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Titolo:
Measurement of the rate of nu(e)+d -> p+p+e(-) interactions produced by B-8 solar neutrinos at the sudbury neutrino observatory - art. no. 071301
Autore:
Ahmad, QR; Allen, RC; Andersen, TC; Anglin, JD; Buhler, G; Barton, JC; Beier, EW; Bercovitch, M; Bigu, J; Biller, S; Black, RA; Blevis, I; Boardman, RJ; Boger, J; Bonvin, E; Boulay, MG; Bowler, MG; Bowles, TJ; Brice, SJ; Browne, MC; Bullard, TV; Burritt, TH; Cameron, K; Cameron, J; Chan, YD; Chen, M; Chen, HH; Chen, X; Chon, MC; Cleveland, BT; Clifford, ETH; Cowan, JHM; Cowen, DF; Cox, GA; Dai, Y; Dai, X; Dalnoki-Veress, F; Davidson, WF; Doe, PJ; Doucas, G; Dragowsky, MR; Duba, CA; Duncan, FA; Dunmore, J; Earle, ED; Elliott, SR; Evans, HC; Ewan, GT; Farine, J; Fergani, H; Ferraris, AP; Ford, RJ; Fowler, MM; Frame, K; Frank, ED; Frati, W; Germani, JV; Gil, S; Goldschmidt, A; Grant, DR; Hahn, RL; Hallin, AL; Hallman, ED; Hamer, A; Hamian, AA; Haq, RU; Hargrove, CK; Harvey, PJ; Hazama, R; Heaton, R; Heeger, KM; Heintzelman, WJ; Heise, J; Helmer, RL; Hepburn, JD; Heron, H; Hewett, J; Hime, A; Howe, M; Hykawy, JG; Isaac, MCP; Jagam, P; Jelley, NA; Jillings, C; Jonkmans, G; Karn, J; Keener, PT; Kirch, K; Klein, JR; Knox, AB; Komar, RJ; Kouzes, R; Kutter, T; Kyba, CCM; Law, J; Lawson, IT; Lay, M; Lee, HW; Lesko, KT; Leslie, JR; Levine, I; Locke, W; Lowry, MM; Luoma, S; Lyon, J; Majerus, S; Mak, HB; Marino, AD; McCauley, N; McDonald, AB; McDonald, DS; McFarlane, K; McGregor, G; McLatchie, W; Drees, RM; Mes, H; Mifflin, C; Miller, GG; Milton, G; Moffat, BA; Moorhead, M; Nally, CW; Neubauer, MS; Newcomer, FM; Ng, HS; Noble, AJ; Norman, EB; Novikov, VM; ONeill, M; Okada, CE; Ollerhead, RW; Omori, M; Orrell, JL; Oser, SM; Poon, AWP; Radcliffe, TJ; Roberge, A; Robertson, BC; Robertson, RGH; Rowley, JK; Rusu, VL; Saettler, E; Schaffer, KK; Schuelke, A; Schwendener, MH; Seifert, H; Shatkay, M; Simpson, JJ; Sinclair, D; Skensved, P; Smith, AR; Smith, MWE; Starinsky, N; Steiger, TD; Stokstad, RG; Storey, RS; Sur, B; Tafirout, R; Tagg, N; Tanner, NW; Taplin, RK; Thorman, M; Thornewell, P; Trent, PT; Tserkovnyak, YI; Van Berg, R; Van de Water, RG; Virtue, CJ; Waltham, CE; Wang, JX; Wark, DL; West, N; Wilhelmy, JB; Wilkerson, JF; Wilson, J; Wittich, P; Wouters, JM; Yeh, M;
Indirizzi:
Univ Washington, Ctr Expt Nucl Phys & Astrophys, Seattle, WA 98195 USA Univ Washington Seattle WA USA 98195 s & Astrophys, Seattle, WA 98195 USA Atom Energy Canada Ltd, Chalk River Nucl Labs, Chalk River, ON K0J 1J0, Canada Atom Energy Canada Ltd Chalk River ON Canada K0J 1J0 , ON K0J 1J0, Canada Brookhaven Natl Lab, Dept Chem, Upton, NY 11973 USA Brookhaven Natl Lab Upton NY USA 11973 ab, Dept Chem, Upton, NY 11973 USA Carleton Univ, Ottawa, ON K1S 5B6, Canada Carleton Univ Ottawa ON Canada K1S 5B6 n Univ, Ottawa, ON K1S 5B6, Canada Laurentian Univ, Dept Phys & Astron, Sudbury, ON P3E 2C6, Canada Laurentian Univ Sudbury ON Canada P3E 2C6 on, Sudbury, ON P3E 2C6, Canada Univ Calif Berkeley, Lawrence Berkeley Lab, Inst Nucl & Particle Astrophys, Berkeley, CA 94720 USA Univ Calif Berkeley Berkeley CA USA 94720 trophys, Berkeley, CA 94720 USA Univ Calif Berkeley, Lawrence Berkeley Lab, Div Nucl Sci, Berkeley, CA 94720 USA Univ Calif Berkeley Berkeley CA USA 94720 ucl Sci, Berkeley, CA 94720 USA Los Alamos Natl Lab, Los Alamos, NM 87545 USA Los Alamos Natl