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We use gamma-ray observations by the Fermi Large Area Telescope (Fermi-LAT) to impose limits on the properties of the hypothetical particle Weyl meson. Such mesons arise in theories which display local scale invariance and act as dark…

High Energy Physics - Phenomenology · Physics 2014-08-14 Gopal Kashyap

Galaxy clusters are one of the prime sites to search for dark matter (DM) annihilation signals. Depending on the substructure of the DM halo of a galaxy cluster and the cross sections for DM annihilation channels, these signals might be…

High Energy Astrophysical Phenomena · Physics 2016-08-07 M. Ackermann , M. Ajello , A. Albert , W. B. Atwood , L. Baldini , G. Barbiellini , D. Bastieri , K. Bechtol , R. Bellazzini , E. Bissaldi , E. D. Bloom , R. Bonino , E. Bottacini , T. J. Brandt , J. Bregeon , P. Bruel , R. Buehler , S. Buson , G. A. Caliandro , R. A. Cameron , R. Caputo , M. Caragiulo , P. A. Caraveo , J. M. Casandjian , E. Cavazzuti , C. Cecchi , E. Charles , A. Chekhtman , G. Chiaro , S. Ciprini , J. Cohen-Tanugi , J. Conrad , S. Cutini , F. D'Ammando , A. de Angelis , F. de Palma , R. Desiante , S. W. Digel , L. Di Venere , P. S. Drell , C. Favuzzi , S. J. Fegan , W. B. Focke , A. Franckowiak , Y. Fukazawa , S. Funk , P. Fusco , F. Gargano , D. Gasparrini , N. Giglietto , F. Giordano , M. Giroletti , T. Glanzman , G. Godfrey , G. A. Gomez-Vargas , I. A. Grenier , S. Guiriec , M. Gustafsson , J. W. Hewitt , A. B. Hill , D. Horan , T. E. Jeltema , T. Jogler , A. S. Johnson , M. Kuss , S. Larsson , L. Latronico , J. Li , L. Li , F. Longo , F. Loparco , M. N. Lovellette , P. Lubrano , S. Maldera , D. Malyshev , A. Manfreda , M. Mayer , M. N. Mazziotta , P. F. Michelson , T. Mizuno , M. E. Monzani , A. Morselli , I. V. Moskalenko , S. Murgia , E. Nuss , T. Ohsugi , M. Orienti , E. Orlando , J. F. Ormes , D. Paneque , J. S. Perkins , M. Pesce-Rollins , V. Petrosian , F. Piron , G. Pivato , T. A. Porter , S. Rainò , R. Rando , M. Razzano , A. Reimer , O. Reimer , M. Sánchez-Conde , A. Schulz , C. Sgró , E. J. Siskind , F. Spada , G. Spandre , P. Spinelli , E. Storm , H. Tajima , H. Takahashi , J. B. Thayer , D. F. Torres , G. Tosti , E. Troja , G. Vianello , K. S. Wood , M. Wood , G. Zaharijas , S. Zimmer , A. Pinzke

Recent gamma-ray observations and radio observations put strong constraints on the parameters of dark matter annihilation. In this article, we derive new constraints for six standard model annihilation channels by using the recent radio…

High Energy Astrophysical Phenomena · Physics 2016-08-03 Man Ho Chan

We consider constraints on $p$-wave dark matter in a dark matter spike surrounding the supermassive black hole at the center of M87. Owing to the large mass of the black hole, and resulting large velocity dispersion for the dark matter…

High Energy Physics - Phenomenology · Physics 2023-11-29 Katharena Christy , Jason Kumar , Pearl Sandick

Short-lived mediators are often used to describe dark matter interactions with Standard Model particles. When the dark matter mass is heavier than the mass of the mediator, it may self-annihilate into short-lived mediators, and in some…

High Energy Physics - Phenomenology · Physics 2018-03-21 Stefano Profumo , Farinaldo S. Queiroz , Joseph Silk , Clarissa Siqueira

