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Article: Measurement of the rate of ve + d → p + p + e- interactions produced by 8B solar neutrinos at the sudbury neutrino observatory

TitleMeasurement of the rate of ve + d → p + p + e- interactions produced by 8B solar neutrinos at the sudbury neutrino observatory
Authors
Ahmad, QRAllen, RCAndersen, TCAnglin, JDBühler, GBarton, JCBeier, EWBercovitch, MBigu, JBiller, SBlack, RABlevis, IBoardman, RJBoger, JBonvin, EBoulay, MGBowler, MGBowles, TJBrice, SJBrowne, MCBullard, TVBurritt, THCameron, KCameron, JChan, YDChen, MChen, HHChen, XChon, MCCleveland, BTClifford, ETHCowan, JHMCowen, DFCox, GADai, YDai, XDalnoki-Veress, FDavidson, WFDoe, PJDoucas, GDragowsky, MRDuba, CADuncan, FADunmore, JEarle, EDElliott, SREvans, HCEwan, GTFarine, JFergani, HFerraris, APFord, RJFowler, MMFrame, KFrank, EDFrati, WGermani, JVGil, SGoldschmidt, AGrant, DRHahn, RLHallin, ALHallman, EDHamer, AHamian, AAHaq, RUHargrove, CKHarvey, PJHazama, RHeaton, RHeeger, KMHeintzelman, WJHeise, JHelmer, RLHepburn, JDHeron, HHewett, JHime, AHowe, MHykawy, JGIsaac, MCPJagam, PJelley, NAJillings, CJonkmans, GKarn, JKeener, PTKirch, KKlein, JRKnox, ABKomar, RJKouzes, RKutter, TKyba, CCMLaw, JLawson, ITLay, MLee, HWLesko, KT
KeywordsAstrophysics
Calculations
Cerenkov Counters
Computer Simulation
Deuterium
Electron Energy Levels
Electron Scattering
Monte Carlo Methods
Neutron Sources
Issue Date2001
PublisherAmerican Physical Society. The Journal's web site is located at http://prl.aps.org
Citation
Physical Review Letters, 2001, v. 87 n. 7, article no. 071301 , p. 1-6 How to Cite?
DOI: http://dx.doi.org/10.1103/PhysRevLett.87.071301
AbstractThe 8B flux from elastic scattering (ES) and charged current (CC) of electrons was recorded at the Sudbury Neutrino Observatory (SNO) between November 2, 1999 and January 15, 2001. Data were partitioned into two sets then analyzed. As a result, the first direct indication of a nonelectron flavor component in the solar neutrino flux was established.
Persistent Identifierhttp://hdl.handle.net/10722/91361
ISSN
0031-9007
2023 Impact Factor: 8.1
2023 SCImago Journal Rankings: 3.040
ISI Accession Number ID
WOS:000170478300005
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorAhmad, QRen_HK
dc.contributor.authorAllen, RCen_HK
dc.contributor.authorAndersen, TCen_HK
dc.contributor.authorAnglin, JDen_HK
dc.contributor.authorBühler, Gen_HK
dc.contributor.authorBarton, JCen_HK
dc.contributor.authorBeier, EWen_HK
dc.contributor.authorBercovitch, Men_HK
dc.contributor.authorBigu, Jen_HK
dc.contributor.authorBiller, Sen_HK
dc.contributor.authorBlack, RAen_HK
dc.contributor.authorBlevis, Ien_HK
dc.contributor.authorBoardman, RJen_HK
dc.contributor.authorBoger, Jen_HK
dc.contributor.authorBonvin, Een_HK
dc.contributor.authorBoulay, MGen_HK
dc.contributor.authorBowler, MGen_HK
dc.contributor.authorBowles, TJen_HK
dc.contributor.authorBrice, SJen_HK
dc.contributor.authorBrowne, MCen_HK
dc.contributor.authorBullard, TVen_HK
dc.contributor.authorBurritt, THen_HK
dc.contributor.authorCameron, Ken_HK
dc.contributor.authorCameron, Jen_HK
dc.contributor.authorChan, YDen_HK
dc.contributor.authorChen, Men_HK
dc.contributor.authorChen, HHen_HK
dc.contributor.authorChen, Xen_HK
dc.contributor.authorChon, MCen_HK
dc.contributor.authorCleveland, BTen_HK
dc.contributor.authorClifford, ETHen_HK
dc.contributor.authorCowan, JHMen_HK
dc.contributor.authorCowen, DFen_HK
dc.contributor.authorCox, GAen_HK
dc.contributor.authorDai, Yen_HK
dc.contributor.authorDai, Xen_HK
dc.contributor.authorDalnoki-Veress, Fen_HK
dc.contributor.authorDavidson, WFen_HK
dc.contributor.authorDoe, PJen_HK
dc.contributor.authorDoucas, Gen_HK
dc.contributor.authorDragowsky, MRen_HK
dc.contributor.authorDuba, CAen_HK
dc.contributor.authorDuncan, FAen_HK
dc.contributor.authorDunmore, Jen_HK
