High Sensitivity Search For (Nu)Over-Bar(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,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,H. J. Karwowski, D. M. Marko,J. A. Messimore,K. Nakamura,R. M. Rohm,W. Tornow,M. J. Chen,Y. F. Wang PHYSICAL REVIEW LETTERS（2004）
摘要
Data corresponding to a KamLAND detector exposure of 0.28 kton yr has been used to search for (v) over bar (e)'s in the energy range 8.3更多
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