hydrogen deep within our star continuously fuses to form helium. And stars don't stop there. When they exhaust their hydrogen, they begin to burn new fuels and create new elements, which are spewed out into the universe when the stars eventually explode, as burnt-out stars are wont to do. "The carbon, oxygen, nitrogen, and hydrogen that make up living organisms were baked in the innards of a star," Rigden says. "In terms of what goes on in stars, we owe our existence to E = mc2."

Einstein's equation even tells of what transpires at black holes, which can contain the mass of millions of stars. Here, E = mc2 is taking place on an astronomical-and highly efficient-scale. "In a nuclear process, you convert something like one part in 1,000 of your rest mass into energy, whereas if you fall into a black hole, you can convert something like 20, 30, 40 percent," Hogg says. "So from the point of view of the energetics of the universe, these black holes are important, because they are big converters of rest mass into energy."

On the largest scale of all-the beginning of the universe-E = mc2 is the only accepted explanation for what was going on. In the first seconds after the big bang, energy and matter went back and forth indiscriminately in exact accordance with the equation. "The description of how the big bang unfolds would be much, much different if you couldn't interconvert mass to energy," Crotts says. If it weren't for E = mc2, the universe would have ended up with a completely different collection of particles than we have now. "I'm not sure what we would have, but we definitely wouldn't be here," he says.

Intangible aspects

The equation's legacy extends into realms well beyond the scientific. David Hogg finds it very useful in teaching, for instance. "I use the equation a lot in class because it's the one equation that all students have definitely heard of," he says. "So one of its legacies is very sociological: it just captures the imagination of everyone." It also helps students remember the units of energy. "A joule is a kilogram meter squared per second squared, and the way you remember that is E = mc2," he says.

Arlin Crotts notes the world Einstein's equation opened up for us. "It just laid bare the fact that all this stuff lying around us is potentially a tremendous reservoir of energy, almost beyond the imagination, if only we could devise ways to get at it," he says. "And that's just an amazing fact." For John Rigden, the equation and Einstein's other leaps of imagination revealed how scientists can be just as visionary as artists, writers, and other "creative" types. "What he did," Rigden says, "has all the creativity in it of Absalom, Absalom or Monet's lily pads."

Jim Gates seconds that. Until Einstein's time, scientists typically would observe things, record them, then find a piece of mathematics that explained the results, he says. "Einstein exactly reverses that process. He starts off with a beautiful piece of mathematics that's based on some very deep insights into the way the universe works and then, from that, makes predictions about what ought to happen in the world. It's a stunning reversal to the usual ordering in which science is done. So that's one of the legacies, that we've learned the power of human creativity in the sciences-or, as Einstein himself might have said, 'to know the mind of God.'"

In the end, the equation's influence, on both scientific and sociological fronts, is indeed hard to separate from Einstein's influence as a whole-which, like E = mc2-derived heat from the sun, shows no sign of diminishing.

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E = mc2

Hear Einstein himself briefly explain E = mc2.

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Walnut

Energy in a nutshell: though it hardly looks full of pep, a simple walnut has enough potential energy locked within it to power a city.

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PET scan

Every time a patient undergoes a positron emission tomography, or PET, scan, she is "paying direct homage to Einstein's insight," Jim Gates says.

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Hand and Sun

Astounding as it seems, the elements that make up our bodies and all other matter on Earth originated within stars like our sun, which are veritable E = mc2 factories.

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Water lilies

Many people today, and not just historians of science, would argue that Einstein's brainstorms and the papers that resulted from them have all the beauty and imagination of a Monet painting.

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Einstein's Big Idea

Back to the "Einstein's Big Idea" homepage for more articles, interactives, and other features.



Peter Tyson is editor in chief of NOVA online.



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The Producer's Story:
Why Einstein Was Like Picasso
by Gary Johnstone


Einstein's Big Idea homepage

"After a certain high level of technical skill is achieved, science and art tend to coalesce in esthetics, plasticity, and form. The greatest scientists are always artists as well."
-Albert Einstein

I couldn't agree more with Einstein's point of view here. I've long taken issue with the false dichotomy presumed to exist between art and science. The idea that artists possess a special sensitivity and insight that is their exclusive preserve is laughable. The idea that the great human leaps of imagination that catapult science onto new levels are somehow different to remarkable insights in painting or sculpture also doesn't hold water. To me, creativity is something we are all born with, and it either gets encouraged or stamped on. Either way, creativity is vital to progress in all human fields.

I've discussed this notion with the great Hollywood director James Cameron, with whom I codirected a film about the battleship Bismarck a couple of years back. Being at sea for four weeks, we eventually got onto the subject of our respective parents. It turns out we have similar backgrounds: parents who were both engineers and artists. When you grow up immersed in both of these areas, you don't see them as separate. In fact, there is no separation. Art and science are only ripped asunder by culture.

With backgrounds on both sides of the camp, it's also not surprising that Jim and I became filmmakers. Filmmaking is, most people would assume, at least a craft, at times an art. But it is also hugely technical. Federico Fellini once said that filmmakers have to know how everything on the set works and what it costs, down to the last lightbulb. Only then can they wrestle every last piece of beauty out of their limited resources. No one embodies this more than Jim Cameron. He may have had $270 million to make Titanic, but after everyone had gone to bed every night on the shoot, he and his brother Mike were still setting up special cameras for the next day, cameras they had built themselves.

So what does all this have to do with the NOVA program "Einstein's Big Idea"? Well, I just wanted to point out that I tend to be overreceptive to stories that demonstrate the deep unity of creativity in all human endeavor. When I was asked to write and direct a film based on David Bodanis' book E = mc2: A Biography of the World's Most Famous Equation, I jumped at the opportunity.

