Measurement of atmospheric neutrino flux consistent with tau neutrino appearance
A search for the appearance of tau neutrinos from nu(mu) nu(tau) oscillations in the atmospheric neutrinos has been performed using 1489.2 days of atmospheric neutrino data from the Super-Kamiokande-I experiment. A best fit tau neutrino appearance signal of 138+/-48(stat)-32(+15)(syst) events is ob...
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| Veröffentlicht in: | Physical review letters 2006-10, Vol.97 (17), p.171801-171801, Article 171801 |
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| creator | Abe, K Hayato, Y Iida, T Ishihara, K Kameda, J Koshio, Y Minamino, A Mitsuda, C Miura, M Moriyama, S Nakahata, M Obayashi, Y Ogawa, H Shiozawa, M Suzuki, Y Takeda, A Takeuchi, Y Ueshima, K Higuchi, I Ishihara, C Ishitsuka, M Kajita, T Kaneyuki, K Mitsuka, G Nakayama, S Nishino, H Okumura, K Saji, C Takenaga, Y Totsuka, Y Clark, S Desai, S Dufour, F Kearns, E Likhoded, S Litos, M Raaf, J L Stone, J L Sulak, L R Wang, W Goldhaber, M Casper, D Cravens, J P Kropp, W R Liu, D W Mine, S Regis, C Smy, M B Sobel, H W Vagins, M R Ganezer, K S Hill, J E Keig, W E Jang, J S Kim, J Y Lim, I T Scholberg, K Tanimoto, N Walter, C W Wendell, R Ellsworth, R W Tasaka, S Guillian, E Learned, J G Matsuno, S Messier, M D Ichikawa, A K Ishida, T Ishii, T Iwashita, T Kobayashi, T Nakadaira, T Nakamura, K Nitta, K Oyama, Y Suzuki, A T Hasegawa, M Kato, I Maesaka, H Nakaya, T Nishikawa, K Sasaki, T Sato, H Yamamoto, S Yokoyama, M Haines, T J Dazeley, S Hatakeyama, S Svoboda, R Sullivan, G W Habig, A Gran, R Fukuda, Y Sato, T Itow, Y Koike, T Jung, C K Kato, T Kobayashi, K Malek, M |
| description | A search for the appearance of tau neutrinos from nu(mu) nu(tau) oscillations in the atmospheric neutrinos has been performed using 1489.2 days of atmospheric neutrino data from the Super-Kamiokande-I experiment. A best fit tau neutrino appearance signal of 138+/-48(stat)-32(+15)(syst) events is obtained with an expectation of 78+/-26(syst). The hypothesis of no tau neutrino appearance is disfavored by 2.4 sigma. |
| doi_str_mv | 10.1103/PhysRevLett.97.171801 |
| format | Article |
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A best fit tau neutrino appearance signal of 138+/-48(stat)-32(+15)(syst) events is obtained with an expectation of 78+/-26(syst). 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S</creatorcontrib><creatorcontrib>Hill, J E</creatorcontrib><creatorcontrib>Keig, W E</creatorcontrib><creatorcontrib>Jang, J S</creatorcontrib><creatorcontrib>Kim, J Y</creatorcontrib><creatorcontrib>Lim, I T</creatorcontrib><creatorcontrib>Scholberg, K</creatorcontrib><creatorcontrib>Tanimoto, N</creatorcontrib><creatorcontrib>Walter, C W</creatorcontrib><creatorcontrib>Wendell, R</creatorcontrib><creatorcontrib>Ellsworth, R W</creatorcontrib><creatorcontrib>Tasaka, S</creatorcontrib><creatorcontrib>Guillian, E</creatorcontrib><creatorcontrib>Learned, J G</creatorcontrib><creatorcontrib>Matsuno, S</creatorcontrib><creatorcontrib>Messier, M D</creatorcontrib><creatorcontrib>Ichikawa, A K</creatorcontrib><creatorcontrib>Ishida, T</creatorcontrib><creatorcontrib>Ishii, T</creatorcontrib><creatorcontrib>Iwashita, T</creatorcontrib><creatorcontrib>Kobayashi, T</creatorcontrib><creatorcontrib>Nakadaira, T</creatorcontrib><creatorcontrib>Nakamura, K</creatorcontrib><creatorcontrib>Nitta, K</creatorcontrib><creatorcontrib>Oyama, Y</creatorcontrib><creatorcontrib>Suzuki, A T</creatorcontrib><creatorcontrib>Hasegawa, M</creatorcontrib><creatorcontrib>Kato, I</creatorcontrib><creatorcontrib>Maesaka, H</creatorcontrib><creatorcontrib>Nakaya, T</creatorcontrib><creatorcontrib>Nishikawa, K</creatorcontrib><creatorcontrib>Sasaki, T</creatorcontrib><creatorcontrib>Sato, H</creatorcontrib><creatorcontrib>Yamamoto, S</creatorcontrib><creatorcontrib>Yokoyama, M</creatorcontrib><creatorcontrib>Haines, T