0000000000587660

AUTHOR

Samuel D. Mcdermott

0000-0001-5513-1938

showing 2 related works from this author

The Cosmological Evolution of Light Dark Photon Dark Matter

2020

Light dark photons are subject to various plasma effects, such as Debye screening and resonant oscillations, which can lead to a more complex cosmological evolution than is experienced by conventional cold dark matter candidates. Maintaining a consistent history of dark photon dark matter requires ensuring that the super-thermal abundance present in the early Universe $\textit{(i)}$ does not deviate significantly after the formation of the CMB, and $\textit{(ii)}$ does not excessively leak into the Standard Model plasma after BBN. We point out that the role of non-resonant absorption, which has previously been neglected in cosmological studies of this dark matter candidate, produces strong …

PhysicsCold dark matterCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsmedia_common.quotation_subjectDark matterCosmic microwave backgroundFOS: Physical sciencesAstrophysicsPlasmaAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesUniverseDark photonHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)13. Climate actionNucleosynthesis0103 physical sciencesOptical depth (astrophysics)010306 general physicsmedia_commonAstrophysics - 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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