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Meaney KD, Kim Y, Herrmann HW, Young CY, Archuleta TA, Hamilton CE, Duke DL, Haines TJ, Corredor AC, Green JA, Fegenbush L, Kaufman MI, Malone RM, Baker SA, Richardson S, Zier J, Engelbrecht J, Culver A. Characterization of the Mercury pulsed power x-ray source spectrum using multichannel density aerogel Cherenkov detectors. Rev Sci Instrum 2018; 89:10F113. [PMID: 30399895 DOI: 10.1063/1.5038745] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/04/2018] [Accepted: 08/02/2018] [Indexed: 06/08/2023]
Abstract
The Aerogel Cherenkov Detector for Cygnus (ACD/C) is a time-dependent, x-ray spectral detector that uses SiO2 aerogels spanning an index of refraction (n = 1.02-1.07) corresponding to a 1.1-2.3 MeV x-ray energy threshold. The ACD/C was developed for pulsed power x-ray sources like Cygnus located at the Nevada National Site and Mercury located at the Naval Research Laboratory (NRL). Aerogels sit between the measurement capabilities of gas (>2 MeV) and solids such as fused silica (>0.3 MeV). The detector uses an aluminum converter to Compton scatter incoming x-rays and create relativistic electrons, which produce Cherenkov light in an aerogel or a fused silica medium. The ACD/C was fielded at the NRL when Mercury was tuned to produce up to 4.8 MeV endpoint bremsstrahlung. Despite a high radiation and electromagnetic interference background, the ACD/C was able to achieve high signal over noise across five aerogel densities and fused silica, including a signal to noise for a 1.1 MeV aerogel threshold. Previous experiments at Cygnus observed a signal that was comparable to the noise (1×) at the same threshold. The ACD/C observed time-resolved rise and fall times for different energy thresholds of the photon spectrum. Monte Carlo simulations of the ACD/C's aerogel response curves were folded with a simulation of Mercury's photon energy spectrum and agree within the error to the observed result.
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Affiliation(s)
- K D Meaney
- Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - Y Kim
- Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - H W Herrmann
- Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - C Y Young
- Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - T A Archuleta
- Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - C E Hamilton
- Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - D L Duke
- Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - T J Haines
- Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - A C Corredor
- Mission Support and Test Services, Las Vegas, Nevada 89193, USA
| | - J A Green
- Mission Support and Test Services, Las Vegas, Nevada 89193, USA
| | - L Fegenbush
- Mission Support and Test Services, Las Vegas, Nevada 89193, USA
| | - M I Kaufman
- Mission Support and Test Services, Las Vegas, Nevada 89193, USA
| | - R M Malone
- Mission Support and Test Services, Las Vegas, Nevada 89193, USA
| | - S A Baker
- Mission Support and Test Services, Las Vegas, Nevada 89193, USA
| | - S Richardson
- Naval Research Laboratory, Washington, District of Columbia 20375, USA
| | - J Zier
- Naval Research Laboratory, Washington, District of Columbia 20375, USA
| | - J Engelbrecht
- Naval Research Laboratory, Washington, District of Columbia 20375, USA
| | - A Culver
- Naval Research Laboratory, Washington, District of Columbia 20375, USA
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Abe K, Hayato Y, Iida T, Ikeda M, Kameda J, Koshio Y, Minamino A, Miura M, Moriyama S, Nakahata M, Nakayama S, Obayashi Y, Ogawa H, Sekiya H, Shiozawa M, Suzuki Y, Takeda A, Takeuchi Y, Ueshima K, Watanabe H, Yamada S, Higuchi I, Ishihara C, Kajita T, Kaneyuki K, Mitsuka G, Nishino H, Okumura K, Saji C, Takenaga Y, Clark S, Desai S, Dufour F, Kearns E, Likhoded S, Litos M, Raaf JL, Stone JL, Sulak LR, Wang W, Goldhaber M, Casper D, Cravens JP, Dunmore J, Kropp WR, Liu DW, Mine S, Regis C, Smy MB, Sobel HW, Vagins MR, Ganezer KS, Hartfield B, Hill J, Keig WE, Jang JS, Jeong IS, Kim JY, Lim IT, Scholberg K, Fechner M, Tanimoto N, Walter CW, Wendell R, Tasaka S, Guillian G, Learned JG, Matsuno S, Messier MD, Hasegawa T, Ishida T, Ishii T, Kobayashi T, Nakadaira T, Nakamura K, Nishikawa K, Oyama Y, Totsuka Y, Suzuki AT, Nakaya T, Tanaka H, Yokoyama M, Haines TJ, Dazeley S, Svoboda R, Habig A, Fukuda Y, Sato T, Itow Y, Koike T, Tanaka T, Jung CK, Kato T, Kobayashi K, McGrew C, Sarrat A, Terri R, Yanagisawa C, Tamura N, Idehara Y, Sakuda M, Sugihara M, Kuno Y, Yoshida M, Kim SB, Yang BS, Ishizuka T, Okazawa H, Choi Y, Seo HK, Gando Y, Inoue K, Furuse Y, Ishii H, Nishijima K, Watanabe Y, Koshiba M, Chen S, Deng Z, Liu Y, Kielczewska D, Berns H, Shiraishi KK, Thrane E, Wilkes RJ. Search for matter-dependent atmospheric neutrino oscillations in Super-Kamiokande. Int J Clin Exp Med 2008. [DOI: 10.1103/physrevd.77.052001] [Citation(s) in RCA: 12] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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3
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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 JL, Stone JL, Sulak LR, Wang W, Goldhaber M, Casper D, Cravens JP, Kropp WR, Liu DW, Mine S, Regis C, Smy MB, Sobel HW, Vagins MR, Ganezer KS, Hill JE, Keig WE, Jang JS, Kim JY, Lim IT, Scholberg K, Tanimoto N, Walter CW, Wendell R, Ellsworth RW, Tasaka S, Guillian E, Learned JG, Matsuno S, Messier MD, Ichikawa AK, Ishida T, Ishii T, Iwashita T, Kobayashi T, Nakadaira T, Nakamura K, Nitta K, Oyama Y, Suzuki AT, Hasegawa M, Kato I, Maesaka H, Nakaya T, Nishikawa K, Sasaki T, Sato H, Yamamoto S, Yokoyama M, Haines TJ, Dazeley S, Hatakeyama S, Svoboda R, Sullivan GW, Habig A, Gran R, Fukuda Y, Sato T, Itow Y, Koike T, Jung CK, Kato T, Kobayashi K, Malek M, McGrew C, Sarrat A, Terri R, Yanagisawa C, Tamura N, Sakuda M, Sugihara M, Kuno Y, Yoshida M, Kim SB, Yoo J, Ishizuka T, Okazawa H, Choi Y, Seo HK, Gando Y, Hasegawa T, Inoue K, Ishii H, Nishijima K, Ishino H, Watanabe Y, Koshiba M, Kielczewska D, Zalipska J, Berns HG, Shiraishi KK, Washburn K, Wilkes RJ. Measurement of atmospheric neutrino flux consistent with tau neutrino appearance. Phys Rev Lett 2006; 97:171801. [PMID: 17155460 DOI: 10.1103/physrevlett.97.171801] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/25/2006] [Indexed: 05/12/2023]
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.
