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相关论文: Looking for dark matter annihilations in dwarf gal…

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We provide a ``Baedecker'' or travel guide to the directions on the sky where the dark matter annihilation signal may be expected. We calculate the flux of high energy gamma-rays from annihilation of neutralino dark matter in the centre of…

天体物理学 · 物理学 2008-11-26 N. W. Evans , F. Ferrer , Subir Sarkar

If the dark matter in the Universe is made of weakly self-interacting particles, they may self-annihilate and emit gamma-rays. We use high resolution numerical simulations to estimate directly the annihilation flux from the central regions…

天体物理学 · 物理学 2009-09-25 Felix Stoehr , Simon D. M. White , Volker Springel , Giuseppe Tormen , Naoki Yoshida

Dark Matter annihilation holds great potential for directly probing the clumpiness of the Galactic halo that is one of the key predictions of the Cold Dark Matter paradigm of hierarchical structure formation. Here we review the gamma-ray…

星系天体物理 · 物理学 2015-05-13 Michael Kuhlen

We examine the prospects for detecting gamma-rays from dark matter annihilation in the six most promising dwarf spheroidal (dSph) satellite galaxies of the Milky Way. We use recently-measured velocity dispersion profiles to provide a…

天体物理学 · 物理学 2008-11-26 Louis E. Strigari , Savvas M. Koushiappas , James S. Bullock , Manoj Kaplinghat

The mass to luminosity ratio of the dwarf satellite galaxies in the Milky Way suggests that these dwarf galaxies may contain substantial dark matter. The dark matter at the dense region such as within or at the vicinity of the centres of…

宇宙学与河外天体物理 · 物理学 2021-01-13 Ashadul Halder , Shibaji Banerjee , Madhurima Pandey , Debasish Majumdar

We present a new analysis of the relative detectability of dark matter annihilation in the Milky Way's eight classical dwarf spheroidal satellite galaxies. Ours is similar to previous analyses in that we use Markov-Chain Monte Carlo…

高能天体物理现象 · 物理学 2011-07-05 M. G. Walker , C. Combet , J. A. Hinton , D. Maurin , M. I. Wilkinson

Dwarf Spheroidal galaxies are amongst the best targets to search for a Dark Matter annihilation signal. The annihilation of WIMPs in the center of Sagittarius dwarf spheroidal (Sgr dSph) galaxy would produce high energy gamma-rays in the…

At present, dwarf spheroidal galaxies satellites of the Milky Way may represent the best astrophysical objects for dark matter (DM) searches with gamma-ray telescopes. They present the highest mass-to-light ratios known in the Universe.…

宇宙学与河外天体物理 · 物理学 2019-08-13 Miguel A. Sanchez-Conde

Some candidate dark matter particles, such as neutralinos in supersymmetry, would annihilate producing GeV/TeV gamma rays. We report on recent observations of two dwarf spheroid galaxies, Draco, Ursa Minor, the compact elliptical galaxy…

天体物理学 · 物理学 2019-08-14 J. Hall

We present a new formalism designed to discover dark matter annihilation occurring in the Milky Way's dwarf galaxies. The statistical framework extracts all available information in the data by simultaneously combining observations of all…

宇宙学与河外天体物理 · 物理学 2015-04-28 Alex Geringer-Sameth , Savvas M. Koushiappas , Matthew G. Walker

The dwarf spheroidal satellite galaxies of the Milky Way are some of the most dark-matter-dominated objects known. Due to their proximity, high dark matter content, and lack of astrophysical backgrounds, dwarf spheroidal galaxies are widely…

高能天体物理现象 · 物理学 2019-08-14 Matthew Wood , Brandon Anderson , Alex Drlica-Wagner , Johann Cohen-Tanugi , Jan Conrad

Gamma-ray searches for dark matter annihilation and decay in dwarf galaxies rely on an understanding of the dark matter density profiles of these systems. Conversely, uncertainties in these density profiles propagate into the derived…

宇宙学与河外天体物理 · 物理学 2015-03-12 Alex Geringer-Sameth , Savvas M. Koushiappas , Matthew Walker

The dark matter halo of the Milky Way is predicted to contain a very large number of smaller subhalos. As a result of the dark matter annihilations taking place within such objects, the most nearby and massive subhalos could appear as…

高能物理 - 唯象学 · 物理学 2014-01-22 Asher Berlin , Dan Hooper

The dwarf spheroidal galaxy Draco has long been considered likely to be one of the brightest point sources of gamma-rays generated through dark matter annihilations. Recent studies of this object have found that it remains largely intact…

