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相关论文: BBN with Late Electron-Sterile Neutrino Oscillatio…

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In this article we discuss lepton asymmetry effect on BBN with neutrino oscillations. We argue that asymmetry much smaller than 0.01, although not big enough to influence directly the nucleosynthesis kinetics, can effect considerably BBN…

高能物理 - 唯象学 · 物理学 2007-05-23 M. V. Chizhov , D. P. Kirilova

We discuss the interplay between lepton asymmetry L and neutrino oscillations in the early Universe. Neutrino oscillations may suppress or enhance previously existing L. On the other hand L is capable to suppress or enhance neutrino…

宇宙学与河外天体物理 · 物理学 2013-02-14 Daniela Kirilova

Oscillations between ordinary and sterile neutrinos can generate large neutrino asymmetries in the early universe. These asymmetries can significantly affect big bang nucleosynthesis (BBN) through modification of nuclear reaction rates. We…

高能物理 - 唯象学 · 物理学 2011-07-19 N. F. Bell , R. Foot , R. R. Volkas

Ordinary-sterile neutrino oscillations can generate a significant lepton number asymmetry in the early Universe. We study this phenomenon in detail. We show that the dynamics of ordinary-sterile neutrino oscillations in the early Universe…

高能物理 - 唯象学 · 物理学 2011-03-10 R. Foot , R. R. Volkas

The relic cosmic background neutrinos accompanying the cosmic microwave background (CMB) photons may hide a universal lepton asymmetry orders of magnitude larger than the universal baryon asymmetry. At present, the only direct way to probe…

高能物理 - 唯象学 · 物理学 2008-11-26 Vimal Simha , Gary Steigman

Primordial Big-Bang Nucleosynthesis (BBN) tightly constrains the existence of any additional relativistic degrees of freedom at that epoch. However a large asymmetry in electron neutrino number shifts the chemical equilibrium between the…

高能物理 - 唯象学 · 物理学 2009-10-31 J. March-Russell , H. Murayama , A. Riotto

We analyze the effects of lepton asymmetry on neutrino oscillations and on cosmological nucleosynthesis with active-sterile oscillating neutrinos. It is shown that small lepton asymmetries, L < 0.01, whose direct kinetic effect on…

天体物理学 · 物理学 2009-11-06 Daniela Kirilova , Mihail Chizhov

While the cosmic baryon asymmetry has been measured at high accuracy to be 6.1*10^-10, a corresponding lepton asymmetry could be as large as 10^-2 if it hides in the neutrino sector. It has been known for some time that a large asymmetry…

宇宙学与河外天体物理 · 物理学 2013-10-23 Steen Hannestad , Rasmus Sloth Hansen , Thomas Tram

Leptogenesis induced by the oscillations of GeV-scale neutrinos provides a minimal and testable explanation of the baryon asymmetry of the Universe. In this work we extend previous studies invoking only two heavy neutrinos to the case of…

高能物理 - 唯象学 · 物理学 2019-02-05 Asmaa Abada , Giorgio Arcadi , Valerie Domcke , Marco Drewes , Juraj Klaric , Michele Lucente

We propose a resonant leptogenesis scenario in a U(1)_{B-L} gauge extension of the standard model to generate large lepton asymmetries for cosmological baryon asymmetry and dark matter. After B-L number is spontaneously broken, inflaton can…

高能物理 - 唯象学 · 物理学 2010-12-09 Pei-Hong Gu

While the baryon asymmetry of the Universe is nowadays well measured by cosmological observations, the bounds on the lepton asymmetry in the form of neutrinos are still significantly weaker. We place limits on the relic neutrino asymmetries…

We discuss the bounds on the cosmological lepton number from Big Bang Nucleosynthesis (BBN), in light of recent evidences for a large value of the neutrino mixing angle theta13. The largest asymmetries for electron and muon or tau neutrinos…

高能物理 - 唯象学 · 物理学 2012-02-01 Gianpiero Mangano , Gennaro Miele , Sergio Pastor , Ofelia Pisanti , Srdjan Sarikas

The detection of a sterile neutrino could constitute the first observation of a particle that could have been produced before Big-Bang Nucleosynthesis (BBN), and could provide information about the yet untested pre-BBN era. The cosmological…

高能物理 - 唯象学 · 物理学 2020-06-19 Graciela B. Gelmini , Philip Lu , Volodymyr Takhistov

In this work we present the results of our numerical analysis of the effect of lepton asymmetries L on neutrino oscillations and consequently on helium production in a model of cosmological nucleosynthesis with active-sterile neutrino…

高能物理 - 唯象学 · 物理学 2009-10-31 Daniela Kirilova , Mihail Chizhov

Ordinary-sterile neutrino oscillations can generate significant neutrino asymmetry in the early Universe. In this paper we extend this work by computing the evolution of neutrino asymmetries and light element abundances during the Big Bang…

高能物理 - 唯象学 · 物理学 2014-11-17 R. Foot , R. R. Volkas

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

Using a new sample of extremely metal poor systems, the EMPRESS survey has recently reported a primordial helium abundance that is $3\sigma$ smaller than the prediction from the standard big bang nucleosynthesis (BBN) scenario. This…

高能物理 - 唯象学 · 物理学 2023-03-08 Miguel Escudero , Alejandro Ibarra , Victor Maura

Primordial neutrino-antineutrino asymmetries can be constrained through big-bang nucleosynthesis (BBN) relic abundances and cosmic microwave background (CMB) anisotropies, both observables being sensitive to neutrino properties. The latter…

高能物理 - 唯象学 · 物理学 2024-11-28 Julien Froustey , Cyril Pitrou

The generation of lepton asymmetry below the electroweak scale has a considerable impact on production of dark matter sterile neutrinos. Oscillations or decays of the heavier sterile neutrinos in the neutrino minimal standard model can give…

高能物理 - 唯象学 · 物理学 2010-11-09 Ananda Roy , Mikhail Shaposhnikov

Effects of light millicharged dark matter particles on primordial nucleosynthesis are considered. It is shown that if the mass of such particles is much smaller than the electron mass, they lead to strong overproduction of Helium-4. An…

宇宙学与河外天体物理 · 物理学 2015-06-12 Zurab Berezhiani , Aleksander Dolgov , Igor Tkachev
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