ATTENTION: The software behind KU ScholarWorks is being upgraded to a new version. Starting July 15th, users will not be able to log in to the system, add items, nor make any changes until the new version is in place at the end of July. Searching for articles and opening files will continue to work while the system is being updated. If you have any questions, please contact Marianne Reed at mreed@ku.edu .

Show simple item record

dc.contributor.authorMarfatia, Danny
dc.contributor.authorHuber, P.
dc.contributor.authorBarger, Vernon
dc.date.accessioned2007-10-08T19:53:19Z
dc.date.available2007-10-08T19:53:19Z
dc.date.issued2005-11-18
dc.identifier.citationBarger, V; Huber, P; Marfatia, D. Solar mass-varying neutrino oscillations. PHYSICAL REVIEW LETTERS. NOV 18 2005. 95(21).
dc.identifier.urihttp://hdl.handle.net/1808/1702
dc.description.abstractWe propose that the solar neutrino deficit may be due to oscillations of mass-varying neutrinos (MaVaNs). This scenario elucidates solar neutrino data beautifully while remaining comfortably compatible with atmospheric neutrino and K2K data and with reactor antineutrino data at short and long baselines (from CHOOZ and KamLAND). We find that the survival probability of solar MaVaNs is independent of how the suppression of neutrino mass caused by the acceleron-matter couplings varies with density. Measurements of MeV and lower energy solar neutrinos will provide a rigorous test of the idea.
dc.language.isoen_US
dc.publisherAMERICAN PHYSICAL SOC
dc.titleSolar mass-varying neutrino oscillations
dc.typeArticle
dc.identifier.doi10.1103/PhysRevLett.95.211802
dc.rights.accessrightsopenAccess


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record