High Sensitivity Search for ν̄e's from the Sun and Other Sources at KamLAND

K. Eguchi; S. Enomoto; K. Furuno; H. Ikeda; K. Ikeda; K. Inoue; K. Ishihara; 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

High Sensitivity Search for ν̄_e's from the Sun and Other Sources at KamLAND

K. Eguchi, S. Enomoto, K. Furuno, H. Ikeda, K. Ikeda, K. Inoue, K. Ishihara, Iwamoto, T. Kawashima, Y. Kishimoto, M. Koga, Y. Koseki, T. Maeda, T. Mitsui, M. Motoki, K. Nakajima, H. Ogawa, K. Owada, F. Piquemal, I. ShimizuJ. 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

Research output: Contribution to journal › Article › peer-review

149 Citations (Scopus)

Abstract

The data corresponding to a KamLAND detector exposure of 0.28 kton yr, that has been used to search for v̄_e's was analyzed. It was assumed that all v̄_e flux had its origin in the Sun and had the characteristics ⁸B solar v₈ energy spectrum. An upper limit of 3.7 ×10² cm^-1s^-1 on the v̄_e flux was obtained. The limit on the product of the neutrino transition magnetic moment μ and the transverse component of the magnetic field B_T in the Sun at a radius of 0.05R_s was also obtained.

Original language	English
Article number	071301
Pages (from-to)	713011-713015
Number of pages	5
Journal	Physical review letters
Volume	92
Issue number	7
Publication status	Published - 2004 Feb 20

ASJC Scopus subject areas

Physics and Astronomy(all)

Access to Document

Fingerprint Dive into the research topics of 'High Sensitivity Search for ν̄<sub>e</sub>'s from the Sun and Other Sources at KamLAND'. Together they form a unique fingerprint.

Cite this

Eguchi, K., Enomoto, S., Furuno, K., Ikeda, H., Ikeda, K., Inoue, K., Ishihara, K., Iwamoto, Kawashima, T., Kishimoto, Y., Koga, M., Koseki, Y., Maeda, T., Mitsui, T., Motoki, M., Nakajima, K., Ogawa, H., Owada, K., Piquemal, F., ... Wang, Y. F. (2004). High Sensitivity Search for ν̄_e's from the Sun and Other Sources at KamLAND. Physical review letters, 92(7), 713011-713015. [071301].

High Sensitivity Search for ν̄_e's from the Sun and Other Sources at KamLAND. / Eguchi, K.; Enomoto, S.; Furuno, K.; Ikeda, H.; Ikeda, K.; Inoue, K.; Ishihara, K.; Iwamoto; Kawashima, T.; Kishimoto, Y.; Koga, M.; Koseki, Y.; Maeda, T.; Mitsui, T.; Motoki, M.; Nakajima, K.; Ogawa, H.; Owada, K.; Piquemal, F.; Shimizu, I.; Shirai, J.; Suekane, F.; Suzuki, A.; Tada, K.; Tajima, O.; Takayama, T.; Tamae, K.; Watanabe, H.; Busenitz, J.; Djurcic, Z.; McKinny, K.; Mei, D. M.; Piepke, A.; Yakushev, E.; Berger, B. E.; Chan, Y. D.; Decowski, M. P.; Dwyer, D. A.; Freedman, S. J.; Fu, Y.; Fujikawa, B. K.; Goldman, J.; Heeger, K. M.; Lesko, K. T.; Luk, K. B.; Murayama, H.; Nygren, D. R.; Okada, C. E.; Poon, A. W.P.; Steiner, H. M.; Winslow, L. A.; Horton-Smith, G. A.; Mauger, C.; McKeown, R. D.; Tipton, B.; Vogel, P.; Lane, C. E.; Miletic, T.; Gorham, P. W.; Guillian, G.; Learned, J. G.; Maricic, J.; Matsuno, S.; Pakvasa, S.; Dazeley, S.; Hatakeyama, S.; Svoboda, R.; Dieterle, B. D.; DiMauro, M.; Detwiler, J.; Gratta, G.; Ishii, K.; Tolich, N.; Uchida, Y.; Batygov, M.; Bugg, W.; Efremenko, Y.; Kamyshkov, Y.; Kozlov, A.; Nakamura, Y.; Gould, C. R.; Karwowski, H. J.; Markoff, D. M.; Messimore, J. A.; Nakamura, K.; Rohm, R. M.; Tornow, W.; Young, A. R.; Chen, M. J.; Wang, Y. F.

In: Physical review letters, Vol. 92, No. 7, 071301, 20.02.2004, p. 713011-713015.

