Search for invisible modes of nucleon decay in water with the SNO plus detector

被引:21
|
作者
Anderson, M. [1 ]
Andringa, S. [2 ]
Arushanova, E. [3 ]
Asahi, S. [1 ]
Askins, M. [4 ,5 ,6 ]
Auty, D. J. [7 ]
Back, A. R. [3 ,8 ]
Barnard, Z. [9 ]
Barros, N. [2 ,10 ,11 ]
Bartlett, D. [1 ]
Barao, F. [2 ,12 ]
Bayes, R. [9 ]
Beier, E. W. [10 ]
Bialek, A. [7 ,13 ]
Biller, S. D. [14 ]
Blucher, E. [15 ,16 ]
Bonventre, R. [4 ,5 ,10 ]
Boulay, M. [1 ]
Braid, D. [9 ]
Caden, E. [9 ,13 ]
Callaghan, E. J. [4 ,5 ]
Caravaca, J. [4 ,5 ]
Carvalho, J. [17 ,18 ]
Cavalli, L. [14 ]
Chauhan, D. [1 ,2 ,9 ,13 ]
Chen, M. [1 ]
Chkvorets, O. [9 ]
Clark, K. J. [1 ,8 ,14 ]
Cleveland, B. [9 ,13 ]
Connors, C. [9 ]
Coulter, I. T. [10 ,14 ]
Cressy, D. [9 ]
Dai, X. [1 ]
Darrach, C. [9 ]
Davis-Purcell, B. [19 ]
Depatie, M. M. [9 ]
Descamps, F. [4 ,5 ]
Di Lodovico, F. [3 ]
Duhaime, N. [9 ]
Duncan, F. [13 ]
Dunger, J. [14 ]
Falk, E. [8 ]
Fatemighomi, N. [1 ]
Fischer, V [6 ]
Fletcher, E. [1 ]
Ford, R. [9 ,13 ]
Gagnon, N. [13 ]
Gilje, K. [7 ]
Gorel, P. [7 ]
Graham, K. [1 ]
机构
[1] Queens Univ, Dept Phys Engn Phys & Astron, Kingston, ON K7L 3N6, Canada
[2] Lab Instrumentacao & Fis Expt Particulas LIP, Av Prof Gama Pinto 2, P-1649003 Lisbon, Portugal
[3] Queen Mary Univ London, Sch Phys & Astron, 327 Mile End Rd, London E1 4NS, England
[4] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
[5] Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
[6] Univ Calif Davis, 1 Shields Ave, Davis, CA 95616 USA
[7] Univ Alberta, Dept Phys, 4-181 CCIS, Edmonton, AB T6G 2E1, Canada
[8] Univ Sussex, Phys & Astron, Pevensey 2, Brighton BN1 9QH, E Sussex, England
[9] Laurentian Univ, Dept Phys, 935 Ramsey Lake Rd, Sudbury, ON P3E 2C6, Canada
[10] Univ Penn, Dept Phys & Astron, 209 South 33rd St, Philadelphia, PA 19104 USA
[11] Tech Univ Dresden, Inst Kern & Teilchenphys, Zellescher Weg 19, D-01069 Dresden, Germany
[12] Univ Lisbon, Inst Super Tecn, Av Rovisco Pais, P-1049001 Lisbon, Portugal
[13] SNOLAB, Creighton Mine 9,1039 Reg Rd 24, Sudbury, ON P3Y 1N2, Canada
[14] Univ Oxford, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England
[15] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA
[16] Univ Chicago, Dept Phys, Chicago, IL 60637 USA
[17] Univ Coimbra, Dept Fis, P-3004516 Coimbra, Portugal
[18] Univ Coimbra, Lab Instrumentacao & Fis Expt Particulas LIP, P-3004516 Coimbra, Portugal
[19] TRIUMF, 4004 Wesbrook Mall, Vancouver, BC V6T 2A3, Canada
[20] Boston Univ, Dept Phys, 590 Commonwealth Ave, Boston, MA 02215 USA
[21] Brookhaven Natl Lab, Chem Dept, Bldg 555,POB 5000, Upton, NY 11973 USA
[22] Univ Nacl Autonoma Mexico, Inst Fis, Apartado Postal 20-364, Mexico City 01000, DF, Mexico
[23] Univ Lisbon, Fac Ciencias FCUL, Dept Fis, Campo Grande,Ediffcio C8, P-1749016 Lisbon, Portugal
[24] Univ Washington, Ctr Expt Nucl Phys & Astrophys, Seattle, WA 98195 USA
[25] Univ Washington, Dept Phys, Seattle, WA 98195 USA
[26] Idaho State Univ, 921 S 8th Ave,Mail Stop 8106, Pocatello, ID 83209 USA
[27] Norwich Univ, 158 Harmon Dr, Northfield, MN 05663 USA
[28] Univ Lancaster, Phys Dept, Lancaster LA1 4YB, England
[29] Boston Univ, Dept Phys, 590 Corrunonwealth Ave, Boston, MA 02215 USA
[30] Univ Liverpool, Dept Phys, Liverpool L69 3BX, Merseyside, England
[31] Univ Sheffield, Dept Phys & Astron, Hicks Bldg,Hounsfield Rd, Sheffield S3 7RH, S Yorkshire, England
[32] Armstrong Atlantic State Univ, 11935 Abercorn St, Savannah, GA 31419 USA
[33] Univ Alberta, Dept Chem, 11227 Saskatchewan Dr, Edmonton, AB T6G 2G2, Canada
[34] Tech Univ Dresden, Fac Chem & Food Chem, D-01062 Dresden, Germany
[35] MTA Atomki, H-4001 Debrecen, Hungary
基金
加拿大创新基金会; 欧洲研究理事会; 加拿大自然科学与工程研究理事会; 美国国家科学基金会; 英国科学技术设施理事会;
关键词
NEUTRINO; LIMITS;
D O I
10.1103/PhysRevD.99.032008
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This paper reports results from a search for nucleon decay through invisible modes, where no visible energy is directly deposited during the decay itself, during the initial water phase of SNO+. However, such decays within the oxygen nucleus would produce an excited daughter that would subsequently deexcite, often emitting detectable gamma rays. A search for such gamma rays yields limits of 2.5 x 10(29) y at 90% Bayesian credibility level (with a prior uniform in rate) for the partial lifetime of the neutron, and 3.6 x 10(29) y for the partial lifetime of the proton, the latter a 70% improvement on the previous limit from SNO. We also present partial lifetime limits for invisible dinucleon modes of 1.3 x 10(28) y for nn, 2.6 x 10(28) y for pn and 4.7 x 10(28) y for pp, an improvement over existing limits by close to 3 orders of magnitude for the latter two.
引用
收藏
页数:13
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