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相关论文: The Neutrino Mass Window for Baryogenesis

200 篇论文

The baryon asymmetry of the universe can be explained by the out-of-equilibrium decays of heavy right-handed neutrinos. We analyse this mechanism in the framework of a supersymmetric extension of the Standard Model and show that lepton…

高能物理 - 唯象学 · 物理学 2016-09-06 M. Plumacher

In this work, we classify all the effective $U(1)$ symmetries and their associated Noether charges in the Standard Model (SM) and its minimal supersymmetric extension (MSSM) from the highest scale after inflation down to the weak scale. We…

高能物理 - 唯象学 · 物理学 2021-08-26 Chee Sheng Fong

We present a simple mechanism which allows the simultaneous generation of the baryon asymmetry of the Universe along with its dark matter content. To this goal, we employ the out-of-equilibrium decays of heavy bath states into a feebly…

高能物理 - 唯象学 · 物理学 2022-02-17 Andreas Goudelis , Pantelis Papachristou , Vassilis C. Spanos

Leptogenesis can successfully explain the matter-antimatter asymmetry via out-of-equilibrium decays of heavy Majorana neutrinos in the early Universe. In this article, we focus on non-resonant thermal leptogenesis and the possibility of…

高能物理 - 唯象学 · 物理学 2018-09-06 K. Moffat , S. Pascoli , S. T. Petcov , H. Schulz , J. Turner

We calculate the baryonic asymmetry of the universe in the baryogenesis-via-leptogenesis framework, assuming first a quark-lepton symmetry and then a charged-neutral lepton symmetry. We match the results with the experimentally favoured…

高能物理 - 唯象学 · 物理学 2009-10-31 D. Falcone , F. Tramontano

We study a set of textures giving rise to correct masses and mixings of the charged fermions in the context of leptogenesis. The Dirac neutrino texture pattern is assumed to be identical with the up quark texture. The heavy Majonana…

高能物理 - 唯象学 · 物理学 2011-07-19 Micheal S. Berger , Biswajoy Brahmachari

We study the possibility of generating tiny Dirac neutrino masses at one loop level through the \textit{scotogenic} mechanism such that one of the particles going inside the loop can be a stable cold dark matter (DM) candidate. Majorana…

高能物理 - 唯象学 · 物理学 2016-12-28 Debasish Borah , Arnab Dasgupta

The Standard Model of particle physics fails to explain the important pieces in the standard cosmology, such as inflation, baryogenesis, and dark matter of the Universe. We consider the possibility that the sector to generate small neutrino…

高能物理 - 唯象学 · 物理学 2015-06-19 Tetsutaro Higaki , Ryuichiro Kitano , Ryosuke Sato

We study in detail the mechanism of baryon and lepton asymmetry generation in the framework of the $\nu$MSM (an extension of the Standard Model by three singlet fermions with masses smaller than the electroweak scale). We elucidate the…

高能物理 - 唯象学 · 物理学 2008-11-26 Mikhail Shaposhnikov

It is quite possible that the reheat temperature of the universe is extremely low close to the scale of Big Bang nucleosynthesis, i.e. $T_{R}\sim 1-10$ MeV. At such low reheat temperatures generating matter anti-matter asymmetry and…

高能物理 - 唯象学 · 物理学 2009-11-10 Kazunori Kohri , Anupam Mazumdar , Narendra Sahu

We propose a model with an $U(1)_{B-L}$ gauge symmetry, in which small neutrino masses, dark matter and the matter-antimatter asymmetry in the Universe can be simultaneously explained. In particular, the neutrino masses are generated…

高能物理 - 唯象学 · 物理学 2018-02-19 Chao-Qiang Geng , Hiroshi Okada

In the last years we have learnt a lot about neutrino masses and mixings. Neutrinos are not all massless but their masses are very small. Probably masses are small because neutrinos are Majorana particles with masses inversely proportional…

高能物理 - 唯象学 · 物理学 2011-11-29 Guido Altarelli

We work out the thermodynamic equations for the decays and scatterings of heavy Majorana neutrinos including the constraints from unitarity. The Boltzmann equations depend on the CP asymmetry parameter which contains both, a self-energy and…

高能物理 - 唯象学 · 物理学 2009-10-31 Marion Flanz , Emmanuel A. Paschos

In models for thermal baryogenesis from particle decays, the mass of the decaying particle is typically many orders of magnitude above the TeV scale. We will discuss different ways to lower the energy scale of baryogenesis and present the…

高能物理 - 唯象学 · 物理学 2015-06-16 J. Racker

Radiative neutrino mass models have interesting features, which make it possible to relate neutrino masses to the existence of dark matter. However, the explanation of the baryon number asymmetry in the universe seems to be generally…

高能物理 - 唯象学 · 物理学 2015-03-17 H. Higashi , T. Ishima , D. Suematsu

We developed a previous model fitting all quark and lepton -- including neutrino quantities in the region of the Large Mixing Angle-MSW solar solution -- order of magnitudewise by only six adjustable parameters (Higgs vacuum expectation…

高能物理 - 唯象学 · 物理学 2015-06-25 H. B. Nielsen , Y. Takanishi

We have studied the scenario of baryogenesis via leptogenesis in an $A_4$ flavor symmetric framework considering type I seesaw as the origin of neutrino mass. Because of the presence of the fifth generation right handed neutrino the model…

高能物理 - 唯象学 · 物理学 2018-03-23 Ananya Mukherjee , Mrinal Kumar Das , Jayanta Kumar Sarma

A brief review is given of some recent works where baryogenesis and dark matter have a common origin within the $U(1)$ extensions of the standard model and of the minimal supersymmetric standard model. The models considered generate the…

高能物理 - 唯象学 · 物理学 2017-05-31 Wan-Zhe Feng , Pran Nath

We consider theories in which the generation of neutrino masses is associated with the breaking of an approximate global lepton number symmetry. In such a scenario the spectrum of light states includes the Majoron, the pseudo-Nambu…

高能物理 - 唯象学 · 物理学 2019-08-07 Zackaria Chacko , Peizhi Du , Michael Geller

In these lectures I examine some of the principal issues in cosmology from a particle physics point of view. I begin with nucleosynthesis and show how the primordial abundance of the light elements can help fix the number of (light)…

高能物理 - 唯象学 · 物理学 2007-05-23 R. D. Peccei