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Euclidean Quantum Gravity
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Bibliographic Detail
Publisher World Scientific Pub Co Inc
Publication date May 1, 1993
Binding Paperback
Book category Adult Non-Fiction
ISBN-13 9789810205164
ISBN-10 9810205163
Dimensions 1.25 by 6.50 by 9.75 in.
Weight 2.15 lbs.
Original list price $65.00
Other format details sci/tech
Summaries and Reviews
Amazon.com description: Product Description: The Euclidean approach to Quantum Gravity was initiated almost 15 years ago in an attempt to understand the difficulties raised by the spacetime singularities of classical general relativity which arise in the gravitational collapse of stars to form black holes and the entire universe in the Big Bang. An important motivation was to develop an approach capable of dealing with the nonlinear, non-perturbative aspects of quantum gravity due to topologically non-trivial spacetimes. There are important links with a Riemannian geometry. Since its inception the theory has been applied to a number of important physical problems including the thermodynamic properties of black holes, quantum cosmology and the problem of the cosmological constant. It is currently at the centre of a great deal of interest.This is a collection of survey lectures and reprints of some important lectures on the Euclidean approach to quantum gravity in which one expresses the Feynman path integral as a sum over Riemannian metrics. As well as papers on the basic formalism there are sections on Black Holes, Quantum Cosmology, Wormholes and Gravitational Instantons.

Editions
Hardcover
Book cover for 9789810205157
 
from World Scientific Pub Co Inc (August 1, 1993)
9789810205157 | details & prices | 7.25 × 10.50 × 1.50 in. | 2.50 lbs | List price $145.00
Paperback
Book cover for 9789810205164
 
The price comparison is for this edition
from World Scientific Pub Co Inc (May 1, 1993)
9789810205164 | details & prices | 6.50 × 9.75 × 1.25 in. | 2.15 lbs | List price $65.00
About: The Euclidean approach to Quantum Gravity was initiated almost 15 years ago in an attempt to understand the difficulties raised by the spacetime singularities of classical general relativity which arise in the gravitational collapse of stars to form black holes and the entire universe in the Big Bang.

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