Recent observations suggest that some high-velocity clouds may be confined by massive dark matter halos. In particular, the proximity and proposed dark matter content of the Smith Cloud make it a tempting target for the indirect detection…

High Energy Astrophysical Phenomena · Physics 2014-07-01 Alex Drlica-Wagner , German A. Gomez-Vargas , John W. Hewitt , Tim Linden , Luigi Tibaldo

An excess of gamma rays at GeV energies has been detected in the Fermi-LAT data. This signal comes from a narrow region around the Galactic Center and has been interpreted as possible evidence for light (30 GeV) dark matter particles.…

High Energy Astrophysical Phenomena · Physics 2015-01-30 Thomas Lacroix

Dark matter particle annihilation or decay can produce monochromatic gamma-ray lines and contribute to the diffuse gamma-ray background. Flux upper limits are presented for gamma-ray spectral lines from 7 to 200 GeV and for the diffuse…

High Energy Astrophysical Phenomena · Physics 2015-06-05 LAT Collaboration , M. Ackermann , M. Ajello , A. Albert , L. Baldini , G. Barbiellini , K. Bechtol , R. Bellazzini , B. Berenji , R. D. Blandford , E. D. Bloom , E. Bonamente , A. W. Borgland , M. Brigida , R. Buehler , S. Buson , G. A. Caliandro , R. A. Cameron , P. A. Caraveo , J. M. Casandjian , C. Cecchi , E. Charles , A. Chekhtman , J. Chiang , S. Ciprini , R. Claus , J. Cohen-Tanugi , J. Conrad , F. D'Ammando , F. de Palma , C. D. Dermer , E. do Couto e Silva , P. S. Drell , A. Drlica-Wagner , Y. Edmonds , R. Essig , C. Favuzzi , S. J. Fegan , Y. Fukazawa , S. Funk , P. Fusco , F. Gargano , D. Gasparrini , S. Germani , N. Giglietto , F. Giordano , M. Giroletti , T. Glanzman , G. Godfrey , I. A. Grenier , S. Guiriec , M. Gustafsson , D. Hadasch , M. Hayashida , D. Horan , R. E. Hughes , T. Kamae , J. Knödlseder , M. Kuss , J. Lande , A. M. Lionetto , M. Llena Garde , F. Longo , F. Loparco , M. N. Lovellette , P. Lubrano , M. N. Mazziotta , P. F. Michelson , W. Mitthumsiri , T. Mizuno , A. A. Moiseev , C. Monte , M. E. Monzani , A. Morselli , I. V. Moskalenko , S. Murgia , M. Naumann-Godo , J. P. Norris , E. Nuss , T. Ohsugi , A. Okumura , E. Orlando , J. F. Ormes , D. Paneque , J. H. Panetta , M. Pesce-Rollins , F. Piron , G. Pivato , T. A. Porter , D. Prokhorov , S. Rainò , R. Rando , M. Razzano , O. Reimer , M. Roth , C. Sbarra , J. D. Scargle , C. Sgrò , E. J. Siskind , A. Snyder , P. Spinelli , D. J. Suson , H. Takahashi , T. Tanaka , J. G. Thayer , J. B. Thayer , L. Tibaldo , M. Tinivella , D. F. Torres , G. Tosti , E. Troja , J. Vandenbroucke , V. Vasileiou , G. Vianello , V. Vitale , A. P. Waite , B. L. Winer , K. S. Wood , Z. Yang , S. Zimmer

Numerical simulations of structure formation have recorded a remarkable progress in the recent years, in particular due to the inclusion of baryonic physics evolving with the dark matter component. We generate Monte Carlo realizations of…

High Energy Astrophysical Phenomena · Physics 2017-09-20 Francesca Calore , Valentina De Romeri , Mattia Di Mauro , Fiorenza Donato , Federico Marinacci

The Galactic center $\gamma$-ray excess, detected by the Fermi-LAT, is a very attractive tentative signal from dark matter annihilation. Searching for associated synchrotron emissions can test the dark matter interpretation for this excess.…

