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相关论文: Thermal Relic Right-Handed Neutrino Dark Matter

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The seesaw mechanism with three right-handed neutrinos has one as a well-motivated dark matter candidate if stable and the other two can explain baryon asymmetry via the thermal leptogenesis scenario. We explore the possibility of…

高能物理 - 唯象学 · 物理学 2023-11-09 Yu Cheng , Shao-Feng Ge , Jie Sheng , Tsutomu T. Yanagida

$SU(2)_L \times SU(2)_R$ gauge symmetry requires three right-handed neutrinos ($ N _i $), one of which, $N_1$, can be sufficiently stable to be dark matter. In the early universe, $ W _R $ exchange with the Standard Model thermal bath keeps…

高能物理 - 唯象学 · 物理学 2020-09-04 Jeff A. Dror , David Dunsky , Lawrence J. Hall , Keisuke Harigaya

We study the right-handed neutrino (RHN) dark matter candidate in the minimal U(1)_{B-L} gauge extension of the standard model. The U(1)_{B-L} gauge symmetry offers three RHNs which can address the origin of the neutrino mass, the relic…

高能物理 - 唯象学 · 物理学 2017-03-08 Kunio Kaneta , Zhaofeng Kang , Hye-Sung Lee

It has been pointed out in ref.[1] that in the nuMSM (Standard Model extended by three right-handed neutrinos with masses smaller than the electroweak scale), there is a corner in the parameter space where CP-violating resonant oscillations…

高能物理 - 唯象学 · 物理学 2009-01-06 M. Laine , M. Shaposhnikov

We investigate the viability of having dark matter in the minimal left-right symmetric theory. We find the lightest right-handed neutrino with a mass around keV as the only viable candidate consistent with a TeV scale of left-right…

高能物理 - 唯象学 · 物理学 2015-06-05 Miha Nemevsek , Goran Senjanovic , Yue Zhang

A right-handed neutrino is a promising candidate for dark matter (DM) which has no interaction with nuclei. Since two right-handed neutrinos explain neutrino oscillation data and baryon number asymmetry through both the seesaw mechanism and…

高能物理 - 唯象学 · 物理学 2026-02-17 Daijiro Suematsu

We study the scenario of dark matter in the minimal left-right symmetric theory at the TeV scale. The only viable candidate is found to be the lightest right-handed neutrino with a mass of keV. To satisfy the dark matter relic abundance,…

高能物理 - 唯象学 · 物理学 2015-06-12 Miha Nemevsek

We consider the interplay between dark matter and leptogenesis in a common framework, where three right-handed neutrinos, one fermionic dark matter and two singlet scalars are introduced into the Standard Model. The mixing of the two…

高能物理 - 唯象学 · 物理学 2023-03-28 XinXin Qi , Hao Sun

$B-L$ is known to be a symmetry somewhat linked to the origin of neutrino masses, which turns out to be anomaly free upon the sole introduction of right handed neutrinos. We suggest a simple extension of the electroweak group,…

高能物理 - 唯象学 · 物理学 2015-03-19 R. J. Hernandez-Pinto , A. Perez-Lorenzana

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 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

We investigate the Standard Model (SM) with a $U(1)_{B-L}$ gauge extension where a $B-L$ charged scalar is a viable dark matter (DM) candidate. The dominant annihilation process, for the DM particle is through the $B-L$ symmetry breaking…

高能物理 - 唯象学 · 物理学 2018-01-08 Priyotosh Bandyopadhyay , Eung Jin Chun , Rusa Mandal

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 supersymmetric extension of the minimal $B-L$ model where we consider a new $Z_2$-parity under which one right-handed neutrino is assigned odd parity. When the Majorana Yukawa coupling of a $Z_2$-even right-handed neutrino is…

高能物理 - 唯象学 · 物理学 2012-05-15 Zachary M. Burell , Nobuchika Okada

We consider minimal $U(1)$ extensions of the Standard Model in which one of the right-handed neutrinos is charged under the new gauge symmetry and plays the role of dark matter. In particular, we perform a detailed phenomenological study…

高能物理 - 唯象学 · 物理学 2018-01-19 Peter Cox , Chengcheng Han , Tsutomu T. Yanagida

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 show that in a class of non-supersymmetric left-right extensions of the Standard Model (SM), the lightest right-handed neutrino (RHN) can play the role of thermal Dark Matter (DM) in the Universe for a wide mass range from TeV to PeV.…

高能物理 - 唯象学 · 物理学 2017-04-28 P. S. Bhupal Dev , Rabindra N. Mohapatra , Yongchao Zhang

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

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

In the minimal supersymmetric standard model (MSSM) the lightest superpartner of the left-handed neutrinos is ruled out of being a candidate of dark matter because of its large elastic cross-section with the nucleus mediated via Z-boson. We…

高能物理 - 唯象学 · 物理学 2014-11-26 Arindam Chatterjee , Narendra Sahu
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