Inflation and nonminimal scalar-curvature coupling in gravity and supergravity

被引:71
|
作者
Ketov, Sergei V. [1 ,2 ]
Starobinsky, Alexei A. [3 ,4 ]
机构
[1] Tokyo Metropolitan Univ, Dept Phys, Hachioji, Tokyo 1920397, Japan
[2] Univ Tokyo, Kavli Inst Phys & Math Universe IPMU, Chiba 2778568, Japan
[3] RAS, LD Landau Theoret Phys Inst, Moscow 119334, Russia
[4] Univ Tokyo, Grad Sch Sci, Res Ctr Early Universe RESCEU, Tokyo 1130033, Japan
基金
俄罗斯基础研究基金会;
关键词
modified gravity; inflation; supersymmetry and cosmology; MODEL HIGGS-BOSON; 4TH-ORDER GRAVITY; STANDARD; COSMOLOGY;
D O I
10.1088/1475-7516/2012/08/022
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Inflationary slow-roll dynamics in Einstein gravity wit h a nonminimal scalar-curvature coupling can be equivalent to that in the certain f (R) gravity theory. We review the correspondence and extend it to N-1 supergravity. the nonminimal coupling in supergravity is rewritten in terms of the standard ('minimal) N=1 matter-coupled supergravity by using curved superspace. The established equivalence between two different inflationary theories means the same inflaton scalar potential, and does not imply the same post-inflationary dynamics and reheating.
引用
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页数:16
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