Putting E = mc2 to film

Adapting David's book for the small screen was an enormous challenge. To be honest, any sane person would have turned it down. Making a biographical film means immersing yourself in the minutiae of a character's life; having to do that for lots of famous scientists is a monumental task. Very quickly I decided that the list of 20 or so scientists that David featured in his book would have to be rationalized down to about six: Einstein, of course; Michael Faraday as an example of "E" (energy); Antoine-Laurent Lavoisier for "m" (mass); James Clerk Maxwell for "c" (the speed of light); and Emilie du Châtelet for "2"(squared). And finally, one great example of how the whole equation works in practice: Lise Meitner and unlocking the atom.

All I had to do then was understand the last 200 years of physics and chemistry!

So what sustained me in the three months I had to educate myself in relativity, nuclear physics, and advanced mathematics? Well, in between the mind-blowing conversations with patient professors, the headaches from the strain of trying to comprehend complex theories, and the backaches from lifting dusty tomes off library shelves, a single thought kept nagging at me. It was the kernel of an idea that probably seems insignificant to most, but it inspired me: Einstein was just like Picasso. What, you say? I repeat: Einstein was just like Picasso.

Birds of a feather

Awhile ago I made a film about the groundbreaking painter, and when I took the E = mc2 project on, I was instantly struck with the notion that Einstein was just as creative as Pablo Picasso. The great scientist was also just as bohemian in his lifestyle as the great artist. He was equally promiscuous, poetic, and playful. Above all, the two shared an indomitable self-determination. To both men, their personal project, their journey of discovery was the most important aspect of their lives.

The more I read about the other scientists in E = mc2, the more I realized they were all united by this quality of character. The greats of history are those who are utterly committed to going beyond the bounds of what already exists in their field. It is an obsession to know, to see, to feel the unknowable. Along the way, these singular individuals all have moments of incredible creativity, moments when the world they are immersed in suddenly shifts in front of their eyes. A crack opens up, and how we all conceive of the world changes irrevocably.

My hope is that viewers get even a tenth of the excitement I felt when reading David's book for the first time.

Of course, what happens in those peoples' lives is that everything and everyone else inevitably plays second fiddle. The attraction of exploring the world of E = mc2, at least for me, was this proposition: that achieving greatness somehow leads to a bittersweet compromise in other areas of life. What fascinated me was that behind each of these iconic, idealized characters of science was a life that was as messy, complex, and difficult as the next person's.

It would be wrong, however, to view any of these leading thinkers' lives purely as personal tragedy. Their achievements are unquestionably triumphs. The trick with the film was to somehow unite an illumination of their creative, scientific insights with the moving drama of the struggles they underwent to achieve those insights.

The power of drama

So how do you make a film about nuclear physics, abstract ideas, and some of the most creative individuals that have ever lived, all rolled into one, and still entertain a wide audience? After all, this was to be a film about ideas-there wasn't going to be much to point the camera at.

Drama seemed to me the only answer. And to make the experience as compelling as the real thing, the drama had to be full dialogue. I wanted top actors to delve into the personality of each character and capture the moment. An actor's job is to be emotionally real on screen. Just having some extras wander about looking a bit like Einstein and company while a narrator insists that this is one of history's seminal moments seemed lame. On the other hand, you simply can't have actors, no matter how good they are, explaining what is going on in the realm of abstract ideas. It's false and tacky. Real people don't do that. That is the job of narration or on-screen experts.

So I ended up with a hybrid. To cut a long story short, I then just sat down and wrote the darn thing. I came up with a five-act structure that seemed to work. I drew character charts. I used as many real scenes as I could. Everything is based to a large extent on real events. Obviously dialogue is largely invented, though it's sometimes based on quotations. I tried to write in a sprightly way. The last thing I wanted to produce was a turgid encyclopedia of E = mc2. If anything, the finished script has a fairytale quality. Many people may take exception to that. I admit that the finished film is at times hyperreal.

Getting it

My hope is that viewers get even a tenth of the excitement I felt when reading David's book for the first time. Here was a subject that most would assume closed to them, but by the end of the book I got it. I understood not just E = mc2 but also the beauty, pain, and wonder behind its creation. I was very lucky that NOVA largely liked my script. God knows what would have happened had they not bought into it.

The script, of course, was just the beginning. The film shoot was a ludicrous proposition: a six-week period drama on location in England, France, and Switzerland, all on a TV drama-doc budget. That is a long, long story in itself. Suffice to say I owe a lot of people a lot of favors.

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Einstein and Picasso

Promiscuity, playfulness, genius: just some of the traits that Einstein and Picasso had in common, says Gary Johnstone.

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Gary and McArdle on platform

Chilled by a morning mist, Gary Johnstone (right) prepares to shoot a scene with the young Einstein, played by Aidan McArdle.

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Einstein and Mileva at work

Einstein became so obsessed with his work that he seriously neglected his marriage to his wife Mileva Maric (played here by Shirley Henderson). The couple eventually divorced.

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Crew in Cafe

Johnstone's film crew shoots a scene of the 26-year-old Einstein (far right) holding forth in a café.

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Einstein's Big Idea

Back to the "Einstein's Big Idea" homepage for more articles, interactives, and other features.



Futher Reading
E = mc2: A Biography of the World's Most Famous Equation
by David Bodanis
New York: Berkley Books, 2000

Einstein, Picasso: Space, Time, and the Beauty That Causes Havoc
by Arthur I. Miller
New York: Basic Books, 2002



Gary Johnstone Gary Johnstone, the director and producer of "Einstein's Big Idea," has directed and/or produced many films, including the PBS documentaries "The Battle of Hood and Bismarck" and "Secrets of the Dead: Catastrophe!"



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Einstein the Nobody
by David Bodanis


Einstein's Big Idea homepage

13 April 1901

Professor Wilhelm Ostwald
University of Leipzig
Leipzig, Germany

Esteemed Herr Professor!

