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In this work we study a classically scale invariant extension of the Standard Model that can explain simultaneously dark matter and the baryon asymmetry in the universe. In our set-up we introduce a dark sector, namely a non-Abelian SU(2)…

高能物理 - 唯象学 · 物理学 2016-11-23 Valentin V. Khoze , Alexis D. Plascencia

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

We propose an extension of the standard model (SM) by including a dark sector comprising of three generations of heavy right-handed neutrinos, a singlet scalar and a singlet Dirac fermion, where the latter two particles are stable and are…

高能物理 - 唯象学 · 物理学 2020-01-07 Nimmala Narendra , Sudhanwa Patra , Narendra Sahu , Sujay Shil

We construct two anomaly-free supersymmetric $U(1)'$ models with a secluded $U(1)'$-breaking sector. For the one with $E_6$ embedding we show that there exists a strong enough first order electroweak phase transition for electroweak…

高能物理 - 唯象学 · 物理学 2011-04-28 Junhai Kang , Paul Langacker , Tianjun Li , Tao Liu

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

The extension of the Standard Model by heavy right-handed neutrinos can simultaneously explain the observed neutrino masses via the seesaw mechanism and the baryon asymmetry of the Universe via leptogenesis. If the mass of the heavy…

高能物理 - 唯象学 · 物理学 2020-07-10 Marco Drewes , Bjorn Garbrecht , Dario Gueter , Juraj Klaric

Considering $Z_4$ symmetry in Type I seesaw scenario, one could obtain mass-squared differences of light neutrinos, mixings and $CP$ violating phase within $3 \sigma$ confidence level based on neutrino oscillation data. This is possible…

高能物理 - 唯象学 · 物理学 2026-04-07 Kunal Pandey , Rathin Adhikari

The generation of the right amount of baryon asymmetry $\eta$ of the Universe from supersymmetric leptogenesis is studied within the type-I seesaw framework with three heavy singlet Majorana neutrinos $N_i\,\,(i = 1,2,3)$ and their…

高能物理 - 唯象学 · 物理学 2011-01-28 Biswajit Adhikary , Ambar Ghosal , Probir Roy

By extending the minimal scotogenic model with a spontaneously broken global symmetry $U(1)'$ and a preserved $\mathbb{Z}_2$ symmetry, we build a seesaw model for generating neutrino masses at three-loop level. The new particles have masses…

We investigate the electroweak phase transition patterns for a recently proposed baryogenesis model with CP violation originated in the dark sector. The model includes a complex scalar singlet-Higgs boson portal, a $U(1)_l$ gauge lepton…

高能物理 - 唯象学 · 物理学 2023-03-22 Marcela Carena , Ying-Ying Li , Tong Ou , Yikun Wang

We argue that the creation of a baryon asymmetry in the early universe is an intriguing case where several aspects of ``Beyond'' physics are needed. We then concentrate on baryogenesis in a strong first-order phase transition and discuss…

高能物理 - 唯象学 · 物理学 2014-11-17 Michael G. Schmidt

We propose a class of models providing an explanation of the origin of light neutrino masses, the baryon asymmetry of the Universe via leptogenesis and offering viable dark matter candidates. In these models the Majorana masses of the…

高能物理 - 唯象学 · 物理学 2024-04-11 Asmaa Abada , Nicolás Bernal , Antonio E. Cárcamo Hernández , Sergey Kovalenko , Téssio B. de Melo

We discuss a model which would explain neutrino oscillation, dark matter, and baryon asymmetry of the Universe simultaneously by the physics at TeV scales. Tiny neutrino masses are generated at the three loop level due to the exact $Z_2$…

高能物理 - 唯象学 · 物理学 2009-01-08 Mayumi Aoki , Shinya Kanemura , Osamu Seto

We propose a minimal model based on lepton number symmetry (and violation), to address a common origin of baryon asymmetry, dark matter and neutrino mass generation. The model consists of a vector like fermion to constitute the dark sector,…

高能物理 - 唯象学 · 物理学 2022-10-12 Subhaditya Bhattacharya , Rishav Roshan , Arunansu Sil , Drona Vatsyayan

A mechanism is presented, in which the mixing of right handed heavy Majorana neutrinos creates a $CP-$asymmetric universe. When these Majorana neutrinos subsequently decay more leptons than anti-leptons are produced. The lepton asymmetry…

高能物理 - 唯象学 · 物理学 2009-10-28 Marion Flanz , Emmanuel A. Paschos , Utpal Sarkar , Jan Weiss

A possible solution to the observed baryon asymmetry in the universe is described, based on the physics of the standard model of electroweak interactions. At temperatures high enough electroweak physics provides violation of baryon number,…

高能物理 - 唯象学 · 物理学 2007-05-23 Nicholas Petropoulos

We discuss a TeV scale model which would explain neutrino oscillation, dark matter, and baryon asymmetry of the Universe simultaneously by the dynamics of the extended Higgs sector and TeV-scale right-handed neutrinos with imposed an exact…

高能物理 - 唯象学 · 物理学 2009-05-26 Mayumi Aoki , Shinya Kanemura , Osamu Seto

We explore lepton-flavored electroweak baryogenesis, driven by CP-violation in leptonic Yukawa sector, using the $\tau-\mu$ system in the two Higgs doublet model as an example. This setup generically yields, together with the…

高能物理 - 唯象学 · 物理学 2018-01-03 Huai-Ke Guo , Ying-Ying Li , Tao Liu , Michael Ramsey-Musolf , Jing Shu

Electroweak baryogenesis (EWBG) remains a theoretically attractive and experimentally testable scenario for explaining the cosmic baryon asymmetry. We review recent progress in computations of the baryon asymmetry within this framework and…

高能物理 - 唯象学 · 物理学 2015-06-05 David E. Morrissey , Michael J. Ramsey-Musolf

The Standard Model fulfills the three Sakharov conditions for baryogenesis. The smallness of quark masses suppresses, however, the CP violation from the Kobayashi-Maskawa phase to a level that is many orders of magnitude below what is…

高能物理 - 唯象学 · 物理学 2009-11-10 Micha Berkooz , Yosef Nir , Tomer Volansky