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相关论文: Radiative Seesaw Dark Matter

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We consider a minimal type Ib seesaw model where the effective neutrino mass operator involves two different Higgs doublets, and the two right-handed neutrinos form a heavy Dirac mass. We propose a minimal dark matter extension of this…

高能物理 - 唯象学 · 物理学 2021-05-25 Marco Chianese , Bowen Fu , Stephen F. King

In this paper, we perform a detail analysis on leptogenesis and dark matter form low scale seesaw. In the framework of $\nu$2HDM, we further introduce one scalar singlet $\phi$ and one Dirac fermion singlet $\chi$, which are charged under a…

高能物理 - 唯象学 · 物理学 2020-05-13 Ang Liu , Zhi-Long Han , Yi Jin , Fa-Xin Yang

Although the seesaw mechanism is a natural explanation for the small neutrino masses, there are cases when the Majorana mass terms for the right-handed neutrinos are not allowed due to symmetry. In that case, if neutrino-specific Higgs…

高能物理 - 唯象学 · 物理学 2017-04-05 Seungwon Baek , Takaaki Nomura

We discuss phenomenology of the radiative seesaw model in which spontaneous breaking of the U(1)$_{B-L}$ gauge symmetry at the TeV scale gives the common origin for masses of neutrinos and dark matter (Kanemura et al., 2012). In this model,…

高能物理 - 唯象学 · 物理学 2013-05-30 Shinya Kanemura , Takehiro Nabeshima , Hiroaki Sugiyama

We consider the singlet Majoron model with softly broken lepton number. This model contains three right-handed neutrinos and a singlet scalar besides the standard model fields. The real part of the singlet scalar develops a vacuum…

高能物理 - 唯象学 · 物理学 2014-11-20 Pei-Hong Gu , Ernest Ma , Utpal Sarkar

The seesaw mechanism is attractive not only because it "explains'' small neutrino mass, but also because of its packaging with the SUSY-GUT, leptogenesis, Dark Matter, and electroweak symmetry breaking. However, this package has the flavor,…

高能物理 - 唯象学 · 物理学 2009-09-29 Hitoshi Murayama

In an attempt to unfold (if any) a possible connection between two apparently uncorrelated sectors, namely neutrino and dark matter, we consider the type-I seesaw and a fermion singlet dark matter to start with. Our construction suggests…

高能物理 - 唯象学 · 物理学 2018-12-26 Subhaditya Bhattacharya , Ivo de Medeiros Varzielas , Biswajit Karmakar , Stephen F. King , Arunansu Sil

An attractive way to generate neutrino masses as required to account for current neutrino oscillation data involves the spontaneous breaking of lepton number. The resulting majoron may pick up a mass due to gravity. If its mass lies in the…

天体物理学 · 物理学 2009-09-17 Federica Bazzocchi , Massimiliano Lattanzi , Signe Riemer-Sorensen , Jose W. F. Valle

The see-saw mechanism for neutrino masses based on the Grand Unification leads to the mass of the heaviest neutrino ($\approx \nu_{\tau}$) in the range $(2 - 3)\cdot 10^{-3}$ eV and hence to a solution of the solar neutrino problem through…

高能物理 - 唯象学 · 物理学 2011-07-19 Anjan S. Joshipura , A. Yu. Smirnov

In this paper we work in the framework of a radiative seesaw model with triplet fermion $\Sigma$. Due to the $Z_2$ discrete flavor symmetry, the lightest neutral component of $\Sigma$ is stable and thus can be a dark matter candidate. Its…

高能物理 - 唯象学 · 物理学 2012-03-01 Wei Chao

The $SU(3)_c^{}\times SU(2)_L^{} \times U(1)_Y^{}$ standard model is extended by a $U(1)_{B-L}^{}$ gauge symmetry with four right-handed neutrinos. Because of their Yukawa couplings to a Higgs singlet for spontaneously breaking the…

高能物理 - 唯象学 · 物理学 2025-08-21 Pei-Hong Gu

We consider a model for a Z'-boson coupled only to baryon minus lepton number and hypercharge. Besides the usual right-handed neutrinos, we add a pair of fermions with a fractional lepton charge, which we therefore call leptinos. One of the…

高能物理 - 唯象学 · 物理学 2013-02-14 Lorenzo Basso , Oliver Fischer , J. J. van der Bij

It is shown that in extensions of the standard model of quarks and leptons where additive lepton number $L$ is broken by two units, so that $Z_2$ lepton parity, i.e. $(-1)^L$ which is either even or odd, remains exactly conserved, there is…

高能物理 - 唯象学 · 物理学 2015-07-08 Ernest Ma

It has recently been pointed out that the underlying symmetry of dark matter may well be $U(1)_\chi$ (coming from $SO(10) \to SU(5) \times U(1)_\chi$) with the dark parity of any given particle determined by $(-1)^{Q_\chi+2j}$, where…

高能物理 - 唯象学 · 物理学 2019-02-07 Ernest Ma

The minimal seesaw extension of the Standard Model requires two electroweak singlet fermions in order to accommodate the neutrino oscillation parameters at tree level. Here we consider a next to minimal extension where light neutrino masses…

高能物理 - 唯象学 · 物理学 2016-06-15 Roberto A. Lineros

We study a three loop induced neutrino mass model with exotic vector-like isospin doublet leptons which contain a dark matter candidate. Then we explore lepton flavor violations, and dark matter physics in co-annihilation system. In this…

高能物理 - 唯象学 · 物理学 2016-06-22 Takaaki Nomura , Hiroshi Okada , Yuta Orikasa

Majorons are the Goldstone bosons of spontaneously broken lepton number and hence intimately connected to Majorana neutrino masses. Since all majoron couplings are heavily suppressed by the seesaw scale they are interesting candidates for…

高能物理 - 唯象学 · 物理学 2018-09-26 Julian Heeck

High energy accelerators may probe into dark matter and the seesaw neutrino mass scales if they are not much heavier than ~O(TeV). In the absence of supersymmetry, we extend a class of SO(10) models to predict well known cold dark matter…

高能物理 - 唯象学 · 物理学 2011-09-27 Mina K. Parida

The linear seesaw mechanism provides a simple way to generate neutrino masses. In addition to Standard Model particles, it includes quasi-Dirac leptons as neutrino mass mediators, and a leptophilic scalar doublet seeding small neutrino…

高能物理 - 唯象学 · 物理学 2023-08-21 Aditya Batra , Praveen Bharadwaj , Sanjoy Mandal , Rahul Srivastava , José W. F. Valle

Neutrino masses may arise from spontaneous breaking of ungauged lepton number. Due to quantum gravity effects the associated Goldstone boson - the majoron - will pick up a mass. We determine the lifetime and mass required by cosmic…

天体物理学 · 物理学 2008-12-18 M. Lattanzi , J. W. F. Valle