Please forgive a father who is so bold as to turn to you, esteemed Herr Professor, in the interest of his son.

I shall start by telling you that my son Albert is 22 years old, that ... he feels profoundly unhappy with his present lack of position, and his idea that he has gone off the tracks with his career & is now out of touch gets more and more entrenched each day. In addition, he is oppressed by the thought that he is a burden on us, people of modest means....

I have taken the liberty of turning [to you] with the humble request to ... write him, if possible, a few words of encouragement, so that he might recover his joy in living and working.

If, in addition, you could secure him an Assistant's position for now or the next autumn, my gratitude would know no bounds....

I am also taking the liberty of mentioning that my son does not know anything about my unusual step.

I remain, highly esteemed Herr Professor,
your devoted

Hermann Einstein

-From the collected papers of Albert Einstein, Volume I. No answer from Professor Ostwald was ever received.

Before the miracle year

The world of 1905 seems distant to us now, but there were many similarities to life today. European newspapers complained that there were too many American tourists, while Americans were complaining that there were too many immigrants. The older generation everywhere complained that the young were disrespectful, while politicians in Europe and America worried about the disturbing turbulence in Russia. There were newfangled "aerobics" classes; there was a trend-setting vegetarian society, and calls for sexual freedom (which were rebuffed by traditionalists standing for family values), and much else.

The year 1905 was also when Einstein wrote a series of papers that changed our view of the universe forever. On the surface, he seemed to have been leading a pleasant, quiet life until then. He had often been interested in physics puzzles as a child, and was now a recent university graduate, easygoing enough to have many friends. He had married a bright fellow student, Mileva Maric, and was earning enough money from a civil service job in the patent office to spend his evenings and Sundays in pub visits, or long walks-above all, he had a great deal of time to think.

Although his father's letter hadn't succeeded, a friend of Einstein's from the university, Marcel Grossman, had pulled the right strings to get Einstein the patent job in 1902. Grossman's help was necessary not so much because Einstein's final university grades were unusually low-through cramming with the ever-useful Grossman's notes, Einstein had just managed to reach a 4.91 average out of a possible 6, which was almost average-but because one professor, furious at Einstein for telling jokes and cutting classes, had spitefully written unacceptable references. Teachers over the years had been irritated by his lack of obedience, most notably Einstein's high school Greek grammar teacher, Joseph Degenhart, the one who has achieved immortality in the history books through insisting that "nothing would ever become of you." Later, when told it would be best if he left the school, Degenhart had explained, "Your presence in the class destroys the respect of the students."

Slipping behind

Outwardly Einstein appeared confident and would joke with his friends about the way everyone in authority seemed to enjoy putting him down. The year before, in 1904, he had applied for a promotion from patent clerk third class to patent clerk second class. His supervisor, Dr. Friedrich Haller, had rejected him, writing in an assessment that although Einstein had "displayed some quite good achievements," he would still have to wait "until he has become fully familiar with mechanical engineering."

In reality, though, the lack of success was becoming serious. Einstein and his wife had given away their first child, a daughter born before they were married, and were now trying to raise the second on a patent clerk's salary. Einstein was 26. He couldn't even afford the money for part-time help to let his wife go back to her studies. Was he really as wise as his adoring younger sister, Maja, had told him?

He managed to get a few physics articles published, but they weren't especially impressive. He was always aiming for grand linkages-his very first paper, published back in 1901, had tried to show that the forces controlling the way liquid rises up in a drinking straw were similar, fundamentally, to Newton's laws of gravitation. But he could not quite manage to get these great linkages to work, and he got almost no response from other physicists. He wrote to his sister, wondering if he'd ever make it.

"The idea is amusing and enticing, but whether the Lord is laughing at it ... that I cannot know."

Even the hours he had to keep at the patent office worked against him. By the time he got off for the day, the one science library in Bern was usually closed. How would he have a chance if he couldn't even stay up to date with the latest findings? When he did have a few free moments during the day, he would scribble on sheets he kept in one drawer of his desk-which he jokingly called his department of theoretical physics. But Haller kept a strict eye on him, and the drawer stayed closed most of the time. Einstein was slipping behind, measurably, compared to the friends he'd made at the university. He talked with his wife about quitting Bern and trying to find a job teaching high school. But even that wasn't any guarantee: he had tried it before, only four years earlier, but never managed to get a permanent post.

The turning point

And then, on what Einstein later remembered as a beautiful day in the spring of 1905, he met his best friend, Michele Besso ("I like him a great deal," Einstein wrote, "because of his sharp mind and his simplicity"), for one of their long strolls on the outskirts of the city. Often they just gossiped about life at the patent office, and music, but today Einstein was uneasy. In the past few months a great deal of what he'd been thinking about had started coming together, but there was still something Einstein felt he was very near to understanding but couldn't quite see. That night Einstein still couldn't quite grasp it, but the next day he suddenly woke up feeling "the greatest excitement."

It took just five or six weeks to write up a first draft of the article, filling 30-some pages. It was the start of his theory of relativity. He sent the article to Annalen der Physik to be published, but a few weeks later, he realized that he had left something out. A three-page supplement was soon delivered to the same physics journal. He admitted to another friend that he was a little unsure how accurate the supplement was: "The idea is amusing and enticing, but whether the Lord is laughing at it and has played a trick on me-that I cannot know."

But in the text itself he began confidently: "The results of an electrodynamic investigation recently published by me in this journal lead to a very interesting conclusion, which will be derived here." And then, four paragraphs from the end of this supplement, he wrote it out.

E = mc2 had arrived in the world.

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Einstein at lectern

It's almost impossible today to imagine Albert Einstein having trouble gaining a foothold in the world of physics, but such was the case for him in his early 20s. Here, he stands at a lectern in the Bern patent office in 1904.

