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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

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

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

The lepton asymmetry that could be generated in the early universe through oscillations of active to sterile neutrinos is calculated (almost) analytically for small mixing angles, sin 2\theta < 10^{-2}. It is shown that for a mass squared…

高能物理 - 唯象学 · 物理学 2011-05-23 A. D. Dolgov , S. H. Hansen , S. Pastor , D. V. Semikoz

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…

高能物理 - 唯象学 · 物理学 2011-02-24 D. P. Kirilova , M. V. Chizhov

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

A large lepton asymmetry could be generated in the Early Universe by oscillations of active to sterile neutrinos with a small mixing angle sin 2 \theta < 10^-2. The final order of magnitude of the lepton asymmetry \eta is mainly determined…

高能物理 - 唯象学 · 物理学 2009-10-31 R. Buras , D. V. Semikoz

Light sterile neutrinos mixing with the active ones have been recently proposed to solve different anomalies observed in short-baseline oscillation experiments. These neutrinos can also be produced by oscillations of the active neutrinos in…

高能物理 - 唯象学 · 物理学 2013-05-30 Alessandro Mirizzi , Ninetta Saviano , Gennaro Miele , Pasquale Dario Serpico

We consider active-sterile neutrino oscillations in the early universe in an inhomogeneous isocurvature background. We show that very small initial baryonic seed-inhomogeneities can trigger a growth of very large amplitude spatial…

高能物理 - 唯象学 · 物理学 2009-10-31 Kari Enqvist , Kimmo Kainulainen , Antti Sorri

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…

高能物理 - 唯象学 · 物理学 2009-10-31 D. P. Kirilova , M. V. 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

We review the consequences of neutrino mixing in the early universe. For both active-sterile mixing or mixing between three active neutrinos only, the consequences of oscillations depend crucially upon the size of the universe's lepton…

高能物理 - 唯象学 · 物理学 2014-11-17 Nicole F. Bell

We consider some consequences of the presence of a cosmological lepton asymmetry in the form of neutrinos. Relic neutrino degeneracy enhances the contribution of massive neutrinos to the present energy density of the Universe, and modifies…

高能物理 - 唯象学 · 物理学 2016-08-25 Julien Lesgourgues , Sergio Pastor

The primordial neutrino asymmetry leaves profound imprints on the evolution history of the universe, which can be constrained by cosmological observations, including Big Bang Nucleosynthesis (BBN), Cosmic Microwave Background (CMB), and…

高能物理 - 唯象学 · 物理学 2025-09-05 Yuan-Zhen Li , Jiang-Hao Yu

Effects of neutrino free streaming is evaluated on the primordial spectrum of gravitational radiation taking both neutrino chemical potential and masses into account. The former or the lepton asymmetry induces two competitive effects,…

高能物理 - 唯象学 · 物理学 2008-11-26 Kiyotomo Ichiki , Masahide Yamaguchi , Jun'Ichi Yokoyama

It has been proposed that an asymmetry in the electron neutrino sector may be generated by resonant active-sterile neutrino transformations during Big Bang Nucleosynthesis (BBN). We calculate the change in the primordial $^4$He yield $Y$…

天体物理学 · 物理学 2009-10-31 Xiangdong Shi , George M. Fuller , Kevork Abazajian

We calculate Boltzmann neutrino energy transport with self-consistently coupled nuclear reactions through the weak-decoupling-nucleosynthesis epoch in an early universe with significant lepton numbers. We find that the presence of lepton…

宇宙学与河外天体物理 · 物理学 2017-03-08 E. Grohs , George M. Fuller , C. T. Kishimoto , Mark W. Paris

We examine the sterile neutrino dark matter production in the primordial plasma with lepton asymmetry unequally distributed over different neutrino flavors. We argue that with the specific flavor fractions, one can mitigate limits from the…

高能物理 - 唯象学 · 物理学 2025-07-29 Dmitry Gorbunov , Dmitry Kalashnikov , George Krugan

A large neutrino asymmetry is an interesting possibility for cosmology, which can have significant observable consequences for nucleosynthesis and the cosmic microwave background. However, although it is a possibility, there is no obvious…

高能物理 - 唯象学 · 物理学 2009-10-31 John McDonald
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