Uncertainties in limits on TeV-gravity from neutrino-induced showers

被引：25

作者：

Ahn, EJ

Cavaglià, M

Olinto, AV

机构：

[1] Univ Mississippi, Dept Phys & Astron, University, MS 38677 USA

[2] Univ Chicago, Dept Astron & Astrophys, Enrico Fermi Inst, Chicago, IL 60637 USA

[3] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA

来源：

ASTROPARTICLE PHYSICS | 2005年 / 22卷 / 5-6期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1016/j.astropartphys.2004.06.008

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In models with TeV-scale gravity, ultrahigh energy cosmic rays can generate microscopic black holes in the collision with atmospheric and terrestrial nuclei. It has been proposed that stringent bounds on TeV-scale gravity can be obtained from the absence of neutrino cosmic ray showers mediated by black holes. However, uncertainties in the cross section of black hole formation and, most importantly, large uncertainties in the neutrino flux affects these bounds. As long as the cosmic neutrino flux remains unknown, the non-observation of neutrino induced showers implies less stringent limits than present collider limits. (C) 2004 Elsevier B.V. All rights reserved.

引用

页码：377 / 385

页数：9

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