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Indirect detection of dark matter with γ rays.Ruling out dark matter interpretation of the galactic GeV excess by gamma-ray data of galaxy clusters.A unified model for the spatial and mass distribution of subhaloesDark matter annihilation radiation in hydrodynamic simulations of Milky Way haloesCharacterization of dark-matter-induced anisotropies in the diffuse gamma-ray backgroundConstraining extended gamma-ray emission from galaxy clustersThe Phoenix Project: the dark side of rich Galaxy clustersIceCube search for dark matter annihilation in nearby galaxies and galaxy clustersConstraining cosmic rays and magnetic fields in the Perseus galaxy cluster with TeV observations by the MAGIC telescopesAngular power spectrum of the diffuse gamma-ray emission as measured by the Fermi Large Area Telescope and constraints on its dark matter interpretation
P2860
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P2860
description
im Oktober 2011 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в жовтні 2011
@uk
name
Where will supersymmetric dark matter first be seen?
@en
Where will supersymmetric dark matter first be seen?
@nl
type
label
Where will supersymmetric dark matter first be seen?
@en
Where will supersymmetric dark matter first be seen?
@nl
prefLabel
Where will supersymmetric dark matter first be seen?
@en
Where will supersymmetric dark matter first be seen?
@nl
P2093
P1476
Where will supersymmetric dark matter first be seen?
@en
P2093
C. S. Frenk
S. D. M. White
P304
P356
10.1111/J.1365-2966.2011.19836.X
P407
P577
2011-10-28T00:00:00Z
P818
P819
2012MNRAS.419.1721G