6533b859fe1ef96bd12b6e52

RESEARCH PRODUCT

Dark matter-neutrino interactions through the lens of their cosmological implications

Andres Olivares-del CampoSilvia PascoliCéline BœhmSergio Palomares-ruiz

subject

Particle physicsStructure formationdark matter: interactionPhysics beyond the Standard ModelDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsParameter space01 natural sciencesdark matterdark matter: couplingHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesneutrino: coupling010306 general physicsneutrino: interactionPhysics010308 nuclear & particles physicsnew physicsdark matter: massdark matter: mediationHigh Energy Physics - PhenomenologyCoupling (physics)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Particle[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]NeutrinoDark fluiddark matter: parameter space

description

Dark matter and neutrinos provide the two most compelling pieces of evidence for new physics beyond the Standard Model of Particle Physics but they are often treated as two different sectors. The aim of this paper is to determine whether there are viable particle physics frameworks in which dark matter can be coupled to active neutrinos. We use a simplified model approach to determine all possible renormalizable scenarios where there is such a coupling, and study their astrophysical and cosmological signatures. We find that dark matter-neutrino interactions have an impact on structure formation and lead to indirect detection signatures when the coupling between dark matter and neutrinos is sufficiently large. This can be used to exclude a large fraction of the parameter space. In most cases, dark matter masses up to a few MeV and mediator masses up to a few GeV are ruled out. The exclusion region can be further extended when dark matter is coupled to a spin-1 mediator or when the dark matter particle and the mediator are degenerate in mass if the mediator is a spin-0 or spin-1/2 particle.

10.1103/physrevd.97.075039https://hal.archives-ouvertes.fr/hal-01797819