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相关论文: Gravitational Effects on Particle Dark Matter and …

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If dark matter self-annihilates then it may produce an observable signal when its density is high. The details depend on the intrinsic properties of dark matter and how it clusters in space. For example, the density profile of some dark…

高能天体物理现象 · 物理学 2015-06-03 Benjamin C. Bromley

We analyse the effect of the compression of the dark matter due to the infall of baryons to the galactic center on the gamma-ray flux. In addition, we also consider the effect of non-universal supersymmetric soft terms. This analysis shows…

高能物理 - 唯象学 · 物理学 2007-05-23 Y. Mambrini

Detection of gamma rays from dark matter annihilation in the galactic center is one of the feasible techniques to search for dark matter. We evaluate the gamma ray flux in the case that the dark matter has an electroweak SU(2)_L charge.…

高能物理 - 唯象学 · 物理学 2009-11-10 Junji Hisano , Shigeki. Matsumoto , Mihoko M. Nojiri , Osamu Saito

In this paper we consider dark matter particle annihilation in the gravitational field of black holes. We obtain exact distribution function of the infalling dark matter particles, and compute the resulting flux and spectra of gamma rays…

天体物理学 · 物理学 2009-10-08 A. N. Baushev

Recent studies have suggested the possibility that the lightest supersymmetric particle is a suitable dark matter candidate. In this theoretical framework, annihilations in high density environments like the center of dark matter haloes may…

天体物理学 · 物理学 2007-05-23 Lidia Pieri , Enzo Branchini

In a large region of the supersymmetry parameter space, the annihilation cross section for neutralino dark matter is strongly dependent on the relative velocity of the incoming particles. We explore the consequences of this velocity…

天体物理学 · 物理学 2008-11-26 Mustafa A. Amin , Tommer Wizansky

The annihilation of neutralino dark matter may result in observable signals in different wavelength. In the present paper we will discuss the effect of neutralino annihilation in the halo of our Galaxy and in its center. According to high…

天体物理学 · 物理学 2016-11-09 Roberto Aloisio

Annihilations of weakly interacting dark matter particles provide an important signature for the possibility of indirect detection of dark matter in galaxy halos. These self-annihilations can be greatly enhanced in the vicinity of a massive…

天体物理学 · 物理学 2009-11-06 G. Bertone , G. Sigl , J. Silk

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…

高能天体物理现象 · 物理学 2012-11-14 Steve Blanchet , Julien Lavalle

We describe cosmic gamma-ray and neutrino signals of dark matter annihilation, explaining how the complementarity of these signals provides additional information that, if observable, can enlighten the particle nature of dark matter. This…

高能物理 - 唯象学 · 物理学 2013-05-30 Rouzbeh Allahverdi , Sheldon Campbell , Bhaskar Dutta

We analyse the effect of the compression of the dark matter due to the infall of baryons to the galactic center on the gamma-ray flux. In addition, we also consider the effect of non-universal supersymmetric soft terms. This analysis shows…

高能物理 - 唯象学 · 物理学 2009-11-11 Y. Mambrini

We study the impact of astrophysical processes on the gamma-ray background produced by the annihilation of dark matter particles in cosmological halos, with particular attention to the consequences of the formation of supermassive black…

天体物理学 · 物理学 2010-04-29 Eun-Joo Ahn , Gianfranco Bertone , David Merritt , Pengjie Zhang

In the frame of indirect dark matter searches we investigate the flux of high-energy $\gamma$-ray photons produced by annihilation of dark matter in caustics within our Galaxy under the hypothesis that the bulk of dark matter is composed of…

天体物理学 · 物理学 2009-11-11 Lidia Pieri , Enzo Branchini

Particle dark matter near the galactic center is accreted by the central black hole into a dense spike, strongly enhancing its annihilation rate. Searching for its annihilation products may give us information on the presence or absence of…

高能物理 - 唯象学 · 物理学 2009-10-31 Paolo Gondolo , Joseph Silk

Under the hypothesis of a Dark Matter composed by supersymmetric particles like neutralinos, we investigate the possibility that their annihilation in the haloes of nearby galaxies could produce detectable fluxes of $\gamma$-photons.…

天体物理学 · 物理学 2009-11-10 Lidia Pieri , Enzo Branchini

We study annihilation radiation of neutralinos in the Galactic centre, assuming the existence of a 'spike' in the dark matter density profile, due to adiabatic accretion onto the massive black hole lying at the Galactic centre. Under this…

天体物理学 · 物理学 2009-11-07 Gianfranco Bertone , Guenter Sigl , Joseph Silk

Recent advances in N-body simulations of cold dark matter halos point to a substantial density enhancement near the center. This means that, e.g., the $\gamma$ ray signals from neutralino dark matter annihilations would be significantly…

天体物理学 · 物理学 2010-11-30 L. Bergstrom , P. Ullio , J. Buckley

We study the annihilating dark matter contribution to the extra-galactic diffuse gamma-ray background spectrum, motivated by the recent observations of cosmic-ray positron/electron anomalies. The observed diffuse gamma-ray flux provides…

宇宙学与河外天体物理 · 物理学 2009-09-02 Masahiro Kawasaki , Kazunori Kohri , Kazunori Nakayama

Gamma rays from the annihilation of dark matter particles in the Galactic halo provide a particularly promising means of indirectly detecting dark matter. Here, we demonstrate that pronounced spectral features at energies near the dark…

高能物理 - 唯象学 · 物理学 2011-12-05 Torsten Bringmann , Francesca Calore , Gilles Vertongen , Christoph Weniger

We use high resolution numerical simulations of the formation of cold dark matter halos to simulate the background of decay products from neutralino annihilation, such as gamma-rays or neutrinos. Halos are non-spherical, have steep singular…

天体物理学 · 物理学 2008-11-26 Carlos Calcaneo-Roldan , Ben Moore
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