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Einstein as a boy

Even as a boy, Albert, seen here with his sister Maja about 1884, enjoyed physics-related puzzles.

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Einstein in 1905

Einstein in 1905, the year he published a series of groundbreaking papers that would forever change our view of the world

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Einstein's Big Idea

Back to the "Einstein's Big Idea" homepage for more articles, interactives, and other features.



Bodanis David Bodanis is the author of E = mc2: A Biography of the World's Most Famous Equation (Berkley Books, 2000), on which the NOVA program "Einstein's Big Idea" is based and from which this article is excerpted with kind permission of the publisher.



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Relativity and the Cosmos
by Alan Lightman


Einstein's Big Idea homepage

In November of 1919, at the age of 40, Albert Einstein became an overnight celebrity, thanks to a solar eclipse. An experiment had confirmed that light rays from distant stars were deflected by the gravity of the sun in just the amount he had predicted in his theory of gravity, general relativity. General relativity was the first major new theory of gravity since Isaac Newton's more than 250 years earlier.

Einstein became a hero, and the myth-building began. Headlines appeared in newspapers all over the world. On November 8, 1919, for example, the London Times had an article headlined: "The Revolution In Science/Einstein Versus Newton." Two days later, The New York Times' headlines read: "Lights All Askew In The Heavens/Men Of Science More Or Less Agog Over Results Of Eclipse Observations/Einstein Theory Triumphs." The planet was exhausted from World War I, eager for some sign of humankind's nobility, and suddenly here was a modest scientific genius, seemingly interested only in pure intellectual pursuits.

The essence of gravity

What was general relativity? Einstein's earlier theory of time and space, special relativity, proposed that distance and time are not absolute. The ticking rate of a clock depends on the motion of the observer of that clock; likewise for the length of a "yardstick." Published in 1915, general relativity proposed that gravity, as well as motion, can affect the intervals of time and of space. The key idea of general relativity, called the equivalence principle, is that gravity pulling in one direction is completely equivalent to an acceleration in the opposite direction. A car accelerating forwards feels just like sideways gravity pushing you back against your seat. An elevator accelerating upwards feels just like gravity pushing you into the floor.

If gravity is equivalent to acceleration, and if motion affects measurements of time and space (as shown in special relativity), then it follows that gravity does so as well. In particular, the gravity of any mass, such as our sun, has the effect of warping the space and time around it. For example, the angles of a triangle no longer add up to 180 degrees, and clocks tick more slowly the closer they are to a gravitational mass like the sun.

Many of the predictions of general relativity, such as the bending of starlight by gravity and a tiny shift in the orbit of the planet Mercury, have been quantitatively confirmed by experiment. Two of the strangest predictions, impossible ever to completely confirm, are the existence of black holes and the effect of gravity on the universe as a whole (cosmology).

Collapsed stars

A black hole is a region of space whose attractive gravitational force is so intense that no matter, light, or communication of any kind can escape. A black hole would thus appear black from the outside. (However, gas around a black hole can be very bright.) It is believed that black holes form from the collapse of stars. As long as they are emitting heat and light into space, stars are able to support themselves against their own inward gravity with the outward pressure generated by heat from nuclear reactions in their deep interiors.

Every star, however, must eventually exhaust its nuclear fuel. When it does so, its unbalanced self-gravitational attraction causes it to collapse. According to theory, if a burned-out star has a mass larger than about three times the mass of our sun, no amount of additional pressure can stave off total gravitational collapse. The star collapses to form a black hole. For a nonrotating collapsed star, the size of the resulting black hole is proportional to the mass of the parent star; a black hole with a mass three times that of our sun would have a diameter of about 10 miles.

General relativity may be the biggest leap of the scientific imagination in history.

The possibility that stars could collapse to form black holes was first theoretically "discovered" in 1939 by J. Robert Oppenheimer and Hartland Snyder, who were manipulating the equations of Einstein's general relativity. The first black hole believed to be discovered in the physical world, as opposed to the mathematical world of pencil and paper, was Cygnus X-1, about 7,000 light-years from Earth. (A light-year, the distance light travels in a year, is about six trillion miles.) Cygnus X-1 was found in 1970. Since then, a dozen excellent black hole candidates have been identified. Many astronomers and astrophysicists believe that massive black holes, with sizes up to 10 million times that of our sun, inhabit the centers of energetic galaxies and quasars and are responsible for their enormous energy release. Ironically, Einstein himself did not believe in the existence of black holes, even though they were predicted by his theory.

The start of everything

Beginning in 1917, Einstein and others applied general relativity to the structure and evolution of the universe as a whole. The leading cosmological theory, called the big bang theory, was formulated in 1922 by the Russian mathematician and meteorologist Alexander Friedmann. Friedmann began with Einstein's equations of general relativity and found a solution to those equations in which the universe began in a state of extremely high density and temperature (the so-called big bang) and then expanded in time, thinning out and cooling as it did so. One of the most stunning successes of the big bang theory is the prediction that the universe is approximately 10 billion years old, a result obtained from the rate at which distant galaxies are flying away from each other. This prediction accords with the age of the universe as obtained from very local methods, such as the dating of radioactive rocks on Earth.

According to the big bang theory, the universe may keep expanding forever, if its inward gravity is not sufficiently strong to counterbalance the outward motion of galaxies, or it may reach a maximum point of expansion and then start collapsing, growing denser and denser, gradually disrupting galaxies, stars, planets, people, and eventually even individual atoms. Which of these two fates awaits our universe can be determined by measuring the density of matter versus the rate of expansion. Much of modern cosmology, including the construction of giant new telescopes such as the new Keck telescope in Hawaii, has been an attempt to measure these two numbers with better and better accuracy. With the present accuracy of measurement, the numbers suggest that our universe will keep expanding forever, growing colder and colder, thinner and thinner.

