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Motivated by the complex gamma-ray spectrum of the Galactic Center source now measured over five decades in energy, we revisit the issue of the role of dark matter annihilations in this interesting region. We reassess whether the emission…

High Energy Astrophysical Phenomena · Physics 2013-05-30 Alexander V. Belikov , Gabrijela Zaharijas , Joseph Silk

A number of signals involving charged cosmic rays and high-energy photons have been interpreted as being due to annihilating dark matter. This article provides an overview of the experimental evidence and discusses in particular detections…

Astrophysics · Physics 2007-05-23 U. Schwanke

We present the first MAGIC/Fermi-LAT joint search for dark matter annihilation gamma-ray signals from dwarf satellite galaxies. We combine 158 hours of observations of Segue 1 by MAGIC with 6-years observations of 15 dwarf satellite…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Javier Rico , Matthew Wood , Alex Drlica-Wagner , Jelena Aleksić

We search for gamma-ray emission from OJ287 in the energy range from 0.1-300 GeV during 2015-2023, in coincidence with an extensive observing campaign to monitor the optical flux variability and polarization, as discussed in…

High Energy Astrophysical Phenomena · Physics 2024-07-29 Vibhavasu Pasumarti , Shantanu Desai

Cosmological $N$-body simulations show that Milky Way-sized galaxies harbor a population of unmerged dark matter subhalos. These subhalos could shine in gamma-rays and be eventually detected in gamma-ray surveys as unidentified sources. We…

High Energy Astrophysical Phenomena · Physics 2021-09-01 H. E. S. S. Collaboration , H. Abdallah , F. Aharonian , F. Ait Benkhali , E. O. Angüner , C. Arcaro , C. Armand , T. Armstrong , H. Ashkar , M. Backes , V. Baghmanyan , V. Barbosa Martins , A. Barnacka , M. Barnard , Y. Becherini , D. Berge , K. Bernlöhr , B. Bi , M. Böttcher , C. Boisson , J. Bolmont , M. de Bony de Lavergne , M. Breuhaus , R. Brose , F. Brun , T. Bulik , T. Bylund , F. Cangemi , S. Caroff , S. Casanova , P. Chambery , J. Catalano T. Chand , A. Chen , G. Cotter , M. Curylo , H. Dalgleish , J. Damascene Mbarubucyeye , I. D. Davids , J. Davies , J. Devin , A. Djannati-Ataï , A. Dmytriiev , A. Donath , V. Doroshenko , L. Dreyer , L. Du Plessis , C. Duffy , K. Egberts , S. Einecke , G. Emery , J. -P. Ernenwein , K. Feijen , S. Fegan , A. Fiasson , G. Fichet de Clairfontaine , G. Fontaine , S. Funk , M. Füßling , S. Gabici , Y. A. Gallant , G. Giavitto , L. Giunti , D. Glawion , J. F. Glicenstein , M. -H. Grondin , S. Hattingh , M. Haupt , G. Hermann , J. A. Hinton , W. Hofmann , C. Hoischen , T. L. Holch , M. Holler , M. Hörbe , D. Horns , Z. Huang , D. Huber , M. Jamrozy , D. Jankowsky , F. Jankowsky , V. Joshi , I. Jung-Richardt , E. Kasai , K. Katarzyński , U. Katz , D. Khangulyan , B. Khèlifi , S. Klepser , W. Kluzniak , Nu. Komin , R. Konno , K. Kosack , D. Kostunin , M. Kreter , G. Kukec Mezek , A. Kundu , G. Lamanna , S. Le Stum , A. Lemière , M. Lemoine-Goumard , J. -P. Lenain , F. Leuschner , C. Levy , T. Lohse , A. Luashvili , I. Lypova , J. Mackey , J. Majumdar , D. Malyshev , D. Malyshev , V. Marandon , P. Marchegiani , A. Marcowith , A. Mares , G. Martì-Devesa , R. Marx , G. Maurin , P. J. Meintjes , M. Meyer , A. Mitchell , R. Moderski , L. Mohrmann , A. Montanari , C. Moore , P. Morris , E. Moulin , J. Muller , T. Murach , K. Nakashima , A. Nayerhoda , M. de Naurois , H. Ndiyavala , J. Niemiec , A. Noel , L. Oberholzer , P. O'Brien , S. Ohm , L. Olivera-Nieto , E. de Ona Wilhelmi , M. Ostrowski , M. Panter , S. Panny , R. D. Parsons , G. Peron , S. Pita , V. Poireau , D. A. Prokhorov , H. Prokoph , G. Pühlhofer , M. Punch , A. Quirrenbach , P. Reichherzer , A. Reimer , O. Reimer , Q. Remy , M. Renaud , F. Rieger , C. Romoli , G. Rowell , B. Rudak , H. Rueda Ricarte , E. Ruiz-Velasco , V. Sahakian , S. Sailer , H. Salzmann , D. A. Sanchez , A. Santangelo , M. Sasaki , F. Schüssler , H. M. Schutte , U. Schwanke , M. Senniappan , A. S. Seyffert , J. N. S. Shapopi , K. Shiningayamwe , R. Simoni , A. Sinha , H. Sol , H. Spackman , A. Specovius , S. Spencer , M. Spir-Jacob , L. Stawarz , L. Sun , R. Steenkamp , C. Stegmann , S. Steinmassl , C. Steppa , T. Takahashi , T. Tanaka , T. Tavernier , A. M. Taylor , R. Terrier , C. Thorpe Morgan , J. H. E. Thiersen , M. Tluczykont , L. Tomankova , C. Trichard , M. Tsirou , M. Tsuji , R. Tuffs , Y. Uchiyama , D. J. van der Walt , C. van Eldik , C. van Rensburg , B. van Soelen , G. Vasileiadis , J. Veh , C. Venter , A. Viana , P. Vincent , J. Vink , H. J. Völk , S. J. Wagner , F. Werner , R. White , A. Wierzcholska , Yu Wun Wong , H. Yassin , A. Yusafzai , M. Zacharias , R. Zanin , D. Zargaryan , A. A. Zdziarski , A. Zech , S. Zhu , A. Zmija , J. Zorn , S. Zouari , N. Zywucka

