Solar neutrino detection sensitivity in DARWIN via electron scattering

被引：37

作者：

Aalbers, J. ^{[1
]}

Agostini, F. ^{[2
,3
]}

Maouloud, S. E. M. Ahmed ^{[4
]}

Alfonsi, M. ^{[5
]}

Althueser, L. ^{[6
]}

Amaro, F. D. ^{[7
]}

Angevaare, J. ^{[8
,9
]}

Antochi, V. C. ^{[1
]}

Antunovic, B. ^{[10
]}

Aprile, E. ^{[11
]}

Arazi, L. ^{[12
]}

Arneodo, F. ^{[13
]}

Balzer, M. ^{[14
]}

Baudis, L. ^{[15
]}

Baur, D. ^{[16
]}

Benabderrahmane, M. L. ^{[13
]}

Biondi, Y. ^{[15
]}

Bismark, A. ^{[15
,16
]}

Bourgeois, C. ^{[17
]}

Breskin, A. ^{[12
]}

Breur, P. A. ^{[8
,9
]}

Brown, A. ^{[15
]}

Brown, E. ^{[18
]}

Bruenner, S. ^{[8
,9
]}

Bruno, G. ^{[13
]}

Budnik, R. ^{[12
]}

Capelli, C. ^{[15
]}

Cardoso, J. ^{[7
]}

Cichon, D. ^{[19
]}

Clark, M. ^{[20
]}

Colijn, A. P. ^{[8
,9
]}

Conrad, J. ^{[1
,38
]}

Cuenca-Garcia, J. J. ^{[21
]}

Cussonneau, J. P. ^{[22
]}

Decowski, M. P. ^{[8
,9
]}

Depoian, A. ^{[20
]}

Dierle, J. ^{[16
]}

Di Gangi, P. ^{[2
,3
]}

Di Giovanni, A. ^{[13
]}

Diglio, S. ^{[22
]}

Douillet, D. ^{[17
]}

Drexlin, G. ^{[23
]}

Eitel, K. ^{[21
]}

Engel, R. ^{[21
]}

Erdal, E. ^{[12
]}

Ferella, A. D. ^{[24
,25
,26
]}

Fischer, H. ^{[16
]}

Fischer, P. ^{[27
]}

Fulgione, W. ^{[25
,26
]}

Gaemers, P. ^{[8
,9
]}

机构：

[1] Stockholm Univ, Dept Phys, Oskar Klein Ctr, S-10691 Stockholm, SE, Sweden

[2] Univ Bologna, Dept Phys & Astron, I-40126 Bologna, Italy

[3] INFN Bologna, I-40126 Bologna, Italy

[4] Univ Paris Diderot, Univ Pierre & Marie Curie, LPNHE, CNRS,IN2P3, F-75252 Paris, France

[5] Johannes Gutenberg Univ Mainz, Inst Phys & Exzellenzcluster PRISMA, D-55099 Mainz, Germany

[6] Westfal Wilhelms Univ Munster, Inst Kernphys, D-48149 Munster, Germany

[7] Univ Coimbra, Dept Phys, LIBPhys, P-3004516 Coimbra, Portugal

[8] Nikhef, Sci Pk, NL-1098XG Amsterdam, Netherlands

[9] Univ Amsterdam, Sci Pk, NL-1098XG Amsterdam, Netherlands

[10] Univ Belgrade, Vinca Inst Nucl Sci, Mihajla Petrov Alasa 12-14, Belgrade, Serbia

[11] Columbia Univ, Phys Dept, New York, NY 10027 USA

[12] Weizmann Inst Sci, Dept Particle Phys & Astrophys, IL-7610001 Rehovot, Israel

[13] New York Univ Abu Dhabi, Abu Dhabi, U Arab Emirates

[14] Karlsruhe Inst Technol KIT, Inst Data Proc & Elect IPE, D-76344 Eggenstein Leopoldshafen, Germany

