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相关论文: Neutrino conversions in hot plasma

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Big Bang Nucleosynthesis imposes stringent bounds on light sterile neutrinos mixing with the active flavors. Here we discuss how altered dispersion relations can weaken such bounds and allow compatibility of new sterile neutrino degrees of…

高能物理 - 唯象学 · 物理学 2016-12-28 Elke Aeikens , Heinrich Päs , Sandip Pakvasa , Thomas J. Weiler

The role of neutrinos in big bang nucleosynthesis is reviewed. Neutrino oscillations in the early universe both in resonance and non-resonance case are briefly discussed. BBN and supernova limits on heavy sterile neutrinos with the mass in…

高能物理 - 唯象学 · 物理学 2007-05-23 A. D. Dolgov

We investigate quantitatively the extent to which having a primordial leptonic asymmetry (n_nu \neq n_nubar) relaxes the bounds on light sterile neutrinos imposed by BBN and LSS. We adopt a few assumptions that allow us to solve the…

天体物理学 · 物理学 2008-11-26 Yi-Zen Chu , Marco Cirelli

We consider active-sterile neutrino conversions in a supernova in the presence of random magnetic field domains. For large enough fields the magnetization of the medium may enhance the active to sterile neutrino conversion rates. Neglecting…

高能物理 - 唯象学 · 物理学 2009-09-25 V. Semikoz , J. W. F. Valle

We reanalyze the effect of magnetic fields in BBN, incorporating several features which were omitted in previous analyses. We find that the effects of coherent magnetic fields on the weak interaction rates and the electron thermodynamic…

天体物理学 · 物理学 2014-10-13 Peter. J. Kernan , Glenn D. Starkman , Tammay Vachaspati

We investigate how sterile neutrinos with a range of masses influence cosmology in MeV-scale reheating temperature scenarios. By computing the production of sterile neutrinos through the combination of mixing and scattering in the early…

高能物理 - 唯象学 · 物理学 2020-08-13 Takuya Hasegawa , Nagisa Hiroshima , Kazunori Kohri , Rasmus S. L. Hansen , Thomas Tram , Steen Hannestad

Assuming that there exists a species of heavy sterile neutrinos($m_{\nu}>1$ keV) and their decays can serve as a heating source of the hot gas in galaxy clusters, we study how the observational constraints on cooling flow limit the mass of…

天体物理学 · 物理学 2010-11-11 M. H. Chan , M. -C. Chu

Local Universe observations find a value of the Hubble constant $H_0$ that is larger than the value inferred from the Cosmic Microwave Background and other early Universe measurements, assuming known physics and the $\Lambda$CDM…

宇宙学与河外天体物理 · 物理学 2021-06-10 Graciela B. Gelmini , Alexander Kusenko , Volodymyr Takhistov

Neutrinos with a magnetic moment $\mu$ change their helicity when interacting with an electromagnetic field. Various aspects of this effect have been described as spin precession, spin-flip scattering, and magnetic Cherenkov radiation.…

高能物理 - 唯象学 · 物理学 2008-11-26 Per Elmfors , Kari Enqvist , Georg Raffelt , Günter Sigl

The helicity evolution of a neutrino interacting with randomly moving and polarized matter is studied. We derive the equation for the averaged neutrino helicity. The type of the neutrino interaction with background fermions is not fixed. In…

高能物理 - 唯象学 · 物理学 2008-07-31 Maxim Dvornikov

We study the dynamics of the early universe in massive conformal gravity. In particular, we show that the theory is consistent with the observed values of the primordial abundances of light elements if we consider the existence of…

综合物理 · 物理学 2023-02-15 F. F. Faria

Neutrino masses and quantum gravity are strong reasons to extend the standard model of particle physics. A large extra dimension can be motivated by quantum gravity and can explain the small neutrino masses with new singlet states that…

高能物理 - 唯象学 · 物理学 2024-10-08 David McKeen , John Ng , Michael Shamma

We discuss how a laboratory detection of a sterile neutrino not only would constitute a fundamental discovery of a new particle, but could also provide an indication of the evolution of the Universe before Big-Bang Nucleosynthesis (BBN), a…

高能物理 - 唯象学 · 物理学 2019-12-19 Graciela B. Gelmini , Philip Lu , Volodymyr Takhistov

Several long-standing anomalies from short-baseline neutrino oscillation experiments -- most recently corroborated by new data from MiniBooNE -- have led to the hypothesis that extra, 'sterile', neutrino species might exist. Models of this…

高能物理 - 唯象学 · 物理学 2022-12-06 Xiaoyong Chu , Basudeb Dasgupta , Mona Dentler , Joachim Kopp , Ninetta Saviano

Sterile neutrinos, fermions with no standard model couplings [SU(2) singlets], are predicted by most extensions of the standard model, and may be the dark matter. I describe the nonthermal production and linear perturbation evolution in the…

天体物理学 · 物理学 2008-11-26 Kevork Abazajian

Lepton asymmetry generated in the early universe by neutrino oscillations into sterile partners is calculated. Kinetic equations are analytically reduced to a simple form that permits an easy numerical treatment. Asymptotic values of the…

高能物理 - 唯象学 · 物理学 2009-11-07 A. D. Dolgov

Recent experiment proposed to observe induced radiative neutrino transitions are confronted to existing bounds on neutrino magnetic moments from earth-based experiments. These are found to exclude any observation by several orders of…

高能物理 - 唯象学 · 物理学 2016-08-15 J. -M. Frère , R. B. Nevzorov , M. I. Vysotsky

The study of sterile neutrinos has recently acquired a different flavor: being now excluded as the dominant solution for the solar or atmospheric conversions, sterile neutrinos, still attractive for many other reasons, have thus become even…

天体物理学 · 物理学 2007-05-23 Marco Cirelli

We solve the problem of coherent Mikheyev-Smirnov-Wolfenstein (MSW) resonant active-to-sterile neutrino flavor conversion driven by an initial lepton number in the early universe. We find incomplete destruction of lepton number in this…

天体物理学 · 物理学 2007-05-23 Chad T. Kishimoto , George M. Fuller , Christel J. Smith

Distortion of the equilibrium spectra of cosmic neutrinos due to interaction with hotter electrons and positrons in the primeval cosmic plasma is considered. The set of integro-differential kinetic equations for neutrinos is accurately…

高能物理 - 唯象学 · 物理学 2009-10-30 A. D. Dolgov , S. H. Hansen , D. V. Semikoz