高能物理 - 唯象学 · 物理学 2008-11-26 Lars Bergstrom , Dan Hooper

We use kinematic data from three new, nearby, extremely low-luminosity Milky Way dwarf galaxies (Ursa Major II, Willman 1, and Coma Berenices) to constrain the properties of their dark matter halos, and from these make predictions for the…

We discuss the gamma-ray signal from dark matter annihilation in our Galaxy and in external objects, namely the Large Magellanic Cloud, the Andromeda Galaxy (M31) and M87. We derive predictions for the fluxes in a low energy realization of…

高能物理 - 唯象学 · 物理学 2008-11-26 N. Fornengo , L. Pieri , S. Scopel

The dwarf spheroidal satellite galaxies (dSphs) of the Milky Way are some of the most dark matter (DM) dominated objects known. We report on gamma-ray observations of Milky Way dSphs based on 6 years of Fermi Large Area Telescope data…

高能天体物理现象 · 物理学 2015-12-09 LAT Collaboration

Context. The sterile neutrino is an excellent dark matter candidate, which can be searched for in a wide range of astrophysical sites. It has previously been shown that the optimal search strategy is to consider dwarf galaxies belonging to…

宇宙学与河外天体物理 · 物理学 2009-05-15 Signe Riemer-Sorensen , Steen H. Hansen

If dark matter (DM), which is considered to constitute most of the mass of galaxies, is made of supersymmetric (SUSY) particles, the centers of galaxies should emit gamma-rays produced by their self-annihilation. We present accurate…

天体物理学 · 物理学 2008-11-26 Francisco Prada , Anatoly Klypin , J. Flix , M. Martinez , E. Simonneau

The dwarf spheroidal satellite galaxies of the Milky Way are some of the most dark-matter-dominated objects known. Due to their proximity, high dark matter content, and lack of astrophysical backgrounds, dwarf spheroidal galaxies are widely…

高能天体物理现象 · 物理学 2014-02-20 LAT Collaboration , M. Ackermann , A. Albert , B. Anderson , L. Baldini , J. Ballet , G. Barbiellini , D. Bastieri , K. Bechtol , R. Bellazzini , E. Bissaldi , E. D. Bloom , E. Bonamente , A. Bouvier , T. J. Brandt , J. Bregeon , M. Brigida , P. Bruel , R. Buehler , S. Buson , G. A. Caliandro , R. A. Cameron , M. Caragiulo , P. A. Caraveo , C. Cecchi , E. Charles , A. Chekhtman , J. Chiang , S. Ciprini , R. Claus , J. Cohen-Tanugi , J. Conrad , F. D'Ammando , A. de Angelis , C. D. Dermer , S. W. Digel , E. do Couto e Silva , P. S. Drell , A. Drlica-Wagner , R. Essig , C. Favuzzi , E. C. Ferrara , A. Franckowiak , Y. Fukazawa , S. Funk , P. Fusco , F. Gargano , D. Gasparrini , N. Giglietto , M. Giroletti , G. Godfrey , G. A. Gomez-Vargas , I. A. Grenier , S. Guiriec , M. Gustafsson , M. Hayashida , E. Hays , J. Hewitt , R. E. Hughes , T. Jogler , T. Kamae , J. Knödlseder , D. Kocevski , M. Kuss , . Larsson , L. Latronico , M. Llena Garde , F. Longo , F. Loparco , M. N. Lovellette , P. Lubrano , G. Martinez , M. Mayer , M. N. Mazziotta , P. F. Michelson , W. Mitthumsiri , T. Mizuno , A. A. Moiseev , M. E. Monzani , A. Morselli , I. V. Moskalenko , S. Murgia , R. Nemmen , E. Nuss , T. Ohsugi , E. Orlando , J. F. Ormes , J. S. Perkins , F. Piron , G. Pivato , T. A. Porter , S. Rainò , R. Rando , M. Razzano , S. Razzaque , A. Reimer , O. Reimer , S. Ritz , M. Sànchez-Conde , N. Sehgal , C. Sgrò , E. J. Siskind , P. Spinelli , L. Strigari , D. J. Suson , H. Tajima , H. Takahashi , J. B. Thayer , L. Tibaldo , M. Tinivella , D. F. Torres , Y. Uchiyama , T. L. Usher , J. Vandenbroucke , G. Vianello , V. Vitale , M. Werner , B. L. Winer , K. S. Wood , M. Wood , G. Zaharijas , S. Zimmer
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