Warming up brane-antibrane inflation

被引:42
|
作者
Bastero-Gil, Mar [1 ]
Berera, Arjun [2 ]
Rosa, Joao G. [2 ]
机构
[1] Univ Granada, Dept Fis Teor & Cosmos, E-18071 Granada, Spain
[2] Univ Edinburgh, SUPA, Sch Phys & Astron, Edinburgh EH9 3JZ, Midlothian, Scotland
关键词
UNIVERSE; MODEL; DYNAMICS; FLATNESS; HORIZON;
D O I
10.1103/PhysRevD.84.103503
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show that, in constructions with additional intersecting D-branes, brane-antibrane inflation may naturally occur in a warm regime, such that strong dissipative effects damp the inflaton's motion, greatly alleviating the associated eta-problem. We illustrate this for D3-D3 inflation in flat space with additional flavor D7 branes, where for a Coulomb-like or quadratic hybrid potential a sufficient number of e-folds may be obtained for perturbative couplings and O(10-10(4)) branes. This is in clear contrast with the corresponding cold scenarios, thus setting the stage for more realistic constructions within fully stabilized compactifications. Such models generically predict a negligible amount of tensor perturbations and non-Gaussianity f(NL) similar to O(10).
引用
收藏
页数:8
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