Physics potential of a long-baseline neutrino oscillation experiment using a J-PARC neutrino beam and Hyper-Kamiokande

被引：239

作者：

Abe, K. ^{[61
,63
]}

Aihara, H. ^{[63
,64
]}

Andreopoulos, C. ^{[32
]}

Anghel, I. ^{[26
]}

Ariga, A. ^{[1
,26
,29
,34
,42
,52
,63
]}

Ariga, T. ^{[1
]}

Asfandiyarov, R. ^{[15
]}

Askins, M. ^{[4
]}

Back, J. J. ^{[69
]}

Ballett, P. ^{[11
]}

Barbi, M. ^{[46
]}

Barker, G. J. ^{[69
]}

Barr, G. ^{[44
]}

Bay, F. ^{[14
]}

Beltrame, P. ^{[13
]}

Berardi, V. ^{[18
,19
]}

Bergevin, M. ^{[4
]}

Berkman, S. ^{[3
]}

Berry, T. ^{[50
]}

Bhadra, S. ^{[74
]}

Blaszczyk, F. D. M. ^{[34
]}

Blondel, A. ^{[15
]}

Bolognesi, S. ^{[7
]}

Boyd, S. B. ^{[69
]}

Bravar, A. ^{[15
]}

Bronner, C. ^{[63
]}

Cafagna, F. S. ^{[18
,19
]}

Carminati, G. ^{[5
]}

Cartwright, S. L. ^{[52
]}

Catanesi, M. G. ^{[18
,19
]}

Choi, K. ^{[38
]}

Choi, J. H. ^{[9
]}

Collazuol, G. ^{[22
,23
]}

Cowan, G. ^{[13
]}

Cremonesi, L. ^{[49
]}

Davies, G. ^{[26
]}

De Rosa, G. ^{[20
,21
]}

Densham, C. ^{[56
,57
]}

Detwiler, J. ^{[70
]}

Dewhurst, D. ^{[44
]}

Di Lodovico, F. ^{[49
]}

Di Luise, S. ^{[14
]}

Drapier, O. ^{[12
]}

Emery, S. ^{[7
]}

Ereditato, A. ^{[1
]}

Fernandez, P. ^{[35
]}

Feusels, T. ^{[3
]}

Finch, A. ^{[31
]}

Fitton, M. ^{[56
,57
]}

Friend, M. ^{[27
,75
]}

机构：

[1] Univ Bern, Albert Einstein Ctr Fundamental Phys, LHEP, Bern, Switzerland

[2] Boston Univ, Dept Phys, Boston, MA 02215 USA

[3] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V5Z 1M9, Canada

[4] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA

[5] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA USA

[6] Calif State Univ, Dept Phys, Carson, CA USA

[7] CEA Saclay, IRFU, F-91191 Gif Sur Yvette, France

[8] Chonnam Natl Univ, Dept Phys, Kwangju, South Korea

[9] Dongshin Univ, Dept Phys, Naju, South Korea

[10] Duke Univ, Dept Phys, Durham, NC 27706 USA

[11] Univ Durham, Sci Labs, Durham DH1 3LE, England

[12] Ecole Polytech, CNRS, IN2P3, Lab Leprince Ringuet, F-91128 Palaiseau, France

[13] Univ Edinburgh, Sch Phys & Astron, Edinburgh, Midlothian, Scotland

[14] ETH, Inst Particle Phys, Zurich, Switzerland

[15] Univ Geneva, DPNC, Sect Phys, CH-1211 Geneva, Switzerland

[16] Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 USA

[17] Univ London Imperial Coll Sci Technol & Med, Dept Phys, London, England

[18] Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy

[19] Univ & Politecn Bari, Dipartimento Interuniv Fis, Bari, Italy

[20] Ist Nazl Fis Nucl, Sez Napoli, I-80125 Naples, Italy

[21] Univ Naples Federico II, Dipartimento Fis, Naples, Italy

[22] Ist Nazl Fis Nucl, Sez Padova, Padua, Italy

[23] Univ Padua, Dipartimento Fis, Padua, Italy

[24] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy

[25] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia

[26] Iowa State Univ, Dept Phys & Astron, Ames, IA USA

[27] High Energy Accelerator Res Org KEK, Tsukuba, Ibaraki, Japan

[28] Kobe Univ, Dept Phys, Kobe, Hyogo 657, Japan

[29] Kyoto Univ, Dept Phys, Kyoto 606, Japan

[30] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy

[31] Univ Lancaster, Dept Phys, Lancaster, England

[32] Univ Liverpool, Dept Phys, Liverpool L69 3BX, Merseyside, England

[33] Los Alamos Natl Lab, Los Alamos, NM 87545 USA

[34] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA

[35] Univ Autonoma Madrid, Dept Theoret Phys, Madrid, Spain

[36] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA

[37] Miyagi Univ Educ, Dept Phys, Sendai, Miyagi, Japan

[38] Nagoya Univ, Grad Sch Sci, Nagoya, Aichi 4648601, Japan

[39] Nagoya Univ, Kobayashi Maskawa Inst Origin Particles & Univers, Nagoya, Aichi 4648601, Japan

[40] Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan

[41] Natl Ctr Nucl Res, Warsaw, Poland

[42] Okayama Univ, Dept Phys, Okayama 700, Japan

[43] Osaka City Univ, Dept Phys, Osaka 558, Japan

[44] Univ Oxford, Dept Phys, Oxford, England

[45] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA

[46] Univ Regina, Dept Phys, Regina, SK S4S 0A2, Canada

[47] Pontificia Univ Catolica Rio de Janeiro, Dept Fis, Rio De Janeiro, Brazil

[48] Univ Rochester, Dept Phys & Astron, Rochester, NY 14627 USA

[49] Queen Mary Univ London, Sch Phys & Astron, London, England

[50] Royal Holloway Univ London, Dept Phys, Egham, Surrey, England

来源：

PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS | 2015年 / 2015卷 / 05期

基金：

美国国家科学基金会; 欧盟地平线“2020”;

关键词：

CP-VIOLATION; MASS; MODEL;

D O I：

10.1093/ptep/ptv061

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Hyper-Kamiokande will be a next-generation underground water Cherenkov detector with a total (fiducial) mass of 0.99 (0.56) million metric tons, approximately 20 (25) times larger than that of Super-Kamiokande. One of the main goals of Hyper-Kamiokande is the study of CP asymmetry in the lepton sector using accelerator neutrino and anti-neutrino beams. In this paper, the physics potential of a long-baseline neutrino experiment using the Hyper-Kamiokande detector and a neutrino beam from the J-PARC proton synchrotron is presented. The analysis uses the framework and systematic uncertainties derived from the ongoing T2K experiment. With a total exposure of 7.5 MW x 10(7) s integrated proton beam power (corresponding to 1.56 x 10(22) protons on target with a 30 GeV proton beam) to a 2.5 degrees off-axis neutrino beam, it is expected that the leptonic CP phase delta(CP) can be determined to better than 19 degrees for all possible values of delta(CP), and CP violation can be established with a statistical significance of more than 3 sigma (5 sigma) for 76% (58%) of the delta(CP) parameter space. Using both nu(e) appearance and nu(mu) disappearance data, the expected 1 sigma uncertainty of sin(2) theta(23) is 0.015(0.006) for sin(2) theta(23) = 0.5(0.45).

引用

页数：35

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