J</creatorcontrib><creatorcontrib>Dazeley, S</creatorcontrib><creatorcontrib>Hatakeyama, S</creatorcontrib><creatorcontrib>Svoboda, R</creatorcontrib><creatorcontrib>Sullivan, G W</creatorcontrib><creatorcontrib>Habig, A</creatorcontrib><creatorcontrib>Gran, R</creatorcontrib><creatorcontrib>Fukuda, Y</creatorcontrib><creatorcontrib>Sato, T</creatorcontrib><creatorcontrib>Itow, Y</creatorcontrib><creatorcontrib>Koike, T</creatorcontrib><creatorcontrib>Jung, C K</creatorcontrib><creatorcontrib>Kato, T</creatorcontrib><creatorcontrib>Kobayashi, K</creatorcontrib><creatorcontrib>Malek, M</creatorcontrib><creatorcontrib>Super-Kamiokande Collaboration</creatorcontrib><title>Measurement of atmospheric neutrino flux consistent with tau neutrino appearance</title><title>Physical review letters</title><addtitle>Phys Rev Lett</addtitle><description>A search for the appearance of tau neutrinos from nu(mu) <--> nu(tau) oscillations in the atmospheric neutrinos has been performed using 1489.2 days of atmospheric neutrino data from the Super-Kamiokande-I experiment. A best fit tau neutrino appearance signal of 138+/-48(stat)-32(+15)(syst) events is obtained with an expectation of 78+/-26(syst). The hypothesis of no tau neutrino appearance is disfavored by 2.4 sigma.</description><subject>MEASURING METHODS</subject><subject>MUON NEUTRINOS</subject><subject>NEUTRON OSCILLATION</subject><subject>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</subject><subject>QUANTUM CHROMODYNAMICS</subject><subject>SIGNALS</subject><subject>TAU 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E</creatorcontrib><creatorcontrib>Jang, J S</creatorcontrib><creatorcontrib>Kim, J Y</creatorcontrib><creatorcontrib>Lim, I T</creatorcontrib><creatorcontrib>Scholberg, K</creatorcontrib><creatorcontrib>Tanimoto, N</creatorcontrib><creatorcontrib>Walter, C W</creatorcontrib><creatorcontrib>Wendell, R</creatorcontrib><creatorcontrib>Ellsworth, R W</creatorcontrib><creatorcontrib>Tasaka, S</creatorcontrib><creatorcontrib>Guillian, E</creatorcontrib><creatorcontrib>Learned, J G</creatorcontrib><creatorcontrib>Matsuno, S</creatorcontrib><creatorcontrib>Messier, M D</creatorcontrib><creatorcontrib>Ichikawa, A K</creatorcontrib><creatorcontrib>Ishida, T</creatorcontrib><creatorcontrib>Ishii, T</creatorcontrib><creatorcontrib>Iwashita, T</creatorcontrib><creatorcontrib>Kobayashi, T</creatorcontrib><creatorcontrib>Nakadaira, T</creatorcontrib><creatorcontrib>Nakamura, K</creatorcontrib><creatorcontrib>Nitta, K</creatorcontrib><creatorcontrib>Oyama, Y</creatorcontrib><creatorcontrib>Suzuki, A T</creatorcontrib><creatorcontrib>Hasegawa, M</creatorcontrib><creatorcontrib>Kato, I</creatorcontrib><creatorcontrib>Maesaka, H</creatorcontrib><creatorcontrib>Nakaya, T</creatorcontrib><creatorcontrib>Nishikawa, K</creatorcontrib><creatorcontrib>Sasaki, T</creatorcontrib><creatorcontrib>Sato, H</creatorcontrib><creatorcontrib>Yamamoto, S</creatorcontrib><creatorcontrib>Yokoyama, M</creatorcontrib><creatorcontrib>Haines, T J</creatorcontrib><creatorcontrib>Dazeley, S</creatorcontrib><creatorcontrib>Hatakeyama, S</creatorcontrib><creatorcontrib>Svoboda, R</creatorcontrib><creatorcontrib>Sullivan, G W</creatorcontrib><creatorcontrib>Habig, A</creatorcontrib><creatorcontrib>Gran, R</creatorcontrib><creatorcontrib>Fukuda, Y</creatorcontrib><creatorcontrib>Sato, T</creatorcontrib><creatorcontrib>Itow, Y</creatorcontrib><creatorcontrib>Koike, T</creatorcontrib><creatorcontrib>Jung, C K</creatorcontrib><creatorcontrib>Kato, T</creatorcontrib><creatorcontrib>Kobayashi, K</creatorcontrib><creatorcontrib>Malek, M</creatorcontrib><creatorcontrib>Super-Kamiokande Collaboration</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><collection>OSTI.GOV</collection><jtitle>Physical review letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Abe, K</au><au>Hayato, Y</au><au>Iida, T</au><au>Ishihara, K</au><au>Kameda, J</au><au>Koshio, Y</au><au>Minamino, A</au><au>Mitsuda, C</au><au>Miura, M</au><au>Moriyama, S</au><au>Nakahata, M</au><au>Obayashi, Y</au><au>Ogawa, H</au><au>Shiozawa, M</au><au>Suzuki, Y</au><au>Takeda, A</au><au>Takeuchi, Y</au><au>Ueshima, K</au><au>Higuchi, I</au><au>Ishihara, C</au><au>Ishitsuka, M</au><au>Kajita, T</au><au>Kaneyuki, K</au><au>Mitsuka, G</au><au>Nakayama, S</au><au>Nishino, H</au><au>Okumura, K</au><au>Saji, C</au><au>Takenaga, Y</au><au>Totsuka, Y</au><au>Clark, S</au><au>Desai, S</au><au>Dufour, F</au><au>Kearns, E</au><au>Likhoded, S</au><au>Litos, M</au><au>Raaf, J L</au><au>Stone, J L</au><au>Sulak, L R</au><au>Wang, W</au><au>Goldhaber, M</au><au>Casper, D</au><au>Cravens, J P</au><au>Kropp, W R</au><au>Liu, D W</au><au>Mine, S</au><au>Regis, C</au><au>Smy, M B</au><au>Sobel, H W</au><au>Vagins, M R</au><au>Ganezer, K S</au><au>Hill, J E</au><au>Keig, W E</au><au>Jang, J S</au><au>Kim, J Y</au><au>Lim, I T</au><au>Scholberg, K</au><au>Tanimoto, N</au><au>Walter, C W</au><au>Wendell, R</au><au>Ellsworth, R W</au><au>Tasaka, S</au><au>Guillian, E</au><au>Learned, J G</au><au>Matsuno, S</au><au>Messier, M D</au><au>Ichikawa, A K</au><au>Ishida, T</au><au>Ishii, T</au><au>Iwashita, T</au><au>Kobayashi, T</au><au>Nakadaira, T</au><au>Nakamura, K</au><au>Nitta, K</au><au>Oyama, Y</au><au>Suzuki, A T</au><au>Hasegawa, M</au><au>Kato, I</au><au>Maesaka, H</au><au>Nakaya, T</au><au>Nishikawa, K</au><au>Sasaki, T</au><au>Sato, H</au><au>Yamamoto, S</au><au>Yokoyama, M</au><au>Haines, T J</au><au>Dazeley, S</au><au>Hatakeyama, S</au><au>Svoboda, R</au><au>Sullivan, G W</au><au>Habig, A</au><au>Gran, R</au><au>Fukuda, Y</au><au>Sato, T</au><au>Itow, Y</au><au>Koike, T</au><au>Jung, C K</au><au>Kato, T</au><au>Kobayashi, K</au><au>Malek, M</au><aucorp>Super-Kamiokande Collaboration</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Measurement of atmospheric neutrino flux consistent with tau neutrino appearance</atitle><jtitle>Physical review letters</jtitle><addtitle>Phys Rev Lett</addtitle><date>2006-10-27</date><risdate>2006</risdate><volume>97</volume><issue>17</issue><spage>171801</spage><epage>171801</epage><pages>171801-171801</pages><artnum>171801</artnum><issn>0031-9007</issn><eissn>1079-7114</eissn><abstract>A search for the appearance of tau neutrinos from nu(mu) <--> nu(tau) oscillations in the atmospheric neutrinos has been performed using 1489.2 days of atmospheric neutrino data from the Super-Kamiokande-I experiment. A best fit tau neutrino appearance signal of 138+/-48(stat)-32(+15)(syst) events is obtained with an expectation of 78+/-26(syst). The hypothesis of no tau neutrino appearance is disfavored by 2.4 sigma.</abstract><cop>United States</cop><pmid>17155460</pmid><doi>10.1103/PhysRevLett.97.171801</doi><tpages>1</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0031-9007 |
| ispartof | Physical review letters, 2006-10, Vol.97 (17), p.171801-171801, Article 171801 |
| issn | 0031-9007 1079-7114 |
| language | eng |
| recordid | cdi_osti_scitechconnect_20861034 |
| source | American Physical Society Journals |
| subjects | MEASURING METHODS MUON NEUTRINOS NEUTRON OSCILLATION PHYSICS OF ELEMENTARY PARTICLES AND FIELDS QUANTUM CHROMODYNAMICS SIGNALS TAU NEUTRINOS |
| title | Measurement of atmospheric neutrino flux consistent with tau neutrino appearance |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-26T02%3A14%3A20IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Measurement%20of%20atmospheric%20neutrino%20flux%20consistent%20with%20tau%20neutrino%20appearance&rft.jtitle=Physical%20review%20letters&rft.au=Abe,%20K&rft.aucorp=Super-Kamiokande%20Collaboration&rft.date=2006-10-27&rft.volume=97&rft.issue=17&rft.spage=171801&rft.epage=171801&rft.pages=171801-171801&rft.artnum=171801&rft.issn=0031-9007&rft.eissn=1079-7114&rft_id=info:doi/10.1103/PhysRevLett.97.171801&rft_dat=%3Cproquest_osti_%3E68238021%3C/proquest_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=68238021&rft_id=info:pmid/17155460&rfr_iscdi=true |