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One-loop f(R) gravity in de Sitter universe

Guido Cognola et al JCAP02(2005)010   doi: 10.1088/1475-7516/2005/02/010  Help

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Guido Cognola1, Emilio Elizalde2, Shin'ichi Nojiri3, Sergei D Odintsov4,5 and Sergio Zerbini1
1 Dipartimento di Fisica, Università di Trento and Istituto Nazionale di Fisica Nucleare, Gruppo Collegato di Trento, Italy
2 Consejo Superior de Investigaciones Científicas (ICE/CSIC) and Institut d'Estudis Espacials de Catalunya (IEEC), Campus UAB, Fac Ciencies, Torre C5-Par-2a pl, E-08193 Bellaterra, Barcelona, Spain
3 Department of Applied Physics, National Defence Academy, Hashirimizu, Yokosuka 239-8686, Japan
4 ICREA and Institut d'Estudis Espacials de Catalunya (IEEC), Campus UAB, Fac Ciencies, Torre C5-Par-2a pl, E-08193 Bellaterra, Barcelona, Spain
5 TSPU, Tomsk, Russia
E-mail: cognola@science.unitn.it, elizalde@ieec.fcr.es, nojiri@nda.ac.jp, snojiri@yukawa.kyoto-u.ac.jp, odintsov@ieec.fcr.es and zerbini@science.unitn.it

Abstract. Motivated by the dark energy issue, the one-loop quantization approach for a family of relativistic cosmological theories is discussed in some detail. Specifically, general f(R) gravity at the one-loop level in a de Sitter universe is investigated, extending a similar program developed for the case of pure Einstein gravity. Using generalized zeta regularization, the one-loop effective action is explicitly obtained off shell, which allows us to study in detail the possibility of (de)stabilization of the de Sitter background by quantum effects. The one-loop effective action may also be useful for the study of the constant curvature black hole nucleation rate and it provides a plausible way of resolving the cosmological constant problem.

Key words: dark energy theory; quantum field theory on curved space

Received 14 January 2005, accepted for publication 14 February 2005
Published 24 February 2005

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