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 91
... rotating black holes . These " Kerr " black holes rotate at a constant rate , their size and shape depending only on their mass and rate of rotation . If the rotation is zero , the black hole is perfectly round and the solution is ...
... rotating black holes . These " Kerr " black holes rotate at a constant rate , their size and shape depending only on their mass and rate of rotation . If the rotation is zero , the black hole is perfectly round and the solution is ...
Página 92
... rotating black hole had an axis of symmetry , like a spinning top , its size and shape would depend only on its mass and rate of rotation . Then , in 1971 , I proved that any stationary rotating black hole would indeed have such an axis ...
... rotating black hole had an axis of symmetry , like a spinning top , its size and shape would depend only on its mass and rate of rotation . Then , in 1971 , I proved that any stationary rotating black hole would indeed have such an axis ...
Página 119
... rotating galaxies were born . Other regions , which did not happen to pick up a rotation , would become oval - shaped objects called elliptical galaxies . In these , the region would stop collapsing because individual parts of the ...
... rotating galaxies were born . Other regions , which did not happen to pick up a rotation , would become oval - shaped objects called elliptical galaxies . In these , the region would stop collapsing because individual parts of the ...
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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