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Affiliation(s)
- K Abe
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
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4
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Atkins R, Benbow W, Berley D, Blaufuss E, Coyne DG, DeYoung T, Dingus BL, Dorfan DE, Ellsworth RW, Fleysher L, Fleysher R, Gisler G, Gonzalez MM, Goodman JA, Haines TJ, Hays E, Hoffman CM, Kelley LA, Lansdell CP, Linnemann JT, McEnery JE, Miller RS, Mincer AI, Morales MF, Nemethy P, Noyes D, Ryan JM, Samuelson FW, Parkinson PMS, Shoup A, Sinnis G, Smith AJ, Sullivan GW, Williams DA, Wilson ME, Xu XW, Yodh GB. Evidence for TeV gamma-ray emission from a region of the galactic plane. Phys Rev Lett 2005; 95:251103. [PMID: 16384445 DOI: 10.1103/physrevlett.95.251103] [Citation(s) in RCA: 9] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/15/2005] [Revised: 10/05/2005] [Indexed: 05/05/2023]
Abstract
Gamma-ray emission from a narrow band at the galactic equator has previously been detected up to 30 GeV. We report evidence for a TeV gamma-ray signal from a region of the galactic plane by Milagro, a large-field-of-view water Cherenkov detector for extensive air showers. An excess with a significance of 4.5 standard deviations has been observed from the region of galactic longitude l E (40 degrees, 100 degrees) and latitude /b/ < 5 degrees. Under the assumption of a simple power law spectrum, with no cutoff in the EGRET-Milagro energy range, the measured integral flux is phi gamma(>3.5 TeV) = (6.4 +/- 1.4 +/- 2.1) x 10(-11) cm(-2) s(-1) sr(-1). This flux is consistent with an extrapolation of the EGRET spectrum between 1 and 30 GeV in this galactic region.
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Affiliation(s)
- R Atkins
- Department of Physics, University of Wisconsin, 1150 University Avenue, Madison, Wisconsin 53706, USA
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5
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Ashie Y, Hosaka J, Ishihara K, Itow Y, Kameda J, Koshio Y, Minamino A, Mitsuda C, Miura M, Moriyama S, Nakahata M, Namba T, Nambu R, Obayashi Y, Shiozawa M, Suzuki Y, Takeuchi Y, Taki K, Yamada S, Ishitsuka M, Kajita T, Kaneyuki K, Nakayama S, Okada A, Okumura K, Ooyabu T, Saji C, Takenaga Y, Desai S, Kearns E, Likhoded S, Stone JL, Sulak LR, Walter CW, Wang W, Goldhaber M, Casper D, Cravens JP, Gajewski W, Kropp WR, Liu DW, Mine S, Smy MB, Sobel HW, Sterner CW, Vagins MR, Ganezer KS, Hill J, Keig WE, Jang JS, Kim JY, Lim IT, Ellsworth RW, Tasaka S, Guillian G, Kibayashi A, Learned JG, Matsuno S, Takemori D, Messier MD, Hayato Y, Ichikawa AK, Ishida T, Ishii T, Iwashita T, Kobayashi T, Maruyama T, Nakamura K, Nitta K, Oyama Y, Sakuda M, Totsuka Y, Suzuki AT, Hasegawa M, Hayashi K, Inagaki T, Kato I, Maesaka H, Morita T, Nakaya T, Nishikawa K, Sasaki T, Ueda S, Yamamoto S, Haines TJ, Dazeley S, Hatakeyama S, Svoboda R, Blaufuss E, Goodman JA, Sullivan GW, Turcan D, Scholberg K, Habig A, Fukuda Y, Jung CK, Kato T, Kobayashi K, Malek M, Mauger C, McGrew C, Sarrat A, Sharkey E, Yanagisawa C, Toshito T, Miyano K, Tamura N, Ishii J, Kuno Y, Nagashima Y, Takita M, Yoshida M, Kim SB, Yoo J, Okazawa H, Ishizuka T, Choi Y, Seo HK, Gando Y, Hasegawa T, Inoue K, Shirai J, Suzuki A, Koshiba M, Nakajima Y, Nishijima K, Harada T, Ishino H, Nishimura R, Watanabe Y, Kielczewska D, Zalipska J, Berns HG, Gran R, Shiraishi KK, Stachyra A, Washburn K, Wilkes RJ. Evidence for an oscillatory signature in atmospheric neutrino oscillations. Phys Rev Lett 2004; 93:101801. [PMID: 15447395 DOI: 10.1103/physrevlett.93.101801] [Citation(s) in RCA: 51] [Impact Index Per Article: 2.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/27/2004] [Indexed: 05/14/2023]
Abstract
Muon neutrino disappearance probability as a function of neutrino flight length L over neutrino energy E was studied. A dip in the L/E distribution was observed in the data, as predicted from the sinusoidal flavor transition probability of neutrino oscillation. The observed L/E distribution constrained nu(micro)<-->nu(tau) neutrino oscillation parameters; 1.9x10(-3)<Deltam(2)<3.0x10(-3) eV(2) and sin((2)2theta>0.90 at 90% confidence level.
