NEUTRINO FLUXES AND RESONANCE PHYSICS WITH NEUTRINO TELESCOPES

被引:2
|
作者
BANDER, M
RUBINSTEIN, HR
机构
[1] UPPSALA UNIV,DEPT THEORET PHYS,UPPSALA,SWEDEN
[2] HEBREW UNIV JERUSALEM,DEPT THEORET PHYS,JERUSALEM,ISRAEL
来源
PHYSICAL REVIEW D | 1995年 / 51卷 / 03期
基金
美国国家科学基金会;
关键词
D O I
10.1103/PhysRevD.51.1410
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Expected atmospheric ν̄e fluxes will result in a significant number of resonantly produced low mass hadronic vector states, as the ρ, in large volume neutrino telescopes. The existence of sources of higher energy neutrinos will result in the production of higher mass states, as the Ds* and the (t̄b)J=1. We calculate the rates of production of these states and discuss their signals. Independent of theoretical flux determinations, the detection of these states will be a tool for experimentally determining these fluxes. © 1995 The American Physical Society.
引用
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页码:1410 / 1411
页数:2
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