High Sensitivity Search for [Formula presented]’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

doi:10.1103/PhysRevLett.92.071301

High Sensitivity Search for [Formula presented]’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. 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

2 Citations (Scopus)

Abstract

Data corresponding to a KamLAND detector exposure of 0.28 kton yr has been used to search for [Formula presented]’s in the energy range [Formula presented]. No candidates were found for an expected background of [Formula presented] events. This result can be used to obtain a limit on [Formula presented] fluxes of any origin. Assuming that all [Formula presented] flux has its origin in the Sun and has the characteristic [Formula presented] solar [Formula presented] energy spectrum, we obtain an upper limit of [Formula presented] (90% C.L.) on the [Formula presented] flux. We interpret this limit, corresponding to [Formula presented] of the standard solar model [Formula presented] [Formula presented] flux, in the framework of spin-flavor precession and neutrino decay models.

Original language	English
Journal	Physical review letters
Volume	92
Issue number	7
DOIs	https://doi.org/10.1103/PhysRevLett.92.071301
Publication status	Published - 2004

ASJC Scopus subject areas

Physics and Astronomy(all)

Access to Document

10.1103/PhysRevLett.92.071301

Cite this

Eguchi, K., Enomoto, S., Furuno, K., Ikeda, H., Ikeda, K., Inoue, K., Ishihara, K., Iwamoto, T., 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 [Formula presented]’s from the Sun and Other Sources at KamLAND. Physical review letters, 92(7). https://doi.org/10.1103/PhysRevLett.92.071301

Eguchi, K, Enomoto, S, Furuno, K, Ikeda, H, Ikeda, K, Inoue, K, Ishihara, K, Iwamoto, T, 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 [Formula presented]’s from the Sun and Other Sources at KamLAND', Physical review letters, vol. 92, no. 7. https://doi.org/10.1103/PhysRevLett.92.071301

@article{8f6a46377e164f1b91d4e85158005240,

title = "High Sensitivity Search for [Formula presented]{\textquoteright}s from the Sun and Other Sources at KamLAND",

abstract = "Data corresponding to a KamLAND detector exposure of 0.28 kton yr has been used to search for [Formula presented]{\textquoteright}s in the energy range [Formula presented]. No candidates were found for an expected background of [Formula presented] events. This result can be used to obtain a limit on [Formula presented] fluxes of any origin. Assuming that all [Formula presented] flux has its origin in the Sun and has the characteristic [Formula presented] solar [Formula presented] energy spectrum, we obtain an upper limit of [Formula presented] (90% C.L.) on the [Formula presented] flux. We interpret this limit, corresponding to [Formula presented] of the standard solar model [Formula presented] [Formula presented] flux, in the framework of spin-flavor precession and neutrino decay models.",

author = "K. Eguchi and S. Enomoto and K. Furuno and H. Ikeda and K. Ikeda and K. Inoue and K. Ishihara and T. 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",

doi = "10.1103/PhysRevLett.92.071301",

language = "English",

volume = "92",

journal = "Physical Review Letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "7",

}

TY - JOUR

T1 - High Sensitivity Search for [Formula presented]’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, 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, 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

Y1 - 2004

N2 - Data corresponding to a KamLAND detector exposure of 0.28 kton yr has been used to search for [Formula presented]’s in the energy range [Formula presented]. No candidates were found for an expected background of [Formula presented] events. This result can be used to obtain a limit on [Formula presented] fluxes of any origin. Assuming that all [Formula presented] flux has its origin in the Sun and has the characteristic [Formula presented] solar [Formula presented] energy spectrum, we obtain an upper limit of [Formula presented] (90% C.L.) on the [Formula presented] flux. We interpret this limit, corresponding to [Formula presented] of the standard solar model [Formula presented] [Formula presented] flux, in the framework of spin-flavor precession and neutrino decay models.

AB - Data corresponding to a KamLAND detector exposure of 0.28 kton yr has been used to search for [Formula presented]’s in the energy range [Formula presented]. No candidates were found for an expected background of [Formula presented] events. This result can be used to obtain a limit on [Formula presented] fluxes of any origin. Assuming that all [Formula presented] flux has its origin in the Sun and has the characteristic [Formula presented] solar [Formula presented] energy spectrum, we obtain an upper limit of [Formula presented] (90% C.L.) on the [Formula presented] flux. We interpret this limit, corresponding to [Formula presented] of the standard solar model [Formula presented] [Formula presented] flux, in the framework of spin-flavor precession and neutrino decay models.

UR - http://www.scopus.com/inward/record.url?scp=84867377459&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84867377459&partnerID=8YFLogxK

U2 - 10.1103/PhysRevLett.92.071301

DO - 10.1103/PhysRevLett.92.071301

M3 - Article

AN - SCOPUS:84867377459

SN - 0031-9007

VL - 92

JO - Physical Review Letters

JF - Physical Review Letters

IS - 7

ER -

High Sensitivity Search for [Formula presented]’s from the Sun and Other Sources at KamLAND

Abstract

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this