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Article: Independent measurement of the total active B8 solar neutrino flux using an array of He3 proportional counters at the sudbury neutrino observatory
Title | Independent measurement of the total active B8 solar neutrino flux using an array of He3 proportional counters at the sudbury neutrino observatory | ||||||||||||||||||||||||||||
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Authors | Aharmim, BAhmed, SNAmsbaugh, JFAnthony, AEBanar, JBarros, NBeier, EWBellerive, ABeltran, BBergevin, MBiller, SDMyers, ANickel, BGNoble, AJOblath, NSO'Keeffe, HMOllerhead, RWGann, GDOOser, SMOtt, RAPeeters, SJMBoudjemline, KPoon, AWPPrior, GReitzner, SDRielage, KRobertson, BCRobertson, RGHRollin, ESchwendener, MHSecrest, JASeibert, SRBoulay, MGSimard, OSimpson, JJSinclair, LSkensved, PSmith, MWESteiger, TDStonehill, LCTešić, GThornewell, PMTolich, NBowles, TJTsui, TTunnell, CDVan Wechel, TVan Berg, RVandevender, BAVirtue, CJWalker, TJWall, BLWaller, DTseung, HWCBrowne, MCWendland, JWest, NWilhelmy, JBWilkerson, JFWilson, JRWouters, JMWright, AYeh, MZhang, FZuber, KBullard, TVBurritt, THCai, BChan, YDChauhan, DChen, MCleveland, BTCox-Mobrand, GACurrat, CADai, XDeng, HDetwiler, JDimarco, MDoe, PJDoucas, GDrouin, P-LDuba, CADuncan, FADunford, MEarle, EDElliott, SREvans, HCEwan, GTFarine, JFergani, HFleurot, FFord, RJFormaggio, JAFowler, MMGagnon, NGermani, JVGoldschmidt, AGoon, JTMGraham, KGuillian, EHabib, SHahn, RLHallin, ALHallman, EDHamian, AAHarper, GCHarvey, PJHazama, RHeeger, KMHeintzelman, WJHeise, JHelmer, RLHenning, RHime, AHoward, CHowe, MAHuang, MJagam, PJamieson, BJelley, NAKeeter, KJKlein, JRKormos, LLKos, MKrüger, AKraus, CKrauss, CBKutter, TKyba, CCMLange, RLaw, JLawson, ITLesko, KTLeslie, JRLoach, JCMacLellan, RMajerus, SMak, HBManeira, JMartin, RMcBryde, KMcCauley, NMcDonald, ABMcGee, SMifflin, CMiller, GGMiller, MLMonreal, BMonroe, JMorissette, B | ||||||||||||||||||||||||||||
Keywords | Buildings Counting Circuits Heavy Water High Energy Physics Observatories Proportional Counters Solar Radiation | ||||||||||||||||||||||||||||
Issue Date | 2008 | ||||||||||||||||||||||||||||
Publisher | American Physical Society. The Journal's web site is located at http://prl.aps.org | ||||||||||||||||||||||||||||
Citation | Physical Review Letters, 2008, v. 101 n. 11, article no. 111301 How to Cite? | ||||||||||||||||||||||||||||
Abstract | The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rate of neutral-current interactions in heavy water and precisely determined the total active (νx) B8 solar neutrino flux. This technique is independent of previous methods employed by SNO. The total flux is found to be 5.54-0.31+0.33(stat)-0.34+0.36(syst)×106cm-2s-1, in agreement with previous measurements and standard solar models. A global analysis of solar and reactor neutrino results yields Δm2=7.59-0.21+0.19×10-5eV2 and θ=34.4-1.2+1.3 degrees. The uncertainty on the mixing angle has been reduced from SNO's previous results. © 2008 The American Physical Society. | ||||||||||||||||||||||||||||
Persistent Identifier | http://hdl.handle.net/10722/91410 | ||||||||||||||||||||||||||||
ISSN | 2023 Impact Factor: 8.1 2023 SCImago Journal Rankings: 3.040 | ||||||||||||||||||||||||||||
ISI Accession Number ID |
Funding Information: This research was supported by: Canada: NSERC, Industry Canada, NRC, Northern Ontario Heritage Fund, Vale Inco, AECL, Ontario Power Generation, HPCVL, CFI, CRC, Westgrid; US: Department of Energy, NERSC PDSF; UK: STFC (formerly PPARC); Portugal: FCT. We thank the SNO technical staff for their strong contributions. | ||||||||||||||||||||||||||||
References |
DC Field | Value | Language |
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dc.contributor.author | Aharmim, B | en_HK |
dc.contributor.author | Ahmed, SN | en_HK |
dc.contributor.author | Amsbaugh, JF | en_HK |
dc.contributor.author | Anthony, AE | en_HK |
dc.contributor.author | Banar, J | en_HK |
dc.contributor.author | Barros, N | en_HK |
dc.contributor.author | Beier, EW | en_HK |
dc.contributor.author | Bellerive, A | en_HK |