Research output: Contribution to journal › Article › peer-review

Eguchi, K, Enomoto, S, Furuno, K, Ikeda, H, Ikeda, K, Inoue, K, Ishihara, K, Iwamoto, Kawashima, T, Kishimoto, Y , Koga, M, Koseki, Y, Maeda, T, Mitsui, T , Motoki, M, Nakajima, K, Ogawa, H, Owada, K, Piquemal, F, Shimizu, I, Shirai, J, Suekane, F, Suzuki, A, Tada, K, Tajima, O, Takayama, T, Tamae, K, Watanabe, H, Busenitz, J, Djurcic, Z, McKinny, K, Mei, DM, Piepke, A, Yakushev, E, Berger, BE, Chan, YD, Decowski, MP, Dwyer, DA, Freedman, SJ, Fu, Y, Fujikawa, BK, Goldman, J, Heeger, KM, Lesko, KT, Luk, KB, Murayama, H, Nygren, DR, Okada, CE, Poon, AWP, Steiner, HM, Winslow, LA, Horton-Smith, GA, Mauger, C, McKeown, RD, Tipton, B, Vogel, P, Lane, CE, Miletic, T, Gorham, PW, Guillian, G, Learned, JG, Maricic, J, Matsuno, S, Pakvasa, S, Dazeley, S, Hatakeyama, S, Svoboda, R, Dieterle, BD, DiMauro, M, Detwiler, J, Gratta, G, Ishii, K, Tolich, N, Uchida, Y, Batygov, M, Bugg, W, Efremenko, Y, Kamyshkov, Y, Kozlov, A, Nakamura, Y, Gould, CR, Karwowski, HJ, Markoff, DM, Messimore, JA, Nakamura, K, Rohm, RM, Tornow, W, Young, AR, Chen, MJ & Wang, YF 2004, 'High Sensitivity Search for ν̄_e's from the Sun and Other Sources at KamLAND', Physical review letters, vol. 92, no. 7, 071301, pp. 713011-713015.

Eguchi, K. ; Enomoto, S. ; Furuno, K. ; Ikeda, H. ; Ikeda, K. ; Inoue, K. ; Ishihara, K. ; Iwamoto ; Kawashima, T. ; Kishimoto, Y. ; Koga, M. ; Koseki, Y. ; Maeda, T. ; Mitsui, T. ; Motoki, M. ; Nakajima, K. ; Ogawa, H. ; Owada, K. ; Piquemal, F. ; Shimizu, I. ; Shirai, J. ; Suekane, F. ; Suzuki, A. ; Tada, K. ; Tajima, O. ; Takayama, T. ; Tamae, K. ; Watanabe, H. ; Busenitz, J. ; Djurcic, Z. ; McKinny, K. ; Mei, D. M. ; Piepke, A. ; Yakushev, E. ; Berger, B. E. ; Chan, Y. D. ; Decowski, M. P. ; Dwyer, D. A. ; Freedman, S. J. ; Fu, Y. ; Fujikawa, B. K. ; Goldman, J. ; Heeger, K. M. ; Lesko, K. T. ; Luk, K. B. ; Murayama, H. ; Nygren, D. R. ; Okada, C. E. ; Poon, A. W.P. ; Steiner, H. M. ; Winslow, L. A. ; Horton-Smith, G. A. ; Mauger, C. ; McKeown, R. D. ; Tipton, B. ; Vogel, P. ; Lane, C. E. ; Miletic, T. ; Gorham, P. W. ; Guillian, G. ; Learned, J. G. ; Maricic, J. ; Matsuno, S. ; Pakvasa, S. ; Dazeley, S. ; Hatakeyama, S. ; Svoboda, R. ; Dieterle, B. D. ; DiMauro, M. ; Detwiler, J. ; Gratta, G. ; Ishii, K. ; Tolich, N. ; Uchida, Y. ; Batygov, M. ; Bugg, W. ; Efremenko, Y. ; Kamyshkov, Y. ; Kozlov, A. ; Nakamura, Y. ; Gould, C. R. ; Karwowski, H. J. ; Markoff, D. M. ; Messimore, J. A. ; Nakamura, K. ; Rohm, R. M. ; Tornow, W. ; Young, A. R. ; Chen, M. J. ; Wang, Y. F. / High Sensitivity Search for ν̄_e's from the Sun and Other Sources at KamLAND. In: Physical review letters. 2004 ; Vol. 92, No. 7. pp. 713011-713015.

@article{5db581ec8aed4ce2a667d28a58608a77,

title = "High Sensitivity Search for {\=ν}e's from the Sun and Other Sources at KamLAND",

abstract = "The data corresponding to a KamLAND detector exposure of 0.28 kton yr, that has been used to search for {\=v}e's was analyzed. It was assumed that all {\=v}e flux had its origin in the Sun and had the characteristics 8B solar v8 energy spectrum. An upper limit of 3.7 ×102 cm-1s-1 on the {\=v}e flux was obtained. The limit on the product of the neutrino transition magnetic moment μ and the transverse component of the magnetic field BT in the Sun at a radius of 0.05Rs was also obtained.",