[15] Univ Zurich, Phys Inst, CH-8057 Zurich, Switzerland

[16] Univ Freiburg, Phys Inst, D-79104 Freiburg, Germany

[17] Univ Paris Saclay, IJCLab, CNRS, IN2P3, F-91405 Orsay, France

[18] Rensselaer Polytech Inst, Dept Phys Appl Phys & Astron, Troy, NY 12180 USA

[19] Max Planck Inst Kernphys, D-69117 Heidelberg, Germany

[20] Purdue Univ, Dept Phys & Astron, W Lafayette, IN 47907 USA

[21] Karlsruhe Inst Technol KIT, Inst Astroparticle Phys IAP, D-76344 Eggenstein Leopoldshafen, Germany

[22] Univ Nantes, SUBATECH, IMT Atlantique, CNRS,IN2P3, F-44307 Nantes, France

[23] Karlsruhe Inst Technol KIT, Inst Expt Particle Phys ETP, D-76344 Eggenstein Leopoldshafen, Germany

[24] Univ Aquila, Dept Chem & Phys, I-67100 Laquila, Italy

[25] INFN Lab Nazl Gran Sasso, I-67100 Laquila, Italy

[26] Gran Sasso Sci Inst, I-67100 Laquila, Italy

[27] Heidelberg Univ, Phys Inst, Heidelberg, Germany

[28] Univ Chicago, Dept Phys, Chicago, IL 60637 USA

[29] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA

[30] Karlsruhe Inst Technol KIT, Inst Tech Phys ITEP, D-76344 Eggenstein Leopoldshafen, Germany

[31] Origins Project Fdn, Phoenix, AZ 85020 USA

[32] Univ Calif San Diego, Dept Phys, San Diego, CA 92093 USA

[33] Univ Melbourne, Sch Phys, Melbourne, Vic 3010, Australia

[34] Univ Alabama, Dept Phys, Tuscaloosa, AL 35487 USA

[35] Rice Univ, Dept Phys & Astron, Houston, TX 77005 USA

[36] Imperial Coll London, Dept Phys, Imperial Ctr Inference & Cosmol, London SW7 2AZ, England

[37] Tech Univ Dresden, Inst Nucl & Particle Phys, D-01069 Dresden, Germany

[38] Univ Banja Luka, Banja Luka, Bosnia & Herceg

[39] Univ Utrecht, Inst Subat Phys, Utrecht, Netherlands

[40] ISEC, Coimbra Polytech, Coimbra, Portugal

来源：

EUROPEAN PHYSICAL JOURNAL C | 2020年 / 80卷 / 12期

基金：

欧洲研究理事会; 美国国家科学基金会; 瑞士国家科学基金会; 英国科学技术设施理事会;

关键词：

XENON;

D O I：

10.1140/epjc/s10052-020-08602-7

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

We detail the sensitivity of the proposed liquid xenon DARWIN observatory to solar neutrinos via elastic electron scattering. We find that DARWIN will have the potential to measure the fluxes of five solar neutrino components: pp, 7Be, 13N, 15O and pep. The precision of the 13N, 15O and pep components is hindered by the double-beta decay of 136Xe and, thus, would benefit from a depleted target. A high-statistics observation of pp neutrinos would allow us to infer the values of the electroweak mixing angle, sin2 theta w, and the electron-type neutrino survival probability, Pee, in the electron recoil energy region from a few keV up to 200 keV for the first time, with relative precision of 5% and 4%, respectively, with 10 live years of data and a 30 tonne fiducial volume. An observation of pp and 7Be neutrinos would constrain the neutrino-inferred solar luminosity down to 0.2%. A combination of all flux measurements would distinguish between the high- (GS98) and low-metallicity (AGS09) solar models with 2.1-2.5 sigma significance, independent of external measurements from other experiments or a measurement of 8B neutrinos through coherent elastic neutrino-nucleus scattering in DARWIN. Finally, we demonstrate that with a depleted target DARWIN may be sensitive to the neutrino capture process of 131Xe.

引用

页数：10

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