Direct detection of Kaluza-Klein particles in neutrino telescopes

被引:6
作者
Albuquerque, Ivone F. M. [1 ]
Burdman, Gustavo [1 ]
Krenke, Christopher A. [2 ,3 ]
Nosratpour, Baran [2 ]
机构
[1] Univ Sao Paulo, Inst Fis, BR-01498 Sao Paulo, Brazil
[2] Univ Arizona, Dept Phys, Tucson, AZ 85721 USA
[3] Univ Maryland, Dept Phys, College Pk, MD 20742 USA
来源
PHYSICAL REVIEW D | 2008年 / 78卷 / 01期
基金
巴西圣保罗研究基金会;
关键词
D O I
10.1103/PhysRevD.78.015010
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In theories with universal extra dimensions, all standard model fields propagate in the bulk and the lightest state of the first Kaluza-Klein (KK) level can be made stable by imposing a Z(2) parity. We consider a framework where the lightest KK particle (LKP) is a neutral, extremely weakly interacting particle such as the first KK excitation of the graviton, while the next-to-lightest KK particle (NLKP) is the first KK mode of a charged right-handed lepton. In such a scenario, due to its very small couplings to the LKP, the NLKP is long-lived. We investigate the production of these particles from the interaction of high energy neutrinos with nucleons in the Earth and determine the rate of NLKP events in neutrino telescopes. Using the Waxman-Bahcall limit for the neutrino flux, we find that the rate can be as large as a few hundreds of events a year for realistic values of the NLKP mass.
引用
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页数:8
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