General relativity may be the biggest leap of the scientific imagination in history. Unlike many previous scientific breakthroughs, such as the principle of natural selection, or the discovery of the physical existence of atoms, general relativity had little foundation upon the theories or experiments of the time. No one except Einstein was thinking of gravity as equivalent to acceleration, as a geometrical phenomenon, as a bending of time and space. Although it is impossible to know, many physicists believe that without Einstein, it could have been another few decades or more before another physicist worked out the concepts and mathematics of general relativity.


Note: This feature originally appeared on NOVA's "Einstein Revealed" Web site, which has been subsumed into the "Einstein's Big Idea" Web site.

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Einstein

If it were not for Einstein, several decades might have passed before another physicist worked out the concepts and mathematics of general relativity, Lightman says.





Einstein in elevator

Click the image above to see narrated animations of:

  • Einstein racing a light beam, a thought experiment that led him to special relativity;
  • Einstein in an elevator, which shows how gravity and acceleration are the same;
  • and the sun warping space-time, a visualization of general relativity




Black hole

A swirling gas disk around a probable black hole in M87 Galaxy





Distant galaxies

An image of distant galaxies taken by Hubble Deep Field








Einstein's Big Idea

Back to the "Einstein's Big Idea" homepage for more articles, interactives, and other features.



Lightman Alan Lightman, a physicist and novelist, is currently Adjunct Professor of Humanities at MIT. Some of his recent books are Einstein's Dreams, The Diagnosis, Reunion, A Sense of the Mysterious, and The Discoveries.



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Genius Among Geniuses
by Thomas Levenson


Einstein's Big Idea homepage

There is a parlor game physics students play: Who was the greater genius? Galileo or Kepler? (Galileo.) Maxwell or Bohr? (Maxwell, but it's closer than you might think.) Hawking or Heisenberg? (A no-brainer, whatever the best-seller lists might say. It's Heisenberg.) But there are two figures who are simply off the charts. Isaac Newton is one. The other is Albert Einstein. If pressed, physicists give Newton pride of place, but it's a photo finish-and no one else is in the race.

Newton's claim is obvious. He created modern physics. His system described the behavior of the entire cosmos, and while others before him had invented grand schemes, Newton's was different. His theories were mathematical, making specific predictions to be confirmed by experiments in the real world. Little wonder that those after Newton called him lucky-"for there is only one universe to discover, and he discovered it."

But what of Einstein? Well, Einstein felt compelled to apologize to Newton. "Newton, forgive me," Einstein wrote in his Autobiographical Notes. "You found the only way which, in your age, was just about possible for a man of highest thought and creative power." Forgive him? For what? For replacing Newton's system with his own-and, like Newton, for putting his mark on virtually every branch of physics.

Miracle year

That's the difference. Young physicists who play the "who's smarter" game are really asking "How will I measure up?" Is there a shot to match-if not Maxwell, then perhaps Lorentz? But Einstein? Don't go there. Match this:

  • In 1905, Einstein is 26, a patent examiner, working on physics on his own. After hours, he creates the special theory of relativity, in which he demonstrates that measurements of time and distance vary systematically as anything moves relative to anything else. Which means that Newton was wrong. Space and time are not absolute, and the relativistic universe we inhabit is not the one Newton "discovered."

That's pretty good, but one idea, however spectacular, does not make a demigod. But now add the rest of what Einstein did in 1905:

  • In March, Einstein creates the quantum theory of light, the idea that light exists as tiny packets, or particles, that we now call photons. Alongside Max Planck's work on quanta of heat, and Niels Bohr's later work on quanta of matter, Einstein's work anchors the most shocking idea in 20th-century physics: we live in a quantum universe, one built out of tiny, discrete chunks of energy and matter.

  • Next, in April and May, Einstein publishes two papers. In one he invents a new method of counting and determining the size of the atoms or molecules in a given space, and in the other he explains the phenomenon of Brownian motion. The net result is a proof that atoms actually exist-still an issue at that time-and the end to a millennia-old debate on the fundamental nature of the chemical elements.

  • And then, in June, Einstein completes special relativity, which adds a twist to the story: Einstein's March paper treated light as particles, but special relativity sees light as a continuous field of waves. Alice's Red Queen can accept many impossible things before breakfast, but it takes a supremely confident mind to do so. Einstein, age 26, sees light as wave and particle, picking the attribute he needs to confront each problem in turn. Now that's tough.

  • And, of course, Einstein isn't finished. Later in 1905 comes an extension of special relativity in which Einstein proves that energy and matter are linked in the most famous relationship in physics: E = mc2. (The energy content of a body is equal to the mass of the body times the speed of light squared.) At first, even Einstein does not grasp the full implications of his formula, but even then he suggests that the heat produced by radium could mark the conversion of tiny amounts of the mass of the radium salts into energy.

In sum, an amazing outburst: Einstein's 1905 still evokes awe. Historians call it the annus mirabilis, the miracle year. Einstein ranges from the smallest scale to the largest (for special relativity is embodied in all motion throughout the universe), through fundamental problems about the nature of energy, matter, motion, time, and space-all the while putting in 40 hours a week at the patent office.

Who's smarter? No one since Newton comes close.

Further miracles

And that alone would have been enough to secure Einstein's reputation. But it is what comes next that is almost more remarkable. After 1905, Einstein achieves what no one since has equaled: a 20-year run at the cutting edge of physics. For all the miracles of his miracle year, his best work is still to come:

  • In 1907, he confronts the problem of gravitation, the same problem that Newton confronted and solved (almost). Einstein begins his work with one crucial insight: gravity and acceleration are equivalent, two facets of the same phenomenon. Where this "principle of equivalence" will lead remains obscure, but to Einstein, it offers the first hint of a theory that could supplant Newton's.

