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We study the possibility that light dark matter can be produced with right relic density by the decay of other dark sector particles. We study this possibility in a model with right-handed neutrinos, a dark sector singlet scalar and a dark…

高能物理 - 唯象学 · 物理学 2021-03-24 Yu Cheng , Wei Liao

Our present work explores the possibility of neutrino mass generation through {\em Type-I see-saw} mechanism and provides an explanation of the baryon asymmetry of the Universe via thermal leptogenesis in the framework of $Z_3$-symmetric…

高能物理 - 唯象学 · 物理学 2020-09-08 Indrani Chakraborty , Himadri Roy

Standard thermal leptogenesis in the type-I seesaw model requires very heavy right-handed neutrinos (RHNs). This makes it hard to probe this scenario experimentally and results in large radiative corrections to the Higgs boson mass. In this…

高能物理 - 唯象学 · 物理学 2019-04-24 Tommi Alanne , Thomas Hugle , Moritz Platscher , Kai Schmitz

We revisit leptogenesis in the minimal non-supersymmetric type I see-saw mechanism with two right-handed (RH) neutrinos, including flavour effects and allowing both RH neutrinos N_1 and N_2 to contribute, rather than just the lightest RH…

高能物理 - 唯象学 · 物理学 2015-05-30 S. Antusch , P. Di Bari , D. A. Jones , S. F. King

We study a seesaw-type extension of the Standard Model in which the symmetry group is enlarged by a global U(1). We introduce adequate scalar and fermion representations which naturally explain the smallness of neutrino masses. With the…

高能物理 - 唯象学 · 物理学 2011-11-23 Francois-Xavier Josse-Michaux , Emiliano Molinaro

Contrary to the common lore based on naive dimensional analysis, the seesaw scale for neutrino masses can be naturally in the TeV range, with small parameters coming from radiative corrections. We present one such class of type-I seesaw…

高能物理 - 唯象学 · 物理学 2015-08-03 P. S. Bhupal Dev , Chang-Hun Lee , R. N. Mohapatra

We consider a U(1)' gauge symmetry acting on three generations of right-handed neutrinos. The U(1)' symmetry is broken at the TeV scale and its remnant discrete symmetry makes one of the right-handed neutrinos stable. As a natural…

高能物理 - 唯象学 · 物理学 2014-01-29 Manfred Lindner , Daniel Schmidt , Atsushi Watanabe

In this talk we show how a natural neutrino mass hierarchy can follow from the type I see-saw mechanism, and a natural neutrino mass degeneracy from the type II see-saw mechanism, where the bi-large mixing angles can arise from either the…

高能物理 - 唯象学 · 物理学 2009-11-10 S. F. King

We discuss the possibility of light scalar dark matter generated by right-handed neutrino in a $L_{\mu}-L_{\tau}$ model, in which the dark matter $\phi_{dm}$ carries $U(1)_{L_{\mu}-L_{\tau}}$ charge but it is a singlet in the Standard…

高能物理 - 唯象学 · 物理学 2023-09-12 XinXin Qi , Hao Sun

We propose a gauged $U(1)_{B-L}$ extension of the standard model (SM) to explain simultaneously the light neutrino masses and dark matter (DM). The generation of neutrino masses occurs through a variant of type-II seesaw mechanism in which…

高能物理 - 唯象学 · 物理学 2020-02-18 Satyabrata Mahapatra , Nimmala Narendra , Narendra Sahu

I suggest a left-right mirror symmetric particle model as the natural and aesthetic extension of the SM. As the left-right mirror symmetry breaking, the tiny neutrino mass is generated by the radiative mechanism, the baryon asymmetry…

高能物理 - 唯象学 · 物理学 2020-02-19 Wei-Min Yang

The generation of neutrino masses by inverse seesaw mechanisms has advantages over other seesaw models since the potential new physics can be produced at the TeV scale. We propose a model that generates the inverse seesaw mechanism via…

高能物理 - 唯象学 · 物理学 2020-06-29 N. Rojas , R. A. Lineros , F. Gonzalez-Canales

In this work, the standard model (SM) is extended with two right-handed (RH) neutrinos and two singlet neutral fermions to yield active neutrino masses via (2,2) inverse see-saw mechanism. We first validate the multi-dimensional model…

高能物理 - 唯象学 · 物理学 2023-04-26 Indrani Chakraborty , Himadri Roy , Tripurari Srivastava

We discuss a left-right symmetric extension of the Standard Model in which the three additional right-handed neutrinos play a central role in explaining the baryon asymmetry of the Universe, the dark matter abundance and the ultra energetic…

高能物理 - 唯象学 · 物理学 2016-11-18 M. Re Fiorentin , V. Niro , N. Fornengo

We make an analytic and numerical study of leptogenesis in the framework of the (Supersymmetric) Standard Model plus the see-saw mechanism with a U(1) family symmetry and single right-handed neutrino dominance. In presenting our analytic…

高能物理 - 唯象学 · 物理学 2009-11-07 M. Hirsch , S. F. King

We construct a loop induced seesaw model in a TeV scale theory with gauged U(1)_{B-L} symmetry. Light neutrino masses are generated at two-loop level and right-handed neutrinos also obtain their masses by one-loop effect. Multi-component…

高能物理 - 唯象学 · 物理学 2013-08-09 Yuji Kajiyama , Hiroshi Okada , Takashi Toma

We propose a UV completion of the inverse see-saw scenario using fermion SU(2) triplet representations. Within this framework, a variation of the standard thermal leptogenesis is achievable at the O(TeV) scale, owing to the presence of a…

高能物理 - 唯象学 · 物理学 2013-03-14 Francois-Xavier Josse-Michaux , Emiliano Molinaro

We discuss a simple non-supersymmetric model based on the electroweak gauge group $SU(2)_L\times SU(2)^\prime\times U(1)_{B-L}$ where the lightest of the right-handed neutrinos, which are part of the leptonic doublet of $SU(2)^\prime$, play…

高能物理 - 唯象学 · 物理学 2016-08-22 P. S. Bhupal Dev , D. Kazanas , R. N. Mohapatra , V. L. Teplitz , Yongchao Zhang

Cosmological and astrophysical observations suggest that both energy densities of baryon and dark matter take the same order values in the present Universe. We propose a scenario to give an answer for this problem in a scotogenic model and…

高能物理 - 唯象学 · 物理学 2024-05-29 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