0000000000267630

AUTHOR

Lorenzo Ubaldi

0000-0002-9567-9719

showing 2 related works from this author

On baryogenesis from dark matter annihilation

2013

We study in detail the conditions to generate the baryon asymmetry of the universe from the annihilation of dark matter. This scenario requires a low energy mechanism for thermal baryogenesis, hence we first discuss some of these mechanisms together with the specific constraints due to the connection with the dark matter sector. Then we show that, contrary to what stated in previous studies, it is possible to generate the cosmological asymmetry without adding a light sterile dark sector, both in models with violation and with conservation of B – L. In addition, one of the models we propose yields some connection to neutrino masses.

Particle physicsmedia_common.quotation_subjectDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesAsymmetryHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetry0103 physical sciencesThermalBaryon asymmetry010306 general physicsmedia_commonPhysicsleptogenesisdark matter theoryAnnihilation010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsConnection (mathematics)BaryogenesisHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoJournal of Cosmology and Astroparticle Physics
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Gamma rays from cosmic-ray proton scattering in AGN jets: the intra-cluster gas vastly outshines dark matter

2013

Active Galactic Nuclei (AGN) host powerful jets containing high-energy electrons and protons. The astrophysical environment where AGNs and their jets are found is characterized by large concentrations of both dark matter (DM) and intra-cluster medium (ICM) gas. As the high-energy jet particles transverse the DM and the ICM, elastic and inelastic scattering processes generically lead to the production of final-state photons. As first envisioned by Bloom and Wells (1998), and as more recently pointed out by us and others, the scattering of electrons off of DM could lead to a potentially detectable gamma-ray signal, with the parton-level contribution from protons offering dimmer perspectives. …

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusScatteringAstrophysics::High Energy Astrophysical PhenomenaDark matterGamma rayFOS: Physical sciencesAstronomy and AstrophysicsCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsElectronAstrophysicsInelastic scatteringHadronizationHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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