Accidental inflation from Kahler uplifting

被引:12
|
作者
Ben-Dayan, Ido [1 ]
Jing, Shenglin [2 ,3 ]
Westphal, Alexander [1 ]
Wieck, Clemens [1 ]
机构
[1] Deutsch Elektronen Synchrotron DESY, Theory Grp, D-22603 Hamburg, Germany
[2] Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada
[3] Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 3H4, Canada
关键词
inflation; string theory and cosmology; power spectrum; physics of the early universe; HUBBLE-SPACE-TELESCOPE; POWER SPECTRUM; CONSTRAINTS; FIELD;
D O I
10.1088/1475-7516/2014/03/054
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We analyze the possibility of realizing inflation with a subsequent dS vacuum in the Kahler uplifting scenario. The inclusion of several quantum corrections to the 4d effective action evades previous no-go theorems and allows for construction of simple and successful models of string inflation. The predictions of several benchmark models are in accord with current observations, i.e., a red spectral index, negligible non-gaussianity, and spectral distortions similar to the simplest models of inflation. A particularly interesting subclass of models are "left-rolling" ones, where the overall volume of the compactified dimensions shrinks during inflation. We call this phenomenon "inflation by deflation" (IBD), where deflation refers to the internal manifold. This subclass has the appealing features of being insensitive to initial conditions, avoiding the overshooting problem, and allowing for observable running alpha similar to 0.012 and enhanced tensor-to-scalar ratio r similar to 10(-5). The latter results differ signifi cantly from many string inflation models.s.
引用
收藏
页数:20
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