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Enhanced Constraints on theta13 from A Three-Flavor Oscillation Analysis of Reactor Antineutrinos at KamLAND
We present new constraints on the neutrino oscillation parameters {Delta}m{sub 21}{sup 2}, {theta}{sub 12}, and {theta}{sub 13} from a three-flavor analysis of solar and KamLAND data. The KamLAND data set includes data acquired following a radiopurity upgrade and amounts to a total exposure of 3.49...
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Published in: | Physical review. D, Particles, fields, gravitation, and cosmology Particles, fields, gravitation, and cosmology, 2010-09 |
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creator | The KamLAND Collaboration Gando, A. Gando, Y. Ichimura, K. Ikeda, H. Inoue, K. Kibe, Y. Kishimoto, Y. Koga, M. Minekawa, Y. Mitsui, T. Morikawa, T. Nagai, N. Nakajima, K. Nakamura, K. Narita, K. Shimizu, I. Shimizu, Y. Shirai, J. Suekane, F. Suzuki, A. Takahashi, H. Takahashi, N. Takemoto, Y. Tamae, K. Watanabe, H. Xu, B. D. Yabumoto, H. Yoshida, H. Yoshida, S. Enomoto, S. Kozlov, A. Murayama, H. Grant, C. Keefer, G. Piepke, A. Banks, T. I. Bloxham, T. Detwiler, J. A. Freedman, S. J. Fujikawa, B. K. Han, K. Kadel, R. O'Donnell, T. Steiner, H. M. Dwyer, D. A. McKeown, R. D. Zhang, C. Berger, B. E. Lane, C. E. Maricic, J. Miletic, T. Batygov, M. Learned, J. G. Matsuno, S. Sakai, M. Horton-Smith, G. A. Downum, K. E. Gratta, G. Efremenko, Y. Perevozchikov, O. Karwowski, H. J. Markoff, D. M. Tornow, W. Heeger, K. M. Decowski, M. P. |
description | We present new constraints on the neutrino oscillation parameters {Delta}m{sub 21}{sup 2}, {theta}{sub 12}, and {theta}{sub 13} from a three-flavor analysis of solar and KamLAND data. The KamLAND data set includes data acquired following a radiopurity upgrade and amounts to a total exposure of 3.49 x 10{sup 32} target-proton-year. Under the assumption of CPT invariance, a two-flavor analysis ({theta}{sub 13} = 0) of the KamLAND and solar data yields the best-fit values tan{sup 2} {theta}{sub 12} = 0.444{sub -0.030}{sup +0.036} and {Delta}m{sub 21}{sup 2} = 7.50{sub -0.20}{sup +0.19} x 10{sup -5} eV{sup 2}; a three-flavor analysis with {theta}{sub 13} as a free parameter yields the best-fit values tan{sup 2} {theta}{sub 12} = 0.452{sub -0.033}{sup +0.035}, {Delta}m{sub 21}{sup 2} = 7.50{sub -0.20}{sup +0.19} x 10{sup -5}eV{sup 2}, and sin{sup 2} {theta}{sub 13} = 0.020{sub -0.016}{sup +0.016}. This {theta}{sub 13} interval is consistent with other recent work combining the CHOOZ, atmospheric and long-baseline accelerator experiments. We also present a new global {theta}{sub 13} analysis, incorporating the CHOOZ, atmospheric and accelerator data, which indicates sin{sup 2} {theta}{sub 13} = 0.017{sub -0.009}{sup +0.010}, a nonzero value at the 93% C.L. This finding will be further tested by upcoming accelerator and reactor experiments. |
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D. ; Yabumoto, H. ; Yoshida, H. ; Yoshida, S. ; Enomoto, S. ; Kozlov, A. ; Murayama, H. ; Grant, C. ; Keefer, G. ; Piepke, A. ; Banks, T. I. ; Bloxham, T. ; Detwiler, J. A. ; Freedman, S. J. ; Fujikawa, B. K. ; Han, K. ; Kadel, R. ; O'Donnell, T. ; Steiner, H. M. ; Dwyer, D. A. ; McKeown, R. D. ; Zhang, C. ; Berger, B. E. ; Lane, C. E. ; Maricic, J. ; Miletic, T. ; Batygov, M. ; Learned, J. G. ; Matsuno, S. ; Sakai, M. ; Horton-Smith, G. A. ; Downum, K. E. ; Gratta, G. ; Efremenko, Y. ; Perevozchikov, O. ; Karwowski, H. J. ; Markoff, D. M. ; Tornow, W. ; Heeger, K. M. ; Decowski, M. P.