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High energy neutrin...
High energy neutrinos from charm in astrophysical sources
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- Enberg, Rikard (author)
- Uppsala universitet,Kärn- och partikelfysik
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- Reno, Mary Hall (author)
- Department of Physics and Astronomy, University of Iowa
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- Sarcevic, Ina (author)
- Department of Physics, University of Arizona
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(creator_code:org_t)
- The American Physical Society, 2009
- 2009
- English.
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In: Physical Review D. - : The American Physical Society. - 1550-7998 .- 1550-2368. ; 79:5, s. 053006-
- Related links:
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http://link.aps.org/...
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https://urn.kb.se/re...
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https://doi.org/10.1...
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Abstract
Subject headings
Close
- Charm production gives rise to a flux of very high energy neutrinos from astrophysical sources with jets driven by central engines, such as gamma ray bursts or supernovae with jets. The neutrino flux from semileptonic decays of charmed mesons is subject to much less hadronic and radiative cooling than the conventional flux from pion and kaon decays and therefore has a dominant contribution at higher energies, which is of relevance to future ultrahigh energy neutrino experiments.
Subject headings
- NATURVETENSKAP -- Fysik (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences (hsv//eng)
Keyword
- High energy neutrinos
- supernovae
- gamma ray bursts
- cosmic rays
- Physics
- Fysik
- Fysik
- Physics
Publication and Content Type
- ref (subject category)
- art (subject category)
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