Lab Los Alamos NM USA 87545 Lab, Los Alamos, NM 87545 USA Natl Res Council Canada, Ottawa, ON K1A 0R6, Canada Natl Res Council Canada Ottawa ON Canada K1A 0R6 tawa, ON K1A 0R6, Canada Princeton Univ, Dept Phys, Princeton, NJ 08544 USA Princeton Univ Princeton NJ USA 08544 Dept Phys, Princeton, NJ 08544 USA Queens Univ, Dept Phys, Kingston, ON K7L 3N6, Canada Queens Univ KingstonON Canada K7L 3N6 Phys, Kingston, ON K7L 3N6, Canada Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada Univ British Columbia Vancouver BC Canada V6T 1Z1 ver, BC V6T 1Z1, Canada Univ Calif Irvine, Dept Phys, Irvine, CA 92717 USA Univ Calif Irvine Irvine CA USA 92717 ne, Dept Phys, Irvine, CA 92717 USA Univ Guelph, Dept Phys, Guelph, ON N1G 2W1, Canada Univ Guelph Guelph ON Canada N1G 2W1 ept Phys, Guelph, ON N1G 2W1, Canada Univ Oxford, Nucl & Astrophys Lab, Oxford OX1 3RH, England Univ Oxford Oxford England OX1 3RH strophys Lab, Oxford OX1 3RH, England Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA Univ Penn Philadelphia PA USA 19104 & Astron, Philadelphia, PA 19104 USA Univ Washington, Dept Phys, Seattle, WA 98195 USA Univ Washington SeattleWA USA 98195 on, Dept Phys, Seattle, WA 98195 USA Univ London Birkbeck Coll, London WC1E 7HX, England Univ London Birkbeck Coll London England WC1E 7HX ndon WC1E 7HX, England TRIUMF, Vancouver, BC V6T 2A3, Canada TRIUMF Vancouver BC Canada V6T 2A3TRIUMF, Vancouver, BC V6T 2A3, Canada Rutherford Appleton Lab, Didcot OX11 0QX, Oxon, England Rutherford Appleton Lab Didcot Oxon England OX11 0QX 1 0QX, Oxon, England Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England Univ Sussex Brighton E Sussex England BN1 9QH BN1 9QH, E Sussex, England
Titolo Testata:
PHYSICAL REVIEW LETTERS
fascicolo: 7, volume: 8707, anno: 2001,
pagine: 1301 -
SICI:
0031-9007(20010813)8707:7<1301:MOTRON>2.0.ZU;2-Y
Fonte:
ISI
Lingua:
ENG
Soggetto:
RADIATIVE-CORRECTIONS; REAL-TIME; SCATTERING; KAMIOKANDE; DETECTOR;
Tipo documento:
Article
Natura:
Periodico
Settore Disciplinare:
Physical, Chemical & Earth Sciences
--discip_EC--
Citazioni:
32
Recensione:
Indirizzi per estratti:
Indirizzo: Ahmad, QR Univ Washington, Ctr Expt Nucl Phys & Astrophys, Seattle, WA 98195 USA Univ Washington Seattle WA USA 98195 hys, Seattle, WA 98195 USA
Citazione:
Q.R. Ahmad et al., "Measurement of the rate of nu(e)+d -> p+p+e(-) interactions produced by B-8 solar neutrinos at the sudbury neutrino observatory - art. no. 071301", PHYS REV L, 8707(7), 2001, pp. 1301

Abstract

Solar neutrinos from B-8 decay have been detected at the Sudbury Neutrino Observatory via the charged current (CC) reaction on deuterium and the elastic scattering (ES) of electrons. The flux of nu (e)'s is measured by the CC reaction rate to be phi (CC)(nu (e)) = 1.75 +/-0.07(stat)(-0.11)(+0.12)(syst) +/-0.05(theor) x 10(6) cm(-2) s(-1). Comparison of phi (CC)(nu (e)) tothe Super-Kamiokande Collaboration's precision value of the flux inferred from the ES reaction yields a 3.3o sigma difference, assuming the systematic uncertainties are normally distributed, providing evidence of an active non=nu (e) component in the solar flux. The total flux of active B-8 neutrinos is determined to be 5.44 +/-0.99 x 10(6) cm(-2) s(-1).

ASDD Area Sistemi Dipartimentali e Documentali, Università di Bologna, Catalogo delle riviste ed altri periodici
Documento generato il 05/12/20 alle ore 14:13:20