6533b7d4fe1ef96bd1262834

RESEARCH PRODUCT

Determining the dark matter mass with DeepCore

Silvia PascoliOlga MenaSergio Palomares-ruizSergio Palomares-ruizChitta R. Das

subject

AstrofísicaNuclear and High Energy PhysicsLarge Underground Xenon experimentAstrophysics::High Energy Astrophysical PhenomenaDark matterScalar field dark matterFOS: Physical sciencesAnnihilationAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Baryonic dark matter0103 physical sciencesWarm dark matter010306 general physicsLight dark matterPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Cosmologia010308 nuclear & particles physicsHot dark matterAstronomyDetectorsHigh Energy Physics - Phenomenology13. Climate actionWeakly interacting massive particlesHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical Phenomena

description

Cosmological and astrophysical observations provide increasing evidence of the existence of dark matter in our Universe. Dark matter particles with a mass above a few GeV can be captured by the Sun, accumulate in the core, annihilate, and produce high energy neutrinos either directly or by subsequent decays of Standard Model particles. We investigate the prospects for indirect dark matter detection in the IceCube/DeepCore neutrino telescope and its capabilities to determine the dark matter mass.

10.1016/j.physletb.2013.07.006http://hdl.handle.net/10261/126817