Search for heavy neutrinos in K + → μ + ν H decays

Here, evidence of a heavy neutrino, νH, in the K+→μ+νH decays was sought using the E949 experimental data with an exposure of 1.70 × 1012 stopped kaons. With the major background from the radiative K+→μ+νμγ decay understood and suppressed, upper limits (90% C.L.) on the neutrino mixing matrix elemen...

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Veröffentlicht in:Physical review. D, Particles, fields, gravitation, and cosmology Particles, fields, gravitation, and cosmology, 2015-03, Vol.91 (5), Article 052001
Hauptverfasser: Artamonov, A. V., Bassalleck, B., Bhuyan, B., Blackmore, E. W., Bryman, D. A., Chen, S., Chiang, I-H., Christidi, I.-A., Cooper, P. S., Diwan, M. V., Frank, J. S., Fujiwara, T., Hu, J., Ives, J., Izmaylov, A. O., Jaffe, D. E., Kabe, S., Kettell, S. H., Khabibullin, M. M., Khotjantsev, A. N., Kitching, P., Kobayashi, M., Komatsubara, T. K., Konaka, A., Kudenko, Yu. G., Landsberg, L. G., Lewis, B., Li, K. K., Littenberg, L. S., Macdonald, J. A., Mildenberger, J., Mineev, O. V., Miyajima, M., Mizouchi, K., Muramatsu, N., Nakano, T., Nomachi, M., Nomura, T., Numao, T., Obraztsov, V. F., Omata, K., Patalakha, D. I., Poutissou, R., Redlinger, G., Sato, T., Sekiguchi, T., Shaikhiev, A. T., Shinkawa, T., Strand, R. C., Sugimoto, S., Tamagawa, Y., Tschirhart, R., Tsunemi, T., Vavilov, D. V., Viren, B., Wang, Zhe, Wei, Hanyu, Yershov, N. V., Yoshimura, Y., Yoshioka, T.
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container_title Physical review. D, Particles, fields, gravitation, and cosmology
container_volume 91
creator Artamonov, A. V.
Bassalleck, B.
Bhuyan, B.
Blackmore, E. W.
Bryman, D. A.
Chen, S.
Chiang, I-H.
Christidi, I.-A.
Cooper, P. S.
Diwan, M. V.
Frank, J. S.
Fujiwara, T.
Hu, J.
Ives, J.
Izmaylov, A. O.
Jaffe, D. E.
Kabe, S.
Kettell, S. H.
Khabibullin, M. M.
Khotjantsev, A. N.
Kitching, P.
Kobayashi, M.
Komatsubara, T. K.
Konaka, A.
Kudenko, Yu. G.
Landsberg, L. G.
Lewis, B.
Li, K. K.
Littenberg, L. S.
Macdonald, J. A.
Mildenberger, J.
Mineev, O. V.
Miyajima, M.
Mizouchi, K.
Muramatsu, N.
Nakano, T.
Nomachi, M.
Nomura, T.
Numao, T.
Obraztsov, V. F.
Omata, K.
Patalakha, D. I.
Poutissou, R.
Redlinger, G.
Sato, T.
Sekiguchi, T.
Shaikhiev, A. T.
Shinkawa, T.
Strand, R. C.
Sugimoto, S.
Tamagawa, Y.
Tschirhart, R.
Tsunemi, T.
Vavilov, D. V.
Viren, B.
Wang, Zhe
Wei, Hanyu
Yershov, N. V.
Yoshimura, Y.
Yoshioka, T.
description Here, evidence of a heavy neutrino, νH, in the K+→μ+νH decays was sought using the E949 experimental data with an exposure of 1.70 × 1012 stopped kaons. With the major background from the radiative K+→μ+νμγ decay understood and suppressed, upper limits (90% C.L.) on the neutrino mixing matrix element between the muon and heavy neutrinos, |UμH|2, were set at the level of 10–7 to 10–9 for the heavy neutrino mass region 175 to 300 MeV/c2.