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Affiliation(s)
- Y Ashie
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu, 506-1205, Japan
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6
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Liu DW, Ashie Y, Fukuda S, Fukuda Y, Ishihara K, Itow Y, Koshio Y, Minamino A, Miura M, Moriyama S, Nakahata M, Namba T, Nambu R, Obayashi Y, Sakurai N, Shiozawa M, Suzuki Y, Takeuchi H, Takeuchi Y, Yamada S, Ishitsuka M, Kajita T, Kaneyuki K, Nakayama S, Okada A, Ooyabu T, Saji C, Desai S, Earl M, Kearns E, Messier MD, Stone JL, Sulak LR, Walter CW, Wang W, Barszczak T, Casper D, Cravens JP, Gajewski W, Kropp WR, Mine S, Smy MB, Sobel HW, Sterner CW, Vagins MR, Ganezer KS, Hill J, Keig WE, Kim JY, Lim IT, Ellsworth RW, Tasaka S, Kibayashi A, Learned JG, Matsuno S, Takemori D, Hayato Y, Ichikawa AK, Ishida T, Ishii T, Iwashita T, Kameda J, Kobayashi T, Maruyama T, Nakamura K, Nitta K, Oyama Y, Sakuda M, Totsuka Y, Suzuki AT, Hasegawa M, Hayashi K, Inagaki T, Kato I, Maesaka H, Morita T, Nakaya T, Nishikawa K, Sasaki T, Ueda S, Yamamoto S, Haines TJ, Dazeley S, Hatakeyama S, Svoboda R, Blaufuss E, Goodman JA, Guillian G, Sullivan GW, Turcan D, Scholberg K, Habig A, Ackermann M, Jung CK, Kato T, Kobayashi K, Martens K, Malek M, Mauger C, McGrew C, Sharkey E, Viren B, Yanagisawa C, Toshito T, Mitsuda C, Miyano K, Shibata T, Ishii J, Kajiyama Y, Kuno Y, Nagashima Y, Takita M, Yoshida M, Kim HI, Kim SB, Yoo J, Okazawa H, Ishizuka T, Choi Y, Seo HK, Gando Y, Hasegawa T, Inoue K, Shirai J, Suzuki A, Koshiba M, Hashimoto T, Nakajima Y, Nishijima K, Ishino H, Morii M, Nishimura R, Watanabe Y, Kielczewska D, Zalipska J, Gran R, Shiraishi KK, Washburn K, Wilkes RJ. Limits on the neutrino magnetic moment using 1496 days of Super-Kamiokande-I solar neutrino data. Phys Rev Lett 2004; 93:021802. [PMID: 15323899 DOI: 10.1103/physrevlett.93.021802] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/07/2004] [Indexed: 05/24/2023]
Abstract
A search for a nonzero neutrino magnetic moment has been conducted using 1496 live days of solar neutrino data from Super-Kamiokande-I. Specifically, we searched for distortions to the energy spectrum of recoil electrons arising from magnetic scattering due to a nonzero neutrino magnetic moment. In the absence of a clear signal, we found micro(nu)</=(3.6x10(-10))micro(B) at 90% C.L. by fitting to the Super-Kamiokande day-night spectra. The fitting took into account the effect of neutrino oscillation on the shapes of energy spectra. With additional information from other solar neutrino and KamLAND experiments constraining the oscillation region, a limit of micro(nu)</=(1.1x10(-10))micro(B) at 90% C.L. was obtained.
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Affiliation(s)
- D W Liu
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
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7
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Gando Y, Fukuda S, Fukuda Y, Ishitsuka M, Itow Y, Kajita T, Kameda J, Kaneyuki K, Kobayashi K, Koshio Y, Miura M, Moriyama S, Nakahata M, Nakayama S, Namba T, Obayashi Y, Okada A, Ooyabu T, Saji C, Sakurai N, Shiozawa M, Suzuki Y, Takeuchi H, Takeuchi Y, Totsuka Y, Yamada S, Desai S, Earl M, Kearns E, Messier MD, Stone JL, Sulak LR, Walter CW, Goldhaber M, Barszczak T, Casper D, Gajewski W, Kropp WR, Mine S, Liu DW, Smy MB, Sobel HW, Vagins MR, Gago A, Ganezer KS, Hill J, Keig WE, Ellsworth RW, Tasaka S, Kibayashi A, Learned JG, Matsuno S, Takemori D, Hayato Y, Ichikawa AK, Ishii T, Kobayashi T, Maruyama T, Nakamura K, Oyama Y, Sakuda M, Yoshida M, Kohama M, Iwashita T, Suzuki AT, Inagaki T, Kato I, Nakaya T, Nishikawa K, Haines TJ, Dazeley S, Hatakeyama S, Svoboda R, Blaufuss E, Chen ML, Goodman JA, Guillian G, Sullivan GW, Turcan D, Scholberg K, Habig A, Ackermann M, Jung CK, Martens K, Malek M, Mauger C, McGrew C, Sharkey E, Viren B, Yanagisawa C, Toshito T, Mitsuda C, Miyano K, Shibata T, Kajiyama Y, Nagashima Y, Nitta K, Takita M, Kim HI, Kim SB, Yoo J, Okazawa H, Ishizuka T, Etoh M, Hasegawa T, Inoue K, Ishihara K, Shirai J, Suzuki A, Koshiba M, Hatakeyama Y, Ichikawa Y, Koike M, Nishijima K, Ishino H, Morii M, Nishimura R, Watanabe Y, Kielczewska D, Berns HG, Boyd SC, Stachyra AL, Wilkes RJ. Search for nu(e) from the sun at Super-Kamiokande-I. Phys Rev Lett 2003; 90:171302. [PMID: 12786067 DOI: 10.1103/physrevlett.90.171302] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/30/2002] [Indexed: 05/24/2023]
Abstract
We present the results of a search for low energy nu(e) from the Sun using 1496 days of data from Super-Kamiokande-I. We observe no significant excess of events and set an upper limit for the conversion probability to nu(e) of the 8B solar neutrino. This conversion limit is 0.8% (90% C.L.) of the standard solar model's neutrino flux for total energy=8-20 MeV. We also set a flux limit for monochromatic nu(e) for E(nu(e))=10-17 MeV.
