The Large Scale Structure of Space-Time (1973) - Stephen
Hawking
The Large Scale Structure of Space-Time is 1973 book
by Stephen Hawking and George Ellis on the theoretical
physics of spacetime.
Hawking and Ellis attempt to describe the foundation of space
itself and its nature of infinite expansion, using differential
geometry to examine the consequences of Einstein's General Theory of
Relativity.
Hawking co-wrote the book with Ellis, while a post doc at Cambridge
University. In his 1988 book A Brief History of Time, he describes The
Large Scale Structure of Space-Time as "highly technical" and
unreadable for the common reader.
Einstein's General Theory of Relativity leads to two
remarkable predictions: first, that the ultimate destiny of many massive stars
is to undergo gravitional collapse and to disappear from view, leaving behind
a' black hole' in space; and secondly, that there will exist singularities in
space -time itself. These singularities are places where space-time begins or
ends, and the presently known laws of physics break down. They will occur
inside black holes, and in the past are what might be construed as the
beginning of the universe.
Einstein's General Theory of Relativity leads to two
remarkable predictions: first, that the ultimate destiny of many massive stars
is to undergo gravitational collapse and to disappear from view, leaving behind
a 'black hole' in space; and secondly, that there will exist singularities in
space-time itself. These singularities are places where space-time begins or
ends, and the presently known laws of physics break down. They will occur
inside black holes, and in the past are what might be construed as the
beginning of the universe. To show how these predictions arise, the authors
discuss the General Theory of Relativity in the large. Starting with a precise
formulation of the theory and an account of the necessary background of
differential geometry, the significance of space-time curvature is discussed
and the global properties of a number of exact solutions of Einstein's field
equations are examined. The theory of the causal structure of a general space-time
is developed, and is used to study black holes and to prove a number of
theorems establishing the inevitability of singualarities under certain
conditions. A discussion of the Cauchy problem for General Relativity is also
included in this 1973 book.
Book Description:
This 1973 book discusses Einstein's General Theory of
Relativity and its two remarkable predictions: first, that the ultimate destiny
of many massive stars is to undergo gravitational collapse and to disappear
from view, leaving behind a 'black hole' in space; and secondly, that there
will exist singularities in space-time itself.
"About this title" may belong to another edition of
this title.
Wormholes, although theoretical, are 'tunnels' or shortcuts predicted by Einstein's theory of relativity that link two places in space-time --- as visualized above --- where negative energy pulls space and time into the mouth of a tunnel, emerging in another time or place in the universe, or possibly even another universe. Wormholes remain hypothetical but have been used in science fiction and films as conduits for time travel, for example as found in the movie Time Bandits (1981), where their locations are shown on a celestial.
Wormholes, although theoretical, are 'tunnels' or shortcuts predicted by Einstein's theory of relativity that link two places in space-time --- as visualized above --- where negative energy pulls space and time into the mouth of a tunnel, emerging in another time or place in the universe, or possibly even another universe. Wormholes remain hypothetical but have been used in science fiction and films as conduits for time travel, for example as found in the movie Time Bandits (1981), where their locations are shown on a celestial.
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