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A scenario that relates the abundance of dark matter to the baryon asymmetry of the Universe is presented. In this scenario, based on a left-right extension of the Standard Model, dark matter is made of light, ~ 1 GeV, right-handed Majorana…

高能物理 - 唯象学 · 物理学 2007-05-23 Michel H. G. Tytgat

We consider a generic type of leptogenesis model which can successfully produce the correct value of the observed baryon number to entropy ratio. The main feature of this model is that it is a simple TeV scale model, a scale accessible in…

高能物理 - 唯象学 · 物理学 2010-04-05 Asmaa Abada , Marta Losada

We propose a unified solution with $Z_4$ discrete symmetry for small neutrino masses and stability of dark matter. The Standard Model is extended with an inert doublet scalar, a dark singlet scalar, a spurion scalar and right-handed…

高能物理 - 唯象学 · 物理学 2025-01-03 Jongkuk Kim , Seong-Sik Kim , Hyun Min Lee , Rojalin Padhan

A simple model is constructed based on the gauge symmetry $SU(3)_c \times SU(2)_L \times U(1)_Y \times SU(2)_\ell$, with only the leptons transforming nontrivially under $SU(2)_\ell$. The extended symmetry is broken down to the Standard…

高能物理 - 唯象学 · 物理学 2017-06-14 Bartosz Fornal

In some classes of flavour models based on unified theories with a type I see-saw mechanism, the prediction for the mass of the lightest right-handed neutrino is in conflict with the lower bound from the requirement of successful thermal…

高能物理 - 唯象学 · 物理学 2009-11-11 Stefan Antusch , Steve F. King

Instead of creating the observed baryon asymmetry of the universe by the decay of right-handed (RH) neutrinos to left-handed leptons, we propose to generate it dominantly by the decay of the RH neutrinos to RH leptons. This mechanism turns…

高能物理 - 唯象学 · 物理学 2009-11-11 Michele Frigerio , Thomas Hambye , Ernest Ma

We construct a model realizing the inverse seesaw mechanism. The model has two types of gauge singlet fermions in addition to right-handed neutrinos. A required Majorana mass scale (keV scale) for generating the light active neutrino mass…

高能物理 - 唯象学 · 物理学 2015-11-30 Mayumi Aoki , Naoyuki Haba , Ryo Takahashi

An extension of the Standard Model by three right-handed neutrinos with masses smaller than the electroweak scale (the $\nu$MSM) can explain simultaneously dark matter and baryon asymmetry of the Universe, being consistent with the data on…

天体物理学 · 物理学 2016-11-15 Mikhail Shaposhnikov

We propose a novel and minimal framework where a light scalar field can give rise to dark matter (DM) self-interactions, while enhancing the CP symmetry required for successful baryon asymmetry of the Universe via leptogenesis route. For…

高能物理 - 唯象学 · 物理学 2022-12-07 Debasish Borah , Arnab Dasgupta , Satyabrata Mahapatra , Narendra Sahu

We study a scenario where both dark matter and heavy right handed neutrino (RHN) responsible for leptogenesis acquire masses by crossing the relativistic bubble walls formed as a result of a TeV scale supercooled first order phase…

高能物理 - 唯象学 · 物理学 2022-12-14 Debasish Borah , Arnab Dasgupta , Indrajit Saha

Under the assumption of hierarchical right-handed neutrino masses, masses of right-handed neutrinos must be larger than $10^8$ GeV in the standard thermal leptogenesis scenario, while the mass can be reduced to around 5 TeV in a…

高能物理 - 唯象学 · 物理学 2013-08-15 Naoyuki Haba , Osamu Seto , Yuya Yamaguchi

We perform a systematic study of the phenomenology associated to models where the dark matter consists in the neutral component of a scalar SU(2)_L n-uplet, up to n=7. If one includes only the pure gauge induced annihilation cross-sections…

高能物理 - 唯象学 · 物理学 2010-12-15 T. Hambye , F. -S. Ling , L. Lopez Honorez , J. Rocher

We propose a novel framework for low-scale leptogenesis within an extension of the Standard Model (SM) that includes three SU(2) singlet right-handed neutrinos, a singlet charged neutral fermion, and a real scalar field. In this setup, the…

高能物理 - 唯象学 · 物理学 2026-01-01 Suresh Chand , Avnish , Poulose Poulose

The seesaw mechanism with three heavy Majorana right-handed neutrinos provides an elegant explanation for neutrino masses and, combined with leptogenesis, can generate the baryon asymmetry of the universe (BAU). Naturally embedded in a…

高能物理 - 唯象学 · 物理学 2025-05-06 Juan Herrero-Garcia , Giacomo Landini , Tsutomu T. Yanagida

In this paper we consider generation of naturally small neutrino masses from a dimension-7 operator. Such a term can arise in presence of a scalar quadruplet and a pair of vector-like fermion triplets and enables one to obtain small…

高能物理 - 唯象学 · 物理学 2013-12-03 Gulab Bambhaniya , Joydeep Chakrabortty , Srubabati Goswami , Partha Konar

We consider an extension of the Standard Model with the global symmetry breaking pattern SO(5)/SO(4), where the Higgs boson arises as a pseudo-Nambu-Goldstone boson. The scalar content of the theory consists of a Standard-Model-like Higgs…

高能物理 - 唯象学 · 物理学 2017-12-11 Tommi Alanne , Aurora Meroni , Kimmo Tuominen

The singlet-doublet dark matter (SDDM) model is a well-motivated WIMP framework that accommodates viable dark matter over a broad range of parameter space. In this work, we explore the possibility of TeV-scale leptogenesis within two…

高能物理 - 唯象学 · 物理学 2026-05-07 Partha Kumar Paul , Narendra Sahu , Shashwat Sharma

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 show that existing laboratory experiments have the potential to unveil the origin of matter by probing leptogenesis in the type-I seesaw model with three right-handed neutrinos and Majorana masses in the GeV range. The baryon asymmetry…

高能物理 - 唯象学 · 物理学 2015-05-25 Laurent Canetti , Marco Drewes , Björn Garbrecht

We study the minimal scotogenic model constituting an additional inert Higgs doublet and three sets of right-handed neutrinos. The scotogenic model connects dark matter, baryon asymmetry of the Universe and neutrino oscillation data. In our…

高能物理 - 唯象学 · 物理学 2021-02-24 Lavina Sarma , Pritam Das , Mrinal Kumar Das