2021
DOI: 10.1140/epjc/s10052-021-09760-y
|View full text |Cite
|
Sign up to set email alerts
|

Inverse Seesaw, dark matter and the Hubble tension

Abstract: 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 $$\Delta N_\text {eff}$$ Δ N eff and late decays to neutrinos… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1

Citation Types

0
10
0

Year Published

2021
2021
2024
2024

Publication Types

Select...
7
3

Relationship

0
10

Authors

Journals

citations
Cited by 26 publications
(12 citation statements)
references
References 76 publications
(95 reference statements)
0
10
0
Order By: Relevance
“…In the latter case, we assume that any explicit symmetry breaking term is small compared to the electroweak scale such that the mass of the (P)NGB can be set to zero in the following analysis. Using the exponential parametrization, the field a disappears from the scalar potential and the only coupling between the Higgs boson at 125 GeV and the (P)NGB is generated via mixing from the kinetic terms of the scalar after spontaneous symmetry breaking [85,86],…”
Section: (Pseudo) Nambu-goldstone Bosonsmentioning
confidence: 99%
“…In the latter case, we assume that any explicit symmetry breaking term is small compared to the electroweak scale such that the mass of the (P)NGB can be set to zero in the following analysis. Using the exponential parametrization, the field a disappears from the scalar potential and the only coupling between the Higgs boson at 125 GeV and the (P)NGB is generated via mixing from the kinetic terms of the scalar after spontaneous symmetry breaking [85,86],…”
Section: (Pseudo) Nambu-goldstone Bosonsmentioning
confidence: 99%
“…Although not as phenomenologically successful as NEDE, different attempts to relate the Hubble tension and the neutrino sector have been made in the past[34,40,52,53], most notably[20,24] explores the possibility that the EDE field is pushed up its potential when neutrinos become non-relativistic (see also[54] for a DE neutrino interaction). To our knowledge, our work is the first to use the NEDE phase transition for higgsing the neutrino sector.…”
mentioning
confidence: 99%
“…For M 0 N < 1 GeV, the decays of N during the recombination period releases entropy into the thermal bath and impacts Big Bang Nucleosynthesis, which in general places strong limits on the mixing and mass parameters and requires in particular M 0 N ≥ O(0.1) GeV [11]. On the other hand, it has been shown that decaying heavy neutrinos with masses O(30) MeV [35] and sterile neutrinos that interact with additional scalars can alleviate the Hubble tension [36]. We will limit our discussion to M 0 N ≥ 0.1 GeV in the following.…”
Section: Constraintsmentioning
confidence: 99%