ITP OpenIR  > SCI期刊论文
von Doetinchem, P.; Perez, K.; Aramaki, T.; Baker, S.; Barwick, S.; Bird, R.; Boezio, M.; Boggs, S. E.; Cui, M.; Datta, A.; Donato, F.; Evoli, C.; Fabris, L.; Fabbietti, L.; Bueno, E. Ferronato; Fornengo, N.; Fuke, H.; Gerrity, C.; Coral, D. Gomez; Hailey, C.; Hooper, D.; Kachelriess, M.; Korsmeier, M.; Kozai, M.; Lea, R.; Li, N.; Lowell, A.; Manghisoni, M.; Moskalenko, I., V; Munini, R.; Naskret, M.; Nelson, T.; Ng, K. C. Y.; Nozzoli, F.; Oliva, A.; Ong, R. A.; Osteria, G.; Pierog, T.; Poulin, V37; Profumo, S.; Poschl, T.; Quinn, S.; Re, V27,28; Rogers, F.; Ryan, J.; Saffold, N.; Sakai, K.; Salati, P.; Schael, S.; Serksnyte, L.; Shukla, A.; Stoessl, A.; Tjemsland, J.; Vannuccini, E.; Vecchi, M.; Winkler, M. W.; Wright, D.; Xiao, M.; Xu, W.; Yoshida, T.; Zampa, G.; Zuccon, P.
Cosmic-ray antinuclei as messengers of new physics: status and outlook for the new decade
AbstractThe precise measurement of cosmic-ray antinuclei serves as an important means for identifying the nature of dark matter and other new astrophysical phenomena, and could be used with other cosmic-ray species to understand cosmic-ray production and propagation in the Galaxy. For instance, low-energy antideuterons would provide a "smoking gun" signature of dark matter annihilation or decay, essentially free of astrophysical background. Studies in recent years have emphasized that models for cosmic-ray antideuterons must be considered together with the abundant cosmic antiprotons and any potential observation of antihelium. Therefore, a second dedicated Antideuteron Workshop was organized at UCLA in March 2019, bringing together a community of theorists and experimentalists to review the status of current observations of cosmic-ray antinuclei, the theoretical work towards understanding these signatures, and the potential of upcoming measurements to illuminate ongoing controversies. This review aims to synthesize this recent work and present implications for the upcoming decade of antinuclei observations and searches. This includes discussion of a possible dark matter signature in the AMS-02 antiproton spectrum, the most recent limits from BESS Polar-II on the cosmic antideuteron flux, and reports of candidate antihelium events by AMS-02; recent collider and cosmic-ray measurements relevant for antinuclei production models; the state of cosmic-ray transport models in light of AMS-02 and Voyager data; and the prospects for upcoming experiments, such as GAPS. This provides a roadmap for progress on cosmic antinuclei signatures of dark matter in the coming years.
Cooperation Status国际
Subject AreaAstronomy & Astrophysics ; Physics
MOST Discipline CatalogueAstronomy & Astrophysics ; Physics, Particles & Fields
Indexed BySCIE
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Document Type期刊论文
Affiliation1.[von Doetinchem, P.; Datta, A.; Gerrity, C.; Coral, D. Gomez; Naskret, M.; Nelson, T.; Shukla, A.; Stoessl, A.] Univ Hawaii Manoa, Dept Phys & Astron, 2505 Correa Rd, Honolulu, HI 96822 USA
2.Perez, K.; Rogers, F.; Xiao, M.] MIT, Dept Phys, 77 Massachusetts Ave, Cambridge, MA 02139 USA
3.Aramaki, T.; Wright, D.] Stanford Linear Accelerator Ctr, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA
4.Baker, S.] Imperial Coll London, London SW7 2AZ, England
5.Barwick, S.] Univ Calif Irvine, Dept Phys & Astron, 4129 Frederick Reines Hall, Irvine, CA 92697 USA
6.Bird, R.; Ong, R. A.; Quinn, S.; Ryan, J.] Univ Calif Los Angeles, Dept Phys & Astron, 475 Portola Plaza, Los Angeles, CA 90095 USA
7.Boezio, M.; Lea, R.; Munini, R.; Zampa, G.] Ist Nazl Fis Nucl, Sez Trieste, Padriciano 99, I-34149 Trieste, Italy
8.Boggs, S. E.; Lowell, A.] Univ Calif San Diego, Dept Phys, 9500 Gilman Dr, La Jolla, CA 90037 USA
9.Cui, M.] Purple Mt Observ, Yuanhua Rd, Nanjing 210033, Peoples R China
10.Donato, F.; Fornengo, N.; Korsmeier, M.] Univ Turin, Dept Phys, Via Pietro Giuria 1, I-10125 Turin, Italy
11.Donato, F.; Fornengo, N.; Korsmeier, M.] Ist Nazl Fis Nucl, Sez Torino, Via Pietro Giuria 1, I-10125 Turin, Italy
12.Evoli, C.] Gran Sasso Sci Inst, Viale Francesco Crispi 7, I-67100 Laquila, Italy
