Paperback ©2000 | -- |
Einstein, Albert,. 1879-1955.
Mathematical physics.
Mass (Physics).
Force and energy.
It's a well-known equation, yet who but physicists really understand E = 2? Bodanis rescues the masses from ignorance in an entertaining story about Einstein's formulation of the equation in 1905 and its association ever after with relativity and nuclear energy. Parallel with the science, Bodanis populates his tale with dramatic lives: Lavoisier mounts the scaffold; Faraday hauls himself up by his bootstraps; Einstein ponders light in his patent office; Lise Meitner gets no credit for discovering atomic fission; and Heisenberg works on a German atom bomb. Alhough Bodanis' elisions of their biographies adequately fill his popularization goal, they inevitably simplify historical complexities, as of Heisenberg's attitude toward Nazidom. On the brighter side, the science the author retells is wholly satisfying, from explaining the origin of each symbol in E = 2 to describing Faraday's unification of electricity and magnetism to Einstein's similar feat with matter, energy, and the weird war pages of time and space at light speeds. With anecdotes and illustrations, Bodanis effectively opens up E = 2 to the widest audience. (Reviewed August 2000)
Kirkus ReviewsA readable history and explanation of the only physics equation that has taken on a life of its own in popular culture. "Everyone knows that E=mc2 is really important, but they usually don't know what it means, and that's frustrating, because the equation is so short that you'd think it would be understandable," Oxford science lecturer Bodanis ( The Secret Family , 1997) confides in the preface. This paradox—that practically everyone can recite the formula, but hardly anyone understands it—spurred the author to write an accessible guide for nonscientists. His tone stays chatty and cheerfully enthusiastic through sketches of the various characters involved in the development of Einstein's equation, technical explanations of each of its components, and discussions of the theoretical and practical applications. His "biography" includes lively if superficial portraits of an assortment of colorful scientists, including Antoine-Laurent Lavoisier (who established the concept of mass before coming to a nasty end in the French Revolution) and Lise Meitner (whose explorations of the mechanisms of matter led to the evolution of laboratory techniques for splitting atoms); unfortunately, the author tends to reduce the physicists' specialized training and exceptional abilities to the kind of spunky rebelliousness familiar from Hollywood versions of scientific genius. The explications of the actual elements of the equation—energy, the equal sign, mass, celeritas , and the exponent—are just as entertaining, but they are also a little too glib (at least for anyone who floundered through high-school physics). There's a vivid explanation of the properties of light, for example, but the function of celeritas (the figure representing the speed of light) as a conversion factor in the equation goes by too quickly to be illuminating, at least for a genuine science dunce. However, the account of the development of the atomic bomb makes clear the interchangeability of matter and energy, as well as providing a fast-paced, suspenseful tale. Bodanis delivers on his promise to make the significance of Einstein's formula at least somewhat understandable for general readers. (20 b&w illustrations, not seen)
Starred Review for Library Journal
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Part 1, Birth
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
No answer from Professor Ostwald was ever received.
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, 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."
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. 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 twenty-six. 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.
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.
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 thirty-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.
—Reprinted from E=mc2, A Biography of the World's Most Famous Equation by David Bodanis by permission of Berkley, a member of Penguin Putnam Inc. Copyright © 2000, David Bodanis. All rights reserved. This excerpt, or any parts thereof, may not be reproduced in any form without permission.
Excerpted from E=mc2: A Biography of the World's Most Famous Equation by David Bodanis
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Already climbing the bestseller lists-and garnering rave reviewsthis "little masterpiece" sheds brilliant light on the equation that changed the world.
Bodanis begins by devoting chapters to each of the equation's letters and symbols, introducing the science and scientists forming the backdrop to Einstein's discoveryfrom Ole Roemer's revelation that the speed of light could be measured to Michael Faraday's pioneering work on energy fields. Having demystified the equation, Bodanis explains its science and brings it to life historically, making clear the astonishing array of discoveries and consequences it made possible. It would prove to be a beacon throughout the twentieth century, important to Ernest Rutherford, who discovered the structure of the atom, Enrico Fermi, who probed the nucleus, and Lise Meitner, who finally understood how atoms could be split wide open. And it has come to inform our daily lives, governing everything from the atomic bomb to a television's cathode-ray tube to the carbon dating of prehistoric paintings.
Preface
Part 1: Birth
1. Bern Patent Office, 1905
Part 2: Ancestors of E=mc²
2. E is for Energy
3. =
4. m Is for mass
5. c Is for celeritas
6. ²
Part 3: The Early Years
7. Einstein and the Equation
8. Into the Atom
9. Quiet in the Midday Snow
Part 4: Adulthood
10. Germany's Turn
11. Norway
12. America's Turn
13. 8:16 AM - Over Japan
Part 5: Til the End of Time
14. The Fires of the Sun
15. Creating the Earth
16. A Brahmin Lifts His Eyes Unto the Sky
Epilogue: What Else Einstein Did
Appendix: Follow-Up of Other Key Participants
Notes
Guide to Further Reading
Acknowledgments
Index