We consider an extension of the Standard Model by a singlet scalar that accounts for the dark matter of the Universe. Within this model we compute the expected gamma ray flux from the annihilation of dark matter particles in a consistent…

High Energy Physics - Phenomenology · Physics 2009-03-27 Carlos E. Yaguna

Observations of cosmic rays are a sensitive probe of dark matter annihilation in our Galaxy. In this article we present an analysis of the AMS-02 antiproton data, reducing cosmic-ray propagation uncertainties by fitting at the same time…

High Energy Astrophysical Phenomena · Physics 2018-04-23 Alessandro Cuoco , Jan Heisig , Michael Korsmeier , Michael Krämer

We study radiative decay of gravitino dark matter with trilinear R-parity violations. We show that the branching ratio of the decay of gravitino into monochromatic photon can be large enough to explain the observed gamma-ray line from the…

High Energy Physics - Phenomenology · Physics 2013-10-22 Seng Pei Liew

The Fermi Gamma-ray Space Telescope was launched more than 13 years ago and since then it has dramatically changed our knowledge of the gamma-ray sky. With more than three billions photons from the whole sky, collected in the energy range…

High Energy Astrophysical Phenomena · Physics 2022-09-09 Giacomo Principe

High energy electrons and positrons from decaying dark matter can produce a significant flux of gamma rays by inverse Compton off low energy photons in the interstellar radiation field. This possibility is inevitably related with the dark…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Le Zhang , Christoph Weniger , Luca Maccione , Javier Redondo , Guenter Sigl

The launch of the Fermi satellite in 2008, with its Large Area Telescope (LAT) on board, has opened a new era for the study of gamma-ray sources at GeV ($10^9$ eV) energies. Similarly, the commissioning of the third generation of imaging…

Instrumentation and Methods for Astrophysics · Physics 2023-11-07 Denys Malyshev , Lars Mohrmann

Supernovae (SNe) exploding in a dense circumstellar medium (CSM) are predicted to accelerate cosmic rays in collisionless shocks and emit GeV gamma rays and TeV neutrinos on a time scale of several months. Here we summarize the results of…

High Energy Astrophysical Phenomena · Physics 2015-07-15 A. Franckowiak , K. Murase , E. O. Ofek

Scenarios with hidden, spontaneously broken, non-abelian gauge groups contain a natural dark matter candidate, the hidden vector, whose longevity is due to an accidental custodial symmetry in the renormalizable Lagrangian. Nevertheless,…

High Energy Physics - Phenomenology · Physics 2015-03-13 Chiara Arina , Thomas Hambye , Alejandro Ibarra , Christoph Weniger

Electroweakly interacting stable spin-1 particle in the $(1-10)$ TeV mass range can be a dark matter candidate with rich testability. In particular, one or even two gamma-ray line-like features are expected to be a smoking-gun signature for…

High Energy Physics - Phenomenology · Physics 2025-03-03 Motoko Fujiwara , Martin Vollmann

In this article, we report a new signature of dark matter annihilation based on the radio continuum data of NGC 1569 galaxy detected in the past few decades. After eliminating the thermal contribution of the radio signal, an abrupt change…

High Energy Astrophysical Phenomena · Physics 2018-06-20 Man Ho Chan

We compute the gamma-ray output of axion-mediated dark matter and derive the corresponding constraints set by recent data. In such scenarios the dark matter candidate is a Dirac fermion that pair-annihilates into axions and/or scalars.…

High Energy Physics - Phenomenology · Physics 2016-04-11 Alejandro Ibarra , Hyun Min Lee , Sergio López Gehler , Wan-Il Park , Miguel Pato

Recently, it was suggested that the gamma rays observed by the Fermi Gamma Ray Space Telescope from the direction of the galactic center could surprisingly well be described by a dark matter annihilation scenario, both in terms of their…

High Energy Physics - Phenomenology · Physics 2009-11-09 Torsten Bringmann

The Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope detected a gamma-ray source that is spatially consistent with the location of Eta Carinae. This source has been persistently bright since the beginning of the LAT…

High Energy Astrophysical Phenomena · Physics 2012-08-27 The Fermi LAT collaboration

A long time ago (in 2014), in galaxies and galaxy clusters far, far away, several groups have reported hints for a yet unidentified line in astrophysical X-ray signals at an energy of 3.5\,keV. While it is not unlikely that this line is…

High Energy Physics - Phenomenology · Physics 2018-02-07 Vedran Brdar , Joachim Kopp , Jia Liu , Xiao-Ping Wang
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