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相关论文: Fermion Dark Matter and Radiative Neutrino Masses …

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In the framework of the scotogenic model, which features radiative generation of neutrino masses, we explore light dark matter scenario. Throughout the paper we chiefly focus on keV-scale dark matter which can be produced either via…

高能物理 - 唯象学 · 物理学 2020-09-25 Sven Baumholzer , Vedran Brdar , Pedro Schwaller , Alexander Segner

We propose a model for radiatively generating the hierarchy of the Standard Model (SM) fermion masses: tree-level top quark mass; 1-loop bottom, charm, tau and muon masses; 2-loop masses for the light up, down and strange quarks as well as…

高能物理 - 唯象学 · 物理学 2017-02-24 A. E. Cárcamo Hernández , Sergey Kovalenko , Ivan Schmidt

We propose a new model where the Dirac mass term for neutrinos, the Majorana mass term for right-handed neutrinos, and the other new fermion masses arise via the spontaneous breakdown of the $U(1)_{B-L}$ gauge symmetry. The anomaly-free…

高能物理 - 唯象学 · 物理学 2014-07-10 Shinya Kanemura , Toshinori Matsui , Hiroaki Sugiyama

In an endeavor to explain the light neutrino masses and dark matter (DM) simultaneously, we study a gauged $U(1)_{\rm B-L}$ extension of the standard model (SM). The neutrino masses are generated through a variant of type-II seesaw…

高能物理 - 唯象学 · 物理学 2022-07-20 Purusottam Ghosh , Satyabrata Mahapatra , Nimmala Narendra , Narendra Sahu

We consider an extension of the Standard Model by right-handed neutrinos and we argue that, under plausible assumptions, a neutrino mass of ${\cal O}(0.1)\,{\rm eV}$ is naturally generated by the breaking of the lepton number at the Planck…

高能物理 - 唯象学 · 物理学 2019-03-06 Alejandro Ibarra , Patrick Strobl , Takashi Toma

The low-energy neutrino physics constraints on the TeV scale type I see-saw scenarios of neutrino mass generation are revisited. It is shown that lepton charge (L) violation, associated to the production and decays of heavy Majorana…

高能物理 - 唯象学 · 物理学 2015-05-27 A. Ibarra , E. Molinaro , S. T. Petcov

We propose a unified explanation for the origin of dark matter and baryon number asymmetry on the basis of a non-supersymmetric model for neutrino masses. Neutrino masses are generated in two distinct ways, that is, a tree-level seesaw…

高能物理 - 唯象学 · 物理学 2008-11-26 Daijiro Suematsu

We propose a class of models providing an explanation of the origin of light neutrino masses, the baryon asymmetry of the Universe via leptogenesis and offering viable dark matter candidates. In these models the Majorana masses of the…

高能物理 - 唯象学 · 物理学 2024-04-11 Asmaa Abada , Nicolás Bernal , Antonio E. Cárcamo Hernández , Sergey Kovalenko , