Ultra-light scalar saving the 3 + 1 neutrino scheme from the cosmological bounds

The LSND and MiniBooNE results as well as the reactor and Gallium anomalies seem to indicate the presence of a sterile neutrino with a mass of ∼1 eV mixed with active neutrinos. Such sterile neutrino can be produced in the early universe before the neutrino decoupling, leading to a contribution to t...

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Main Author: Yasaman Farzan
Format: Article
Language:English
Published: Elsevier 2019-10-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269319306331
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spelling doaj-240aa0fc54c24a399d66c13a10c6439a2020-11-25T01:08:44ZengElsevierPhysics Letters B0370-26932019-10-01797Ultra-light scalar saving the 3 + 1 neutrino scheme from the cosmological boundsYasaman Farzan0Physics school, Institute for Research in Fundamental Sciences (IPM), P.O. Box 19395-5531, Tehran, Iran; The Abdus Salam ICTP, Strada Costiera 11, 34151, Trieste, Italy; Correspondence to: Physics school, Institute for Research in Fundamental Sciences (IPM), P.O. Box 19395-5531, Tehran, Iran.The LSND and MiniBooNE results as well as the reactor and Gallium anomalies seem to indicate the presence of a sterile neutrino with a mass of ∼1 eV mixed with active neutrinos. Such sterile neutrino can be produced in the early universe before the neutrino decoupling, leading to a contribution to the effective number of neutrinos (Neff) as well as to a contribution to the sum of neutrino masses which are in tension with cosmological observations. We propose a scenario to relax this tension by a Yukawa coupling of the sterile neutrinos to ultra-light scalar particles which contribute to the dark matter in the background. The coupling induces an effective mass for νs which prevents its production in the early universe. We discuss the implications for the upcoming KATRIN experiment and future relic neutrino search experiments such as PTOLEMY. We also briefly comment on certain non-renormalizable forms of interaction between νs and the scalar and their consequences for the νs production in the early universe.http://www.sciencedirect.com/science/article/pii/S0370269319306331
collection DOAJ
language English
format Article
sources DOAJ
author Yasaman Farzan
spellingShingle Yasaman Farzan
Ultra-light scalar saving the 3 + 1 neutrino scheme from the cosmological bounds
Physics Letters B
author_facet Yasaman Farzan
author_sort Yasaman Farzan
title Ultra-light scalar saving the 3 + 1 neutrino scheme from the cosmological bounds
title_short Ultra-light scalar saving the 3 + 1 neutrino scheme from the cosmological bounds
title_full Ultra-light scalar saving the 3 + 1 neutrino scheme from the cosmological bounds
title_fullStr Ultra-light scalar saving the 3 + 1 neutrino scheme from the cosmological bounds
title_full_unstemmed Ultra-light scalar saving the 3 + 1 neutrino scheme from the cosmological bounds
title_sort ultra-light scalar saving the 3 + 1 neutrino scheme from the cosmological bounds
publisher Elsevier
series Physics Letters B
issn 0370-2693
publishDate 2019-10-01
description The LSND and MiniBooNE results as well as the reactor and Gallium anomalies seem to indicate the presence of a sterile neutrino with a mass of ∼1 eV mixed with active neutrinos. Such sterile neutrino can be produced in the early universe before the neutrino decoupling, leading to a contribution to the effective number of neutrinos (Neff) as well as to a contribution to the sum of neutrino masses which are in tension with cosmological observations. We propose a scenario to relax this tension by a Yukawa coupling of the sterile neutrinos to ultra-light scalar particles which contribute to the dark matter in the background. The coupling induces an effective mass for νs which prevents its production in the early universe. We discuss the implications for the upcoming KATRIN experiment and future relic neutrino search experiments such as PTOLEMY. We also briefly comment on certain non-renormalizable forms of interaction between νs and the scalar and their consequences for the νs production in the early universe.
url http://www.sciencedirect.com/science/article/pii/S0370269319306331
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