Review of the theoretical and experimental status of dark matter identification with cosmic-ray antideuterons

被引：66

作者：

Aramaki, T. ^{[1
,2
]}

Boggs, S. ^{[3
]}

Bufalino, S. ^{[4
]}

Dal, L. ^{[5
]}

von Doetinchem, P. ^{[6
]}

Donato, F. ^{[4
,7
]}

Fornengo, N. ^{[4
,7
]}

Fuke, H. ^{[8
]}

Grefe, M. ^{[9
]}

Hailey, C. ^{[1
]}

Hamilton, B. ^{[10
]}

Ibarra, A. ^{[11
]}

Mitchell, J. ^{[12
]}

Mognet, I. ^{[13
]}

Ong, R. A. ^{[13
]}

Pereira, R. ^{[6
]}

Perez, K. ^{[14
]}

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

Raklev, A. ^{[5
]}

Salati, P. ^{[15
]}

Sasaki, M. ^{[12
]}

Tarle, G. ^{[17
]}

Urbano, A. ^{[18
]}

Vittino, A. ^{[4
,7
]}

Wild, S. ^{[11
]}

Xue, W. ^{[19
]}

Yoshimura, K. ^{[20
]}

机构：

[1] Columbia Univ, Columbia Astrophys Lab, 538 W 120th St, New York, NY 10027 USA

[2] SLAC Natl Accelerator Lab, Menlo Pk, CA USA

[3] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94709 USA

[4] Ist Nazl Fis Nucl, Sez Torino, I-10125 Turin, Italy

[5] Univ Oslo, Dept Phys, POB 1048, N-0316 Oslo, Norway

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

[7] Univ Turin, Dept Phys, I-10125 Turin, Italy

[8] Japan Aerosp Explorat Agcy ISAS JAXA, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2525210, Japan

[9] Univ Hamburg, Inst Theoret Phys 2, D-22761 Hamburg, Germany

[10] Univ Maryland, Dept Phys, College Pk, MD 20742 USA

[11] Tech Univ Munich, Phys Dept T30D, D-85748 Garching, Germany

[12] NASA, Goddard Space Flight Ctr, Code 661, Greenbelt, MD 20771 USA

[13] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA

[14] Haverford Coll, Haverford, PA 19041 USA

[15] Univ Savoie Mt Blanc, CNRS, LAPTh, F-74941 Annecy Le Vieux, France

[16] Univ Savoie Mt Blanc, CNRS, LAPP, IN2P3, F-74941 Annecy Le Vieux, France

[17] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA

[18] SISSA Int Sch Adv Studies, I-34136 Trieste, Italy

[19] MIT, Ctr Theoret Phys, Cambridge, MA 02139 USA

[20] High Energy Accelerator Res Org KEK, Tsukuba, Ibaraki 3050801, Japan

来源：

PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 2016年 / 618卷

基金：

美国国家科学基金会;

关键词：

Antideuteron; Cosmic ray; Dark matter; Coalescence; Propagation; ENERGY PROTON-BOMBARDMENT; ALPHA MAGNETIC SPECTROMETER; DISTANT SC-1 GALAXIES; VELOCITY ANISOTROPY; PARTICLE PHYSICS; DIFFUSION-MODEL; ANTI-DEUTERONS; PROPAGATION; ANTIPROTONS; SEARCH;

D O I：

10.1016/j.physrep.2016.01.002

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Recent years have seen increased theoretical and experimental effort towards the first ever detection of cosmic-ray antideuterons, in particular as an indirect signature of dark matter annihilation or decay. In contrast to indirect dark matter searches using positrons, antiprotons, or gamma-rays, which suffer from relatively high and uncertain astrophysical backgrounds, searches with antideuterons benefit from very suppressed conventional backgrounds, offering a potential breakthrough in unexplored phase space for dark matter. This article is based on the first dedicated cosmic-ray antideuteron workshop, which was held at UCLA in June 2014. It reviews broad classes of dark matter candidates that result in detectable cosmic-ray antideuteron fluxes, as well as the status and prospects of cur rent experimental searches. The coalescence model of antideuteron production and the influence of antideuteron measurements at particle colliders are discussed. This is followed by a review of the modeling of antideuteron propagation through the magnetic fields, plasma currents, and molecular material of our Galaxy, the solar system, the Earth's geomagnetic field, and the atmosphere. Finally, the three ongoing or planned experiments that are sensitive to cosmic-ray antideuterons, BESS, AMS-02, and GAPS, are detailed. As cosmic-ray antideuteron detection is a rare event search, multiple experiments with orthogonal techniques and backgrounds are essential. Therefore, the combination of AMS-02 and GAPS antideuteron searches is highly desirable. Many theoretical and experimental groups have contributed to these studies over the last decade, this review aims to provide the first coherent discussion of the relevant dark matter theories that antideuterons probe, the challenges to predictions and interpretations of antideuteron signals, and the experimental efforts toward cosmic antideuteron detection. (C) 2016 Elsevier B.V. All rights reserved.

引用

页码：1 / 37

页数：37

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