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Vacuum properties of non-symmetric gravity in de Sitter space

Tomas Janssen and Tomislav Prokopec

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We consider quantum effects of a massive antisymmetric tensor field on the dynamics of de Sitter space–time. Our starting point is the most general, stable, linearized Lagrangian arising in non-symmetric gravitational theories, where part of the antisymmetric field mass is generated by the cosmological term. We construct a renormalization group (RG) improved effective action by integrating out one-loop vacuum fluctuations of the antisymmetric tensor field and show that, in the limit when the RG scale goes to zero, the Hubble parameter—and thus the effective cosmological constant—relaxes rapidly to zero. We thus conclude that quantum loop effects in de Sitter space can dramatically change the infrared sector of the on-shell gravity, making the expansion rate insensitive to the original (bare) cosmological constant.


Keywords

quantum field theory on curved space

inflation

gravity

 

E-print Number: gr-qc/0703050

Cited: by |

Refers: to

PACS

04.60.Pp Loop quantum gravity, quantum geometry, spin foams

98.80.Es Observational cosmology (including Hubble constant, distance scale, cosmological constant, early Universe, etc)

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

11.10.Hi Renormalization group evolution of parameters

Subjects

Gravitation and cosmology

Particle physics and field theory

Astrophysics and astroparticles

Dates

Issue 05 (May 2007)

Received 11 April 2007, accepted for publication 19 April 2007

Published 14 May 2007



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