6533b86ffe1ef96bd12cdfb1

RESEARCH PRODUCT

Testing freeze-in with axial and vector Z′ bosons

Taylor R. GrayCatarina CosmeCatarina CosmeStephen GodfreyMaíra Dutra

subject

High Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectDark matterMassive particleFOS: Physical sciencesContext (language use)QC770-7987. Clean energy01 natural sciencesPartícules (Física nuclear)law.inventionHigh Energy Physics - Phenomenology (hep-ph)WIMPlawNuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesBeam dump010306 general physicsmedia_commonBosonHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCosmologia010308 nuclear & particles physicsCosmology of Theories beyond the SMUniverse3. Good healthHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Beyond Standard ModelAstrophysics - High Energy Astrophysical PhenomenaPhenomenology (particle physics)Astrophysics - Cosmology and Nongalactic Astrophysics

description

The freeze-in production of Feebly Interacting Massive Particle (FIMP) dark matter in the early universe is an appealing alternative to the well-known - and constrained - Weakly Interacting Massive Particle (WIMP) paradigm. Although challenging, the phenomenology of FIMP dark matter has been receiving growing attention and is possible in a few scenarios. In this work, we contribute to this endeavor by considering a $Z^\prime$ portal to fermionic dark matter, with the $Z^\prime$ having both vector and axial couplings and a mass ranging from MeV up to PeV. We evaluate the bounds on both freeze-in and freeze-out from direct detection, atomic parity violation, leptonic anomalous magnetic moments, neutrino-electron scattering, collider, and beam dump experiments. We show that FIMPs can already be tested by most of these experiments in a complementary way, whereas WIMPs are especially viable in the $Z^\prime$ low mass regime, in addition to the $Z^\prime$ resonance region. We also discuss the role of the axial couplings of $Z^\prime$ in our results. We therefore hope to motivate specific realizations of this model in the context of FIMPs, as well as searches for these elusive dark matter candidates.

10.1007/jhep09(2021)056https://doaj.org/article/4ec8645edb0f4e9bb0773d7e567bd0bf