</creator><creatorcontrib>The KamLAND Collaboration ; Gando, A. ; Gando, Y. ; Ichimura, K. ; Ikeda, H. ; Inoue, K. ; Kibe, Y. ; Kishimoto, Y. ; Koga, M. ; Minekawa, Y. ; Mitsui, T. ; Morikawa, T. ; Nagai, N. ; Nakajima, K. ; Nakamura, K. ; Narita, K. ; Shimizu, I. ; Shimizu, Y. ; Shirai, J. ; Suekane, F. ; Suzuki, A. ; Takahashi, H. ; Takahashi, N. ; Takemoto, Y. ; Tamae, K. ; Watanabe, H. ; Xu, B. D. ; Yabumoto, H. ; Yoshida, H. ; Yoshida, S. ; Enomoto, S. ; Kozlov, A. ; Murayama, H. ; Grant, C. ; Keefer, G. ; Piepke, A. ; Banks, T. I. ; Bloxham, T. ; Detwiler, J. A. ; Freedman, S. J. ; Fujikawa, B. K. ; Han, K. ; Kadel, R. ; O'Donnell, T. ; Steiner, H. M. ; Dwyer, D. A. ; McKeown, R. D. ; Zhang, C. ; Berger, B. E. ; Lane, C. E. ; Maricic, J. ; Miletic, T. ; Batygov, M. ; Learned, J. G. ; Matsuno, S. ; Sakai, M. ; Horton-Smith, G. A. ; Downum, K. E. ; Gratta, G. ; Efremenko, Y. ; Perevozchikov, O. ; Karwowski, H. J. ; Markoff, D. M. ; Tornow, W. ; Heeger, K. M. ; Decowski, M. P. ; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)</creatorcontrib><description>We present new constraints on the neutrino oscillation parameters {Delta}m{sub 21}{sup 2}, {theta}{sub 12}, and {theta}{sub 13} from a three-flavor analysis of solar and KamLAND data. The KamLAND data set includes data acquired following a radiopurity upgrade and amounts to a total exposure of 3.49 x 10{sup 32} target-proton-year. Under the assumption of CPT invariance, a two-flavor analysis ({theta}{sub 13} = 0) of the KamLAND and solar data yields the best-fit values tan{sup 2} {theta}{sub 12} = 0.444{sub -0.030}{sup +0.036} and {Delta}m{sub 21}{sup 2} = 7.50{sub -0.20}{sup +0.19} x 10{sup -5} eV{sup 2}; a three-flavor analysis with {theta}{sub 13} as a free parameter yields the best-fit values tan{sup 2} {theta}{sub 12} = 0.452{sub -0.033}{sup +0.035}, {Delta}m{sub 21}{sup 2} = 7.50{sub -0.20}{sup +0.19} x 10{sup -5}eV{sup 2}, and sin{sup 2} {theta}{sub 13} = 0.020{sub -0.016}{sup +0.016}. This {theta}{sub 13} interval is consistent with other recent work combining the CHOOZ, atmospheric and long-baseline accelerator experiments. We also present a new global {theta}{sub 13} analysis, incorporating the CHOOZ, atmospheric and accelerator data, which indicates sin{sup 2} {theta}{sub 13} = 0.017{sub -0.009}{sup +0.010}, a nonzero value at the 93% C.L. This finding will be further tested by upcoming accelerator and reactor experiments.</description><identifier>ISSN: 1550-7998</identifier><identifier>EISSN: 1550-2368</identifier><language>eng</language><publisher>United States</publisher><subject>72 ; 79 ; ACCELERATORS ; ANTINEUTRINOS ; NEUTRINO OSCILLATION ; OSCILLATIONS</subject><ispartof>Physical review. 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(LBNL), Berkeley, CA (United States)</creatorcontrib><title>Enhanced Constraints on theta13 from A Three-Flavor Oscillation Analysis of Reactor Antineutrinos at KamLAND</title><title>Physical review. D, Particles, fields, gravitation, and cosmology</title><description>We present new constraints on the neutrino oscillation parameters {Delta}m{sub 21}{sup 2}, {theta}{sub 12}, and {theta}{sub 13} from a three-flavor analysis of solar and KamLAND data. The KamLAND data set includes data acquired following a radiopurity upgrade and amounts to a total exposure of 3.49 x 