We investigate a consistent scenario of time-varying neutrino masses, and discuss its impact on cosmology, beta decay, and neutrino oscillation experiments. Such time-varying masses are assumed to be generated by the coupling between a sterile neutrino and an ultralight scalar field, which in turn affects the light neutrinos by mixing. Besides, the scalar could act as an ultralight dark matter candidate. We demonstrate how various cosmological bounds, such as those coming from Big Bang nucleosynthesis, the cosmic microwave background, as well as large scale structures, can be evaded in this model. This scenario can be further constrained using multiple terrestrial experiments. In particular, for beta-decay experiments like KATRIN, non-trivi...
A sterile neutrino with a keV-scale mass is a compelling dark matter candidate. We propose a new pro...
Sterile neutrinos are one of the leading dark matter candidates. Their masses may originate from a v...
We show that sterile neutrinos with masses larger than 1 eV, as motivated by several short-baseline ...
We investigate a consistent scenario of time-varying neutrino masses, and discuss its impact on cosm...
Unexplored interactions of neutrinos could be the key to understanding the nature of the dark matter...
We investigate the cosmological consequences of light sterile neutrinos with altered dispersion rela...
We employ state-of-the art cosmological observables including supernova surveys and BAO information ...
If ultralight $(\ll$ eV), bosonic dark matter couples to right handed neutrinos, active neutrino mas...
In this paper we investigate a time-varying neutrino mass model, motivated by the mild tension betwe...
We propose a new production mechanism for keV sterile neutrino dark matter which relies neither on t...
We explore the neutrinoless double beta ($0\nu \beta\beta$) decay induced by an ultralight dark matt...
The presence of light (m_A∼10^(−6) eV) scalar fields in the early universe can modify the cosmology...
We explore a Portalino-like model of dark matter and neutrino masses in which right-handed neutrino ...
Sterile neutrinos can be produced in the early universe via interactions with their active counterpa...
Sterile neutrinos are well-motivated and simple dark matter (DM) candidates. However, sterile neutri...
A sterile neutrino with a keV-scale mass is a compelling dark matter candidate. We propose a new pro...
Sterile neutrinos are one of the leading dark matter candidates. Their masses may originate from a v...
We show that sterile neutrinos with masses larger than 1 eV, as motivated by several short-baseline ...
We investigate a consistent scenario of time-varying neutrino masses, and discuss its impact on cosm...
Unexplored interactions of neutrinos could be the key to understanding the nature of the dark matter...
We investigate the cosmological consequences of light sterile neutrinos with altered dispersion rela...
We employ state-of-the art cosmological observables including supernova surveys and BAO information ...
If ultralight $(\ll$ eV), bosonic dark matter couples to right handed neutrinos, active neutrino mas...
In this paper we investigate a time-varying neutrino mass model, motivated by the mild tension betwe...
We propose a new production mechanism for keV sterile neutrino dark matter which relies neither on t...
We explore the neutrinoless double beta ($0\nu \beta\beta$) decay induced by an ultralight dark matt...
The presence of light (m_A∼10^(−6) eV) scalar fields in the early universe can modify the cosmology...
We explore a Portalino-like model of dark matter and neutrino masses in which right-handed neutrino ...
Sterile neutrinos can be produced in the early universe via interactions with their active counterpa...
Sterile neutrinos are well-motivated and simple dark matter (DM) candidates. However, sterile neutri...
A sterile neutrino with a keV-scale mass is a compelling dark matter candidate. We propose a new pro...
Sterile neutrinos are one of the leading dark matter candidates. Their masses may originate from a v...
We show that sterile neutrinos with masses larger than 1 eV, as motivated by several short-baseline ...