Published 1990 | Version v1
Book

Baby universes

Creators

Description

This paper reports that in a reasonable theory of quantum gravity, the topology of spacetime must be able to be different from that of flat space. Otherwise, the theory would not be able to describe closed universes, or black holes. Presumably, the theory should allow all possible spacetime topologies. In particular, it should allow closed universes to branch off, or join onto, our asymptotic flat region of spacetime. Of course, such behavior is not possible with a real, non singular, Lorentzian metric. However, we now all know that quantum gravity has to be formulated in the Euclidean domain. There, it is no problem: it is just a question of plumbing

Additional details

Publishing Information

Publisher
World Scientific Pub. Co.
Imprint Place
Teaneck, NJ (United States)
ISBN
9971-50-899-0
Imprint Title
Proceedings of the Friedmann centenary conference
Imprint Pagination
327 p.
Journal Page Range
p. 81-92.

Conference

Title
Friedmann centenary conference.
Dates
22-26 Jun 1988.
Place
Leningrad (USSR).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
23055170
Subject category
S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
BLACK HOLES; EUCLIDEAN SPACE; LORENTZ TRANSFORMATIONS; METRICS; QUANTUM GRAVITY; SPACE-TIME; TOPOLOGY; UNIVERSE
Descriptors DEC
FIELD THEORIES; MATHEMATICAL SPACE; MATHEMATICS; QUANTUM FIELD THEORY; RIEMANN SPACE; SPACE

Optional Information

Secondary number(s)
CONF-8806514--.