dc.contributor.author | Beltran, B | en_HK |
dc.contributor.author | Bergevin, M | en_HK |
dc.contributor.author | Biller, SD | en_HK |
dc.contributor.author | Myers, A | en_HK |
dc.contributor.author | Nickel, BG | en_HK |
dc.contributor.author | Noble, AJ | en_HK |
dc.contributor.author | Oblath, NS | en_HK |
dc.contributor.author | O'Keeffe, HM | en_HK |
dc.contributor.author | Ollerhead, RW | en_HK |
dc.contributor.author | Gann, GDO | en_HK |
dc.contributor.author | Oser, SM | en_HK |
dc.contributor.author | Ott, RA | en_HK |
dc.contributor.author | Peeters, SJM | en_HK |
dc.contributor.author | Boudjemline, K | en_HK |
dc.contributor.author | Poon, AWP | en_HK |
dc.contributor.author | Prior, G | en_HK |
dc.contributor.author | Reitzner, SD | en_HK |
dc.contributor.author | Rielage, K | en_HK |
dc.contributor.author | Robertson, BC | en_HK |
dc.contributor.author | Robertson, RGH | en_HK |
dc.contributor.author | Rollin, E | en_HK |
dc.contributor.author | Schwendener, MH | en_HK |
dc.contributor.author | Secrest, JA | en_HK |
dc.contributor.author | Seibert, SR | en_HK |
dc.contributor.author | Boulay, MG | en_HK |
dc.contributor.author | Simard, O | en_HK |
dc.contributor.author | Simpson, JJ | en_HK |
dc.contributor.author | Sinclair, L | en_HK |
dc.contributor.author | Skensved, P | en_HK |
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dc.contributor.author | Stonehill, LC | en_HK |
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dc.contributor.author | Bowles, TJ | en_HK |
dc.contributor.author | Tsui, T | en_HK |
dc.contributor.author | Tunnell, CD | en_HK |
dc.contributor.author | Van Wechel, T | en_HK |
dc.contributor.author | Van Berg, R | en_HK |
dc.contributor.author | Vandevender, BA | en_HK |
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dc.contributor.author | Tseung, HWC | en_HK |
dc.contributor.author | Browne, MC | en_HK |
dc.contributor.author | Wendland, J | en_HK |
dc.contributor.author | West, N | en_HK |
dc.contributor.author | Wilhelmy, JB | en_HK |
dc.contributor.author | Wilkerson, JF | en_HK |
dc.contributor.author | Wilson, JR | en_HK |
dc.contributor.author | Wouters, JM | en_HK |
dc.contributor.author | Wright, A | en_HK |
dc.contributor.author | Yeh, M | en_HK |
dc.contributor.author | Zhang, F | en_HK |
dc.contributor.author | Zuber, K | en_HK |
dc.contributor.author | Bullard, TV | en_HK |
dc.contributor.author | Burritt, TH | en_HK |
dc.contributor.author | Cai, B | en_HK |
dc.contributor.author | Chan, YD | en_HK |
dc.contributor.author | Chauhan, D | en_HK |
dc.contributor.author | Chen, M | en_HK |
dc.contributor.author | Cleveland, BT | en_HK |
dc.contributor.author | Cox-Mobrand, GA | en_HK |
dc.contributor.author | Currat, CA | en_HK |
dc.contributor.author | Dai, X | en_HK |
dc.contributor.author | Deng, H | en_HK |
dc.contributor.author | Detwiler, J | en_HK |
dc.contributor.author | Dimarco, M | en_HK |
dc.contributor.author | Doe, PJ | en_HK |
dc.contributor.author | Doucas, G | en_HK |
dc.contributor.author | Drouin, P-L | en_HK |
dc.contributor.author | Duba, CA | en_HK |
dc.contributor.author | Duncan, FA | en_HK |
dc.contributor.author | Dunford, M | en_HK |
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dc.contributor.author | Fergani, H | en_HK |
dc.contributor.author | Fleurot, F | en_HK |
dc.contributor.author | Ford, RJ | en_HK |
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dc.contributor.author | Fowler, MM | en_HK |
dc.contributor.author | Gagnon, N | en_HK |
dc.contributor.author | Germani, JV | en_HK |
dc.contributor.author | Goldschmidt, A | en_HK |
dc.contributor.author | Goon, JTM | en_HK |
dc.contributor.author | Graham, K | en_HK |
dc.contributor.author | Guillian, E | en_HK |
dc.contributor.author | Habib, S | en_HK |
dc.contributor.author | Hahn, RL | en_HK |
dc.contributor.author | Hallin, AL | en_HK |
dc.contributor.author | Hallman, ED | en_HK |
dc.contributor.author | Hamian, AA | en_HK |
dc.contributor.author | Harper, GC | en_HK |
dc.contributor.author | Harvey, PJ | en_HK |
dc.contributor.author | Hazama, R | en_HK |
dc.contributor.author | Heeger, KM | en_HK |