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Affiliation(s)
- Y Gando
- Research Center for Neutrino Science, Tohoku University, Sendai, Miyagi 980-8578, Japan
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8
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Malek M, Morii M, Fukuda S, Fukuda Y, Ishitsuka M, Itow Y, Kajita T, Kameda J, Kaneyuki K, Kobayashi K, Koshio Y, Miura M, Moriyama S, Nakahata M, Nakayama S, Namba T, Okada A, Ooyabu T, Saji C, Sakurai N, Shiozawa M, Suzuki Y, Takeuchi H, Takeuchi Y, Totsuka Y, Yamada S, Desai S, Earl M, Kearns E, Messier MD, Stone JL, Sulak LR, Walter CW, Goldhaber M, Barszczak T, Casper D, Gajewski W, Kropp WR, Mine S, Liu DW, Smy MB, Sobel HW, Vagins MR, Gago A, Ganezer KS, Keig WE, Ellsworth RW, Tasaka S, Kibayashi A, Learned JG, Matsuno S, Takemori D, Hayato Y, Ishii T, Kobayashi T, Maruyama T, Nakamura K, Obayashi Y, Oyama Y, Sakuda M, Yoshida M, Kohama M, Iwashita T, Suzuki AT, Ichikawa A, Inagaki T, Kato I, Nakaya T, Nishikawa K, Haines TJ, Dazeley S, Hatakeyama S, Svoboda R, Blaufuss E, Goodman JA, Guillian G, Sullivan GW, Turcan D, Scholberg K, Habig A, Ackermann M, Hill J, Jung CK, Martens K, Mauger C, McGrew C, Sharkey E, Viren B, Yanagisawa C, Toshito T, Mitsuda C, Miyano K, Shibata T, Kajiyama Y, Nagashima Y, Nitta K, Takita M, Kim HI, Kim SB, Yoo J, Okazawa H, Ishizuka T, Etoh M, Gando Y, Hasegawa T, Inoue K, Ishihara K, Shirai J, Suzuki A, Koshiba M, Hatakeyama Y, Ichikawa Y, Koike M, Nishijima K, Ishino H, Nishimura R, Watanabe Y, Kielczewska D, Berns HG, Boyd SC, Stachyra AL, Wilkes RJ. Search for supernova relic neutrinos at Super-Kamiokande. Phys Rev Lett 2003; 90:061101. [PMID: 12633283 DOI: 10.1103/physrevlett.90.061101] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/15/2002] [Revised: 10/21/2002] [Indexed: 05/24/2023]
Abstract
A search for the relic neutrinos from all past core-collapse supernovae was conducted using 1496 days of data from the Super-Kamiokande detector. This analysis looked for electron-type antineutrinos that had produced a positron with an energy greater than 18 MeV. In the absence of a signal, 90% C.L. upper limits on the total flux were set for several theoretical models; these limits ranged from 20 to 130 macro nu(e) cm(-2) s(-1). Additionally, an upper bound of 1.2 macro nu(e) cm(-2) s(-1) was set for the supernova relic neutrino flux in the energy region E(nu)>19.3 MeV.
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Affiliation(s)
- M Malek
- Department of Physics and Astronomy, State University of New York, Stony Brook, New York 11794-3800, USA
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9
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Fukuda S, Fukuda Y, Ishitsuka M, Itow Y, Kajita T, Kameda J, Kaneyuki K, Kobayashi K, Koshio Y, Miura M, Moriyama S, Nakahata M, Nakayama S, Okada A, Sakurai N, Shiozawa M, Suzuki Y, Takeuchi H, Takeuchi Y, Toshito T, Totsuka Y, Yamada S, Desai S, Earl M, Kearns E, Messier MD, Scholberg K, Stone JL, Sulak LR, Walter CW, Goldhaber M, Barszczak T, Casper D, Gajewski W, Kropp WR, Mine S, Liu DW, Price LR, Smy MB, Sobel HW, Vagins MR, Ganezer KS, Keig WE, Ellsworth RW, Tasaka S, Kibayashi A, Learned JG, Matsuno S, Takemori D, Hayato Y, Ishii T, Kobayashi T, Nakamura K, Obayashi Y, Oyama Y, Sakai A, Sakuda M, Kohama M, Suzuki AT, Inagaki T, Nakaya T, Nishikawa K, Haines TJ, Blaufuss E, Dazeley S, Lee KB, Svoboda R, Goodman JA, Guillian G, Sullivan GW, Turcan D, Habig A, Hill J, Jung CK, Martens K, Malek M, Mauger C, McGrew C, Sharkey E, Viren B, Yanagisawa C, Mitsuda C, Miyano K, Saji C, Shibata T, Kajiyama Y, Nagashima Y, Nitta K, Takita M, Yoshida M, Kim HI, Kim SB, Yoo J, Okazawa H, Ishizuka T, Etoh M, Gando Y, Hasegawa T, Inoue K, Ishihara K, Maruyama T, Shirai J, Suzuki A, Koshiba M, Hatakeyama Y, Ichikawa Y, Koike M, Nishijima K, Fujiyasu H, Ishino H, Morii M, Watanabe Y, Golebiewska U, Kielczewska D, Boyd SC, Stachyra AL, Wilkes RJ, Young KK. Constraints on neutrino oscillations using 1258 days of Super-Kamiokande solar neutrino data. Phys Rev Lett 2001; 86:5656-5660. [PMID: 11415326 DOI: 10.1103/physrevlett.86.5656] [Citation(s) in RCA: 50] [Impact Index Per Article: 2.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/19/2001] [Indexed: 05/23/2023]
Abstract
We report the result of a search for neutrino oscillations using precise measurements of the recoil electron energy spectrum and zenith angle variations of the solar neutrino flux from 1258 days of neutrino-electron scattering data in Super-Kamiokande. The absence of significant zenith angle variation and spectrum distortion places strong constraints on neutrino mixing and mass difference in a flux-independent way. Using the Super-Kamiokande flux measurement in addition, two allowed regions at large mixing are found.
