Radio telescopes as the detectors of super-high-energy neutrinos
The registration of super high energy neutrinos is a very difficult and also very important problem that requires construction of detectors with large effective target masses. Askaryan pointed out the possibility of registering cascades in dense media by the Cherenkov radio emission of an excess of...
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1991
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ftnasantrs:oai:casi.ntrs.nasa.gov:19920003727 2023-05-15T14:03:21+02:00 Radio telescopes as the detectors of super-high-energy neutrinos Dagkesamansky, R. D. Zheleznykh, I. M. Unclassified, Unlimited, Publicly available JAN 1, 1991 http://ntrs.nasa.gov/search.jsp?R=19920003727 unknown http://ntrs.nasa.gov/search.jsp?R=19920003727 Accession ID: 92N12945 No Copyright CASI 89 NAS-NRC, High-Energy Astrophysics. American and Soviet Perspectives; p 87-90 1991 ftnasantrs 2012-02-15T19:12:38Z The registration of super high energy neutrinos is a very difficult and also very important problem that requires construction of detectors with large effective target masses. Askaryan pointed out the possibility of registering cascades in dense media by the Cherenkov radio emission of an excess of negative charges in the cascades which arose in interaction between high energy particles and the atoms of medium. The telescopes for cosmic high energy neutrino detection by radioemission of cascades induced underground, but whose development continues in the atmosphere were proposed by others. The effective target masses of such detectors could be approx. 10(exp 9) tons and more. The properties of Cherenkov radio emission of cascades and the properties of ice in the Antarctic Region make it possible to propose Radio Antarctic Muon and Neutrino Detection (RAMAND): antennas should be placed on the ice surface of approx. 10 sq km to search for radio signals for neutrino (muon) cascades of energy. It is evident from data given that the largest radio telescopes gives the opportunity for registration of the cascades induced by neutrinos with the energies E is greater than or = 10(exp 20) eV. Other/Unknown Material Antarc* Antarctic NASA Technical Reports Server (NTRS) Antarctic The Antarctic |
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89 Dagkesamansky, R. D. Zheleznykh, I. M. Radio telescopes as the detectors of super-high-energy neutrinos |
topic_facet |
89 |
description |
The registration of super high energy neutrinos is a very difficult and also very important problem that requires construction of detectors with large effective target masses. Askaryan pointed out the possibility of registering cascades in dense media by the Cherenkov radio emission of an excess of negative charges in the cascades which arose in interaction between high energy particles and the atoms of medium. The telescopes for cosmic high energy neutrino detection by radioemission of cascades induced underground, but whose development continues in the atmosphere were proposed by others. The effective target masses of such detectors could be approx. 10(exp 9) tons and more. The properties of Cherenkov radio emission of cascades and the properties of ice in the Antarctic Region make it possible to propose Radio Antarctic Muon and Neutrino Detection (RAMAND): antennas should be placed on the ice surface of approx. 10 sq km to search for radio signals for neutrino (muon) cascades of energy. It is evident from data given that the largest radio telescopes gives the opportunity for registration of the cascades induced by neutrinos with the energies E is greater than or = 10(exp 20) eV. |
format |
Other/Unknown Material |
author |
Dagkesamansky, R. D. Zheleznykh, I. M. |
author_facet |
Dagkesamansky, R. D. Zheleznykh, I. M. |
author_sort |
Dagkesamansky, R. D. |
title |
Radio telescopes as the detectors of super-high-energy neutrinos |
title_short |
Radio telescopes as the detectors of super-high-energy neutrinos |
title_full |
Radio telescopes as the detectors of super-high-energy neutrinos |
title_fullStr |
Radio telescopes as the detectors of super-high-energy neutrinos |
title_full_unstemmed |
Radio telescopes as the detectors of super-high-energy neutrinos |
title_sort |
radio telescopes as the detectors of super-high-energy neutrinos |
publishDate |
1991 |
url |
http://ntrs.nasa.gov/search.jsp?R=19920003727 |
op_coverage |
Unclassified, Unlimited, Publicly available |
geographic |
Antarctic The Antarctic |
geographic_facet |
Antarctic The Antarctic |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_source |
CASI |
op_relation |
http://ntrs.nasa.gov/search.jsp?R=19920003727 Accession ID: 92N12945 |
op_rights |
No Copyright |
_version_ |
1766273972901511168 |