doi_str_mv 10.1103/PhysRevD.91.052001
format Article
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Bassalleck, B. ; Bhuyan, B. ; Blackmore, E. W. ; Bryman, D. A. ; Chen, S. ; Chiang, I-H. ; Christidi, I.-A. ; Cooper, P. S. ; Diwan, M. V. ; Frank, J. S. ; Fujiwara, T. ; Hu, J. ; Ives, J. ; Izmaylov, A. O. ; Jaffe, D. E. ; Kabe, S. ; Kettell, S. H. ; Khabibullin, M. M. ; Khotjantsev, A. N. ; Kitching, P. ; Kobayashi, M. ; Komatsubara, T. K. ; Konaka, A. ; Kudenko, Yu. G. ; Landsberg, L. G. ; Lewis, B. ; Li, K. K. ; Littenberg, L. S. ; Macdonald, J. A. ; Mildenberger, J. ; Mineev, O. V. ; Miyajima, M. ; Mizouchi, K. ; Muramatsu, N. ; Nakano, T. ; Nomachi, M. ; Nomura, T. ; Numao, T. ; Obraztsov, V. F. ; Omata, K. ; Patalakha, D. I. ; Poutissou, R. ; Redlinger, G. ; Sato, T. ; Sekiguchi, T. ; Shaikhiev, A. T. ; Shinkawa, T. ; Strand, R. C. ; Sugimoto, S. ; Tamagawa, Y. ; Tschirhart, R. ; Tsunemi, T. ; Vavilov, D. V. ; Viren, B. ; Wang, Zhe ; Wei, Hanyu ; Yershov, N. V. ; Yoshimura, Y. ; Yoshioka, T.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c189t-42fec60796664fa80646538739260a5e2e4d07fcacaae1a69c1b240a6d1e21753</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</topic><toplevel>online_resources</toplevel><creatorcontrib>Artamonov, A. V.</creatorcontrib><creatorcontrib>Bassalleck, B.</creatorcontrib><creatorcontrib>Bhuyan, B.</creatorcontrib><creatorcontrib>Blackmore, E. W.</creatorcontrib><creatorcontrib>Bryman, D. A.</creatorcontrib><creatorcontrib>Chen, S.</creatorcontrib><creatorcontrib>Chiang, I-H.</creatorcontrib><creatorcontrib>Christidi, I.-A.</creatorcontrib><creatorcontrib>Cooper, P. S.</creatorcontrib><creatorcontrib>Diwan, M. V.</creatorcontrib><creatorcontrib>Frank, J. S.</creatorcontrib><creatorcontrib>Fujiwara, T.</creatorcontrib><creatorcontrib>Hu, J.</creatorcontrib><creatorcontrib>Ives, J.</creatorcontrib><creatorcontrib>Izmaylov, A. O.</creatorcontrib><creatorcontrib>Jaffe, D. E.</creatorcontrib><creatorcontrib>Kabe, S.</creatorcontrib><creatorcontrib>Kettell, S. H.</creatorcontrib><creatorcontrib>Khabibullin, M. M.</creatorcontrib><creatorcontrib>Khotjantsev, A. N.</creatorcontrib><creatorcontrib>Kitching, P.</creatorcontrib><creatorcontrib>Kobayashi, M.</creatorcontrib><creatorcontrib>Komatsubara, T. K.</creatorcontrib><creatorcontrib>Konaka, A.</creatorcontrib><creatorcontrib>Kudenko, Yu. G.</creatorcontrib><creatorcontrib>Landsberg, L. G.</creatorcontrib><creatorcontrib>Lewis, B.</creatorcontrib><creatorcontrib>Li, K. K.</creatorcontrib><creatorcontrib>Littenberg, L. S.</creatorcontrib><creatorcontrib>Macdonald, J. A.</creatorcontrib><creatorcontrib>Mildenberger, J.</creatorcontrib><creatorcontrib>Mineev, O. V.</creatorcontrib><creatorcontrib>Miyajima, M.</creatorcontrib><creatorcontrib>Mizouchi, K.</creatorcontrib><creatorcontrib>Muramatsu, N.</creatorcontrib><creatorcontrib>Nakano, T.</creatorcontrib><creatorcontrib>Nomachi, M.</creatorcontrib><creatorcontrib>Nomura, T.</creatorcontrib><creatorcontrib>Numao, T.</creatorcontrib><creatorcontrib>Obraztsov, V. F.</creatorcontrib><creatorcontrib>Omata, K.</creatorcontrib><creatorcontrib>Patalakha, D. I.</creatorcontrib><creatorcontrib>Poutissou, R.</creatorcontrib><creatorcontrib>Redlinger, G.</creatorcontrib><creatorcontrib>Sato, T.</creatorcontrib><creatorcontrib>Sekiguchi, T.</creatorcontrib><creatorcontrib>Shaikhiev, A. T.</creatorcontrib><creatorcontrib>Shinkawa, T.</creatorcontrib><creatorcontrib>Strand, R. C.