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Phys Rev Lett. 2015 Feb 27;114(8):081301. doi: 10.1103/PhysRevLett.114.081301. Epub 2015 Feb 24.

Constraints on an annihilation signal from a core of constant dark matter density around the milky way center with H.E.S.S.

Physical review letters

A Abramowski, F Aharonian, F Ait Benkhali, A G Akhperjanian, E O Angüner, M Backes, S Balenderan, A Balzer, A Barnacka, Y Becherini, J Becker Tjus, D Berge, S Bernhard, K Bernlöhr, E Birsin, J Biteau, M Böttcher, C Boisson, J Bolmont, P Bordas, J Bregeon, F Brun, P Brun, M Bryan, T Bulik, S Carrigan, S Casanova, P M Chadwick, N Chakraborty, R Chalme-Calvet, R C G Chaves, M Chrétien, S Colafrancesco, G Cologna, J Conrad, C Couturier, Y Cui, I D Davids, B Degrange, C Deil, P deWilt, A Djannati-Ataï, W Domainko, A Donath, L O'C Drury, G Dubus, K Dutson, J Dyks, M Dyrda, T Edwards, K Egberts, P Eger, P Espigat, C Farnier, S Fegan, F Feinstein, M V Fernandes, D Fernandez, A Fiasson, G Fontaine, A Förster, M Füßling, S Gabici, M Gajdus, Y A Gallant, T Garrigoux, G Giavitto, B Giebels, J F Glicenstein, D Gottschall, M-H Grondin, M Grudzińska, D Hadasch, S Häffner, J Hahn, J Harris, G Heinzelmann, G Henri, G Hermann, O Hervet, A Hillert, J A Hinton, W Hofmann, P Hofverberg, M Holler, D Horns, A Ivascenko, A Jacholkowska, C Jahn, M Jamrozy, M Janiak, F Jankowsky, I Jung-Richardt, M A Kastendieck, K Katarzyński, U Katz, S Kaufmann, B Khélifi, M Kieffer, S Klepser, D Klochkov, W Kluźniak, D Kolitzus, Nu Komin, K Kosack, S Krakau, F Krayzel, P P Krüger, H Laffon, G Lamanna, J Lefaucheur, V Lefranc, A Lemière, M Lemoine-Goumard, J-P Lenain, T Lohse, A Lopatin, C-C Lu, V Marandon, A Marcowith, R Marx, G Maurin, N Maxted, M Mayer, T J L McComb, J Méhault, P J Meintjes, U Menzler, M Meyer, A M W Mitchell, R Moderski, M Mohamed, K Morå, E Moulin, T Murach, M de Naurois, J Niemiec, S J Nolan, L Oakes, H Odaka, S Ohm, B Opitz, M Ostrowski, I Oya, M Panter, R D Parsons, M Paz Arribas, N W Pekeur, G Pelletier, P-O Petrucci, B Peyaud, S Pita, H Poon, G Pühlhofer, M Punch, A Quirrenbach, S Raab, I Reichardt, A Reimer, O Reimer, M Renaud, R de Los Reyes, F Rieger, C Romoli, S Rosier-Lees, G Rowell, B Rudak, C B Rulten, V Sahakian, D Salek, D A Sanchez, A Santangelo, R Schlickeiser, F Schüssler, A Schulz, U Schwanke, S Schwarzburg, S Schwemmer, H Sol, F Spanier, G Spengler, F Spies, Ł Stawarz, R Steenkamp, C Stegmann, F Stinzing, K Stycz, I Sushch, J-P Tavernet, T Tavernier, A M Taylor, R Terrier, M Tluczykont, C Trichard, K Valerius, C van Eldik, B van Soelen, G Vasileiadis, J Veh, C Venter, A Viana, P Vincent, J Vink, H J Völk, F Volpe, M Vorster, T Vuillaume, S J Wagner, P Wagner, R M Wagner, M Ward, M Weidinger, Q Weitzel, R White, A Wierzcholska, P Willmann, A Wörnlein, D Wouters, R Yang, V Zabalza, D Zaborov, M Zacharias, A A Zdziarski, A Zech, H-S Zechlin,

