Updated limits on TeV-scale gravity from the absence of neutrino cosmic ray showers mediated by black holes

被引：73

作者：

Anchordoqui, LA ^{[1
]}

Feng, JL

Goldberg, H

Shapere, AD

机构：

[1] Northeastern Univ, Dept Phys, Boston, MA 02115 USA

[2] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

[3] MIT, Ctr Theoret Phys, Cambridge, MA 02139 USA

[4] Univ Kentucky, Dept Phys, Lexington, KY 40506 USA

来源：

PHYSICAL REVIEW D | 2003年 / 68卷 / 10期

关键词：

D O I：

10.1103/PhysRevD.68.104025

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We revise existing limits on the D-dimensional Planck scale M-D from the nonobservation of microscopic black holes produced by high energy cosmic neutrinos in scenarios with D=4+n large extra dimensions. Previous studies have neglected the energy radiated in gravitational waves by the multipole moments of the incoming shock waves. We include the effects of energy loss, as well as form factors for black hole production and recent null results from cosmic ray detectors. For ngreater than or equal to5, we obtain M-D>1.0-1.4 TeV. These bounds are among the most stringent and conservative to date.

引用

页数：6

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