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Neutrino fluxes and resonance physics with neutrino telescopes

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 01 Feb 1995Embargo end date: 01 Jan 1994 United States Publisher:American Physical Society (APS)Journal:Physical Review D, volume 51, pages 1,410-1,411 (issn: 0556-2821,

Authors: H. Rubinstein; H. Rubinstein; Myron Bander;

doi: 10.1103/physrevd.51.1410 , 10.48550/arxiv.hep-ph/9403287

pmid: 10018602

arXiv: http://arxiv.org/abs/hep-ph/9403287

Neutrino fluxes and resonance physics with neutrino telescopes

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Abstract

Expected atmospheric ${\bar ��_e}$ fluxes will result in a significant number of resonantly produced low mass hadronic vector states, as the $��$, in large volume neutrino telescopes. The existence of sources of higher energy neutrinos will result in the production of higher mass states, as the $D_s^*$ and the $({\bar t}b)_{J=1}$. 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.

pages, UCI-TR 94-10

Country

United States

Related Organizations

University of California System
United States
University of California, Irvine
United States
Hebrew University of Jerusalem
Israel
Uppsala University
Sweden

Keywords

High Energy Physics - Phenomenology, High Energy Physics - Phenomenology (hep-ph), Physical Sciences, FOS: Physical sciences, Particle and High Energy Physics, Nuclear and Plasma Physics, 530

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