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Affiliation(s)
- S Fukuda
- Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
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10
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Fukuda S, Fukuda Y, Ishitsuka M, Itow Y, Kajita T, Kameda J, Kaneyuki K, Kobayashi K, Koshio Y, Miura M, Moriyama S, Nakahata M, Nakayama S, Okada A, Sakurai N, Shiozawa M, Suzuki Y, Takeuchi H, Takeuchi Y, Toshito T, Totsuka Y, Yamada S, Desai S, Earl M, Kearns E, Messier MD, Scholberg K, Stone JL, Sulak LR, Walter CW, Goldhaber M, Barszczak T, Casper D, Gajewski W, Kropp WR, Mine S, Liu DW, Price LR, Smy MB, Sobel HW, Vagins MR, Ganezer KS, Keig WE, Ellsworth RW, Tasaka S, Kibayashi A, Learned JG, Matsuno S, Takemori D, Hayato Y, Ishii T, Kobayashi T, Nakamura K, Obayashi Y, Oyama Y, Sakai A, Sakuda M, Kohama M, Suzuki AT, Inagaki T, Nakaya T, Nishikawa K, Haines TJ, Blaufuss E, Dazeley S, Lee KB, Svoboda R, Goodman JA, Guillian G, Sullivan GW, Turcan D, Habig A, Hill J, Jung CK, Martens K, Malek M, Mauger C, McGrew C, Sharkey E, Viren B, Yanagisawa C, Mitsuda C, Miyano K, Saji C, Shibata T, Kajiyama Y, Nagashima Y, Nitta K, Takita M, Yoshida M, Kim HI, Kim SB, Yoo J, Okazawa H, Ishizuka T, Etoh M, Gando Y, Hasegawa T, Inoue K, Ishihara K, Maruyama T, Shirai J, Suzuki A, Koshiba M, Hatakeyama Y, Ichikawa Y, Koike M, Nishijima K, Fujiyasu H, Ishino H, Morii M, Watanabe Y, Golebiewska U, Kielczewska D, Boyd SC, Stachyra AL, Wilkes RJ, Young KK. Solar 8B and hep neutrino measurements from 1258 days of Super-Kamiokande data. Phys Rev Lett 2001; 86:5651-5655. [PMID: 11415325 DOI: 10.1103/physrevlett.86.5651] [Citation(s) in RCA: 59] [Impact Index Per Article: 2.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/19/2001] [Indexed: 05/23/2023]
Abstract
Solar neutrino measurements from 1258 days of data from the Super-Kamiokande detector are presented. The measurements are based on recoil electrons in the energy range 5.0-20.0 MeV. The measured solar neutrino flux is 2.32+/-0.03(stat)+0.08-0.07(syst)x10(6) cm(-2) x s(-1), which is 45.1+/-0.5(stat)+1.6-1.4(syst)% of that predicted by the BP2000 SSM. The day vs night flux asymmetry (Phi(n)-Phi(d))/Phi(average) is 0.033+/-0.022(stat)+0.013-0.012(syst). The recoil electron energy spectrum is consistent with no spectral distortion. For the hep neutrino flux, we set a 90% C.L. upper limit of 40x10(3) cm(-2) x s(-1), which is 4.3 times the BP2000 SSM prediction.
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Affiliation(s)
- S Fukuda
- Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
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11
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Atkins R, Benbow W, Berley D, Chen ML, Coyne DG, Dingus BL, Dorfan DE, Ellsworth RW, Evans D, Falcone A, Fleysher L, Fleysher R, Gisler G, Goodman JA, Haines TJ, Hoffman CM, Hugenberger S, Kelley LA, Leonor I, McConnell M, McCullough JF, McEnery JE, Miller RS, Mincer AI, Morales MF, Nemethy P, Ryan JM, Shen B, Shoup A, Sinnis C, Smith AJ, Sullivan GW, Tumer T, Wang K, Wascko MO, Westerhoff S, Williams DA, Yang T, Yodh GB. Evidence for TeV Emission from GRB 970417a. Astrophys J 2000; 533:L119-L122. [PMID: 10770704 DOI: 10.1086/312629] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/15/1999] [Accepted: 03/03/2000] [Indexed: 05/23/2023]
Abstract
Milagrito, a detector sensitive to very high energy gamma rays, monitored the northern sky from 1997 February through 1998 May. With a large field of view and a high duty cycle, this instrument was well suited to perform a search for TeV gamma-ray bursts (GRBs). We report on a search made for TeV counterparts to GRBs observed by BATSE. BATSE detected 54 GRBs within the field of view of Milagrito during this period. An excess of events coincident in time and space with one of these bursts, GRB 970417a, was observed by Milagrito. The excess has a chance probability of 2.8x10-5 of being a fluctuation of the background. The probability for observing an excess at least this large from any of the 54 bursts is 1.5x10-3. No significant correlations were detected from the other bursts.
