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WIMP neutrinos from the Sun and the Earth
Max-Planck-Institut für Physik.ORCID iD: 0000-0001-5948-9152
Department of Physics, Stockholm University.
KTH, School of Engineering Sciences (SCI), Theoretical Physics, Theoretical Particle Physics.ORCID iD: 0000-0002-3525-8349
2008 (English)In: : idm2008, SISSA , 2008, 4p- p.Conference paper (Refereed)
Abstract [en]

We discuss the propagation treatment of the indirect dark matter detection using WIMP annihilations in the Sun and the Earth. In particular, we focus on treating neutrino interactions and oscillations in a consistent framework, including tau neutrino regeneration and a full three-flavor neutrino oscillation framework. We also discuss the equivalence of using a Monte Carlo approach - suited for inclusion in neutrino telescope Monte Carlos - and the density matrix formalism.

Place, publisher, year, edition, pages
SISSA , 2008. 4p- p.
Series
, Proceedings of Science (PoS), ISSN 1824-8039
National Category
Subatomic Physics
Identifiers
URN: urn:nbn:se:kth:diva-34607ScopusID: 2-s2.0-84882399845OAI: oai:DiVA.org:kth-34607DiVA: diva2:423971
Conference
Identification of Dark Matter 2008, IDM 2008; Stockholm; Sweden; 18-22 August 2008
Funder
Swedish Research Council, 623-2007-8066Swedish Research Council, 622-2003-6025Swedish Research Council, 621-2005-3588
Note

QC 20140925

Available from: 2011-06-16 Created: 2011-06-10 Last updated: 2014-09-25Bibliographically approved

Open Access in DiVA

fulltext(61 kB)70 downloads
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Type fulltextMimetype application/pdf

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Scopushttp://pos.sissa.it/archive/conferences/064/116/idm2008_116.pdf

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