0000000000775223

AUTHOR

Fabio Iocco

0000-0002-4237-0005

showing 2 related works from this author

Effect of low mass dark matter particles on the Sun

2010

We study the effect of dark matter (DM) particles in the Sun, focusing in particular on the possible reduction of the solar neutrinos flux due to the energy carried away by DM particles from the innermost regions of the Sun, and to the consequent reduction of the temperature of the solar core. We find that in the very low-mass range between 4 and 10 GeV, recently advocated to explain the findings of the DAMA and CoGent experiments, the effects on neutrino fluxes are detectable only for DM models with very small, or vanishing, self-annihilation cross section, such as the so-called asymmetric DM models, and we study the combination of DM masses and Spin Dependent cross sections which can be e…

PhysicsAstrophysics and AstronomyNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Solar energetic particles010308 nuclear & particles physics530 PhysicsSolar neutrinoDark matterFOS: Physical sciencesAstrophysics01 natural sciencesMassless particleHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Solar coreConvection zone10231 Institute for Computational Science0103 physical sciencesNeutrino3106 Nuclear and High Energy Physics3101 Physics and Astronomy (miscellaneous)010303 astronomy & astrophysicsLeptonAstrophysics - Cosmology and Nongalactic Astrophysics
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Main Sequence Stars with Asymmetric Dark Matter

2012

We study the effects of feebly or non-annihilating weakly interacting Dark Matter (DM) particles on stars that live in DM environments denser than that of our Sun. We find that the energy transport mechanism induced by DM particles can produce unusual conditions in the core of Main Sequence stars, with effects which can potentially be used to probe DM properties. We find that solar mass stars placed in DM densities of rhochi>= e2 GeV/cm3 are sensitive to Spin-Dependent scattering cross-section sigmsd >= e-37 cm2 and a DM particle mass as low as mchi=5 GeV, accessing a parameter range weakly constrained by current direct detection experiments.

General Physicsastro-ph.SRPhysics MultidisciplinaryDark matterFOS: Physical sciencesGeneral Physics and AstronomyAstrophysics01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsLight dark matterSolar and Stellar Astrophysics (astro-ph.SR)PhysicsSolar massRange (particle radiation)Science & Technology02 Physical Sciences010308 nuclear & particles physicsPhysicsHot dark matter1ST STARShep-phHigh Energy Physics - PhenomenologyStarsAstrophysics - Solar and Stellar AstrophysicsSTELLAR EVOLUTION13. Climate actionPhysical SciencesMixed dark matterAstrophysics::Earth and Planetary AstrophysicsMain sequencePhysical Review Letters
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