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Gravitational waves from WZW models

Giuseppe D'Appollonio

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A brief review is given of the recent solution of a non-compact CFT describing a NS-supported pp-wave background. We will first explain how to compute the three- and four-point correlators using the current algebra techniques, thereby showing that some generic features of the non-compact WZW models become very clear in this simple context. We will then present the Penrose limit as a contraction of an U(1) × SU(2)k WZW model, an approach that could prove useful in order to understand holography for pp-wave spacetimes. We will finally comment on the string amplitudes and on the existence of two flat space limits.


PACS

11.25.Hf Conformal field theory, algebraic structures

11.25.Db Properties of perturbation theory

04.30.-w Gravitational waves

MSC

83C35 Gravitational waves

81T40 Two-dimensional field theories, conformal field theories, etc.

Subjects

Gravitation and cosmology

Particle physics and field theory

Dates

Issue 10 (21 May 2004)

Received 25 February 2004

Published 16 April 2004



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