One-loop f(R) gravity in de Sitter universe -: art. no. 010

被引:303
作者
Cognola, G [1 ]
Elizalde, E
Nojiri, S
Odintsov, SD
Zerbini, S
机构
[1] Univ Trent, Dipartimento Fis, I-38100 Trento, Italy
[2] Ist Nazl Fis Nucl, Grp Collegato Trento, Trento, Italy
[3] CSIC, ICE, E-08193 Barcelona, Spain
[4] Fac Ciencies, IEEC, E-08193 Barcelona, Spain
[5] Natl Def Acad, Dept Appl Phys, Yokosuka, Kanagawa 2398686, Japan
[6] Fac Ciencies, ICREA, E-08193 Barcelona, Spain
[7] TSPU, Tomsk, Russia
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2005年 / 02期
关键词
dark energy theory; quantum field theory on curved space;
D O I
10.1088/1475-7516/2005/02/010
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:217 / 243
页数:27
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