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相关论文: Cosmology Based on f(R) Gravity Admits 1 eV Steril…

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We address the cosmological role of an additional ${\cal O}(1)$ eV sterile neutrino in modified gravity models. We confront the present cosmological data with predictions of the FLRW cosmological model based on a variant of $f(R)$ modified…

宇宙学与河外天体物理 · 物理学 2015-05-14 A. S. Chudaykin , D. S. Gorbunov , A. A. Starobinsky , R. A. Burenin

There are hints, both from cosmology and from neutrino oscillation experiments, that one or two sterile neutrinos with eV masses are favored. We consider the implications of combining data from short baseline neutrino experiments with…

宇宙学与河外天体物理 · 物理学 2013-03-20 Jostein R. Kristiansen , Øystein Elgarøy , Carlo Giunti , Marco Laveder

We show that sterile neutrinos with masses ~1 eV or larger, as motivated by several short-baseline oscillation anomalies, can be consistent with cosmological constraints if they are charged under a hidden sector force mediated by a light…

高能物理 - 唯象学 · 物理学 2014-06-16 Basudeb Dasgupta , Joachim Kopp

We find that the viability of a cosmological model that incorporates 2 sterile neutrinos with masses around 1 eV each, as favored by global neutrino oscillation analyses including short baseline results, is significantly dependent on the…

宇宙学与河外天体物理 · 物理学 2013-03-13 Shahab Joudaki , Kevork N. Abazajian , Manoj Kaplinghat

We introduce a cosmological invisible decay of the sterile neutrino with the eV-scale mass indicated by short-baseline neutrino oscillation experiments in order to allow its full thermalization in the early Universe. We show that the fit of…

宇宙学与河外天体物理 · 物理学 2014-06-12 S. Gariazzo , C. Giunti , M. Laveder

Light sterile neutrinos with a mass around 1 eV have been studied for many years as a possible explanation of the so called short-baseline neutrino oscillation anomalies. Recently, several neutrino oscillation experiments reported…

高能物理 - 唯象学 · 物理学 2020-02-19 S. Gariazzo

We study cosmological models that contain sterile neutrinos with eV-range masses as suggested by reactor and short-baseline oscillation data. We confront these models with both precision cosmological data (probing the CMB decoupling epoch)…

宇宙学与河外天体物理 · 物理学 2015-02-02 Jan Hamann , Steen Hannestad , Georg G. Raffelt , Yvonne Y. Y. Wong

Tensions between several cosmic observations were found recently, such as the inconsistent values of $H_{0}$ (or $\sigma_{8}$) were indicated by the different cosmic observations. Introducing the massive neutrinos in $\Lambda$CDM could…

宇宙学与河外天体物理 · 物理学 2017-01-04 Jianbo Lu , Molin Liu , Yabo Wu , Yan Wang , Weiqiang Yang

Cosmology and short baseline neutrino oscillation data both hint at the existence of light sterile neutrinos with masses in the 1 eV range. Here we perform a detailed analysis of the sterile neutrino scenario using both cosmological and SBL…

宇宙学与河外天体物理 · 物理学 2015-06-15 Maria Archidiacono , Nicolao Fornengo , Carlo Giunti , Steen Hannestad , Alessandro Melchiorri

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…

高能物理 - 唯象学 · 物理学 2022-05-17 Stefan Sandner

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…

宇宙学与河外天体物理 · 物理学 2020-12-18 Maria Archidiacono , Stefano Gariazzo , Carlo Giunti , Steen Hannestad , Thomas Tram

The exponential $f(R)$ gravity model provides a theoretically well-motivated extension of General Relativity, introducing a modified gravitational dynamics at late times consistent with a dynamical dark energy scenario, while recovering the…

广义相对论与量子宇宙学 · 物理学 2025-11-11 Simone D'Onofrio , Sergei Odintsov , Tiziano Schiavone

If all three neutrino oscillation data were to be confirmed in the near future, it is probable that one might need a sterile neutrino, in addition to the three active ones. This sterile neutrino, nu_S, would be very light with mass m_{nu_S}…

高能物理 - 唯象学 · 物理学 2007-05-23 P. Q. Hung

Neutrino masses are usually described by adding to the Standard Model some SU(2)-singlet fermions that have the Yukawa couplings, as well as some Majorana mass terms. The number of such fields and the scales of their Majorana masses are not…

高能物理 - 唯象学 · 物理学 2009-11-13 Alexander Kusenko

A sterile neutrino with mass in the eV range, mixing with the electron antineutrino, is allowed and possibly even preferred by cosmology and oscillation experiments. If such eV-mass neutrinos exist they provide a much better target for…

宇宙学与河外天体物理 · 物理学 2011-03-18 Anna Sejersen Riis , Steen Hannestad

We analyze the most recent cosmological data, including Planck, taking into account the possible existence of a sterile neutrino with a mass at the eV scale indicated by short-baseline neutrino oscillations data in the 3+1 framework. We…

高能物理 - 唯象学 · 物理学 2015-06-17 S. Gariazzo , C. Giunti , M. Laveder

There is a renewed interest in constraining the sum of the masses of the three neutrino flavours by using cosmological measurements. Solar, atmospheric, and reactor neutrino experiments have confirmed neutrino oscillations, implying that…

高能物理 - 唯象学 · 物理学 2008-11-26 Oystein Elgaroy , Ofer Lahav

Although the MiniBooNE experiment has severely restricted the possible existence of light sterile neutrinos, a few anomalies persist in oscillation data, and the possibility of extra light species contributing as a subdominant hot (or warm)…

天体物理学 · 物理学 2010-04-23 Mario A. Acero , Julien Lesgourgues

Cosmology cannot rule out the solution nu_mu <-> nu_s to the atmospheric neutrino data and thus only Earth experiments will be able to give a definitive answer. This conclusion holds when a generation of lepton number is taken into account…

高能物理 - 唯象学 · 物理学 2016-11-03 P. Di Bari

We constrain the neutrino properties in $f(R)$ gravity using the latest observations from cosmic microwave background(CMB) and baryon acoustic oscillation(BAO) measurements. We first constrain separately the total mass of neutrinos $\sum…

宇宙学与河外天体物理 · 物理学 2014-02-25 Jian-hua He
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