Affiliations

  1. Universität Hamburg, Institut für Experimentalphysik, Luruper Chaussee 149, D 22761 Hamburg, Germany.
  2. Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany.
  3. Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland.
  4. National Academy of Sciences of the Republic of Armenia, Marshall Baghramian Avenue, 24, 0019 Yerevan, Republic of Armenia.
  5. Yerevan Physics Institute, 2 Alikhanian Brothers St., 375036 Yerevan, Armenia.
  6. Institut für Physik, Humboldt-Universität zu Berlin, Newtonstr. 15, D 12489 Berlin, Germany.
  7. University of Namibia, Department of Physics, Private Bag 13301, Windhoek, Namibia.
  8. University of Durham, Department of Physics, South Road, Durham DH1 3LE, United Kingdom.
  9. GRAPPA, Anton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands.
  10. Obserwatorium Astronomiczne, Uniwersytet Jagiello?ski, ul. Orla 171, 30-244 Kraków, Poland.
  11. Now at Harvard-Smithsonian Center for Astrophysics, 60 Garden St, MS-20, Cambridge, Massachusetts 02138, USA.
  12. Department of Physics and Electrical Engineering, Linnaeus University, 351 95 Växjö, Sweden.
  13. Institut für Theoretische Physik, Lehrstuhl IV: Weltraum und Astrophysik, Ruhr-Universität Bochum, D 44780 Bochum, Germany.
  14. GRAPPA, Anton Pannekoek Institute for Astronomy and Institute of High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands.
  15. Institut für Astro- und Teilchenphysik, Leopold-Franzens-Universität Innsbruck, A-6020 Innsbruck, Austria.
  16. Laboratoire Leprince-Ringuet, Ecole Polytechnique, CNRS/IN2P3, F-91128 Palaiseau, France.
  17. Now at Santa Cruz Institute for Particle Physics, Department of Physics, University of California at Santa Cruz, Santa Cruz, California 95064, USA.
  18. Centre for Space Research, North-West University, Potchefstroom 2520, South Africa.
  19. LUTH, Observatoire de Paris, CNRS, Université Paris Diderot, 5 Place Jules Janssen, 92190 Meudon, France.
  20. LPNHE, Université Pierre et Marie Curie Paris 6, Université Denis Diderot Paris 7, CNRS/IN2P3, 4 Place Jussieu, F-75252 Paris Cedex 5, France.
  21. Institut für Astronomie und Astrophysik, Universität Tübingen, Sand 1, D 72076 Tübingen, Germany.
  22. Laboratoire Univers et Particules de Montpellier, Université Montpellier 2, CNRS/IN2P3, CC 72, Place Eugène Bataillon, F-34095 Montpellier Cedex 5, France.
  23. DSM/Irfu, CEA Saclay, F-91191 Gif-Sur-Yvette Cedex, France.
  24. Astronomical Observatory, The University of Warsaw, Al. Ujazdowskie 4, 00-478 Warsaw, Poland.
  25. Instytut Fizyki Ja?drowej PAN, ul. Radzikowskiego 152, 31-342 Kraków, Poland.
  26. School of Physics, University of the Witwatersrand, 1 Jan Smuts Avenue, Braamfontein, Johannesburg 2050, South Africa.
  27. Landessternwarte, Universität Heidelberg, Königstuhl, D 69117 Heidelberg, Germany.
  28. Oskar Klein Centre, Department of Physics, Stockholm University, Albanova University Center, SE-10691 Stockholm, Sweden.
  29. Wallenberg Academy Fellow.
  30. School of Chemistry & Physics, University of Adelaide, Adelaide 5005, Australia.
  31. APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France.
  32. Univ. Grenoble Alpes, IPAG, F-38000 Grenoble, France and CNRS, IPAG, F-38000 Grenoble, France.
  33. Department of Physics and Astronomy, The University of Leicester, University Road, Leicester LE1 7RH, United Kingdom.
  34. Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warsaw, Poland.
  35. Institut für Physik und Astronomie, Universität Potsdam, Karl-Liebknecht-Strasse 24/25, D 14476 Potsdam, Germany.
  36. Laboratoire d'Annecy-le-Vieux de Physique des Particules, Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France.
  37. DESY, D-15738 Zeuthen, Germany.
  38. Universität Erlangen-Nürnberg, Physikalisches Institut, Erwin-Rommel-Str. 1, D 91058 Erlangen, Germany.
  39. Centre for Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University, Grudziadzka 5, 87-100 Torun, Poland.
  40. Université Bordeaux 1, CNRS/IN2P3, Centre d'Études Nucléaires de Bordeaux Gradignan, 33175 Gradignan, France.
  41. Department of Physics, University of the Free State, PO Box 339, Bloemfontein 9300, South Africa.
  42. GRAPPA, Institute of High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands.

PMID: 25768750 DOI: 10.1103/PhysRevLett.114.081301

Abstract

An annihilation signal of dark matter is searched for from the central region of the Milky Way. Data acquired in dedicated on-off observations of the Galactic center region with H.E.S.S. are analyzed for this purpose. No significant signal is found in a total of ∼9  h of on-off observations. Upper limits on the velocity averaged cross section, ⟨σv⟩, for the annihilation of dark matter particles with masses in the range of ∼300  GeV to ∼10  TeV are derived. In contrast to previous constraints derived from observations of the Galactic center region, the constraints that are derived here apply also under the assumption of a central core of constant dark matter density around the center of the Galaxy. Values of ⟨σv⟩ that are larger than 3×10^{-24}  cm^{3}/s are excluded for dark matter particles with masses between ∼1 and ∼4  TeV at 95% C.L. if the radius of the central dark matter density core does not exceed 500 pc. This is the strongest constraint that is derived on ⟨σv⟩ for annihilating TeV mass dark matter without the assumption of a centrally cusped dark matter density distribution in the search region.

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