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I discuss BBN with nonequilibrium nu_e<->nu_s oscillations in the more general case of non-zero population of nu_s before oscillations delta N_s>0. I calculate He-4 primordial production Y_p(delta N_s) in the presence of nu_e<->nu_s…

Astrophysics · Physics 2008-11-26 Daniela P. Kirilova

The maximum overproduction of helium-4 in cosmological nucleosynthesis with active--sterile neutrino oscillations, nu_e -> nu_s, efficient after decoupling of electron neutrino, is analyzed. The kinetic effects on primordial nucleosynthesis…

Astrophysics · Physics 2014-07-08 D. P. Kirilova

We study the nonresonant oscillations between left-handed electron neutrinos nu_e and nonthermalized sterile neutrinos nu_s in the early Universe plasma. The case when nu_s do not thermalize till 2 MeV and the oscillations become effective…

High Energy Physics - Phenomenology · Physics 2011-02-24 D. P. Kirilova , M. V. Chizhov

We present a review of cosmological nucleosynthesis (CN) with neutrino oscillations, discussing the different effects of oscillations on CN, namely: increase of the effective degrees of freedom during CN, spectrum distortion of the…

Astrophysics · Physics 2007-05-23 Daniela Kirilova , Mihail Chizhov

We have provided a numerical study of the influence of the resonant active-sterile neutrino oscillations between electron and sterile neutrinos, on the primordial production of helium-4. The evolution of the neutrino ensembles was followed…

High Energy Physics - Phenomenology · Physics 2009-10-31 D. P. Kirilova , M. V. Chizhov

We study the distortion of electron neutrino energy spectrum due to oscillations with the sterile neutrino nu_e <-> nu_s, for different initial populations of the sterile state delta N_s at the onset of oscillations. The influence of this…

High Energy Physics - Phenomenology · Physics 2014-11-17 Daniela Kirilova

Phenomenology of neutrino oscillations in vacuum and in cosmological plasma is considered. Neutrino oscillations in vacuum are usually described in plane wave approximation. In this formalism there is an ambiguity if one should assume…

High Energy Physics - Phenomenology · Physics 2007-05-23 A. D. Dolgov

We discuss the oscillations effects on neutrinos in the early Universe and update the cosmological constraints on the oscillation parameters. It is shown that sterile LOW solution to the solar neutrino problem is almost completely excluded…

High Energy Physics - Phenomenology · Physics 2009-11-07 D. Kirilova , M. Chizhov

We studied nonequilibrium oscillations between left-handed electron neutrinos and nonthermalized sterile neutrinos in medium for resonant and nonresonant cases. The exact kinetic equations for neutrinos, written in terms of neutrino density…

High Energy Physics - Phenomenology · Physics 2009-10-28 D. P. Kirilova , M. V. Chizhov

Several anomalies in neutrino oscillation experiments point to the existence of a $\sim 1\,$eV sterile neutrino $\nu_s$ mixing with $\nu_e$ at the level of $U_{e4}\cong 0.1$, but such a neutrino is strongly disfavored by constraints on…

High Energy Physics - Phenomenology · Physics 2020-01-15 James M. Cline

We analyze the oscillation signals generated by one extra sterile neutrino. We fully take into account the effects of the established oscillations among active neutrinos. We analyze the effects in solar, atmospheric, reactor and beam…

High Energy Physics - Phenomenology · Physics 2007-05-23 Guido Marandella

Sterile neutrinos with a mass in the eV range have been invoked as a possible explanation of a variety of short baseline (SBL) neutrino oscillation anomalies. However, if one considers neutrino oscillations between active and sterile…

Cosmology and Nongalactic Astrophysics · Physics 2020-12-18 Maria Archidiacono , Stefano Gariazzo , Carlo Giunti , Steen Hannestad , Thomas Tram

We consider heavy sterile neutrinos $\nu_s$, with mass in the range 10 MeV $\lesssim m_s \lesssim m_{\pi} \sim 135$ MeV, thermally produced in the early universe and freezing out after the QCD phase transition. The existence of these…

High Energy Physics - Phenomenology · Physics 2022-02-24 L. Mastrototaro

We provide a consistent framework to set limits on properties of light sterile neutrinos coupled to all three active neutrinos using a combination of the latest cosmological data and terrestrial measurements from oscillations, $\beta$-decay…

The light neutrino masses are at present most stringently constraint via cosmological probes. In particular the Planck collaboration reports $ \sum m_\nu \leq 0.12\,\mathrm{eV}$ at $95\%$ CL within the standard cosmological model. This is…

High Energy Physics - Phenomenology · Physics 2022-05-17 Stefan Sandner

We perform a thorough analysis of oscillation signals generated by one extra sterile neutrino, extending previous analyses done in simple limiting cases and including the effects of established oscillations among active neutrinos. We…

High Energy Physics - Phenomenology · Physics 2008-11-26 Marco Cirelli , Guido Marandella , Alessandro Strumia , Francesco Vissani

We present a short discussion of the Neutrino-4 experimental results and the results of other experiments searching for the sterile neutrino. We estimated the contribution of the sterile neutrino with parameters $\Delta m^2_{14} =…

High Energy Physics - Phenomenology · Physics 2023-02-15 A. P. Serebrov , R. M. Samoilov , M. E. Chaikovskii , O. M. Zherebtsov

We investigate cosmological bounds on sterile neutrino masses in the light of the Hubble and $S_8$ tensions. We argue that non-zero masses for sterile neutrinos are inferred at 2$\sigma$ level in some extended models such as varying dark…

Cosmology and Nongalactic Astrophysics · Physics 2024-10-24 Supriya Pan , Osamu Seto , Tomo Takahashi , Yo Toda

Cosmological measurements are affected by the energy density of both active and sterile massive neutrinos. We extend here a recent analysis of current cosmological data to non minimal cosmologies. Several possible scenarios are examined: a…

Cosmology and Nongalactic Astrophysics · Physics 2013-05-30 Elena Giusarma , Maria Archidiacono , Roland de Putter , Alessandro Melchiorri , Olga Mena

We consider relatively heavy neutrinos $\nu_H$, mostly contributing to a sterile state $\nu_s$, with mass in the range 10 MeV $\lesssim m_s \lesssim m_{\pi} \sim 135$ MeV, which are thermally produced in the early universe in collisional…

High Energy Physics - Phenomenology · Physics 2021-08-03 Leonardo Mastrototaro , Pasquale Dario Serpico , Alessandro Mirizzi , Ninetta Saviano
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