Eternal inflation with α'-corrections -: art. no. 003

被引:27
作者
Westphal, A [1 ]
机构
[1] DESY, D-22603 Hamburg, Germany
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2005年 / 11期
关键词
extra dimensions; string theory and cosmology; inflation; power spectrum;
D O I
10.1088/1475-7516/2005/11/003
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Higher-order a alpha'-corrections are a generic feature of type IIB string compactifications. In KKLT-like models of moduli stabilization they provide a mechanism of breaking of the no-scale structure of the volume modulus. We present a model of inflation driven by the volume modulus of flux compactifications of the type IIB superstring. Using the effects of gauginocondensation on D7-branes and perturbative alpha'-corrections the volume modulus can be stabilized in a scalar potential which simultaneously contains saddle points providing slow-roll inflation with about 130 e-foldings. We can accommodate the WMAP data with a spectral index of density. fluctuations n(s) = 0.93. Our model allows for eternal inflation providing the initial conditions of slow-roll inflation.
引用
收藏
页码:37 / 59
页数:23
相关论文
共 76 条
[1]  
ACHARYA BS, 2002, HEPTH0212294
[2]   R-4 couplings in M- and type II theories on Calabi-Yau spaces [J].
Antoniadis, I ;
Ferrara, S ;
Minasian, R ;
Narain, KS .
NUCLEAR PHYSICS B, 1997, 507 (03) :571-588
[3]  
BACHAS C, 1995, HEPTH9503030
[4]  
Balasubramanian V, 2004, J HIGH ENERGY PHYS
[5]   Systematics of moduli stabilisation in Calabi-Yau flux compactifications [J].
Balasubramanian, V ;
Berglund, P ;
Conlon, JP ;
Quevedo, F .
JOURNAL OF HIGH ENERGY PHYSICS, 2005, (03) :133-154
[6]   Warped reheating in brane-antibrane inflation [J].
Barnaby, N ;
Burgess, CP ;
Cline, JM .
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2005, (04) :167-184
[7]  
BARREIRO T, 2005, HEPPH0506045
[8]   M-theory inflation from multi M5-brane dynamics [J].
Becker, K ;
Becker, M ;
Krause, A .
NUCLEAR PHYSICS B, 2005, 715 (1-2) :349-371
[9]  
Becker K, 2001, J HIGH ENERGY PHYS
[10]  
Becker K, 2002, J HIGH ENERGY PHYS