0000000000821462

AUTHOR

Julia Stadler

showing 2 related works from this author

The full Boltzmann hierarchy for dark matter-massive neutrino interactions

2020

The impact of dark matter-neutrino interactions on the measurement of the cosmological parameters has been investigated in the past in the context of massless neutrinos exclusively. Here we revisit the role of a neutrino-dark matter coupling in light of ongoing cosmological tensions by implementing the full Boltzmann hierarchy for three massive neutrinos. Our tightest 95% CL upper limit on the strength of the interactions, parameterized via $u_\chi =\frac{\sigma_0}{\sigma_{Th}}\left(\frac{m_\chi}{100 \text{GeV}}\right)^{-1}$, is $u_\chi\leq3.34 \cdot 10^{-4}$, arising from a combination of Planck TTTEEE data, Planck lensing data and SDSS BAO data. This upper bound is, as expected, slightly …

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesContext (language use)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanckWeak gravitational lensingneutrino propertiesPhysicsdark matter theory010308 nuclear & particles physicsAstronomy and AstrophysicsCoupling (probability)Massless particleHigh Energy Physics - Phenomenologyparticle physics-cosmology connectioncosmological perturbation theorysymbolsNeutrinoHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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Is it mixed dark matter or neutrino masses?

2018

In this paper, we explore a scenario where the dark matter is a mixture of interacting and non interacting species. Assuming dark matter-photon interactions for the interacting species, we find that the suppression of the matter power spectrum in this scenario can mimic that expected in the case of massive neutrinos. Our numerical studies include present limits from Planck Cosmic Microwave Background data, which render the strength of the dark matter photon interaction unconstrained when the fraction of interacting dark matter is small. Despite the large entangling between mixed dark matter and neutrino masses, we show that future measurements from the Dark Energy Instrument (DESI) could he…

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Photon010308 nuclear & particles physicsMatter power spectrumCosmic microwave backgroundDark matterFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencessymbols.namesake0103 physical sciencesMixed dark matterDark energysymbolsNeutrinoPlanck[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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