  • Before anyone else, Einstein recognizes the essential dualism in nature, the coexistence of particles and waves at the level of quanta. In 1911, he declares resolving the quantum issue to be the central problem of physics.

  • Even the minor works resonate. For example, in 1910, Einstein answers a basic question: "Why is the sky blue?" His paper on the phenomenon called critical opalescence solves the problem by examining the cumulative effect of the scattering of light by individual molecules in the atmosphere.

  • Then, in 1915, Einstein completes the general theory of relativity, the product of eight years of work on the problem of gravity. In general relativity, Einstein shows that matter and energy-all the "stuff" in the universe-actually mold the shape of space and the flow of time. What we feel as the "force" of gravity is simply the sensation of following the shortest path we can through curved, four-dimensional space-time. It is a radical vision: space is no longer the box the universe comes in; instead, space and time, matter and energy are, as Einstein proves, locked together in the most intimate embrace.

  • In 1917, Einstein publishes a paper that uses general relativity to model the behavior of an entire universe. General relativity has spawned some of the weirdest and most important results in modern astronomy (see Relativity and the Cosmos), but Einstein's paper is the starting point, the first in the modern field of cosmology-the study of the behavior of the universe as a whole. (It is also the paper in which Einstein makes what he would call his worst blunder-inventing a "cosmological constant" to keep his universe static. When Einstein learned of Edwin Hubble's observations that the universe is expanding, he promptly jettisoned the constant.)

  • Returning to the quantum, by 1919, six years before the invention of quantum mechanics and the uncertainty principle, Einstein recognizes that there might be a problem with the classical notion of cause and effect. Given the peculiar dual nature of quanta as both waves and particles, it might be impossible, he warns, to definitively tie effects to their causes.

  • Yet as late as 1924 and 1925, Einstein still makes significant contributions to the development of quantum theory. His last work on the theory builds on ideas developed by Satyendra Nath Bose and predicts a new state of matter (to add to the list of solid, liquid, and gas) called a Bose-Einstein condensate. The condensate was finally created at exceptionally low temperatures only in 1995.

In sum, Einstein is famous for his distaste for modern quantum theory, largely because its probabilistic nature forbids a complete description of cause and effect. But still he recognizes many of the fundamental implications of the idea of the quantum long before the rest of the physics community does.

The miracle that eluded him

After the quantum mechanical revolution of 1925 through 1927, Einstein spends the bulk of his remaining scientific career searching for a deeper theory to subsume quantum mechanics and eliminate its probabilities and uncertainties. It is the end, as far as his contemporaries believe, of Einstein's active participation in science. He generates pages of equations, geometrical descriptions of fields extending through many dimensions that could unify all the known forces of nature. None of the theories works out. It is a waste of time-and yet:

Contemporary theoretical physics is dominated by what is known as "string theory." It is multidimensional. (Some versions include as many as 26 dimensions, with 15 or 16 curled up in a tiny ball.) It is geometrical: the interactions of one multidimensional shape with another produces the effects we call forces, just as the "force" of gravity in general relativity is what we feel as we move through the curves of four-dimensional space-time. And it unifies, no doubt about it: in the math, at least, all of nature from quantum mechanics to gravity emerges from the equations of string theory.

As it stands, string theory is unproved, and perhaps unprovable, as it involves interactions at energy levels far beyond any we can handle. But to those versed enough in the language of mathematics to follow it, it is beautiful. And in its beauty (and perhaps in its impenetrability), string theory is the heir to Einstein's primitive first attempts to produce a unified field theory.

Between 1905 and 1925, Einstein transformed humankind's understanding of nature on every scale, from the smallest to that of the cosmos as a whole. Now, a century after he began to make his mark, we are still exploring Einstein's universe. The problems he could not solve remain the ones that define the cutting edge, the most tantalizing and compelling.

You can't touch that. Who's smarter? No one since Newton comes close.


Note: This feature originally appeared on NOVA's "Einstein Revealed" Web site, which has been subsumed into the "Einstein's Big Idea" Web site.

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Newton and Einstein

Who was smarter, Newton or Einstein? "It's a photo finish," Levenson says.











Planck and Bohr

Quantum theory owes its existence to Einstein's work as well as that of Max Planck (left) and Niels Bohr (right).











Marie Curie

Marie Curie's research with radium led Einstein to suggest that that radioactive element might be exhibiting E = mc2 in miniature. In time, he was shown to be right.











Bose

Bose-Einstein condensates, a new form of matter that Einstein predicted in the 1920s and that was first seen in the 1990s, are named in his honor and that of Indian physicist Satyendranath Bose (above).











The Elegant Universe

To learn more about string theory, see NOVA's Elegant Universe Web site.














Einstein's Big Idea

Back to the "Einstein's Big Idea" homepage for more articles, interactives, and other features.



Levenson Thomas Levenson, an independent filmmaker, produced the NOVA program "Einstein Revealed," which originally aired in 1996. He has published three books, most recently Einstein in Berlin (Bantam, 2004), and he is also a lecturer in the graduate science writing program at MIT.



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The Theory Behind the Equation
by Michio Kaku


Einstein's Big Idea homepage

Imagine a police officer chasing after a speeding motorist. If he drives fast enough, the officer knows that he can catch the motorist. Anyone who has ever gotten a ticket for speeding knows that. But if we now replace the speeding motorist with a light beam, and an observer witnesses the whole thing, then the observer concludes that the officer is speeding just behind the light beam, traveling almost as fast as light. We are confident that the officer knows he is traveling neck and neck with the light beam.

But later, when we interview him, we hear a strange tale. He claims that instead of riding alongside the light beam as we just witnessed, it sped away from him, leaving him in the dust. He says that no matter how much he gunned his engines, the light beam sped away at precisely the same velocity. In fact, he swears that he could not even make a dent in catching up to the light beam. No matter how fast he traveled, the light beam traveled away from him at the speed of light, as if he were stationary instead of speeding in a police car.

