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20 April 2024
 
  » pubmed » pmid14995837

 Article overview


High sensitivity search for nu;e's from the sun and other sources at KamLAND
K Eguchi ; S Enomoto ; K Furuno ; H Ikeda ; K Ikeda ; K Inoue ; K Ishihara ; T Iwamoto ; T Kawashima ; Y Kishimoto ; M Koga ; Y Koseki ; T Maeda ; T Mitsui ; M Motoki ; K Nakajima ; H Ogawa ; K Owada ; F Piquemal ; I Shimizu ; J Shirai ; F Suekane ; A Suzuki ; K Tada ; O Tajima ; T Takayama ; K Tamae ; H Watanabe ; J Busenitz ; Z Djurcic ; K McKinny ; D-M Mei ; A Piepke ; E Yakushev ; B E Berger ; Y D Chan ; M P Decowski ; D A Dwyer ; S J Freedman ; Y Fu ; B K Fujikawa ; J Goldman ; K M Heeger ; K T Lesko ; K-B Luk ; H Murayama ; D R Nygren ; C E Okada ; A W P Poon ; H M Steiner ; L A Winslow ; G A Horton-Smith ; C Mauger ; R D McKeown ; B Tipton ; P Vogel ; C E Lane ; T Miletic ; P W Gorham ; G Guillian ; J G Learned ; J Maricic ; S Matsuno ; S Pakvasa ; S Dazeley ; S Hatakeyama ; R Svoboda ; B D Dieterle ; M DiMauro ; J Detwiler ; G Gratta ; K Ishii ; N Tolich ; Y Uchida ; M Batygov ; W Bugg ; Y Efremenko ; Y Kamyshkov ; A Kozlov ; Y Nakamura ; C R Gould ; H J Karwowski ; D M Markoff ; J A Messimore ; K Nakamura ; R M Rohm ; W Tornow ; A R Young ; M-J Chen ; Y-F Wang ; ;
Date 20 Feb 2004
Journal Phys Rev Lett, 92 (7), 071301
AbstractData corresponding to a KamLAND detector exposure of 0.28 kton yr has been used to search for nu;(e)’s in the energy range 8.3<E(nu;(e))<14.8 MeV. No candidates were found for an expected background of 1.1+/-0.4 events. This result can be used to obtain a limit on nu;(e) fluxes of any origin. Assuming that all nu;(e) flux has its origin in the Sun and has the characteristic 8B solar nu(e) energy spectrum, we obtain an upper limit of 3.7 x 10(2) cm(-2) s(-1) (90% C.L.) on the nu;(e) flux. We interpret this limit, corresponding to 2.8 x 10(-4) of the standard solar model 8B nu(e) flux, in the framework of spin-flavor precession and neutrino decay models.
Source PubMed, pmid14995837
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