Brane inflation, solitons and cosmological solutions: I

被引:40
作者
Chen, PS [1 ]
Dasgupta, K
Narayan, K
Shmakova, M
Zagermann, M
机构
[1] Stanford Univ, Stanford Linear Accelerator Ctr, Stanford, CA 94309 USA
[2] Univ Illinois, Loomis Lab, Urbana, IL 61801 USA
[3] Tata Inst Fundamental Res, Bombay 400005, Maharashtra, India
[4] Stanford Univ, Varian Lab, Stanford, CA 94309 USA
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2005年 / 09期
关键词
F-theory; supergravity models; D-branes; M-theory;
D O I
10.1088/1126-6708/2005/09/009
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
In this paper we study various cosmological solutions for a D3/D7 system directly from M-theory with fluxes and M2-branes. In M-theory, these solutions exist only if we incorporate higher derivative corrections from the curvatures as well as G-fluxes. We take these corrections into account and study a number of toy cosmologies, including one with a novel background for the D3/D7 system whose supergravity solution can be completely determined. This new background preserves all the good properties of the original model and opens up avenues to investigate cosmological effects from wrapped branes and brane-antibrane annihilation, to name a few. We also discuss in some detail semilocal defects with higher global symmetries, for example exceptional ones, that could occur in a slightly different regime of our D3/D7 model. We show that the D3/D7 system does have the required ingredients to realise these configurations as non-topological solitons of the theory. These constructions also allow us to give a physical meaning to the existence of certain underlying homogeneous quaternionic Kahler manifolds.
引用
收藏
页码:171 / 265
页数:95
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