Inverse Seesaw, dark matter and the Hubble tension
Autor: | Emanuelle Pinsard, S. Rosauro-Alcaraz, Enrique Fernandez-Martinez, Mathias Pierre |
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Přispěvatelé: | UAM. Departamento de Física Teórica, Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA) |
Rok vydání: | 2021 |
Předmět: |
Computer Science::Machine Learning
High Energy Physics - Theory Sterile neutrino Particle physics Cosmology and Nongalactic Astrophysics (astro-ph.CO) Physics and Astronomy (miscellaneous) Spontaneous symmetry breaking Dark matter FOS: Physical sciences dark matter: density QC770-798 Astrophysics Computer Science::Digital Libraries 7. Clean energy 01 natural sciences Statistics::Machine Learning High Energy Physics - Phenomenology (hep-ph) Seesaw molecular geometry Nuclear and particle physics. Atomic energy. Radioactivity 0103 physical sciences Dark Matter neutrino: mass lepton number Neutrinos 010306 general physics Engineering (miscellaneous) Majoron Physics [PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th] 010308 nuclear & particles physics High Energy Physics::Phenomenology spontaneous symmetry breaking Física neutrino: sterile tension Line Lepton number QB460-466 High Energy Physics - Phenomenology Seesaw mechanism High Energy Physics - Theory (hep-th) [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph] Computer Science::Mathematical Software High Energy Physics::Experiment Neutrino [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Astrophysics - Cosmology and Nongalactic Astrophysics |
Zdroj: | European Physical Journal C: Particles and Fields, Vol 81, Iss 10, Pp 1-13 (2021) Biblos-e Archivo. Repositorio Institucional de la UAM instname European Physical Journal Eur.Phys.J.C Eur.Phys.J.C, 2021, 81 (10), pp.954. ⟨10.1140/epjc/s10052-021-09760-y⟩ |
DOI: | 10.48550/arxiv.2106.05298 |
Popis: | We consider the inverse Seesaw scenario for neutrino masses with the approximate Lepton number symmetry broken dynamically by a scalar with Lepton number two. We show that the Majoron associated to the spontaneous symmetry breaking can alleviate the Hubble tension through its contribution to $\Delta N_\text{eff}$ and late decays to neutrinos. Among the additional fermionic states required for realizing the inverse Seesaw mechanism, sterile neutrinos at the keV-MeV scale can account for all the dark matter component of the Universe if produced via freeze-in from the decays of heavier degrees of freedom. Comment: 22 pages, 2 figures |
Databáze: | OpenAIRE |
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