author = "K. Eguchi and S. Enomoto and K. Furuno and H. Ikeda and K. Ikeda and K. Inoue and K. Ishihara and Iwamoto and T. Kawashima and Y. Kishimoto and M. Koga and Y. Koseki and T. Maeda and T. Mitsui and M. Motoki and K. Nakajima and H. Ogawa and K. Owada and F. Piquemal and I. Shimizu and J. Shirai and F. Suekane and A. Suzuki and K. Tada and O. Tajima and T. Takayama and K. Tamae and H. Watanabe and J. Busenitz and Z. Djurcic and K. McKinny and Mei, {D. M.} and A. Piepke and E. Yakushev and Berger, {B. E.} and Chan, {Y. D.} and Decowski, {M. P.} and Dwyer, {D. A.} and Freedman, {S. J.} and Y. Fu and Fujikawa, {B. K.} and J. Goldman and Heeger, {K. M.} and Lesko, {K. T.} and Luk, {K. B.} and H. Murayama and Nygren, {D. R.} and Okada, {C. E.} and Poon, {A. W.P.} and Steiner, {H. M.} and Winslow, {L. A.} and Horton-Smith, {G. A.} and C. Mauger and McKeown, {R. D.} and B. Tipton and P. Vogel and Lane, {C. E.} and T. Miletic and Gorham, {P. W.} and G. Guillian and Learned, {J. G.} and J. Maricic and S. Matsuno and S. Pakvasa and S. Dazeley and S. Hatakeyama and R. Svoboda and Dieterle, {B. D.} and M. DiMauro and J. Detwiler and G. Gratta and K. Ishii and N. Tolich and Y. Uchida and M. Batygov and W. Bugg and Y. Efremenko and Y. Kamyshkov and A. Kozlov and Y. Nakamura and Gould, {C. R.} and Karwowski, {H. J.} and Markoff, {D. M.} and Messimore, {J. A.} and K. Nakamura and Rohm, {R. M.} and W. Tornow and Young, {A. R.} and Chen, {M. J.} and Wang, {Y. F.}",

year = "2004",

month = feb,

day = "20",

language = "English",

volume = "92",

pages = "713011--713015",

journal = "Physical Review Letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "7",

}

TY - JOUR

T1 - High Sensitivity Search for ν̄e's from the Sun and Other Sources at KamLAND

AU - Eguchi, K.

AU - Enomoto, S.

AU - Furuno, K.

AU - Ikeda, H.

AU - Ikeda, K.

AU - Inoue, K.

AU - Ishihara, K.

AU - Iwamoto,

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, B. E.

AU - Chan, Y. D.

AU - Decowski, M. P.

AU - Dwyer, D. A.

AU - Freedman, S. J.

AU - Fu, Y.

AU - Fujikawa, B. K.

AU - Goldman, J.

AU - Heeger, K. M.

AU - Lesko, K. T.

AU - Luk, K. B.

AU - Murayama, H.

AU - Nygren, D. R.

AU - Okada, C. E.

AU - Poon, A. W.P.

AU - Steiner, H. M.

AU - Winslow, L. A.

AU - Horton-Smith, G. A.

AU - Mauger, C.

AU - McKeown, R. D.

AU - Tipton, B.

AU - Vogel, P.

AU - Lane, C. E.

AU - Miletic, T.

AU - Gorham, P. W.

AU - Guillian, G.

AU - Learned, J. G.

AU - Maricic, J.

AU - Matsuno, S.

AU - Pakvasa, S.

AU - Dazeley, S.

AU - Hatakeyama, S.

AU - Svoboda, R.

AU - Dieterle, B. D.

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, C. R.

AU - Karwowski, H. J.

AU - Markoff, D. M.

AU - Messimore, J. A.

AU - Nakamura, K.

AU - Rohm, R. M.

AU - Tornow, W.

AU - Young, A. R.

AU - Chen, M. J.

AU - Wang, Y. F.

PY - 2004/2/20

Y1 - 2004/2/20

N2 - The data corresponding to a KamLAND detector exposure of 0.28 kton yr, that has been used to search for v̄e's was analyzed. It was assumed that all v̄e flux had its origin in the Sun and had the characteristics 8B solar v8 energy spectrum. An upper limit of 3.7 ×102 cm-1s-1 on the v̄e flux was obtained. The limit on the product of the neutrino transition magnetic moment μ and the transverse component of the magnetic field BT in the Sun at a radius of 0.05Rs was also obtained.

AB - The data corresponding to a KamLAND detector exposure of 0.28 kton yr, that has been used to search for v̄e's was analyzed. It was assumed that all v̄e flux had its origin in the Sun and had the characteristics 8B solar v8 energy spectrum. An upper limit of 3.7 ×102 cm-1s-1 on the v̄e flux was obtained. The limit on the product of the neutrino transition magnetic moment μ and the transverse component of the magnetic field BT in the Sun at a radius of 0.05Rs was also obtained.

UR - http://www.scopus.com/inward/record.url?scp=3843141413&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=3843141413&partnerID=8YFLogxK

M3 - Article

AN - SCOPUS:3843141413

VL - 92

SP - 713011

EP - 713015

JO - Physical Review Letters

JF - Physical Review Letters

SN - 0031-9007

IS - 7

M1 - 071301

ER -