dc.contributor.author | Heintzelman, WJ | en_HK |
dc.contributor.author | Heise, J | en_HK |
dc.contributor.author | Helmer, RL | en_HK |
dc.contributor.author | Henning, R | en_HK |
dc.contributor.author | Hime, A | en_HK |
dc.contributor.author | Howard, C | en_HK |
dc.contributor.author | Howe, MA | en_HK |
dc.contributor.author | Huang, M | en_HK |
dc.contributor.author | Jagam, P | en_HK |
dc.contributor.author | Jamieson, B | en_HK |
dc.contributor.author | Jelley, NA | en_HK |
dc.contributor.author | Keeter, KJ | en_HK |
dc.contributor.author | Klein, JR | en_HK |
dc.contributor.author | Kormos, LL | en_HK |
dc.contributor.author | Kos, M | en_HK |
dc.contributor.author | Krüger, A | en_HK |
dc.contributor.author | Kraus, C | en_HK |
dc.contributor.author | Krauss, CB | en_HK |
dc.contributor.author | Kutter, T | en_HK |
dc.contributor.author | Kyba, CCM | en_HK |
dc.contributor.author | Lange, R | en_HK |
dc.contributor.author | Law, J | en_HK |
dc.contributor.author | Lawson, IT | en_HK |
dc.contributor.author | Lesko, KT | en_HK |
dc.contributor.author | Leslie, JR | en_HK |
dc.contributor.author | Loach, JC | en_HK |
dc.contributor.author | MacLellan, R | en_HK |
dc.contributor.author | Majerus, S | en_HK |
dc.contributor.author | Mak, HB | en_HK |
dc.contributor.author | Maneira, J | en_HK |
dc.contributor.author | Martin, R | en_HK |
dc.contributor.author | McBryde, K | en_HK |
dc.contributor.author | McCauley, N | en_HK |
dc.contributor.author | McDonald, AB | en_HK |
dc.contributor.author | McGee, S | en_HK |
dc.contributor.author | Mifflin, C | en_HK |
dc.contributor.author | Miller, GG | en_HK |
dc.contributor.author | Miller, ML | en_HK |
dc.contributor.author | Monreal, B | en_HK |
dc.contributor.author | Monroe, J | en_HK |
dc.contributor.author | Morissette, B | en_HK |
dc.date.accessioned | 2010-09-17T10:18:52Z | - |
dc.date.available | 2010-09-17T10:18:52Z | - |
dc.date.issued | 2008 | en_HK |
dc.identifier.citation | Physical Review Letters, 2008, v. 101 n. 11, article no. 111301 | - |
dc.identifier.issn | 0031-9007 | en_HK |
dc.identifier.uri | http://hdl.handle.net/10722/91410 | - |
dc.description.abstract | The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rate of neutral-current interactions in heavy water and precisely determined the total active (νx) B8 solar neutrino flux. This technique is independent of previous methods employed by SNO. The total flux is found to be 5.54-0.31+0.33(stat)-0.34+0.36(syst)×106cm-2s-1, in agreement with previous measurements and standard solar models. A global analysis of solar and reactor neutrino results yields Δm2=7.59-0.21+0.19×10-5eV2 and θ=34.4-1.2+1.3 degrees. The uncertainty on the mixing angle has been reduced from SNO's previous results. © 2008 The American Physical Society. | en_HK |
dc.language | eng | en_HK |
dc.publisher | American Physical Society. The Journal's web site is located at http://prl.aps.org | en_HK |
dc.relation.ispartof | Physical Review Letters | en_HK |
dc.subject | Buildings | en_HK |
dc.subject | Counting Circuits | en_HK |
dc.subject | Heavy Water | en_HK |
dc.subject | High Energy Physics | en_HK |
dc.subject | Observatories | en_HK |
dc.subject | Proportional Counters | en_HK |
dc.subject | Solar Radiation | en_HK |
dc.title | Independent measurement of the total active B8 solar neutrino flux using an array of He3 proportional counters at the sudbury neutrino observatory | en_HK |
dc.type | Article | en_HK |
dc.identifier.email | Chen, MZ:mzqchen@hku.hk | en_HK |
dc.identifier.authority | Chen, MZ=rp1317 | en_HK |
dc.description.nature | link_to_subscribed_fulltext | - |
dc.identifier.doi | 10.1103/PhysRevLett.101.111301 | en_HK |
dc.identifier.scopus | eid_2-s2.0-51749123510 | en_HK |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-51749123510&selection=ref&src=s&origin=recordpage | en_HK |
dc.identifier.volume | 101 | en_HK |
dc.identifier.issue | 11 | en_HK |
dc.identifier.spage | article no. 111301 | - |
dc.identifier.epage | article no. 111301 | - |
dc.identifier.eissn | 1079-7114 | - |
dc.identifier.isi | WOS:000259188700006 | - |
dc.identifier.issnl | 0031-9007 | - |