10{sup 32} target-proton-year. Under the assumption of CPT invariance, a two-flavor analysis ({theta}{sub 13} = 0) of the KamLAND and solar data yields the best-fit values tan{sup 2} {theta}{sub 12} = 0.444{sub -0.030}{sup +0.036} and {Delta}m{sub 21}{sup 2} = 7.50{sub -0.20}{sup +0.19} x 10{sup -5} eV{sup 2}; a three-flavor analysis with {theta}{sub 13} as a free parameter yields the best-fit values tan{sup 2} {theta}{sub 12} = 0.452{sub -0.033}{sup +0.035}, {Delta}m{sub 21}{sup 2} = 7.50{sub -0.20}{sup +0.19} x 10{sup -5}eV{sup 2}, and sin{sup 2} {theta}{sub 13} = 0.020{sub -0.016}{sup +0.016}. This {theta}{sub 13} interval is consistent with other recent work combining the CHOOZ, atmospheric and long-baseline accelerator experiments. We also present a new global {theta}{sub 13} analysis, incorporating the CHOOZ, atmospheric and accelerator data, which indicates sin{sup 2} {theta}{sub 13} = 0.017{sub -0.009}{sup +0.010}, a nonzero value at the 93% C.L. This finding will be further tested by upcoming accelerator and reactor experiments.</description><subject>72</subject><subject>79</subject><subject>ACCELERATORS</subject><subject>ANTINEUTRINOS</subject><subject>NEUTRINO OSCILLATION</subject><subject>OSCILLATIONS</subject><issn>1550-7998</issn><issn>1550-2368</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNqNjN1qwkAQhRdpwdT6DuMDBPJTTXIZNCK0tCC5D8N2QlbWWdgZhb59c-EDeHU-ON85C5Pk222WFuWufnlw1TT10ryJXLKsLHZVlRjf8YRs6Rf2gUUjOlaBwKATKeYljDFcoYV-ikTp0eM9RPgR67xHdbPXMvo_cfNmhDOh1blvWR3TTaPjIIAKn3j9ar8P7-Z1RC-0fuTKbI5dvz-lQdQN86mSnWxgJqtD0xQfdV4-4_wDKw9JSw</recordid><startdate>20100924</startdate><enddate>20100924</enddate><creator>The KamLAND Collaboration</creator><creator>Gando, A.</creator><creator>Gando, Y.</creator><creator>Ichimura, K.</creator><creator>Ikeda, H.</creator><creator>Inoue, K.</creator><creator>Kibe, Y.</creator><creator>Kishimoto, Y.</creator><creator>Koga, M.</creator><creator>Minekawa, Y.</creator><creator>Mitsui, T.</creator><creator>Morikawa, T.</creator><creator>Nagai, N.</creator><creator>Nakajima, K.</creator><creator>Nakamura, K.</creator><creator>Narita, K.</creator><creator>Shimizu, I.</creator><creator>Shimizu, Y.</creator><creator>Shirai, J.</creator><creator>Suekane, F.</creator><creator>Suzuki, A.</creator><creator>Takahashi, H.</creator><creator>Takahashi, N.</creator><creator>Takemoto, Y.</creator><creator>Tamae, K.</creator><creator>Watanabe, H.</creator><creator>Xu, B. D.</creator><creator>Yabumoto, H.</creator><creator>Yoshida, H.</creator><creator>Yoshida, S.</creator><creator>Enomoto, S.</creator><creator>Kozlov, A.</creator><creator>Murayama, H.</creator><creator>Grant, C.</creator><creator>Keefer, G.</creator><creator>Piepke, A.</creator><creator>Banks, T. I.</creator><creator>Bloxham, T.</creator><creator>Detwiler, J. A.</creator><creator>Freedman, S. J.</creator><creator>Fujikawa, B. K.</creator><creator>Han, K.</creator><creator>Kadel, R.</creator><creator>O'Donnell, T.</creator><creator>Steiner, H. M.</creator><creator>Dwyer, D. A.</creator><creator>McKeown, R. D.</creator><creator>Zhang, C.</creator><creator>Berger, B. E.</creator><creator>Lane, C. E.</creator><creator>Maricic, J.</creator><creator>Miletic, T.</creator><creator>Batygov, M.</creator><creator>Learned, J. G.</creator><creator>Matsuno, S.</creator><creator>Sakai, M.</creator><creator>Horton-Smith, G. A.</creator><creator>Downum, K. E.</creator><creator>Gratta, G.</creator><creator>Efremenko, Y.