Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope

被引：52

作者：

Albert, A. ^{[1
]}

Andre, M. ^{[2
]}

Anghinolfi, M. ^{[3
]}

Anton, G. ^{[4
]}

Ardid, M. ^{[5
]}

Aubert, J. J. ^{[6
]}

Avgitas, T. ^{[7
]}

Baret, B. ^{[7
]}

Barrios-Marti, J. ^{[8
]}

Basa, S. ^{[9
]}

Bertin, V. ^{[6
]}

Biagi, S. ^{[10
]}

Bormuth, R. ^{[11
,12
]}

Bourret, S. ^{[7
]}

Bouwhuis, M. C. ^{[11
]}

Bruijn, R. ^{[11
,13
]}

Brunner, J. ^{[6
]}

Busto, J. ^{[6
]}

Capone, A. ^{[14
,15
]}

Caramete, L. ^{[16
]}

Carr, J. ^{[6
]}

Celli, S. ^{[14
,15
,17
]}

Chiarusi, T. ^{[18
]}

Circella, M. ^{[19
]}

Coelho, J. A. B. ^{[7
]}

Coleiro, A. ^{[7
]}

Coniglione, R. ^{[10
]}

Costantini, H. ^{[6
]}

Coyle, P. ^{[6
]}

Creusot, A. ^{[7
]}

Deschamps, A. ^{[20
]}

De Bonis, G. ^{[14
,15
]}

Distefano, C. ^{[10
]}

Di Palma, I. ^{[14
,15
]}

Donzaud, C. ^{[7
,21
]}

Dornic, D. ^{[6
]}

Drouhin, D. ^{[1
]}

Eberl, T. ^{[4
]}

El Bojaddaini, I. ^{[22
]}

Elsaesser, D. ^{[23
]}

Enzenhofer, A. ^{[6
]}

Felis, I. ^{[5
]}

Fusco, L. A. ^{[18
,24
]}

Galata, S. ^{[7
]}

Gay, P. ^{[7
,25
]}

Geisselsoeder, S. ^{[4
]}

Geyer, K. ^{[4
]}

Giordano, V. ^{[26
]}

Gleixner, A. ^{[4
]}

Glotin, H. ^{[27
,28
,29
]}

机构：

[1] Univ Haute Alsace, GRPHE, Inst Univ Technol Colmar, 34 Rue Grillenbreit,BP 50568, F-68008 Colmar, France

[2] Tech Univ Catalonia, Lab Appl Bioacoust, Rambla Exposicio, Barcelona 08800, Spain

[3] INFN, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy

[4] Friedrich Alexander Univ Erlangen Nurnberg, Erlangen Ctr Astroparticle Phys, Erwin Rommel Str 1, D-91058 Erlangen, Germany

[5] Univ Politecn Valencia, Inst Invest Gestio Integrada Zones Costaneres IGI, C Paranimf 1, Gandia 46730, Spain

[6] Aix Marseille Univ, CNRS, IN2P3, CPPM,UMR 7346, F-13288 Marseille, France

[7] Univ Paris Diderot, APC, Sorbonne Paris Cite, CNRS,IN2P3,CEA,IRFU,Observ Paris, F-75205 Paris, France

[8] Univ Valencia, CSIC, Inst Fis Corpuscular, IFIC, C Catedratico Jose Beltran 2, E-46980 Valencia, Spain

[9] Pole Etoile Site Chateau Gombert, LAM, Rue Frederic Joliot Curie 38, F-13388 Marseille 13, France

[10] INFN, LNS, Via S Sofia 62, I-95123 Catania, Italy

[11] Nikhef, Sci Pk, Amsterdam, Netherlands

[12] Leiden Univ, Huygens Kamerlingh Onnes Lab, Leiden, Netherlands

[13] Univ Amsterdam, Inst Hoge Energie Fys, Sci Pk 105, NL-1098 XG Amsterdam, Netherlands

[14] INFN, Sez Roma, Ple Aldo Moro 2, I-00185 Rome, Italy

[15] Univ Roma La Sapienza, Dipartimento Fis, Ple Aldo Moro 2, I-00185 Rome, Italy