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Atkins R, Benbow W, Berley D, Chen ML, Coyne DG, Delay RS, Dingus BL, Dorfan DE, Ellsworth RW, Espinoza C, Evans D, Falcone A, Fleysher L, Fleysher R, Gisler G, Goodman JA, Haines TJ, Hoffman CM, Hugenberger S, Kelley LA, Leonor I, McConnell M, McCullough JF, McEnery JE, Miller RS, Mincer AI, Morales MF, Murray MM, Nemethy P, Ryan JM, Schneider M, Shen B, Shoup A, Sinnis C, Smith AJ, Sullivan GW, Thompson TN, Tumer T, Wang K, Wascko MO, Westerhoff S, Williams DA, Yang T, Yodh GB. TeV Observations of Markarian 501 with the Milagrito Water Cerenkov Detector. Astrophys J 1999; 525:L25-L28. [PMID: 10511505 DOI: 10.1086/312332] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
Abstract
The Milagrito water Cerenkov detector near Los Alamos, New Mexico, was operated as a sky monitor at energies of a few TeV between 1997 February and 1998 May, including the period of the strong, long-lasting 1997 flare of Markarian 501. Milagrito served as a test run for the full Milagro detector. An event excess with a significance of 3.7 sigma from Markarian 501 was observed, in agreement with expectations.
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Becker-Szendy R, Bratton CB, Breault J, Casper D, Dye ST, Ganezer K, Gajewski W, Goldhaber M, Haines TJ, Halverson PG, Kielczewska D, Kropp WR, Learned JG, LoSecco J, Matsuno S, McGrath G, McGrew C, Miller RS, Price L, Reines F, Schultz J, Sobel HW, Stone JL, Sulak LR, Svoboda R. New magnetic monopole flux limits from the IMB proton decay detector. Phys Rev D Part Fields 1994; 49:2169-2173. [PMID: 10017205 DOI: 10.1103/physrevd.49.2169] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/22/2023]
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14
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Alexandreas DE, Allen GE, Berley D, Biller S, Burman RL, Cavalli-Sforza M, Chang CY, Chen ML, Chumney P, Coyne D, Dion C, Dion GM, Dorfan D, Ellsworth RW, Goodman JA, Haines TJ, Harmon M, Hoffman CM, Kelley L, Klein S, Nagle DE, Schmidt DM, Schnee R, Sinnis C, Shoup A, Stark MJ, Weeks DD, Williams DA, Wu JP, Yang T, Yodh GB, Zhang WP. New limit on the rate-density of evaporating black holes. Phys Rev Lett 1993; 71:2524-2527. [PMID: 10054704 DOI: 10.1103/physrevlett.71.2524] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
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15
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Becker-Szendy R, Bratton CB, Casper D, Dye ST, Gajewski W, Goldhaber M, Haines TJ, Halverson PG, Kielczewska D, Kropp WR, Learned JG, LoSecco JM, Matsuno S, McGrath G, McGrew C, Miller RS, Price L, Reines F, Schultz J, Sobel HW, Stone JL, Sulak LR, Svoboda R. Study of underground muons during the January 1991 radio flare of Cygnus X-3. Int J Clin Exp Med 1993; 47:4203-4205. [PMID: 10015414 DOI: 10.1103/physrevd.47.4203] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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16
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Becker-Szendy R, Bratton CB, Casper D, Dye ST, Gajewski W, Goldhaber M, Haines TJ, Halverson PG, Kielczewska D, Kropp WR, Learned JG, LoSecco JM, Matsuno S, McGrath G, McGrew C, Miller R, Price LR, Reines F, Schultz J, Sobel HW, Stone JL, Sulak LR, Svoboda R. Electron- and muon-neutrino content of the atmospheric flux. Phys Rev D Part Fields 1992; 46:3720-3724. [PMID: 10015325 DOI: 10.1103/physrevd.46.3720] [Citation(s) in RCA: 33] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/22/2023]
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17
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Becker-Szendy R, Bratton CB, Casper D, Dye ST, Gajewski W, Goldhaber M, Haines TJ, Halverson PG, Jones T, Kielczewska D, Kropp WR, Learned JG, LoSecco J, McGrath G, McGrew C, Matthews J, Matsuno S, Miller RS, Mudan MS, Price L, Reines F, Schultz J, Sinclair D, Sobel HW, Stone J, Sulak LR, Svoboda R. Search for muon neutrino oscillations with the Irvine-Michigan-Brookhaven detector. Phys Rev Lett 1992; 69:1010-1013. [PMID: 10047100 DOI: 10.1103/physrevlett.69.1010] [Citation(s) in RCA: 20] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
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18
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Casper D, Becker-Szendy R, Bratton CB, Cady DR, Claus R, Dye ST, Gajewski W, Goldhaber M, Haines TJ, Halverson PG, Jones TW, Kielczewska D, Kropp WR, Learned JG, LoSecco JM, McGrew C, Matsuno S, Matthews J, Mudan MS, Price L, Reines F, Schultz J, Sinclair D, Sobel HW, Stone JL, Sulak LR, Svoboda R, Thornton G. Measurement of atmospheric neutrino composition with the IMB-3 detector. Phys Rev Lett 1991; 66:2561-2564. [PMID: 10043554 DOI: 10.1103/physrevlett.66.2561] [Citation(s) in RCA: 69] [Impact Index Per Article: 2.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
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19
