Great Physicists: The Life and Times of Leading Physicists from Galileo to HawkingHere is a lively history of modern physics, as seen through the lives of thirty men and women from the pantheon of physics. William H. Cropper vividly portrays the life and accomplishments of such giants as Galileo and Isaac Newton, Marie Curie and Ernest Rutherford, Albert Einstein and Niels Bohr, right up to contemporary figures such as Richard Feynman, Murray Gell-Mann, and Stephen Hawking. We meet scientists--all geniuses--who could be gregarious, aloof, unpretentious, friendly, dogged, imperious, generous to colleagues or contentious rivals. As Cropper captures their personalities, he also offers vivid portraits of their great moments of discovery, their bitter feuds, their relations with family and friends, their religious beliefs and education. In addition, Cropper has grouped these biographies by discipline--mechanics, thermodynamics, particle physics, and others--each section beginning with a historical overview. Thus in the section on quantum mechanics, readers can see how the work of Max Planck influenced Niels Bohr, and how Bohr in turn influenced Werner Heisenberg. Our understanding of the physical world has increased dramatically in the last four centuries. With Great Physicists, readers can retrace the footsteps of the men and women who led the way. |
From inside the book
Results 1-5 of 85
Page 5
... experiment a doctrine originated by Aristotle almost two thousand years earlier: that objects fall at a rate proportional to their weight; a ten-pound ball would fall ten times faster than a onepound ball. With a flourish the young ...
... experiment a doctrine originated by Aristotle almost two thousand years earlier: that objects fall at a rate proportional to their weight; a ten-pound ball would fall ten times faster than a onepound ball. With a flourish the young ...
Page 15
... experimental methods seem to us more modern. He devised a system of units that parallels our own and that served him well in his experiments on pendulum motion. His measure of distance, which he called a punto, was equivalent to 0.094 ...
... experimental methods seem to us more modern. He devised a system of units that parallels our own and that served him well in his experiments on pendulum motion. His measure of distance, which he called a punto, was equivalent to 0.094 ...
Page 24
... experimental and other observations. For that, integrated equations are often a necessity. The great misfortune is that some otherwise innocent-looking differential equations are extremely difficult to integrate. In some important cases ...
... experimental and other observations. For that, integrated equations are often a necessity. The great misfortune is that some otherwise innocent-looking differential equations are extremely difficult to integrate. In some important cases ...
Page 26
... experiment employing two prisms. The first prism separated sunlight into the usual red-through-violet components, and all ... experimental evidence; Hooke and Huygens would not grant the weight of that evidence. This was just the lesson ...
... experiment employing two prisms. The first prism separated sunlight into the usual red-through-violet components, and all ... experimental evidence; Hooke and Huygens would not grant the weight of that evidence. This was just the lesson ...
Page 35
... experimental foundations, and an attempt to lay the theoretical foundations, of the science of optics. He describes experiments that demonstrate the main physical properties of light rays: their reflection, “degree of refrangibility ...
... experimental foundations, and an attempt to lay the theoretical foundations, of the science of optics. He describes experiments that demonstrate the main physical properties of light rays: their reflection, “degree of refrangibility ...
Contents
41 | |
Historical Synopsis | 135 |
Historical Synopsis | 177 |
Historical Synopsis | 201 |
Historical Synopsis | 229 |
Historical Synopsis | 293 |
Historical Synopsis | 363 |
Historical Synopsis | 421 |
Chronology of the Main Events | 464 |
Glossary | 469 |
Invitation to More Reading | 478 |
Index | 485 |
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acceleration astronomer atomic became Berlin Bohr Bohr’s Boltzmann calculation called Cambridge Carnot’s Chandra charge chemical chemistry Clausius Clausius’s colleagues concept constant Curie Dirac discovery effect Einstein electric electromagnetic electron elements energy entropy experimental experiments Faraday Faraday’s Fermi Feynman field fission force function galaxy Galileo Gell-Mann Gibbs Gibbs energy Gibbs’s Glenlair Go¨ttingen gravitational Hahn Hawking heat engine Heisenberg Helmholtz Hubble Hubble’s hydrogen isospin Joule Joule’s laboratory later Laura Fermi lecture light Lise Meitner magnetic Marie mass mathematical mathematician matrix mechanics Maxwell Maxwell’s Mayer measured Meitner molecular molecules motion Nernst neutron Newton nuclear nucleus observed paper particles Pauli photons physicists Planck principle problem professor published quantum mechanics quantum number quantum theory quark radiation radioactive radium rays reaction Richard Feynman Rutherford Schro¨dinger scientific scientists speed statistical statistical mechanics temperature theoretical physics theorists thermodynamics Thomson tion University uranium wave writes wrote