</creator><creator>Perevozchikov, O.</creator><creator>Karwowski, H. J.</creator><creator>Markoff, D. M.</creator><creator>Tornow, W.</creator><creator>Heeger, K. M.</creator><creator>Decowski, M. P.</creator><scope>OIOZB</scope><scope>OTOTI</scope></search><sort><creationdate>20100924</creationdate><title>Enhanced Constraints on theta13 from A Three-Flavor Oscillation Analysis of Reactor Antineutrinos at KamLAND</title><author>The KamLAND Collaboration ; Gando, A. ; Gando, Y. ; Ichimura, K. ; Ikeda, H. ; Inoue, K. ; Kibe, Y. ; Kishimoto, Y. ; Koga, M. ; Minekawa, Y. ; Mitsui, T. ; Morikawa, T. ; Nagai, N. ; Nakajima, K. ; Nakamura, K. ; Narita, K. ; Shimizu, I. ; Shimizu, Y. ; Shirai, J. ; Suekane, F. ; Suzuki, A. ; Takahashi, H. ; Takahashi, N. ; Takemoto, Y. ; Tamae, K. ; Watanabe, H. ; Xu, B. D. ; Yabumoto, H. ; Yoshida, H. ; Yoshida, S. ; Enomoto, S. ; Kozlov, A. ; Murayama, H. ; Grant, C. ; Keefer, G. ; Piepke, A. ; Banks, T. I. ; Bloxham, T. ; Detwiler, J. A. ; Freedman, S. J. ; Fujikawa, B. K. ; Han, K. ; Kadel, R. ; O'Donnell, T. ; Steiner, H. M. ; Dwyer, D. A. ; McKeown, R. D. ; Zhang, C. ; Berger, B. E. ; Lane, C. E. ; Maricic, J. ; Miletic, T. ; Batygov, M. ; Learned, J. G. ; Matsuno, S. ; Sakai, M. ; Horton-Smith, G. A. ; Downum, K. E. ; Gratta, G. ; Efremenko, Y. ; Perevozchikov, O. ; Karwowski, H. J. ; Markoff, D. M. ; Tornow, W. ; Heeger, K. M. ; Decowski, M. 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E.</creatorcontrib><creatorcontrib>Lane, C. E.</creatorcontrib><creatorcontrib>Maricic, J.</creatorcontrib><creatorcontrib>Miletic, T.</creatorcontrib><creatorcontrib>Batygov, M.</creatorcontrib><creatorcontrib>Learned, J. G.</creatorcontrib><creatorcontrib>Matsuno, S.</creatorcontrib><creatorcontrib>Sakai, M.</creatorcontrib><creatorcontrib>Horton-Smith, G. A.</creatorcontrib><creatorcontrib>Downum, K. E.</creatorcontrib><creatorcontrib>Gratta, G.</creatorcontrib><creatorcontrib>Efremenko, Y.</creatorcontrib><creatorcontrib>Perevozchikov, O.</creatorcontrib><creatorcontrib>Karwowski, H. J.</creatorcontrib><creatorcontrib>Markoff, D. M.</creatorcontrib><creatorcontrib>Tornow, W.</creatorcontrib><creatorcontrib>Heeger, K. M.</creatorcontrib><creatorcontrib>Decowski, M. P.</creatorcontrib><creatorcontrib>Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)</creatorcontrib><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>Physical review. D, Particles, fields, gravitation, and cosmology</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>The KamLAND Collaboration</au><au>Gando, A.</au><au>Gando, Y.</au><au>Ichimura, K.</au><au>Ikeda, H.</au><au>Inoue, K.</au><au>Kibe, Y.</au><au>Kishimoto, Y.</au><au>Koga, M.</au><au>Minekawa, Y.</au><au>Mitsui, T.</au><au>Morikawa, T.</au><au>Nagai, N.</au><au>Nakajima, K.</au><au>Nakamura, K.</au><au>Narita, K.</au><au>Shimizu, I.</au><au>Shimizu, Y.</au><au>Shirai, J.</au><au>Suekane, F.</au><au>Suzuki, A.</au><au>Takahashi, H.</au><au>Takahashi, N.</au><au>Takemoto, Y.</au><au>Tamae, K.</au><au>Watanabe, H.</au><au>Xu, B. D.</au><au>Yabumoto, H.</au><au>Yoshida, H.</au><au>Yoshida, S.</au><au>Enomoto, S.</au><au>Kozlov, A.</au><au>Murayama, H.</au><au>Grant, C.</au><au>Keefer, G.</au><au>Piepke, A.</au><au>Banks, T. I.</au><au>Bloxham, T.</au><au>Detwiler, J. A.</au><au>Freedman, S. J.</au><au>Fujikawa, B. K.</au><au>Han, K.</au><au>Kadel, R.</au><au>O'Donnell, T.</au><au>Steiner, H. M.</au><au>Dwyer, D. A.