The one-loop effective action in φ4 theory coupled non-linearly with the power of the curvature and the dynamical origin of the cosmological constant -: art. no. 010

被引:36
作者
Inagaki, T [1 ]
Nojiri, S
Odintsov, SD
机构
[1] Flinders Univ S Australia, Sch Chem Phys & Earth Sci, Adelaide, SA 5001, Australia
[2] Hiroshima Univ, Informat Media Ctr, Higashihiroshima 724, Japan
[3] Natl Def Acad, Dept Appl Phys, Yokosuka, Kanagawa 2398686, Japan
[4] Inst Catalana Recerca & Estudis Avancats, Barcelona 08034, Spain
[5] Inst Estudis Espacials Catalunya, Barcelona 08034, Spain
[6] TSPU, Tomsk, Russia
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2005年 / 06期
关键词
dark energy theory; cosmology of theories beyond the SM; quantum field theory on curved space;
D O I
10.1088/1475-7516/2005/06/010
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The functional formulation and one-loop effective action for scalar self-interacting theory non-linearly coupled with some power of the curvature are studied. After the explicit one-loop renormalization at weak curvature, we investigated numerically the phase structure for such unusual phi(4) theory. We demonstrate the possibility of curvature-induced phase transitions for positive values of the curvature power, while for negative values the radiative symmetry breaking does not take place. The dynamical mechanism for the explanation of the current smallness of the cosmological constant is presented for several models from the class of theories under consideration.
引用
收藏
页码:165 / 190
页数:26
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