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相关论文: A TeV-scale model for neutrino mass, DM and baryon…

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We propose an extended version of the standard model, in which neutrino oscillation, dark matter, and baryon asymmetry of the Universe can be simultaneously explained by the TeV-scale physics without assuming unnatural hierarchy among the…

高能物理 - 唯象学 · 物理学 2009-02-27 Mayumi Aoki , Shinya Kanemura , Osamu Seto

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 discuss some details for the model proposed in Ref. \cite{aks-prl}, in which neutrino oscillation, dark matter, and baryon asymmetry of the Universe can be simultaneously explained by the TeV-scale physics without introducing very high…

高能物理 - 唯象学 · 物理学 2009-09-01 Mayumi Aoki , Shinya Kanemura , Osamu Seto

In this talk, 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. By the…

高能物理 - 唯象学 · 物理学 2009-02-19 Mayumi Aoki , Shinya Kanemura , Osamu Seto

We discuss phenomenology in a new 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.…

高能物理 - 唯象学 · 物理学 2010-08-17 Mayumi Aoki , Shinya Kanemura , Osamu Seto

We propose a model to explain tiny masses of neutrinos with the lepton number conservation, where neither too heavy particles beyond the TeV-scale nor tiny coupling constants are required. Assignments of conserving lepton numbers to new…

高能物理 - 唯象学 · 物理学 2017-11-29 Shinya Kanemura , Kodai Sakurai , Hiroaki Sugiyama

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

The radiative neutrino mass model with an inert doublet scalar has been considered as a promising candidate which can explain neutrino masses, dark matter abundance and baryon number asymmetry if dark matter is identified with the lightest…

高能物理 - 唯象学 · 物理学 2015-06-05 Shoichi Kashiwase , Daijiro Suematsu

We propose a simple testable model with mass generation mechanisms for dark matter and neutrino based on the gauged $U(1)_{B-L}$ symmetry and an exact $Z_2$ parity. The $U(1)_{B-L}$ symmetry is spontaneously broken at the TeV scale, by…

高能物理 - 唯象学 · 物理学 2011-08-08 Shinya Kanemura , Osamu Seto , Takashi Shimomura

Realization of the inverted hierarchy is studied in the radiative neutrino mass model with an additional doublet, in which neutrino masses and dark matter could be induced from a common particle. We show that the sufficient baryon number…

高能物理 - 唯象学 · 物理学 2015-06-12 Shoichi Kashiwase , Daijiro Suematsu

The radiative neutrino mass model can relate neutrino masses and dark matter at a TeV scale. If we apply this model to thermal leptogenesis, we need to consider resonant leptogenesis at that scale. It requires both finely degenerate masses…

高能物理 - 唯象学 · 物理学 2016-03-23 Shoichi Kashiwase , Daijiro Suematsu

A simple TeV scale model for baryon and lepton number violation is presented, where neutrino mass arises via a one-loop radiative seesaw effect and B-violation obeys $\Delta B=2$ selection rule. The stability of proton is connected to the…

高能物理 - 唯象学 · 物理学 2015-07-29 P. S. Bhupal Dev , Rabindra N. Mohapatra

It is known that the radiative neutrino mass model proposed by Ma could be a consistent framework for dark matter, leptogenesis and suppressed lepton flavor violation if a neutral component of the inert doublet is identified as dark matter…

高能物理 - 唯象学 · 物理学 2015-05-27 Daijiro Suematsu

We propose a low scale leptogenesis scenario in the framework of composite Higgs models supplemented with singlet heavy neutrinos. One of the neutrinos can also be considered as a dark matter candidate whose stability is guaranteed by a…

高能物理 - 唯象学 · 物理学 2021-04-28 M. Ahmadvand

We study a class of leptogenesis scenarios with decay or scattering being the source of lepton asymmetry, which can not only give rise to the observed baryon asymmetry in the universe but also can leave behind a large remnant neutrino…

高能物理 - 唯象学 · 物理学 2023-08-14 Debasish Borah , Arnab Dasgupta

We construct a list of minimal scale-invariant models at the TeV scale that generate one-loop neutrino mass and give viable dark matter candidates. The models generically contain a singlet scalar and a $Z_2$-odd sector comprised of singlet,…

高能物理 - 唯象学 · 物理学 2016-09-21 Amine Ahriche , Adrian Manning , Kristian L. McDonald , Salah Nasri

We consider a minimal grand unified model where the dark matter arises from non-thermal decays of a messenger particle in the TeV range. The messenger particle compensates for the baryon asymmetry in the standard model and gives similar…

高能物理 - 唯象学 · 物理学 2007-05-23 Ryuichiro Kitano , Ian Low

We propose a new mechanism of TeV scale leptogenesis where the chemical potential of right-handed electron is passed on to the $B-L$ asymmetry of the Universe in the presence of sphalerons. The model has the virtue that the origin of…

高能物理 - 唯象学 · 物理学 2008-11-26 Narendra Sahu , Utpal Sarkar

To explain the dark matter and the baryon asymmetry of the Universe, the parameters of the $\nu$MSM (an extension of the Minimal Standard Model by three singlet neutrinos with masses smaller than the electroweak scale) must be fine-tuned:…

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

We present a TeV scale model for leptogenesis where the origin of neutrino masses are independent of the scale of leptogenesis. As a result, the model could be extended to explain {\it dark matter, neutrino masses and leptogenesis at the…

高能物理 - 唯象学 · 物理学 2008-11-26 Narendra Sahu
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