0000000000345004

AUTHOR

Vivian Poulin

showing 2 related works from this author

The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe

2020

It is commonly assumed that the energy density of the Universe was dominated by radiation between reheating after inflation and the onset of matter domination 54,000 years later. While the abundance of light elements indicates that the Universe was radiation dominated during Big Bang Nucleosynthesis (BBN), there is scant evidence that the Universe was radiation dominated prior to BBN. It is therefore possible that the cosmological history was more complicated, with deviations from the standard radiation domination during the earliest epochs. Indeed, several interesting proposals regarding various topics such as the generation of dark matter, matter-antimatter asymmetry, gravitational waves,…

High Energy Physics - TheoryCosmology and Nongalactic Astrophysics (astro-ph.CO)reheatingmedia_common.quotation_subjectnucleosynthesis: big bangDark matterFOS: Physical sciencesPrimordial black holeGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesCosmologyGeneral Relativity and Quantum Cosmologydark matterGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesis0103 physical sciencesenergy: density010306 general physicsmedia_commonInflation (cosmology)Physics010308 nuclear & particles physicsGravitational wave[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]gravitational radiationAstronomyUniverseinflation: modelBaryogenesisHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph][PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]history[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]black hole: primordialasymmetryAstrophysics - Cosmology and Nongalactic Astrophysics
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Dark photon dark matter in the presence of inhomogeneous structure

2020

Dark photon dark matter will resonantly convert into visible photons when the dark photon mass is equal to the plasma frequency of the ambient medium. In cosmological contexts, this transition leads to an extremely efficient, albeit short-lived, heating of the surrounding gas. Existing work in this field has been predominantly focused on understanding the implications of these resonant transitions in the limit that the plasma frequency of the Universe can be treated as being perfectly homogeneous, i.e. neglecting inhomogeneities in the electron number density. In this work we focus on the implications of heating from dark photon dark matter in the presence of inhomogeneous structure (which …

Nuclear and High Energy PhysicsPhotonCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsPlasma oscillation01 natural sciencesDark photon[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityThermal Field Theory010306 general physicsReionizationPhysicsRange (particle radiation)010308 nuclear & particles physicsStar formationFísicaCosmology of Theories beyond the SMHigh Energy Physics - PhenomenologyOrders of magnitude (time)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]lcsh:QC770-798Astrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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