PQCD analysis of atmospheric tau neutrino

被引：0

作者：

Yeh, TW ^{[1
]}

机构：

[1] Natl Chiao Tung Univ, Inst Phys, Hsinchu 300, Taiwan

来源：

PROCEEDINGS OF THE 2002 INTERNATIONAL SYMPOSIUM ON COSMOLOGY AND PARTICLE ASTROPHYSICS | 2003年

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We calculate the flux of v, produced in the atmosphere by cosmic ray-air collisions. The production channels of v, from the process pA -> X -> v(T)((v) over bar (T))Y with X = D-s W-+/-, Z, h(b), t (t) over bar, are considered. The calculations are performed by employing perturbative QCD (PQCD). The predicted v(T) flux phi v(T)(E) is given for energy range 10(3)GeV <= E <= 10(8)GeV.

引用

页码：191 / 198

页数：8

共 7 条

[1]

ALVAREZMUNIZ J, 2001, DETECTION TAU NEUTRI

[2] Prospects for observations of high-energy cosmic tau neutrinos [J].