13.Evoli, C.] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, Via G Acitelli 22, I-67100 Laquila, Italy
14.Fabris, L.] Oak Ridge Natl Lab, Isotope & Fuel Cycle & Technol Div, POB 2008, Oak Ridge, TN 37831 USA
15.Fabbietti, L.; Poschl, T.; Serksnyte, L.] Tech Univ Munich, Dept Phys, James Franck Str 1, D-85748 Garching, Germany
16.Bueno, E. Ferronato; Vecchi, M.] Univ Groningen, Kapteyn Astron Inst, Landleven 12, NL-9717 AD Groningen, Netherlands
17.Fuke, H.; Kozai, M.; Yoshida, T.] Japan Aerosp Explorat Agcy ISAS JAXA, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2525210, Japan
18.Univ Nacl Autonoma Mexico, Inst Phys, Ciudad De Mexico 04510, Mexico
19.Hailey, C.; Saffold, N.] Columbia Univ, Dept Phys, 500 W 120th St, New York, NY 10027 USA
20.Hooper, D.] Fermilab Natl Accelerator Lab, Theoret Astrophys, Wilson & Kirk Rds, Batavia, IL 60510 USA
21.Hooper, D.] Univ Chicago, Dept Astron & Astrophys, 5640 S Ellis Ave, Chicago, IL 60637 USA
22.Hooper, D.] Univ Chicago, Kavli Inst Cosmol Phys, 5640 S Ellis Ave, Chicago, IL 60637 USA
23.Kachelriess, M.; Tjemsland, J.] Norwegian Univ Sci & Technol, Dept Phys, N-7491 Trondheim, Norway
24.Korsmeier, M.] Rhein Westfal TH Aachen, Inst Theoret Particle Phys & Cosmol, D-52056 Aachen, Germany
25.Lea, R.] Univ Trieste, Dipartimento Fis, Via Valerio 2, I-34127 Trieste, Italy
26.Li, N.] Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China
27.Li, N.] Univ Chinese Acad Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China
28.Ist Nazl Fis Nucl, Sez Pavia, Via Agostino Bassi 6, I-27100 Pavia, Italy
29.Univ Bergamo, Dipartimento Ingn Ind, Viale Marconi 5, I-24044 Dalmine, Italy
30.Stanford Univ, Hansen Expt Phys Lab, 452 Lomita Mall, Stanford, CA 94305 USA
31.Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA
32.Naskret, M.] Univ Wroclaw, Inst Theoret Phys, Pl M Borna 9, PL-50204 Wroclaw, Poland
33.Ng, K. C. Y.] Weizmann Inst Sci, Dept Particle Phys & Astrophys, IL-76100 Rehovot, Israel
34.Nozzoli, F.; Zuccon, P.] Ist Nazl Fis Nucl, Trento Inst Fundamental Phys & Applicat, Via Sommar 14, I-38123 Povo, Italy
35.Oliva, A.] Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy
36.Osteria, G.] Ist Nazl Fis Nucl, Sez Napoli, Str Comunale Cinthia, I-80126 Naples, Italy
37.Pierog, T.] Karlsruhe Inst Technol, Inst Nucl Phys, Hermann von Helmholtz Pl 1, D-76344 Eggenstein Leopoldshafen, Germany
38.Univ Montpellier, Lab Univers & Particules Montpellier, CNRS, Pl Eugene Bataillon, F-34095 Montpellier 05, France
39.Profumo, S.] Univ Calif Santa Cruz, Dept Phys, Santa Cruz, CA 95064 USA
40.Profumo, S.] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA
41.Sakai, K.] NASA, Goddard Space Flight Ctr, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA
42.Sakai, K.] Univ Maryland, CRESST, Baltimore County, MD 21250 USA
43.Salati, P.] Lab Annecy le Vieux Phys Theor, 9 Chemin Bellevue, F-74940 Annecy, France
44.Schael, S.] Rhein Westfal TH Aachen, Phys Inst 1, Sommerfeldstr 14, D-52074 Aachen, Germany
45.Vannuccini, E.] Ist Nazl Fis Nucl, Sez Firenze, I-50019 Florence, Italy
46.Winkler, M. W.] Stockholm Univ, Oskar Klein Ctr Cosmoparticle Phys, Dept Phys, S-10691 Stockholm, Sweden
47.Xu, W.] Harvard Univ, Dept Phys, 17 Oxford St, Cambridge, MA 02138 USA
48.Zuccon, P.] Univ Trento, Dept Phys, Via Sommar 14, I-38123 Povo, Italy
Recommended Citation
GB/T 7714
von Doetinchem, P.,Perez, K.,Aramaki, T.,et al. Cosmic-ray antinuclei as messengers of new physics: status and outlook for the new decade[J]. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS,2020(8):35.
APA von Doetinchem, P..,Perez, K..,Aramaki, T..,Baker, S..,Barwick, S..,...&Zuccon, P..(2020).Cosmic-ray antinuclei as messengers of new physics: status and outlook for the new decade.JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS(8),35.
MLA von Doetinchem, P.,et al."Cosmic-ray antinuclei as messengers of new physics: status and outlook for the new decade".JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS .8(2020):35.
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