IIB String Theory and Sequestered Inflation

被引:12
|
作者
Kallosh, Renata [1 ,2 ]
Linde, Andrei [1 ,2 ]
Wrase, Timm [3 ]
Yamada, Yusuke [4 ]
机构
[1] Stanford Univ, Stanford Inst Theoret Phys, Stanford, CA 94305 USA
[2] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
[3] Lehigh Univ, Dept Phys, 16 Mem Dr East, Bethlehem, PA 18018 USA
[4] Univ Tokyo, Res Ctr Early Universe RESCEU, Grad Sch Sci, Bunkyo Ku, Hongo 7-3-1, Tokyo 1130033, Japan
来源
基金
美国国家科学基金会;
关键词
cosmology; inflation; string theory; supergravity;
D O I
10.1002/prop.202100127
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We develop sequestered inflation models, where inflation occurs along flat directions in supergravity models derived from type IIB string theory. It is compactified on a T6Z2xZ2 orientifold with generalized fluxes and O3/O7-planes. At Step I, we use flux potentials which 1) satisfy tadpole cancellation conditions and 2) have supersymmetric Minkowski vacua with flat direction(s). The 7 moduli are split into heavy and massless Goldstone multiplets. At Step II we add a nilpotent multiplet and uplift the flat direction(s) of the type IIB string theory to phenomenological inflationary plateau potentials: alpha-attractors with 7 discrete values 3 alpha=1,2,3, horizontal ellipsis ,7. Their cosmological predictions are determined by the hyperbolic geometry inherited from string theory. The masses of the heavy fields and the volume of the extra dimensions change during inflation, but this does not affect the inflationary dynamics.
引用
收藏
页数:11
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