</creatorcontrib><creatorcontrib>Sugimoto, S.</creatorcontrib><creatorcontrib>Tamagawa, Y.</creatorcontrib><creatorcontrib>Tschirhart, R.</creatorcontrib><creatorcontrib>Tsunemi, T.</creatorcontrib><creatorcontrib>Vavilov, D. V.</creatorcontrib><creatorcontrib>Viren, B.</creatorcontrib><creatorcontrib>Wang, Zhe</creatorcontrib><creatorcontrib>Wei, Hanyu</creatorcontrib><creatorcontrib>Yershov, N. V.</creatorcontrib><creatorcontrib>Yoshimura, Y.</creatorcontrib><creatorcontrib>Yoshioka, T.</creatorcontrib><creatorcontrib>E949 Collaboration</creatorcontrib><creatorcontrib>Fermi National Accelerator Lab. 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D, Particles, fields, gravitation, and cosmology</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Artamonov, A. V.</au><au>Bassalleck, B.</au><au>Bhuyan, B.</au><au>Blackmore, E. W.</au><au>Bryman, D. A.</au><au>Chen, S.</au><au>Chiang, I-H.</au><au>Christidi, I.-A.</au><au>Cooper, P. S.</au><au>Diwan, M. V.</au><au>Frank, J. S.</au><au>Fujiwara, T.</au><au>Hu, J.</au><au>Ives, J.</au><au>Izmaylov, A. O.</au><au>Jaffe, D. E.</au><au>Kabe, S.</au><au>Kettell, S. H.</au><au>Khabibullin, M. M.</au><au>Khotjantsev, A. N.</au><au>Kitching, P.</au><au>Kobayashi, M.</au><au>Komatsubara, T. K.</au><au>Konaka, A.</au><au>Kudenko, Yu. G.</au><au>Landsberg, L. G.</au><au>Lewis, B.</au><au>Li, K. K.</au><au>Littenberg, L. S.</au><au>Macdonald, J. A.</au><au>Mildenberger, J.</au><au>Mineev, O. V.</au><au>Miyajima, M.</au><au>Mizouchi, K.</au><au>Muramatsu, N.</au><au>Nakano, T.</au><au>Nomachi, M.</au><au>Nomura, T.</au><au>Numao, T.</au><au>Obraztsov, V. F.</au><au>Omata, K.</au><au>Patalakha, D. I.</au><au>Poutissou, R.</au><au>Redlinger, G.</au><au>Sato, T.</au><au>Sekiguchi, T.</au><au>Shaikhiev, A. T.</au><au>Shinkawa, T.</au><au>Strand, R. C.</au><au>Sugimoto, S.</au><au>Tamagawa, Y.</au><au>Tschirhart, R.</au><au>Tsunemi, T.</au><au>Vavilov, D. V.</au><au>Viren, B.</au><au>Wang, Zhe</au><au>Wei, Hanyu</au><au>Yershov, N. V.</au><au>Yoshimura, Y.</au><au>Yoshioka, T.</au><aucorp>E949 Collaboration</aucorp><aucorp>Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)</aucorp><aucorp>Brookhaven National Lab. (BNL), Upton, NY (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Search for heavy neutrinos in K + → μ + ν H decays</atitle><jtitle>Physical review. D, Particles, fields, gravitation, and cosmology</jtitle><date>2015-03-02</date><risdate>2015</risdate><volume>91</volume><issue>5</issue><artnum>052001</artnum><issn>1550-7998</issn><eissn>1550-2368</eissn><abstract>Here, evidence of a heavy neutrino, νH, in the K+→μ+νH decays was sought using the E949 experimental data with an exposure of 1.70 × 1012 stopped kaons. With the major background from the radiative K+→μ+νμγ decay understood and suppressed, upper limits (90% C.L.) on the neutrino mixing matrix element between the muon and heavy neutrinos, |UμH|2, were set at the level of 10–7 to 10–9 for the heavy neutrino mass region 175 to 300 MeV/c2.</abstract><cop>United States</cop><pub>American Physical Society (APS)</pub><doi>10.1103/PhysRevD.91.052001</doi><oa>free_for_read</oa></addata></record>
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1550-2368
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source American Physical Society Journals
subjects PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
title Search for heavy neutrinos in K + → μ + ν H decays
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