Erratum to: Interactions of astrophysical neutrinos with dark matter: a model building perspective
Sujata Pandey, Siddhartha Karmakar, Subhendu Rakshit
Abstract
To satisfy the Big Bang Nucleosynthesis (BBN) constraints on neutrino interactions with ultralight scalar DM , the rate of at the neutrino decoupling temperature T 2 MeV must be less than Hubble expansion rate H. Thus, at T , the cross-section of has to be H/n 3.5 10 -34 eV -2 . For the interaction given by Topology I 3,
Topics & Concepts
PhysicsDark matterNeutrinoPerspective (graphical)Particle physicsComputer scienceArtificial intelligenceDark Matter and Cosmic PhenomenaAstrophysics and Cosmic PhenomenaParticle physics theoretical and experimental studies