Moduli stabilization in warped compactifications at one loop

被引:0
|
作者
Pujolàs, O [1 ]
机构
[1] Univ Autonoma Barcelona, Dept Fis, IFAE, E-08193 Barcelona, Spain
关键词
casimir energy; brane world; warped compactifications;
D O I
10.1023/A:1021189211783
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We review the moduli stabilization mechanism found in Garriga et al. (Garriga, J., Pujolas, O., and Tanaka, T. (2000). Preprint hep-th/0111277.) for a class of five-dimensional warped brane-world scenarios. Specifically, we consider solutions with a power-law warp factor and a bulk dilaton with logarithmic profile in terms of the proper distance in the extra dimension. This includes the Heterotic M-theory brane-world of Lukas et al. (Lukas, A., Ovrut, B. A., Stelle, K. S., and Waldram, D. (1999). Physical Review D 59, 086001.) and Khoury et al. (Khoury, J., Ovrut, B. A., Steinhardt, P. J., and Turok, N. (2001). Preprint hep-th/0103239.) and the Randall-Sundrum (RS) model as a limiting case. In general, there are two moduli fields y(+/-), corresponding to the "positions" of two branes. Classically, the moduli are massless due to a scaling symmetry of the action. However, in the absence of supersymmetry, they develop an effective potential at one loop. Local terms proportional to some powers of the local curvature scale at the location of the corresponding brane are needed in order to remove the divergences in the effective potential. Such terms break the scaling symmetry and therefore act as stabilizers for the moduli. Moreover, for qgreater than or similar to10, the observed hierarchy can be naturally generated by this potential, and the lightest modulus mass is of order m-less than or similar toTeV.
引用
收藏
页码:2233 / 2254
页数:22
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