But when you insist that you saw the police officer speeding neck and neck with the light beam, within a hairsbreadth of catching up to it, he says you are crazy; he never even got close. To Einstein, this was the central, nagging mystery: How was it possible for two people to see the same event in such totally different ways? If the speed of light was really a constant of nature, then how could a witness claim that the officer was neck and neck with the light beam, yet the officer swears that he never even got close?

Einstein had realized earlier that the Newtonian picture (where velocities can be added and subtracted) and the Maxwellian picture (where the speed of light was constant) were in total contradiction. Newtonian theory was a self-contained system, resting on a few assumptions. If only one of these assumptions were changed, it would unravel the entire theory in the same way that a loose thread can unravel a sweater. That thread would be Einstein's daydream of racing a light beam.

Special relativity is born

One day around May of 1905, Einstein went to visit his good friend Michele Besso, who also worked at the patent office, and laid out the dimensions of the problem that had puzzled him for a decade. Using Besso as his favorite sounding board for ideas, Einstein presented the issue: Newtonian mechanics and Maxwell's equations, the two pillars of physics, were incompatible. One or the other was wrong. Whichever theory proved to be correct, the final resolution would require a vast reorganization of all of physics. He went over and over the paradox of racing a light beam. Einstein would later recall, "The germ of the special relativity theory was already present in that paradox." They talked for hours, discussing every aspect of the problem, including Newton's concept of absolute space and time, which seemed to violate Maxwell's constancy of the speed of light. Eventually, totally exhausted, Einstein announced that he was defeated and would give up the entire quest. It was no use; he had failed.

Although Einstein was depressed, his thoughts were still churning in his mind when he returned home that night. In particular, he remembered riding in a streetcar in Bern and looking back at the famous clock tower that dominated the city. He then imagined what would happen if his streetcar raced away from the clock tower at the speed of light. He quickly realized that the clock would appear stopped, since light could not catch up to the streetcar, but his own clock in the streetcar would beat normally.

Then it suddenly hit him, the key to the entire problem. Einstein recalled, "A storm broke loose in my mind." The answer was simple and elegant: time can beat at different rates throughout the universe, depending on how fast you moved. Imagine clocks scattered at different points in space, each one announcing a different time, each one ticking at a different rate. One second on Earth was not the same length as one second on the moon or one second on Jupiter. In fact, the faster you moved, the more time slowed down. (Einstein once joked that in relativity theory, he placed a clock at every point in the universe, each one running at a different rate, but in real life he didn't have enough money to buy even one.) This meant that events that were simultaneous in one frame were not necessarily simultaneous in another frame, as Newton thought. He had finally tapped into "God's thoughts." He would recall excitedly, "The solution came to me suddenly with the thought that our concepts and laws of space and time can only claim validity insofar as they stand in a clear relation to our experiences.... By a revision of the concept of simultaneity into a more malleable form, I thus arrived at the theory of relativity."

"Thank you, I've completely solved the problem."

For example, remember that in the paradox of the speeding motorist, the police officer was traveling neck and neck with the speeding light beam, while the officer himself claimed that the light beam was speeding away from him at precisely the speed of light, no matter how much he gunned his engines. The only way to reconcile these two pictures is to have the brain of the officer slow down. Time slows down for the policeman. If we could have seen the officer's wristwatch from the roadside, we would have seen that it nearly stopped and that his facial expressions were frozen in time. Thus, from our point of view, we saw him speeding neck and neck with the light beam, but his clocks (and his brain) were nearly stopped. When we interviewed the officer later, we found that he perceived the light beam to be speeding away, only because his brain and clocks were running much slower.

The paper that changed everything

The day after this revelation, Einstein went back to Besso's home and, without even saying hello, he blurted out, "Thank you, I've completely solved the problem." He would proudly recall, "An analysis of the concept of time was my solution. Time cannot be absolutely defined, and there is an inseparable relation between time and signal velocity." For the next six weeks, he furiously worked out every mathematical detail of his brilliant insight, leading to a paper that is arguably one of the most important scientific papers of all time. According to his son, he then went straight to bed for two weeks after giving the paper to his wife Mileva to check for any mathematical errors. The final paper, "On the Electrodynamics of Moving Bodies," was scribbled on 31 handwritten pages, but it changed world history.

In the paper, he does not acknowledge any other physicist; he only gives thanks to Michele Besso. It was finally published in Annalen der Physik in September 1905, in volume 17. In fact, Einstein would publish three of his pathbreaking papers in that famous volume 17. His colleague Max Born has written, volume 17 is "one of the most remarkable volumes in the whole scientific literature. It contains three papers by Einstein, each dealing with a different subject and each today acknowledged to be a masterpiece." (Copies of that famous volume sold for $15,000 at an auction in 1994.)

With almost breathtaking sweep, Einstein began his paper by proclaiming that his theories worked not just for light, but were truths about the universe itself. Remarkably, he derived all his work from two simple postulates applying to inertial frames (i.e., objects that move with constant velocity with respect to each other):

  1. The laws of physics are the same in all inertial frames.

  2. The speed of light is a constant in all inertial frames.

These two deceptively simple principles mark the most profound insights into the nature of the universe since Newton's work. From them, one can derive an entirely new picture of space and time.

