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We consider the cosmological effects of sterile neutrinos with the masses of $150- 450$ MeV. The decay of sterile neutrinos changes the thermal history of the Universe and affects the energy density of radiation at the recombination and the…

高能物理 - 唯象学 · 物理学 2020-10-13 Graciela B. Gelmini , Masahiro Kawasaki , Alexander Kusenko , Kai Murai , Volodymyr Takhistov

Theories with large extra dimensions may be tested using sterile neutrinos living in the bulk. A bulk neutrino can mix with a flavor neutrino localized in the brane leading to unconventional patterns of neutrino oscillations. A resonance…

高能物理 - 唯象学 · 物理学 2016-11-27 A. Nicolaidis

Tantalizing cosmological and terrestrial evidence suggests the number of light neutrinos may be greater than 3, motivating a careful re-examination of cosmological bounds on extra light species. Big Bang Nucleosynthesis constrains the…

宇宙学与河外天体物理 · 物理学 2013-04-24 Thomas D. Jacques , Lawrence M. Krauss , Cecilia Lunardini

The existence of bulk sterile neutrinos in theories with large extra dimensions can naturally explain small 4-dimensional Dirac masses for the active neutrinos. We study a model with 3 bulk neutrinos and derive various constraints on the…

高能物理 - 唯象学 · 物理学 2014-11-17 H. Davoudiasl , P. Langacker , M. Perelstein

We discuss in detail the effect of neutrino oscillations in Big Bang nucleosynthesis, between active and sterile neutrinos, as well as between active and active neutrinos. We calculate the constraints on mixings between active and sterile…

天体物理学 · 物理学 2009-10-22 X. Shi , D. N. Schramm , B. D. Fields

Cosmological and astrophysical effects of heavy (10 - 200 MeV) sterile Dirac neutrinos, mixed with the active ones, are considered. The bounds on mass and mixing angle from both supernovae and big-bang nucleosynthesis are presented.

高能物理 - 唯象学 · 物理学 2009-10-31 A. D. Dolgov , S. H. Hansen , G. Raffelt , D. V. Semikoz

We discuss the possibility of sterile neutrinos taking shortcuts in extra dimensions, and the consequences for neutrino oscillations. This effect influences the active-sterile neutrino mixing and provides a possibility to accommodate the…

高能物理 - 唯象学 · 物理学 2008-11-26 Heinrich Päs , Sandip Pakvasa , Thomas J. Weiler

Short-baseline neutrino anomalies suggest the existence of low-mass ( m \sim O(1)~eV) sterile neutrinos \nu_s. These would be efficiently produced in the early universe by oscillations with active neutrino species, leading to a thermal…

宇宙学与河外天体物理 · 物理学 2014-12-24 Ninetta Saviano , Ofelia Pisanti , Gianpiero Mangano , Alessandro Mirizzi

We study the effects of kination and scalar-tensor pre-Big Bang Nucleosynthesis cosmologies on the non-resonant production of sterile neutrinos. We show that if the peak of the production rate of sterile neutrinos occurs during the…

高能物理 - 唯象学 · 物理学 2015-06-18 Thomas Rehagen , Graciela B. Gelmini

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

We re-examine the big bang nucleosynthesis (BBN) bounds on the mixing of neutrinos with sterile species. These bounds depend on the assumption that the relic neutrino asymmetry $L_{\nu}$ is very small. We show that for $L_{\nu}$ large…

高能物理 - 唯象学 · 物理学 2009-10-28 R. Foot , R. R. Volkas

We employ state-of-the art cosmological observables including supernova surveys and BAO information to provide constraints on the mass and mixing angle of a non-resonantly produced sterile neutrino species, showing that cosmology can…

宇宙学与河外天体物理 · 物理学 2015-07-10 Aaron C. Vincent , Enrique Fernandez Martinez , Pilar Hernandez , Massimiliano Lattanzi , Olga Mena

In extra-dimensional scenarios oscillations between active and sterile neutrinos can be governed by a new resonance in the oscillation amplitude. This resonance results when cancelation occurs between two phase differences, the usual…

高能物理 - 唯象学 · 物理学 2015-05-13 Sebastian Hollenberg , Octavian Micu , Heinrich Päs , Thomas J. Weiler

We discuss a possible new resonance in active-sterile neutrino oscillations arising in theories with large extra dimensions. Fluctuations in the brane effectively increase the path-length of active neutrinos relative to the path-length of…

高能物理 - 唯象学 · 物理学 2009-11-11 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 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

We examine the constraints imposed by the requirement of successful big bang nucleosynthesis on models with one large extra dimension and a single bulk neutrino. We solve the Boltzman kinetic equations for the thermal distribution of bulk…

高能物理 - 唯象学 · 物理学 2009-11-07 H. S. Goh , R. N. Mohapatra

We discuss causality properties of extra-dimensional theories allowing for effectively superluminal bulk shortcuts. Such shortcuts for sterile neutrinos have been discussed as a solution to the puzzling LSND and MiniBooNE neutrino…

高能物理 - 唯象学 · 物理学 2007-12-09 James Dent , Heinrich Päs , Sandip Pakvasa , Thomas J. Weiler

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 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…

高能物理 - 唯象学 · 物理学 2022-02-24 L. Mastrototaro
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