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High energy neutrin...
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Enberg, RikardUppsala universitet,Kärn- och partikelfysik
(author)
High energy neutrinos from charm in astrophysical sources
- Article/chapterEnglish2009
Publisher, publication year, extent ...
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The American Physical Society,2009
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printrdacarrier
Numbers
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LIBRIS-ID:oai:DiVA.org:uu-99775
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https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-99775URI
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https://doi.org/10.1103/PhysRevD.79.053006DOI
Supplementary language notes
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Language:English
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Summary in:English
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Subject category:ref swepub-contenttype
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Subject category:art swepub-publicationtype
Notes
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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.
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Reno, Mary HallDepartment of Physics and Astronomy, University of Iowa
(author)
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Sarcevic, InaDepartment of Physics, University of Arizona
(author)
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Uppsala universitetKärn- och partikelfysik
(creator_code:org_t)
Related titles
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In:Physical Review D: The American Physical Society79:5, s. 053006-1550-79981550-2368
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