A Brief History of Time: From the Big Bang to Black HolesBantam Books, 1990 - 198 páginas Stephen Hawking has earned a reputation as the most brilliant theoretical physicist since Einstein. In this landmark volume, Professor Hawking shares his blazing intellect with nonscientists everywhere, guiding us expertly to confront the supreme questions of the nature of time and the universe. Was there a beginning of time? Will there be an end? Is the universe infinite or does it have boundaries? From Galileo and Newton to modern astrophysics, from the breathtakingly cast to the extraordinarily tiny, Professor Hawking leads us on an exhilarating journey to distant galaxies, black holes, alternate dimensions--as close as man has ever ventured to the mind of God. From the vantage point of the wheelchair from which he has spent more than twenty years trapped by Lou Gehrig's disease, Stephen Hawking has transformed our view of the universe. Cogently explained, passionately revealed, "A Brief History of Time is the story of the ultimate quest for knowledge: the ongoing search for the tantalizing secrets at the heart of time and space. |
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Página 74
... weaker at high energies . On the other hand , the electromagnetic and weak forces , which are not asymptotically free , get stronger at high energies . At some very high energy , called the grand unification energy , three forces would ...
... weaker at high energies . On the other hand , the electromagnetic and weak forces , which are not asymptotically free , get stronger at high energies . At some very high energy , called the grand unification energy , three forces would ...
Página 77
... weak force does not in fact obey the symmetry P. In other words , the weak force would make the uni- verse develop in a different way from the way in which the mirror image of the universe would develop . The same year , a colleague ...
... weak force does not in fact obey the symmetry P. In other words , the weak force would make the uni- verse develop in a different way from the way in which the mirror image of the universe would develop . The same year , a colleague ...
Página 124
... weak and the strong . The weak anthropic principle states that in a universe that is large or infinite in space and / or time , the conditions neces- sary for the development of intelligent life will be met only in certain regions that ...
... weak and the strong . The weak anthropic principle states that in a universe that is large or infinite in space and / or time , the conditions neces- sary for the development of intelligent life will be met only in certain regions that ...
Otras ediciones - Ver todas
A Brief History of Time: From the Big Bang to Black Holes Stephen Hawking,Carl Sagan Vista de fragmentos - 1988 |
Términos y frases comunes
able according appear arrow atoms attraction beginning believed big bang black hole body boundary called caused collapse complete contracting density describe developed dimensions direction disorder distance early earth effect Einstein electrons emitted energy event event horizon example exist expanding explain fact fall field FIGURE force galaxies gravitational collapse gravity happen histories idea increase infinite initial known later laws less light limit look mass matter means measure million million million moving neutron Newton objects observe orbits particles past paths phase planets position possible predictions principle probably quantum mechanics quarks question radiation rays reason regions relativity result rotating seems showed single singularity space space-time speed stars started string suggested surface temperature theory thought uncertainty unified theory universe waves weak zero