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Related papers: Gamma Rays from Heavy Neutralino Dark Matter

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The viability of neutralino dark matter as an explanation of the 130 GeV gamma ray signal from the Galactic Center recently observed by the Fermi Large Area Telescope is examined. It is found that the signal can be compatible with a sharp…

High Energy Physics - Phenomenology · Physics 2012-10-17 Bibhushan Shakya

We consider neutralino annihilation in dense extragalactic systems known to be dominated by dark matter, in particular M87 and several local dwarf spheroidal galaxies. These annihilations can produce energetic gamma rays which may be…

Astrophysics · Physics 2008-11-26 E. A. Baltz , C. Briot , P. Salati , R. Taillet , J. 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…

Astrophysics · Physics 2010-11-30 L. Bergstrom , P. Ullio , J. Buckley

We consider extensions of the standard model based on open strings ending on D-branes, in which gauge bosons and their associated gauginos exist as strings attached to stacks of D-branes, and chiral matter exists as strings stretching…

High Energy Physics - Phenomenology · Physics 2010-05-12 Luis A. Anchordoqui , Haim Goldberg , Dan Hooper , Danny Marfatia , Tomasz R. Taylor

MMonochromatic neutrinos from dark matter annihilations ($\chi\chi\to \nu\bar\nu$) are always produced in association with a gamma-ray spectrum generated by electroweak bremsstrahlung. Consequently, these neutrino lines can be searched for…

High Energy Physics - Phenomenology · Physics 2016-07-06 Farinaldo S. Queiroz , Carlos E. Yaguna , Christoph Weniger

We present a detailed study of the effect of internal bremsstrahlung photons in the context of the minimal supersymmetric standard models and their impact on gamma-ray dark matter annihilation searches. We find that although this effect has…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 M. Cannoni , M. E. Gomez , M. A. Sanchez-Conde , F. Prada , O. Panella

We consider a simplified model in which Majorana fermion dark matter annihilates to charged fermions through exchange of charged mediators. We consider the gamma-ray signals arising from the processes $XX \rightarrow \bar f f \gamma$,…

High Energy Physics - Phenomenology · Physics 2016-07-27 Jason Kumar , Pearl Sandick , Fei Teng , Takahiro Yamamoto

We compute the electromagnetic radiative corrections to all leading annihilation processes which may occur in the Galactic dark matter halo, for dark matter in the framework of supersymmetric extensions of the Standard Model (MSSM and…

High Energy Physics - Phenomenology · Physics 2008-11-26 Torsten Bringmann , Lars Bergstrom , Joakim Edsjo

We compute the cosmological background radiation of gamma rays and neutrinos due to neutralino annihilation in evolving dark matter halos, assuming the observed dark matter is comprised of thermally excited neutralinos in the MSSM. The…

Astrophysics · Physics 2014-10-13 Dominik Elsaesser , Karl Mannheim

High energy gamma-rays and neutrinos can be produced both by the annihilation and by the possible slow decay of dark matter particles. We discuss the fluxes and spectra of such secondaries produced by dark matter particles in the universe…

Astrophysics · Physics 2009-10-28 F. W. Stecker

Dark matter annihilation into charged particles is necessarily accompanied by gamma rays, produced via radiative corrections. Internal bremsstrahlung from the final state particles can produce hard gamma rays up to the dark matter mass,…

Astrophysics · Physics 2010-02-01 Nicole F. Bell , Thomas D. Jacques

We consider regions of the parameter space of the Minimal Supersymmetric Standard Model (MSSM) with bino-like neutralino dark matter in which a large fraction of the total dark matter annihilation cross section in the present era arises…

High Energy Physics - Phenomenology · Physics 2013-08-09 Jason Kumar , Pearl Sandick

We calculate, using unitarity, a lower bound on the branching ratio $\chi\chi\to \gamma\gamma$ and $\chi\chi\to \gamma Z$, where $\chi$ is any halo dark matter particle that has $W^+W^-$ as one of the major annihilation modes. Examples of…

High Energy Physics - Phenomenology · Physics 2010-11-30 L. Bergstrom , J. Kaplan

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…

High Energy Physics - Phenomenology · Physics 2011-12-05 Torsten Bringmann , Francesca Calore , Gilles Vertongen , Christoph Weniger

In this study, we present some general features of gamma-ray spectra from dark matter. We find that the spectrum with sharp features could appear in a wide class of dark matter models and mimic the gamma line signals. If all other physical…

High Energy Physics - Phenomenology · Physics 2017-12-05 Yong Tang

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…

Astrophysics · Physics 2007-05-23 Lidia Pieri , Enzo Branchini

The inert doublet model contains a neutral stable particle which is an excellent dark matter candidate. We discuss in this paper the indirect signatures of this model in gamma-rays when the dark matter mass is larger than the $W$ boson…

High Energy Physics - Phenomenology · Physics 2015-06-16 Camilo Garcia-Cely , Alejandro Ibarra

It is widely thought that neutralinos, the lightest supersymmetric particles, could comprise most of the dark matter. If so, then dark halos will emit radio and gamma ray signals initiated by neutralino annihilation. A particularly…

Astrophysics · Physics 2009-11-07 Craig Tyler

The neutralino, the lightest stable supersymmetric particle, is a strong theoretical candidate for the missing astronomical ``dark matter''. A profusion of such neutralinos can accumulate near the Sun when they lose energy upon scattering…

Astrophysics · Physics 2017-01-04 Milagro Collaboration

An upper limit on the total annihilation cross section of dark matter (DM) has recently been derived from the observed atmospheric neutrino background. We show that comparable bounds are obtained for DM masses around the TeV scale by…

High Energy Physics - Phenomenology · Physics 2008-11-26 M. Kachelriess , P. D. Serpico
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