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Wavefunction of the Universe and Chern–Simons perturbation theory

Chopin Soo

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The Chern–Simons exact solution of four-dimensional quantum gravity with nonvanishing cosmological constant is presented in metric variables as the partition function of Chern–Simons theory with nontrivial source. The perturbative expansion is given, and the wavefunction is computed to the lowest order of approximation for the Cauchy surface which is topologically a 3-sphere. The state is well-defined even at degenerate and vanishing values of the dreibein. Reality conditions for the Ashtekar variables are also taken into account, and remarkable features of the Chern–Simons state and their relevance to cosmology are pointed out.


PACS

04.60.-m Quantum gravity

11.15.Bt General properties of perturbation theory

MSC

83Cxx General relativity

81T13 Yang-Mills and other gauge theories (See also 53C07, 58E15)

Subjects

Gravitation and cosmology

Particle physics and field theory

Dates

Issue 6 (21 March 2002)

Received 31 October 2001, in final form 28 January 2002

Published 25 February 2002



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