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Sterile neutrino dark matter in B-L extension of the standard model and galactic 511 keV line

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dc.creator Khalil, Shaaban
dc.creator Seto, Osamu
dc.date 2008-07-02T14:14:59Z
dc.date 2008-07-02T14:14:59Z
dc.date 2008-04-02
dc.date.accessioned 2017-01-31T02:20:32Z
dc.date.available 2017-01-31T02:20:32Z
dc.identifier arXiv:0804.0336v1 [hep-ph]
dc.identifier http://hdl.handle.net/10261/5542
dc.identifier.uri http://dspace.mediu.edu.my:8181/xmlui/handle/10261/5542
dc.description PACS numbers: 95.35.+d, 13.15.+g, 98.80.Cq, 98.70.Rz.-- 10 pages, 1 figure.
dc.description Sterile right-handed neutrinos can be naturally embedded in a low scale gauged U(1)_{B-L} extension of the standard model. We show that, within a low reheating scenario, such a neutrino is an interesting candidate for dark matter. We emphasize that if the neutrino mass is of order of MeV, then it accounts for the measured dark matter relic density and also accommodates the observed flux of 511 keV photons from the galactic bulge.
dc.description The work of O.S. is supported by the MEC project FPA 2004-02015 and the Comunidad de Madrid project HEPHACOS (No. P-ESP-00346).
dc.format 117338 bytes
dc.format application/pdf
dc.language eng
dc.relation IFT-UAM/CSIC-08-19
dc.relation Preprint
dc.rights openAccess
dc.subject Non-baryonic Dark Matter
dc.subject Beyond the Standard Model
dc.subject High Energy Physics - Phenomenology
dc.subject Astrophysics
dc.title Sterile neutrino dark matter in B-L extension of the standard model and galactic 511 keV line
dc.type Pre-print


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