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Alexandreas DE, Allen RC, Berley D, Biller SD, Burman RL, Cady DR, Chang CY, Dingus BL, Dion GM, Ellsworth RW, Gilra MK, Goodman JA, Gupta S, Haines TJ, Hoffman CM, Krakauer DA, Kwok P, Lloyd-Evans J, Lu XQ, Nagle DE, Potter ME, Sandberg VD, Stark MJ, Talaga RL, Vishwanath PR, Yodh GB, Zhang W. Observation of shadowing of ultrahigh-energy cosmic rays by the Moon and the Sun. Phys Rev D Part Fields 1991; 43:1735-1738. [PMID: 10013548 DOI: 10.1103/physrevd.43.1735] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/22/2023]
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20
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Becker-Szendy R, Bratton CB, Cady R, Casper D, Dye ST, Gajewski W, Goldhaber M, Haines TJ, Halverson PG, Jones TW, Kielczewska D, Kropp WR, Learned JG, LoSecco JM, Matsuno S, McGrew C, Mudan MS, Price L, Reines F, Schultz J, Sobel HW, Stone JL, Sulak LR, Svoboda R, Wittel F. Search for Cygnus X-3 in underground muons during the 1989 radio outbursts using the IMB detector. Int J Clin Exp Med 1991; 43:1413-1415. [PMID: 10013512 DOI: 10.1103/physrevd.43.1413] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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21
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Becker-Szendy R, Bratton CB, Cady DR, Casper D, Claus R, Crouch M, Dye ST, Gajewski W, Goldhaber M, Haines TJ, Halverson PG, Jones TW, Kielczewska D, Kropp WR, Learned JG, LoSecco JM, McGrew C, Matsuno S, Mudan MS, Price L, Reines F, Schultz J, Sinclair D, Sobel HW, Stone JL, Sulak LR, Svoboda R, Thornton G. Search for proton decay into e++ pi 0 in the IMB-3 detector. Phys Rev D Part Fields 1990; 42:2974-2976. [PMID: 10013179 DOI: 10.1103/physrevd.42.2974] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/22/2023]
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22
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Alexandreas DE, Allen RC, Berley D, Biller SD, Burman RL, Cady R, Chang CY, Dingus BL, Dion GM, Ellsworth RW, Goodman JA, Haines TJ, Hoffman CM, Lloyd-Evans J, Lu XQ, Nagle DE, Potter ME, Sandberg VD, Stark MJ, Talaga RL, Vishwanath PR, Yodh GB, Zhang W. Study of Cygnus X-3 at ultrahigh energies during the 1989 radio outbursts. Phys Rev Lett 1990; 64:2973-2975. [PMID: 10041862 DOI: 10.1103/physrevlett.64.2973] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
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23
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Haines TJ, Alexandreas DE, Allen RC, Biller S, Berley D, Burman RL, Cady DR, Chang CY, Dingus BL, Dion GM, Ellsworth RW, Goodman JA, Hoffman CM, Lloyd-Evans J, Nagle DE, Potter M, Sandberg VD, Wilkinson CA, Yodh GB. Limit on possible energy-dependent velocities for massless particles. Phys Rev D Part Fields 1990; 41:692-694. [PMID: 10012379 DOI: 10.1103/physrevd.41.692] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/22/2023]
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24
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Dye ST, Annis J, Becker-Szendy R, Bratton CB, Casper D, Claus R, Crouch M, Errede S, Gajewski W, Goldhaber M, Haines TJ, Jones TW, Kielczewska D, Kropp WR, Learned JG, LoSecco JM, McGrew C, Matthews J, Mudan MS, Price LR, Reines F, Schultz J, Seidel S, Sinclair D, Sobel HW, Stone JL, Sulak LR, Svoboda R, Thornton G. Experimental upper limit to the galactic stellar-collapse rate. Phys Rev Lett 1989; 62:2069-2072. [PMID: 10039848 DOI: 10.1103/physrevlett.62.2069] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
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25
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Seidel S, Bionta RM, Blewitt G, Bratton CB, Casper D, Ciocio A, Claus R, Dye ST, Errede S, Foster GW, Gajewski W, Ganezer KS, Goldhaber M, Haines TJ, Jones TW, Kielczewska D, Kropp WR, Learned JG, LoSecco JM, Matthews J, Park HS, Price L, Reines F, Schultz J, Shumard E, Sinclair D, Sobel HW, Stone JL, Sulak L, Svoboda R, Thornton G, Wuest C. Search for multitrack nucleon decay. Phys Rev Lett 1988; 61:2522-2525. [PMID: 10039147 DOI: 10.1103/physrevlett.61.2522] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
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26
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Dingus BL, Alexandreas DE, Allen RC, Burman RL, Butterfield KB, Cady R, Chang CY, Ellsworth RW, Goodman JA, Gupta SK, Haines TJ, Krakauer DA, Lloyd-Evans J, Nagle DE, Potter M, Sandberg VD, Talaga RL, Wilkinson CA, Yodh GB. Ultrahigh-energy pulsed emission from Hercules X-1 with anomalous air-shower muon production. Phys Rev Lett 1988; 61:1906-1909. [PMID: 10038929 DOI: 10.1103/physrevlett.61.1906] [Citation(s) in RCA: 26] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
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27
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Bionta RM, Blewitt G, Bratton CB, Casper D, Claus R, Cortez B, Errede S, Foster G, Gajewski W, Ganezer KS, Goldhaber M, Haines TJ, Jones TW, Kielczewska D, Kropp WR, Learned JG, Lehmann E, LoSecco JM, Park HS, Reines F, Schultz J, Seidel S, Shumard E, Sinclair D, Sobel HW, Stone JL, Sulak L, Svoboda R, Wuest C. Contained neutrino interactions in an underground water detector. Phys Rev D Part Fields 1988; 38:768-775. [PMID: 9959205 DOI: 10.1103/physrevd.38.768] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/22/2023]
