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Aharmim, B, Ahmed, SN, Amsbaugh, JF, Anaya, JM, Anthony, AE, Banar, J, Barros, N, Beier, EW, Bellerive, A, Beltran, B, Bergevin, M, Biller, SD, Boudjemline, K, Boulay, MG, Bowles, TJ, Browne, MC, Bullard, TV, Burritt, TH, Cai, B, Chan, YD, Chauhan, D, Chen, M, Cleveland, BT, Cox, GA, Currat, CA, Dai, X, Deng, H, Detwiler, JA, DiMarco, M, Doe, PJ, Doucas, G, Dragowsky, MR, Drouin, P-L, Duba, CA, Duncan, FA, Dunford, M, Earle, ED, Elliott, SR, Evans, HC, Ewan, GT, Farine, J, Fergani, H, Fleurot, F, Ford, RJ, Formaggio, JA, Fowler, MM, Gagnon, N, Germani, JV
, Kormos, LL, O'Keeffe, HM & SNO Collaboration 2013, '
Measurement of the nu(e) and total B-8 solar neutrino fluxes with the Sudbury Neutrino Observatory phase-III data set',
Physical Review C, vol. 87, no. 1, 015502.
https://doi.org/10.1103/PhysRevC.87.015502APA
Aharmim, B., Ahmed, S. N., Amsbaugh, J. F., Anaya, J. M., Anthony, A. E., Banar, J., Barros, N., Beier, E. W., Bellerive, A., Beltran, B., Bergevin, M., Biller, S. D., Boudjemline, K., Boulay, M. G., Bowles, T. J., Browne, M. C., Bullard, T. V., Burritt, T. H., Cai, B., ... SNO Collaboration (2013).
Measurement of the nu(e) and total B-8 solar neutrino fluxes with the Sudbury Neutrino Observatory phase-III data set.
Physical Review C,
87(1), Article 015502.
https://doi.org/10.1103/PhysRevC.87.015502Vancouver
Author
Bibtex
@article{b8dd6155a011466494f7e317702d4080,
title = "Measurement of the nu(e) and total B-8 solar neutrino fluxes with the Sudbury Neutrino Observatory phase-III data set",
abstract = "This paper details the solar neutrino analysis of the 385.17-day phase-III data set acquired by the Sudbury Neutrino Observatory (SNO). An array of He-3 proportional counters was installed in the heavy-water target to measure precisely the rate of neutrino-deuteron neutral-current interactions. This technique to determine the total active B-8 solar neutrino flux was largely independent of the methods employed in previous phases. The total flux of active neutrinos was measured to be 5.54(-0.31)(+0.33)(stat.)(-0.34)(+0.36)(syst.) x 10(6) cm(-2) s(-1), consistent with previous measurements and standard solar models. A global analysis of solar and reactor neutrino mixing parameters yielded the best-fit values of Delta m(2) = 7.59(-0.21)(+0.19) x 10(-5) eV(2) and theta = 34.4(-1.2)(+1.3) degrees. DOI: 10.1103/PhysRevC.87.015502",
keywords = "CALIBRATION SOURCE, OSCILLATIONS, COUNTERS, MODELS, MATTER, LIGHT, WATER",
author = "B. Aharmim and Ahmed, {S. N.} and Amsbaugh, {J. F.} and Anaya, {J. M.} and Anthony, {A. E.} and J. Banar and N. Barros and Beier, {E. W.} and A. Bellerive and B. Beltran and M. Bergevin and Biller, {S. D.} and K. Boudjemline and Boulay, {M. G.} and Bowles, {T. J.} and Browne, {M. C.} and Bullard, {T. V.} and Burritt, {T. H.} and B. Cai and Chan, {Y. D.} and D. Chauhan and M. Chen and Cleveland, {B. T.} and Cox, {G. A.} and Currat, {C. A.} and X. Dai and H. Deng and Detwiler, {J. A.} and M. DiMarco and Doe, {P. J.} and G. Doucas and Dragowsky, {M. R.} and Drouin, {P. -L.} and Duba, {C. A.} and Duncan, {F. A.} and M. Dunford and Earle, {E. D.} and Elliott, {S. R.} and Evans, {H. C.} and Ewan, {G. T.} and J. Farine and H. Fergani and F. Fleurot and Ford, {R. J.} and Formaggio, {J. A.} and Fowler, {M. M.} and N. Gagnon and Germani, {J. V.} and Kormos, {L. L.} and O'Keeffe, {H. M.} and {SNO Collaboration}",
note = "{\textcopyright}2013 American Physical Society",
year = "2013",
month = jan,
day = "18",
doi = "10.1103/PhysRevC.87.015502",
language = "English",
volume = "87",
journal = "Physical Review C",
issn = "0556-2813",
publisher = "American Physical Society",
number = "1",
}
RIS
TY - JOUR
T1 - Measurement of the nu(e) and total B-8 solar neutrino fluxes with the Sudbury Neutrino Observatory phase-III data set
AU - Aharmim, B.
