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相关论文: The Neutrino Mass Window for Baryogenesis

200 篇论文

I review the origin of the lepton asymmetry which is converted to a baryon excess at the electroweak scale. This scenario becomes more attractive if we can relate it to other physical phenomena. For this reason I elaborate on the conditions…

高能物理 - 唯象学 · 物理学 2009-11-07 E. A. Paschos

Neutrino properties can play a crucial role in determining the matter-antimatter asymmetry of the universe if thermal leptogenesis is the correct solution to the baryogenesis problem. Owing to this, the study of neutrino models goes beyond…

高能物理 - 唯象学 · 物理学 2009-01-12 Sandy S. C. Law

The extension of the Standard Model by right handed neutrinos with masses in the GeV range can simultaneously explain the observed neutrino masses via the seesaw mechanism and the baryon asymmetry of the universe via leptogenesis. It has…

高能物理 - 唯象学 · 物理学 2017-01-18 Marco Drewes , Shintaro Eijima

The observed baryon asymmetry of the Universe is suitably created in thermal leptogenesis through the out-of-equilibrium decay of $N_1$, the lightest of the three heavy singlet neutral fermions which anchor the seesaw mechanism to obtain…

高能物理 - 唯象学 · 物理学 2007-05-23 Ernest Ma , Narendra Sahu , Utpal Sarkar

We study a simple extension of the standard model to simultaneously explain neutrino masses, dark matter and the matter-antimatter asymmetry of the Universe. In our model, the baryon asymmetry is achieved by the leptogenesis mechanism,…

高能物理 - 唯象学 · 物理学 2010-03-26 Chuan-Hung Chen , Chao-Qiang Geng , Dmitry V. Zhuridov

We demonstrate that $CP-$violation in the Majorana mass matrices of the heavy neutrinos can generate a $CP-$asymmetric universe. The subsequent decay of the Majorana particles generates a lepton number asymmetry. During the electroweak…

高能物理 - 唯象学 · 物理学 2010-11-01 Marion Flanz , Emmanuel A. Paschos , Utpal Sarkar

We reconsider the GUT-baryogenesis mechanism for generating the baryon asymmetry of the Universe. The baryon asymmetry is produced by the out of equilibrium decay of coloured Higgs bosons at the GUT scale, conserving B-L. If neutrinos are…

高能物理 - 唯象学 · 物理学 2007-05-23 J. A. Lopez-Perez , N. Rius

In this work, we explain three beyond standard model (BSM) phenomena, namely neutrino masses, the baryon asymmetry of the Universe and Dark Matter, within a single model and in each explanation the right handed (RH) neutrinos play the prime…

高能物理 - 唯象学 · 物理学 2019-06-26 Anirban Biswas , Sandhya Choubey , Laura Covi , Sarif Khan

The origin of neutrino masses can be simply attributed to a new scalar beyond the Standard Model. We demonstrate that leptogenesis can explain the baryon asymmetry of the universe already in such a minimal framework, where the electroweak…

高能物理 - 唯象学 · 物理学 2025-08-06 Shinya Kanemura , Shao-Ping Li

The effects of the lightest neutrino mass in ``flavoured'' leptogenesis are investigated in the case when the CP-violation necessary for the generation of the baryon asymmetry of the Universe is due exclusively to the Dirac and/or Majorana…

高能物理 - 唯象学 · 物理学 2008-11-26 E. Molinaro , S. T. Petcov , T. Shindou , Y. Takanishi

We discuss a model of neutrino mass based on the type I seesaw mechanism embedded in a spontaneously broken global lepton number framework with a $Z_2$ symmetry. We show that the resulting Majoron is a viable freeze-in dark matter…

高能物理 - 唯象学 · 物理学 2025-04-28 Stephen F. King , Soumen Kumar Manna , Rishav Roshan , Arunansu Sil

We review the scenario of baryogenesis through leptogenesis induced by the out-of-equilibrium decays of heavy neutrinos. We pay special attention to the resonant phenomenon of CP violation through mixing of two nearly degenerate heavy…

高能物理 - 唯象学 · 物理学 2007-05-23 Apostolos Pilaftsis

It is clear that matter is dominant in the Universe compared to antimatter. We call this problem baryon asymmetry. The baryon asymmetry is experimentally determined by both cosmic microwave background and big bang nucleosynthesis…

高能物理 - 唯象学 · 物理学 2022-05-18 Dong Woo Kang , Jongkuk Kim , Takaaki Nomura , Hiroshi Okada

We propose a novel framework where baryon asymmetry of the universe can arise due to forbidden decay of dark matter (DM) enabled by finite-temperature effects in the vicinity of a first order phase transition (FOPT). In order to implement…

高能物理 - 唯象学 · 物理学 2023-10-13 Debasish Borah , Arnab Dasgupta , Matthew Knauss , Indrajit Saha

We investigate a minimal extension of the Leptogenesis framework that simultaneously explains the observed baryon asymmetry and dark matter (DM) abundance through the decay of a heavy Majorana neutrino. In this scenario, CP violation arises…

高能物理 - 唯象学 · 物理学 2026-04-22 Henry G. F. McKenna , Juri Smirnov , Martin Gorbahn

We consider a dark electroweak phase transition, during which a baryon asymmetry in the dark neutrons and an equal lepton asymmetry in the dark Dirac neutrinos can be simultaneously induced by the CP-violating reflection of the dark…

高能物理 - 唯象学 · 物理学 2017-10-04 Pei-Hong Gu

Baryogenesis appears to require lepton number violation. This is naturally realized in extensions of the standard model containing right-handed neutrinos. We discuss the generation of a baryon asymmetry by the out-of-equilibrium decay of…

高能物理 - 唯象学 · 物理学 2007-05-23 W. Buchmuller , M. Plumacher

We review observational evidence for a matter-antimatter asymmetry in the early universe, which leads to the remnant matter density we observe today. We also discuss observational bounds on the presence of antimatter in the present day…

高能物理 - 唯象学 · 物理学 2012-11-06 Laurent Canetti , Marco Drewes , Mikhail Shaposhnikov

We study a mechanism through which the cosmic dark matter density can be explained simultaneously with the observed baryon asymmetry of the Universe. At the core of our proposal lie the out-of-equilibrium scattering processes of bath…

高能物理 - 唯象学 · 物理学 2022-09-15 Andreas Goudelis , Dimitrios Karamitros , Pantelis Papachristou , Vassilis C. Spanos

We propose a unified explanation for the origin of dark matter and baryon number asymmetry on the basis of a non-supersymmetric model for neutrino masses. Neutrino masses are generated in two distinct ways, that is, a tree-level seesaw…

高能物理 - 唯象学 · 物理学 2008-11-26 Daijiro Suematsu