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28
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Bratton CB, Casper D, Ciocio A, Claus R, Crouch M, Dye ST, Errede S, Gajewski W, Goldhaber M, Haines TJ, Jones TW, Kielczewska D, Kropp WR, Learned JG, LoSecco JM, Matthews J, Miller R, Mudan M, Price LR, Reines F, Schultz J, Seidel S, Sinclair D, Sobel HW, Stone JL, Sulak L, Svoboda R, Thornton G. Angular distribution of events from SN1987A. Phys Rev D Part Fields 1988; 37:3361-3363. [PMID: 9958631 DOI: 10.1103/physrevd.37.3361] [Citation(s) in RCA: 10] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/22/2023]
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29
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Bionta RM, Blewitt G, Bratton CB, Casper D, Ciocio A, Claus R, Crouch M, Dye ST, Errede S, Foster GW, Gajewski W, Ganezer KS, Goldhaber M, Haines TJ, Jones TW, Kielczewska D, Kropp WR, Learned JG, LoSecco JM, Matthews J, Park HS, Price LR, Reines F, Schulz J, Seidel S, Shumard E, Sinclair D, Sobel HW, Stone JL, Sulak L, Svoboda R, Thornton G, Wuest C. Underground search for muons correlated with Cygnus X-3. Phys Rev D Part Fields 1987; 36:30-36. [PMID: 9958017 DOI: 10.1103/physrevd.36.30] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/22/2023]
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30
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Bionta RM, Blewitt G, Bratton CB, Casper D, Ciocio A, Claus R, Cortez B, Crouch M, Dye ST, Errede S, Foster GW, Gajewski W, Ganezer KS, Goldhaber M, Haines TJ, Jones TW, Kielczewska D, Kropp WR, Learned JG, LoSecco JM, Matthews J, Miller R, Mudan MS, Park HS, Price LR, Reines F, Schultz J, Seidel S, Shumard E, Sinclair D, Sobel HW, Stone JL, Sulak LR, Svoboda R, Thornton G, Wuest C. Observation of a neutrino burst in coincidence with supernova 1987A in the Large Magellanic Cloud. Phys Rev Lett 1987; 58:1494-1496. [PMID: 10034451 DOI: 10.1103/physrevlett.58.1494] [Citation(s) in RCA: 164] [Impact Index Per Article: 4.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
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31
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LoSecco JM, Bionta RM, Blewitt G, Bratton CB, Casper D, Claus R, Cortez B, Errede S, Foster G, Gajewski W, Ganezer KS, Goldhaber M, Haines TJ, Jones TW, Kielczewska D, Kropp WR, Learned JG, Lehmann E, Park HS, Reines F, Schultz J, Seidel S, Shumard E, Sinclair D, Sobel HW, Stone JL, Sulak L, Svoboda R, Wuest C. Limits on the neutrino lifetime. Phys Rev D Part Fields 1987; 35:2073-2076. [PMID: 9957895 DOI: 10.1103/physrevd.35.2073] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/22/2023]
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Haines TJ, Bionta RM, Blewitt G, Bratton CB, Casper D, Claus R, Cortez BG, Errede S, Foster GW, Gajewski W, Ganezer KS, Goldhaber M, Jones TW, Kielczewska D, Kropp WR, Learned JG, Lehmann E, LoSecco JM, Matthews J, Park HS, Price LR, Reines F, Schultz J, Seidel S, Shumard E, Sinclair D, Sobel HW, Stone JL, Sulak L, Svoboda R, Wuest C. Calculation of atmospheric neutrino-induced backgrounds in a nucleon-decay search. Phys Rev Lett 1986; 57:1986-1989. [PMID: 10033603 DOI: 10.1103/physrevlett.57.1986] [Citation(s) in RCA: 13] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
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Blewitt G, LoSecco JM, Bionta RM, Bratton CB, Casper D, Chrysicopoulou P, Claus R, Cortez BG, Errede S, Foster GW, Gajewski W, Ganezer KS, Goldhaber M, Haines TJ, Jones TW, Kielczewska D, Kropp WR, Learned JG, Lehmann E, Park HS, Reines F, Schultz J, Seidel S, Shumard E, Sinclair D, Sobel HW, Stone JL, Sulak L, Svoboda R, Wuest C. Experimental limits on the free-proton lifetime for two- and three-body decay modes. Phys Rev Lett 1985; 55:2114-2117. [PMID: 10032052 DOI: 10.1103/physrevlett.55.2114] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
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LoSecco JM, Bionta RM, Biewitt G, Bratton CB, Casper D, Chrysicopoulou P, Claus R, Cortez BG, Errede S, Foster GW, Gajewski W, Ganezer KS, Goldhaber M, Haines TJ, Jones TW, Kielczewska D, Kropp WR, Learned JG, Lehmann E, Park HS, Reines F, Schultz J, Seidel S, Shumard E, Sinclair D, Sobel HW, Stone JL, Sulak L, Svoboda R, Wuest C. Test of neutrino oscillations using atmospheric neutrinos. Phys Rev Lett 1985; 54:2299-2301. [PMID: 10031304 DOI: 10.1103/physrevlett.54.2299] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
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Park HS, Blewitt G, Cortez BG, Foster GW, Gajewski W, Haines TJ, Kielczewska D, LoSecco JM, Bionta RM, Bratton CB, Casper D, Chrysicopoulou P, Claus R, Errede S, Ganezer KS, Goldhaber M, Jones TW, Kropp WR, Learned JG, Lehmann E, Reines F, Schultz J, Seidel S, Shumard E, Sinclair D, Sobel HW, Stone JL, Sulak LR, Svoboda R, Wuest C. Experimental limits on the nucleon lifetime for two- and three-body decay modes. Phys Rev Lett 1985; 54:22-25. [PMID: 10030874 DOI: 10.1103/physrevlett.54.22] [Citation(s) in RCA: 12] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
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