Length, like time, is relative

First, in one masterful stroke, Einstein elegantly proved that if the speed of light was indeed a constant of nature, then the most general solution was the Lorentz transformation*. He then showed that Maxwell's equations did indeed respect that principle. Last, he showed that velocities add in a peculiar way. Although Newton, observing the motion of sailing ships, concluded that velocities could add without limit, Einstein concluded that the speed of light was the ultimate velocity in the universe. Imagine, for a moment, that you are in a rocket speeding at 90 percent the speed of light away from Earth. Now fire a bullet inside the rocket that is also going at 90 percent the speed of light. According to Newtonian physics, the bullet should be going at 180 percent the speed of light, thus exceeding light velocity. But Einstein showed that because meter sticks are shortening and time is slowing down, the sum of these velocities is actually close to 99 percent the speed of light. In fact, Einstein could show that no matter how hard you tried, you could never boost yourself beyond the speed of light. Light velocity was the ultimate speed limit in the universe.

We never see these bizarre distortions in our experience because we never travel near the speed of light. For everyday velocities, Newton's laws are perfectly fine. This is the fundamental reason why it took over 200 years to discover the first correction to Newton's laws. But now imagine that the speed of light is only 20 miles per hour. If a car were to go down the street, it might look compressed in the direction of motion, being squeezed like an accordion down to perhaps one inch in length, for example, although its height would remain the same. Because the passengers in the car are compressed down to one inch, we might expect them to yell and scream as their bones are crushed. In fact, the passengers see nothing wrong, since everything inside the car, including the atoms in their bodies, is squeezed as well.

As the car slows down to a stop, it would slowly expand from one inch to about 10 feet, and the passengers would walk out as if nothing happened. Who is really compressed? You or the car? According to relativity, you cannot tell, since the concept of length has no absolute meaning.

The greatest afterthought in history

Einstein then pushed further and made the next fateful leap. He wrote a small paper, almost a footnote, late in 1905 that would change world history. If meter sticks and clocks became distorted the faster you moved, then everything you can measure with meter sticks and clocks must also change, including matter and energy. In fact, matter and energy could change into each other. For example, Einstein could show that the mass of an object increased the faster it moved. (Its mass would in fact become infinite if you hit the speed of light-which is impossible, which proves the unattainability of the speed of light.) This meant that the energy of motion was somehow being transformed into increasing the mass of the object. Thus, matter and energy are interchangeable. If you calculated precisely how much energy was being converted into mass, in a few simple lines you could show that E = mc2, the most celebrated equation of all time. Since the speed of light was a fantastically large number, and its square was even larger, this meant that even a tiny amount of matter could release a fabulous amount of energy. A few teaspoons of matter, for example, has the energy of several hydrogen bombs. In fact, a piece of matter the size of a house might be enough to crack the Earth in half.

"Imagine the audacity of such a step ... every speck of dust becoming a prodigious reservoir of untapped energy."

Einstein's formula was not simply an academic exercise, because he believed that it might explain the curious fact discovered by Marie Curie, that just an ounce of radium emitted 4,000 calories of heat per hour indefinitely, seemingly violating the first law of thermodynamics (which states that the total amount of energy is always constant or conserved). He concluded that there should be a slight decrease in its mass as radium radiated away energy (an amount too small to be measured using the equipment of 1905). "The idea is amusing and enticing; but whether the Almighty is laughing at it and is leading me up the garden path-that I cannot know," he wrote. He concluded that a direct verification of his conjecture "for the time being probably lies beyond the realm of possible experience."

Why hadn't this untapped energy been noticed before? He compared this to a fabulously rich man who kept his wealth secret by never spending a cent.

Banesh Hoffman, a former student, wrote, "Imagine the audacity of such a step.... Every clod of earth, every feather, every speck of dust becoming a prodigious reservoir of untapped energy. There was no way of verifying this at the time. Yet in presenting his equation in 1907 Einstein spoke of it as the most important consequence of his theory of relativity. His extraordinary ability to see far ahead is shown by the fact that his equation was not verified ... until some twenty-five years later."

Once again, the relativity principle forced a major revision in classical physics. Before, physicists believed in the conservation of energy, the first law of thermodynamics, which states that the total amount of energy can never be created or destroyed. Now physicists considered the total combined amount of matter and energy as being conserved.


*Named for the Dutch physicist Hendrik Lorentz, who calculated them, the Lorentz transformations are the distortions of space and time inherent in the equations for light, i.e., Maxwell's equations. These transformations state that the faster you move, the slower time beats for you and the more compressed you become. (At the speed of light, hypothetically time would stop and distances would shrink to nothing, both of which are impossible.) These transformations are necessary to keep the speed of light a constant in all inertial frames.

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Newton and Maxell

Einstein realized that the world described by Isaac Newton (left), in which one could add and subtract velocities, and that described by James Clerk Maxwell, in which the speed of light is constant, could not both be right. He decided to solve the problem-and special relativity was the result.

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Einstein in patent office

Einstein in the Bern patent office in 1904, just months away from the brilliant insight that led to his theory of special relativity-and, a few weeks later, to E = mc2

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Bern clock tower

A streetcar trundles below the clock tower in Bern that Einstein made famous with his thought experiment about racing a light beam.

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Journal cover

Volume 17 of the German physics journal Annalen der Physik, in which Einstein published no fewer than three groundbreaking papers at age 26.

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1911 conference

Other scientists came close to stumbling upon relativity before Einstein, including the Dutch physicist Hendrik Lorentz (seated fourth from left) and the French mathematician Henri Poincaré (seated far right, next to Marie Curie). Einstein is standing second from right in this photo from a 1911 conference.

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Equation in manuscript

The world's most famous equation, as it appears in modified form in a manuscript on special relativity theory that Einstein wrote in 1912

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Einstein's Big Idea

Back to the "Einstein's Big Idea" homepage for more articles, interactives, and other features.



Michio Kaku Michio Kaku, a theoretical physicist at the City University of New York, is the author of Einstein's Cosmos: How Albert Einstein's Vision Transformed Our Understanding of Space and Time (Norton, 2004), from which this article was adapted with kind permission of the author and publisher.



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