[16] Inst Space Sci, RO-077125 Bucharest, Magurele, Romania

[17] Gran Sasso Sci Inst, Viale Francesco Crispi 7, I-00167 Laquila, Italy

[18] INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy

[19] INFN, Sez Bari, Via E Orabona 4, I-70126 Bari, Italy

[20] Geoazur, UCA, CNRS, IRD,Observ Cote Azur, Sophia Antipolis, France

[21] Univ Paris Sud, F-91405 Orsay, France

[22] Univ Mohammed 1, Lab Phys Matter & Radiat, BP 717, Oujda 6000, Morocco

[23] Univ Wurzburg, Inst Theoret Phys & Astrophys, Emil Fischer Str 31, D-97074 Wurzburg, Germany

[24] Univ Bologna, Dipartimento Fis & Astron, Viale Berti Pichat 6-2, I-40127 Bologna, Italy

[25] Univ Blaise Pascal, Clermont Univ, Lab Phys Corpusculaire, CNRS,IN2P3, BP 10448, F-63000 Clermont Ferrand, France

[26] INFN, Sez Catania, Viale Andrea Doria 6, I-95125 Catania, Italy

[27] Aix Marseille Univ, LSIS, CNRS, ENSAM,UMR 7296, F-13397 Marseille, France

[28] Univ Toulon & Var, CNRS, LSIS, UMR 7296, F-83957 La Garde, France

[29] Inst Univ France, F-75005 Paris, France

[30] Royal Netherlands Inst Sea Res NIOZ, Landsdiep 4, NL-1797 SZ Thorntje, Texel, Netherlands

[31] Univ Genoa, Dipartimento Fis, Via Dodecaneso 33, I-16146 Genoa, Italy

[32] Univ Erlangen Nurnberg, Dr Remeis Sternwarte, Sternwartstr 7, D-96049 Bamberg, Germany

[33] Univ Erlangen Nurnberg, ECAP, Sternwartstr 7, D-96049 Bamberg, Germany

[34] Moscow MV Lomonosov State Univ, Skobeltsyn Inst Nucl Phys, Moscow 119991, Russia

[35] Aix Marseille Univ, MIO, F-13288 Marseille 9, France

[36] Univ Sud Toulon Var, CNRS, INSU, UM 10,IRD, F-83957 La Garde, France

[37] Univ Catania, Dipartimento Fis & Astron, Viale Andrea Doria 6, I-95125 Catania, Italy

[38] CEA Saclay, Serv Phys Particules, Direct Sci Mat, Inst Rech Sur Fondamentales Univers, F-91191 Gif Sur Yvette, France

[39] INFN, Sez Pisa, Largo B Pontecorvo 3, I-56127 Pisa, Italy

[40] Univ Pisa, Dipartimento Fis, Largo B Pontecorvo 3, I-56127 Pisa, Italy

[41] INFN, Sez Napoli, Via Cintia, I-80126 Naples, Italy

[42] Univ Strasbourg, CNRS, IPHC, UMR 7178, F-67000 Strasbourg, France

[43] Univ Mohammed V Rabat, Fac Sci, 4 Ave Ibn Battouta,BP 1014, RP-10000 Rabat, Morocco

[44] Univ Federico II Napoli, Dipartimento Fis, Via Cintia, I-80126 Naples, Italy

来源：

PHYSICS LETTERS B | 2017年 / 769卷

关键词：

Dark matter; WIMP; Indirect detection; Neutrino telescope; Galactic Centre; ANTARES; ANNIHILATION; LIMITS;

D O I：

10.1016/j.physletb.2017.03.063

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using data recorded with the ANTARES telescope from 2007 to 2015, a new search for dark matter annihilation in the Milky Way has been performed. Three halo models and five annihilation channels, WIMP + WIMP -> b (b) over bar, W+W-, tau(+)tau(-), mu(+)mu(-) and v (v) over bar, with WIMP masses ranging from 50 2 GeV/C-2 to 100 Tev/C-2, were considered. No excess over the expected background was found, and limits on the thermally averaged annihilation cross-section were set. (C) 2017 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license.

引用

页码：249 / 254

页数：6

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