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Neutrinos from WIMP annihilations in the Sun including neutrino oscillations
KTH, School of Engineering Sciences (SCI), Theoretical Physics, Theoretical Particle Physics.ORCID iD: 0000-0001-5948-9152
Fysikum, Stockholm University.
KTH, School of Engineering Sciences (SCI), Theoretical Physics, Theoretical Particle Physics.ORCID iD: 0000-0002-3525-8349
2011 (English)In: The Proceedings of the 22nd International Conference on Neutrino Physics and Astrophysics / [ed] Geoffrey Mills, Steve Elliott, Terrence Goldman, and Thomas Bowles, Elsevier, 2011, Vol. 221, 37-38 p.Conference paper, Published paper (Refereed)
Abstract [en]

The prospects to detect neutrinos from the Sun arising from dark matter annihilations in the core of the Sun are reviewed. Emphasis is placed on new work investigating the effects of neutrino oscillations on the expected neutrino fluxes.

Place, publisher, year, edition, pages
Elsevier, 2011. Vol. 221, 37-38 p.
Series
Nuclear Physics B - Proceedings Supplements, ISSN 0920-5632
National Category
Subatomic Physics
Identifiers
URN: urn:nbn:se:kth:diva-107126DOI: 10.1016/j.nuclphysbps.2011.03.089Scopus ID: 2-s2.0-84859713737OAI: oai:DiVA.org:kth-107126DiVA: diva2:574716
Conference
22nd International Conference on Neutrino Physics and Astrophysics, Santa Fe, NM, USA , 3–19 June 2006
Funder
Swedish Research Council, 621-2002-3577Swedish Research Council, 621-2003-6025Swedish Research Council, 621-2005-3588
Note

QC 20130220

Available from: 2013-02-20 Created: 2012-12-06 Last updated: 2015-01-26Bibliographically approved

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Blennow, MattiasOhlsson, Tommy

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