BibTex format
@article{Eguchi:2004:10.1103/PhysRevLett.92.071301,
author = {Eguchi, K and Enomoto, S and Furuno, K and Ikeda, H and Ikeda, K and Inoue, K and Ishihara, K and Iwamoto, T and Kawashima, T and Kishimoto, Y and Koga, M and Koseki, Y and Maeda, T and Mitsui, T and Motoki, M and Nakajima, K and Ogawa, H and Owada, K and Piquemal, F and Shimizu, I and Shirai, J and Suekane, F and Suzuki, A and Tada, K and Tajima, O and Takayama, T and Tamae, K and Watanabe, H and Busenitz, J and Djurcic, Z and McKinny, K and Mei, D-M and Piepke, A and Yakushev, E and Berger, BE and Chan, YD and Decowski, MP and Dwyer, DA and Freedman, SJ and Fu, Y and Fujikawa, BK and Goldman, J and Heeger, KM and Lesko, KT and Luk, K-B and Murayama, H and Nygren, DR and Okada, CE and Poon, AWP and Steiner, HM and Winslow, LA and Horton-Smith, GA and Mauger, C and McKeown, RD and Tipton, B and Vogel, P and Lane, CE and Miletic, T and Gorham, PW and Guillian, G and Learned, JG and Maricic, J and Matsuno, S and Pakvasa, S and Dazeley, S and Hatakeyama, S and Svoboda, R and Dieterle, BD },
doi = {10.1103/PhysRevLett.92.071301},
journal = {Phys Rev Lett},
title = {High sensitivity search for nu;e's from the sun and other sources at KamLAND.},
url = {http://dx.doi.org/10.1103/PhysRevLett.92.071301},
volume = {92},
year = {2004}
}
RIS format (EndNote, RefMan)
TY - JOUR
AB - Data 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.
AU - Eguchi,K
AU - Enomoto,S
AU - Furuno,K
AU - Ikeda,H
AU - Ikeda,K
AU - Inoue,K
AU - Ishihara,K
AU - Iwamoto,T
AU - Kawashima,T
AU - Kishimoto,Y
AU - Koga,M
AU - Koseki,Y
AU - Maeda,T
AU - Mitsui,T
AU - Motoki,M
AU - Nakajima,K
AU - Ogawa,H
AU - Owada,K
AU - Piquemal,F
AU - Shimizu,I
AU - Shirai,J
AU - Suekane,F
AU - Suzuki,A
AU - Tada,K
AU - Tajima,O
AU - Takayama,T
AU - Tamae,K
AU - Watanabe,H
AU - Busenitz,J
AU - Djurcic,Z
AU - McKinny,K
AU - Mei,D-M
AU - Piepke,A
AU - Yakushev,E
AU - Berger,BE
AU - Chan,YD
AU - Decowski,MP
AU - Dwyer,DA
AU - Freedman,SJ
AU - Fu,Y
AU - Fujikawa,BK
AU - Goldman,J
AU - Heeger,KM
AU - Lesko,KT
AU - Luk,K-B
AU - Murayama,H
AU - Nygren,DR
AU - Okada,CE
AU - Poon,AWP
AU - Steiner,HM
AU - Winslow,LA
AU - Horton-Smith,GA
AU - Mauger,C
AU - McKeown,RD
AU - Tipton,B
AU - Vogel,P
AU - Lane,CE
AU - Miletic,T
AU - Gorham,PW
AU - Guillian,G
AU - Learned,JG
AU - Maricic,J
AU - Matsuno,S
AU - Pakvasa,S
AU - Dazeley,S
AU - Hatakeyama,S
AU - Svoboda,R
AU - Dieterle,BD
AU - DiMauro,M
AU - Detwiler,J
AU - Gratta,G
AU - Ishii,K
AU - Tolich,N
AU - Uchida,Y
AU - Batygov,M
AU - Bugg,W
AU - Efremenko,Y
AU - Kamyshkov,Y
AU - Kozlov,A
AU - Nakamura,Y
AU - Gould,CR
AU - Karwowski,HJ
AU - Markoff,DM
AU - Messimore,JA
AU - Nakamura,K
AU - Rohm,RM
AU - Tornow,W
AU - Young,AR
AU - Chen,M-J
AU - Wang,Y-F
AU - KamLAND,Collaboration
DO - 10.1103/PhysRevLett.92.071301
PY - 2004///
SN - 0031-9007
TI - High sensitivity search for nu;e's from the sun and other sources at KamLAND.
T2 - Phys Rev Lett
UR - http://dx.doi.org/10.1103/PhysRevLett.92.071301
UR - https://www.ncbi.nlm.nih.gov/pubmed/14995837
VL - 92
ER -