dc.contributor.authorEarle, EDen_HK
dc.contributor.authorElliott, SRen_HK
dc.contributor.authorEvans, HCen_HK
dc.contributor.authorEwan, GTen_HK
dc.contributor.authorFarine, Jen_HK
dc.contributor.authorFergani, Hen_HK
dc.contributor.authorFerraris, APen_HK
dc.contributor.authorFord, RJen_HK
dc.contributor.authorFowler, MMen_HK
dc.contributor.authorFrame, Ken_HK
dc.contributor.authorFrank, EDen_HK
dc.contributor.authorFrati, Wen_HK
dc.contributor.authorGermani, JVen_HK
dc.contributor.authorGil, Sen_HK
dc.contributor.authorGoldschmidt, Aen_HK
dc.contributor.authorGrant, DRen_HK
dc.contributor.authorHahn, RLen_HK
dc.contributor.authorHallin, ALen_HK
dc.contributor.authorHallman, EDen_HK
dc.contributor.authorHamer, Aen_HK
dc.contributor.authorHamian, AAen_HK
dc.contributor.authorHaq, RUen_HK
dc.contributor.authorHargrove, CKen_HK
dc.contributor.authorHarvey, PJen_HK
dc.contributor.authorHazama, Ren_HK
dc.contributor.authorHeaton, Ren_HK
dc.contributor.authorHeeger, KMen_HK
dc.contributor.authorHeintzelman, WJen_HK
dc.contributor.authorHeise, Jen_HK
dc.contributor.authorHelmer, RLen_HK
dc.contributor.authorHepburn, JDen_HK
dc.contributor.authorHeron, Hen_HK
dc.contributor.authorHewett, Jen_HK
dc.contributor.authorHime, Aen_HK
dc.contributor.authorHowe, Men_HK
dc.contributor.authorHykawy, JGen_HK
dc.contributor.authorIsaac, MCPen_HK
dc.contributor.authorJagam, Pen_HK
dc.contributor.authorJelley, NAen_HK
dc.contributor.authorJillings, Cen_HK
dc.contributor.authorJonkmans, Gen_HK
dc.contributor.authorKarn, Jen_HK
dc.contributor.authorKeener, PTen_HK
dc.contributor.authorKirch, Ken_HK
dc.contributor.authorKlein, JRen_HK
dc.contributor.authorKnox, ABen_HK
dc.contributor.authorKomar, RJen_HK
dc.contributor.authorKouzes, Ren_HK
dc.contributor.authorKutter, Ten_HK
dc.contributor.authorKyba, CCMen_HK
dc.contributor.authorLaw, Jen_HK
dc.contributor.authorLawson, ITen_HK
dc.contributor.authorLay, Men_HK
dc.contributor.authorLee, HWen_HK
dc.contributor.authorLesko, KTen_HK
dc.date.accessioned2010-09-17T10:17:48Z-
dc.date.available2010-09-17T10:17:48Z-
dc.date.issued2001en_HK
dc.identifier.citationPhysical Review Letters, 2001, v. 87 n. 7, article no. 071301 , p. 1-6-
dc.identifier.issn0031-9007en_HK
dc.identifier.urihttp://hdl.handle.net/10722/91361-
dc.description.abstractThe 8B flux from elastic scattering (ES) and charged current (CC) of electrons was recorded at the Sudbury Neutrino Observatory (SNO) between November 2, 1999 and January 15, 2001. Data were partitioned into two sets then analyzed. As a result, the first direct indication of a nonelectron flavor component in the solar neutrino flux was established.en_HK
dc.languageengen_HK
dc.publisherAmerican Physical Society. The Journal's web site is located at http://prl.aps.orgen_HK
dc.relation.ispartofPhysical Review Lettersen_HK
dc.subjectAstrophysicsen_HK
dc.subjectCalculationsen_HK
dc.subjectCerenkov Countersen_HK
dc.subjectComputer Simulationen_HK
dc.subjectDeuteriumen_HK
dc.subjectElectron Energy Levelsen_HK
dc.subjectElectron Scatteringen_HK
dc.subjectMonte Carlo Methodsen_HK
dc.subjectNeutron Sourcesen_HK
dc.titleMeasurement of the rate of ve + d → p + p + e- interactions produced by 8B solar neutrinos at the sudbury neutrino observatoryen_HK
dc.typeArticleen_HK
dc.identifier.emailChen, MZ:mzqchen@hku.hken_HK
dc.identifier.authorityChen, MZ=rp1317en_HK
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1103/PhysRevLett.87.071301-
dc.identifier.scopuseid_2-s2.0-37649032191en_HK
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-37649032191&selection=ref&src=s&origin=recordpageen_HK
dc.identifier.volume87en_HK
dc.identifier.issue7en_HK
dc.identifier.spagearticle no. 071301, p. 1en_HK
dc.identifier.epagearticle no. 071301, p. 6en_HK
dc.identifier.isiWOS:000170478300005-
dc.identifier.issnl0031-9007-

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