Type II Seesaw and the PAMELA/ATIC Signals

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dc.contributor.author Okada, Nobuchika
dc.date.accessioned 2019-05-29T19:11:11Z
dc.date.available 2019-05-29T19:11:11Z
dc.date.copyright 2009
dc.date.issued 2009-08-24
dc.identifier.citation Gogoladze, I., Okada, N., Shafi, Q. (2009): Type II Seesaw and the PAMELA/ATIC Signals. Physics Letters B, 679(237-241). DOI: https://doi.org/10.1016/j.physletb.2009.07.035 en_US
dc.identifier.issn 0370-2693
dc.identifier.uri http://ir.ua.edu/handle/123456789/5646
dc.description.abstract We discuss how the cosmic ray signals reported by the PAMELA and ATIC/PPB-BETS experiments may be understood in a Standard Model (SM) framework supplemented by type II seesaw and a stable SM singlet scalar boson as dark matter. A particle physics explanation of the ‘boost’ factor can be provided by including an additional SM singlet scalar field. en_US
dc.format.mimetype application/pdf en_US
dc.language English en_US
dc.publisher Elsevier B.V. en_US
dc.title Type II Seesaw and the PAMELA/ATIC Signals en_US
dc.type text en_US
dc.rights.holder Elsevier Science B. V. en_US


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