AU - Ahmed, S. N.
AU - Amsbaugh, J. F.
AU - Anaya, J. M.
AU - Anthony, A. E.
AU - Banar, J.
AU - Barros, N.
AU - Beier, E. W.
AU - Bellerive, A.
AU - Beltran, B.
AU - Bergevin, M.
AU - Biller, S. D.
AU - Boudjemline, K.
AU - Boulay, M. G.
AU - Bowles, T. J.
AU - Browne, M. C.
AU - Bullard, T. V.
AU - Burritt, T. H.
AU - Cai, B.
AU - Chan, Y. D.
AU - Chauhan, D.
AU - Chen, M.
AU - Cleveland, B. T.
AU - Cox, G. A.
AU - Currat, C. A.
AU - Dai, X.
AU - Deng, H.
AU - Detwiler, J. A.
AU - DiMarco, M.
AU - Doe, P. J.
AU - Doucas, G.
AU - Dragowsky, M. R.
AU - Drouin, P. -L.
AU - Duba, C. A.
AU - Duncan, F. A.
AU - Dunford, M.
AU - Earle, E. D.
AU - Elliott, S. R.
AU - Evans, H. C.
AU - Ewan, G. T.
AU - Farine, J.
AU - Fergani, H.
AU - Fleurot, F.
AU - Ford, R. J.
AU - Formaggio, J. A.
AU - Fowler, M. M.
AU - Gagnon, N.
AU - Germani, J. V.
AU - Kormos, L. L.
AU - O'Keeffe, H. M.
AU - SNO Collaboration
N1 - ©2013 American Physical Society
PY - 2013/1/18
Y1 - 2013/1/18
N2 - This paper details the solar neutrino analysis of the 385.17-day phase-III data set acquired by the Sudbury Neutrino Observatory (SNO). An array of He-3 proportional counters was installed in the heavy-water target to measure precisely the rate of neutrino-deuteron neutral-current interactions. This technique to determine the total active B-8 solar neutrino flux was largely independent of the methods employed in previous phases. The total flux of active neutrinos was measured to be 5.54(-0.31)(+0.33)(stat.)(-0.34)(+0.36)(syst.) x 10(6) cm(-2) s(-1), consistent with previous measurements and standard solar models. A global analysis of solar and reactor neutrino mixing parameters yielded the best-fit values of Delta m(2) = 7.59(-0.21)(+0.19) x 10(-5) eV(2) and theta = 34.4(-1.2)(+1.3) degrees. DOI: 10.1103/PhysRevC.87.015502
AB - This paper details the solar neutrino analysis of the 385.17-day phase-III data set acquired by the Sudbury Neutrino Observatory (SNO). An array of He-3 proportional counters was installed in the heavy-water target to measure precisely the rate of neutrino-deuteron neutral-current interactions. This technique to determine the total active B-8 solar neutrino flux was largely independent of the methods employed in previous phases. The total flux of active neutrinos was measured to be 5.54(-0.31)(+0.33)(stat.)(-0.34)(+0.36)(syst.) x 10(6) cm(-2) s(-1), consistent with previous measurements and standard solar models. A global analysis of solar and reactor neutrino mixing parameters yielded the best-fit values of Delta m(2) = 7.59(-0.21)(+0.19) x 10(-5) eV(2) and theta = 34.4(-1.2)(+1.3) degrees. DOI: 10.1103/PhysRevC.87.015502
KW - CALIBRATION SOURCE
KW - OSCILLATIONS
KW - COUNTERS
KW - MODELS
KW - MATTER
KW - LIGHT
KW - WATER
U2 - 10.1103/PhysRevC.87.015502
DO - 10.1103/PhysRevC.87.015502
M3 - Journal article
VL - 87
JO - Physical Review C
JF - Physical Review C
SN - 0556-2813
IS - 1
M1 - 015502
ER -
