0000000000741071

AUTHOR

Enrico Morgante

0000-0001-9389-0353

showing 3 related works from this author

Relaxion fluctuations (self-stopping relaxion) and overview of relaxion stopping mechanisms

2020

Journal of high energy physics 2005(5), 80 (2020). doi:10.1007/JHEP05(2020)080

effect: quantumNuclear and High Energy Physicscosmological modelCosmology and Nongalactic Astrophysics (astro-ph.CO)production [gauge boson]Field (physics)FOS: Physical sciencesParameter spaceHiggs particle01 natural sciences530Theoretical physicsHigh Energy Physics - Phenomenology (hep-ph)gauge boson: productionfluctuation: quantum0103 physical sciencesddc:530lcsh:Nuclear and particle physics. Atomic energy. Radioactivityinflation010306 general physicsQuantum fluctuationInflation (cosmology)PhysicsGauge boson010308 nuclear & particles physicsElectroweak interactionscale: electroweak interactionquantum [fluctuation]electroweak interaction [scale]Cosmology of Theories beyond the SMHigh Energy Physics - PhenomenologyHomogeneousquantum [effect]Beyond Standard Modelaxion-like particleslcsh:QC770-798Electroweak scaleAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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Structure Formation Limits on Axion-Like Dark Matter

2020

We derive structure formation limits on dark matter (DM) composed of keV-scale axion-like particles (ALPs), produced via freeze-in through the interactions with photons and Standard Model (SM) fermions. We employ Lyman-alpha (Ly-{\alpha}) forest data sets as well as the observed number of Milky Way (MW) subhalos. We compare results obtained using Maxwell-Boltzmann and quantum statistics for describing the SM bath. It should be emphasized that the presence of logarithmic divergences complicates the calculation of the production rate, which can not be parameterized with a simple power law behaviour. The obtained results, in combination with X-ray bounds, exclude the possibility for a photophi…

High Energy Physics - TheoryPhysicsParticle physicsStructure formationPhotonCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsDark matterFOS: Physical sciencesAstronomy and AstrophysicsFermion01 natural sciencesStandard ModelMomentumHigh Energy Physics - PhenomenologyDistribution functionHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)0103 physical sciencesAxionAstrophysics - Cosmology and Nongalactic Astrophysics
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Probing photophobic axion and relaxion dark matter

2021

We investigate the interplay between early universe cosmology and dark matter direct detection, considering axion models with naturally suppressed couplings to photons. In the context of the cosmological relaxation of the electroweak scale, we focus on a scenario of relaxion dark matter, in which the relaxion field constitutes all the observed dark matter relic density and its allowed mass range is fixed to a few keV by construction. In particular, we show that a relaxion particle with mass mϕ=3.0 keV which couples to electrons with gϕ,e=6.8×10−14 is consistent with the XENON1T excess, while accounting for the observed dark matter and satisfying astro/cosmo probes. This scenario uses the el…

PhysicsParticle physics010308 nuclear & particles physicsmedia_common.quotation_subjectDark matterContext (language use)Astrophysics::Cosmology and Extragalactic AstrophysicsElectron01 natural sciencesUniverseCosmology0103 physical sciencesProduction (computer science)Electroweak scale010306 general physicsAxionmedia_commonPhysical Review
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