High Energy Astrophysical Phenomena · Physics 2023-05-18 Wen-Qing Guo , Yichao Li , Xiaoyuan Huang , Yin-Zhe Ma , Geoff Beck , Yogesh Chandola , Feng Huang

We reconsider Sommerfeld-enhanced annihilation of dark matter (DM) into leptons to explain PAMELA and Fermi electron and positron observations, in light of possible new effects from substructure. There is strong tension between getting a…

High Energy Physics - Phenomenology · Physics 2010-12-23 Aaron C Vincent , Wei Xue , James M Cline

In this article, we review the prospects for the Fermi satellite (formerly known as GLAST) to detect gamma rays from dark matter annihilations in the Central Region of the Milky Way, in particular on the light of the recent astrophysical…

High Energy Physics - Phenomenology · Physics 2015-03-13 Pasquale Dario Serpico , Dan Hooper

We make a detailed analysis of the indirect diffuse gamma-ray signals from dark matter annihilation in the Galaxy. We include the prompt emission, as well as the emission from inverse Compton scattering whenever the annihilation products…

High Energy Astrophysical Phenomena · Physics 2012-11-14 Steve Blanchet , Julien Lavalle

Clear methods to differentiate between decaying and annihilating dark matter (DM) scenarios are still by and large unavailable. In this note, we study the potential astrophysical signatures of a new class of hidden sector decaying DM…

High Energy Physics - Phenomenology · Physics 2009-08-11 Joshua T. Ruderman , Tomer Volansky

Recently, a preliminary spectrum from the Fermi Gamma-ray Space Telescope has been presented for the inner galaxy (-30 < l < 30, -5 < b < 5), as well as the galactic center (-1 < l < 1, -1< b < 1). We consider the implications of these data…

High Energy Astrophysical Phenomena · Physics 2009-07-29 Ilias Cholis , Gregory Dobler , Douglas P. Finkbeiner , Lisa Goodenough , Tracy R. Slatyer , Neal Weiner

We study the spectra of gamma ray signals that arise from dark matter annihilation in the universe. We focus on the large class of theories where the photon spectrum includes both continuum spectrum of gamma rays that arise from…

High Energy Physics - Phenomenology · Physics 2015-03-19 Kevork N. Abazajian , Prateek Agrawal , Zackaria Chacko , Can Kilic

If dark matter particles are not perfectly stable, their decay products might be seen in the cosmic-ray fluxes. A natural candidate for decaying dark matter is the gravitino in R-parity violating scenarios. In the relevant GeV-TeV energy…

High Energy Astrophysical Phenomena · Physics 2011-10-31 Xiaoyuan Huang , Gilles Vertongen , Christoph Weniger

We search for dark matter (DM) annihilating subhalos of the Milky Way halo among the Fermi Large Area Telescope (LAT) unassociated sources. We construct, for the first time, a statistical model of the unassociated sources at latitudes above…

High Energy Astrophysical Phenomena · Physics 2025-03-20 Aurelio Amerio , Dmitry Malyshev , Bryan Zaldivar , Viviana Gammaldi , Miguel Ángel Sánchez-Conde

Spatial extension has been hailed as a "smoking gun" in the gamma-ray search of dark galactic subhalos, which would appear as unidentified sources for gamma-ray telescopes. In this work, we study the sensitivity of the Fermi-LAT to extended…

High Energy Astrophysical Phenomena · Physics 2022-04-27 J. Coronado-Blazquez , M. Sanchez-Conde , J. Perez-Romero , A. Aguirre-Santaella

The detection of gamma-rays from dark matter (DM) annihilation is among the scientific goals of the Fermi Large Area Telescope (formerly known as GLAST) and Cherenkov telescopes. In this paper we investigate the existence of realistic…

Astrophysics · Physics 2009-11-13 L. Pieri , A. Pizzella , E. M. Corsini , E. Dalla Bonta' , F. Bertola