About: Indirect detection of dark matter

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dbo:wikiPageWikiLink	dbr:IceCube_Neutrino_Observatory dbc:Physics_beyond_the_Standard_Model dbr:Chronology_of_the_universe dbr:Planck_(spacecraft) dbr:Direct_detection_of_dark_matter dbc:Dark_matter dbr:Neutrino dbr:Photon dbr:Photon_energy dbr:Pulsar dbr:Galactic_Center dbr:Super-Kamiokande dbr:Fermi_Gamma-ray_Space_Telescope dbr:Angular_resolution dbr:Cherenkov_Telescope_Array dbr:Cosmic_ray dbr:Galaxy_cluster dbr:Gamma_ray dbr:X-ray dbr:NuSTAR dbr:Electronvolt dbr:High_Energy_Stereoscopic_System dbr:Bremsstrahlung dbc:Physical_cosmology dbr:Milky_Way dbr:Universe dbr:Scale_factor_(cosmology) dbr:Atom dbr:Galactic_halo dbr:Standard_Model dbr:Cosmic_microwave_background dbr:Dark_matter dbr:Geminga dbr:Particle_accelerator dbr:Dwarf_galaxy dbr:Supernova_remnant dbr:Anisotropy dbr:Muon_neutrino dbc:Observational_cosmology dbr:VERITAS dbr:Recombination_(cosmology) dbr:Cross_section_(physics) dbr:Weakly_interacting_massive_particles dbr:File:1e0657_scale.jpg dbr:File:Fermi_5_year_11000x6189.png
dbp:date	June 2022 (en)
dbp:reason	The prevailing theory suggests that we are instead currently in the dark-energy-dominated era. (en)
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dct:subject	dbc:Physics_beyond_the_Standard_Model dbc:Dark_matter dbc:Observational_cosmology
rdfs:label	Indirect detection of dark matter (en)
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