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Title Possibility of detecting relict massive neutrinos
Creator/Author Shvartsman, V.F. ; Braginskii, V.B. ; Gershtein, S.S. ; Zel`dovich, Y.B. ; Khlopov, M.Y.
Publication Date1982 Sep 20
OSTI IdentifierOSTI ID: 6302261
Other Number(s)CODEN: JTPLA
Resource TypeJournal Article
Resource RelationJETP Lett. (Engl. Transl.) ; Vol/Issue: 36:6
Research OrgM. V. Keldysh Institute of Applied Mathematics, Academy of Sciences of the USSR
Subject640106 -- Astrophysics & Cosmology-- Cosmology; ;COSMIC NEUTRINOS-- NEUTRINO DETECTION; BACKGROUND RADIATION;REST MASS
Related SubjectCOSMIC RADIATION;DETECTION;ELEMENTARY PARTICLES;FERMIONS;IONIZING RADIATIONS;LEPTONS;MASS;MASSLESS PARTICLES;NEUTRINOS;RADIATION DETECTION;RADIATIONS
Description/Abstract The coherent intensification of the interaction of relict massive neutrinos with grains of matter with a size on the order of the neutrino wavelength suggests that it might be possible to detect a galactic neutrino sea by virtue of the mechanical pressure which it exerts in the direction opposite that in which the solar system is moving in the galaxy.
Country of PublicationUnited States
LanguageEnglish
FormatPages: 277-279
System Entry Date2001 May 13

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