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From big bang to big crunch and beyond

Shmuel Elitzur1, Amit Giveon1, David Kutasov2 and Eliezer Rabinovici1

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We study a quotient Conformal Field Theory, which describes a 3+1 dimensional cosmological spacetime. Part of this spacetime is the Nappi-Witten (NW) universe, which starts at a ``big bang'' singularity, expands and then contracts to a ``big crunch'' singularity at a finite time. The gauged WZW model contains a number of copies of the NW spacetime, with each copy connected to the preceeding one and to the next one at the respective big bang/big crunch singularities. The sequence of NW spacetimes is further connected at the singularities to a series of non-compact static regions with closed timelike curves. These regions contain boundaries, on which the observables of the theory live. This suggests a holographic interpretation of the physics.


Keywords

AdS-CFT and dS-CFT Correspondence

Conformal Field Models in String Theory

 

E-print Number: hep-th/0204189

Cited: by |

Refers: to

PACS

98.80.Cq Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.)

11.25.Hf Conformal field theory, algebraic structures

11.10.Lm Nonlinear or nonlocal theories and models

Subjects

Gravitation and cosmology

Particle physics and field theory

Astrophysics and astroparticles

Dates

Issue 06 (June 2002)

Received 1 May 2002, accepted for publication 10 June 2002

Published 25 July 2002



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