</au><au>McKeown, R. D.</au><au>Zhang, C.</au><au>Berger, B. E.</au><au>Lane, C. E.</au><au>Maricic, J.</au><au>Miletic, T.</au><au>Batygov, M.</au><au>Learned, J. G.</au><au>Matsuno, S.</au><au>Sakai, M.</au><au>Horton-Smith, G. A.</au><au>Downum, K. E.</au><au>Gratta, G.</au><au>Efremenko, Y.</au><au>Perevozchikov, O.</au><au>Karwowski, H. J.</au><au>Markoff, D. M.</au><au>Tornow, W.</au><au>Heeger, K. M.</au><au>Decowski, M. P.</au><aucorp>Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Enhanced Constraints on theta13 from A Three-Flavor Oscillation Analysis of Reactor Antineutrinos at KamLAND</atitle><jtitle>Physical review. D, Particles, fields, gravitation, and cosmology</jtitle><date>2010-09-24</date><risdate>2010</risdate><issn>1550-7998</issn><eissn>1550-2368</eissn><abstract>We present new constraints on the neutrino oscillation parameters {Delta}m{sub 21}{sup 2}, {theta}{sub 12}, and {theta}{sub 13} from a three-flavor analysis of solar and KamLAND data. The KamLAND data set includes data acquired following a radiopurity upgrade and amounts to a total exposure of 3.49 x 10{sup 32} target-proton-year. Under the assumption of CPT invariance, a two-flavor analysis ({theta}{sub 13} = 0) of the KamLAND and solar data yields the best-fit values tan{sup 2} {theta}{sub 12} = 0.444{sub -0.030}{sup +0.036} and {Delta}m{sub 21}{sup 2} = 7.50{sub -0.20}{sup +0.19} x 10{sup -5} eV{sup 2}; a three-flavor analysis with {theta}{sub 13} as a free parameter yields the best-fit values tan{sup 2} {theta}{sub 12} = 0.452{sub -0.033}{sup +0.035}, {Delta}m{sub 21}{sup 2} = 7.50{sub -0.20}{sup +0.19} x 10{sup -5}eV{sup 2}, and sin{sup 2} {theta}{sub 13} = 0.020{sub -0.016}{sup +0.016}. This {theta}{sub 13} interval is consistent with other recent work combining the CHOOZ, atmospheric and long-baseline accelerator experiments. We also present a new global {theta}{sub 13} analysis, incorporating the CHOOZ, atmospheric and accelerator data, which indicates sin{sup 2} {theta}{sub 13} = 0.017{sub -0.009}{sup +0.010}, a nonzero value at the 93% C.L. This finding will be further tested by upcoming accelerator and reactor experiments.</abstract><cop>United States</cop><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 1550-7998 |
ispartof | Physical review. D, Particles, fields, gravitation, and cosmology, 2010-09 |
issn | 1550-7998 1550-2368 |
language | eng |
recordid | cdi_osti_scitechconnect_992481 |
source | American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list) |
subjects | 72 79 ACCELERATORS ANTINEUTRINOS NEUTRINO OSCILLATION OSCILLATIONS |
title | Enhanced Constraints on theta13 from A Three-Flavor Oscillation Analysis of Reactor Antineutrinos at KamLAND |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-02T03%3A03%3A59IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-osti&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Enhanced%20Constraints%20on%20theta13%20from%20A%20Three-Flavor%20Oscillation%20Analysis%20of%20Reactor%20Antineutrinos%20at%20KamLAND&rft.jtitle=Physical%20review.%20D,%20Particles,%20fields,%20gravitation,%20and%20cosmology&rft.au=The%20KamLAND%20Collaboration&rft.aucorp=Lawrence%20Berkeley%20National%20Lab.%20(LBNL),%20Berkeley,%20CA%20(United%20States)&rft.date=2010-09-24&rft.issn=1550-7998&rft.eissn=1550-2368&rft_id=info:doi/&rft_dat=%3Costi%3E992481%3C/osti%3E%3Cgrp_id%3Ecdi_FETCH-osti_scitechconnect_9924813%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |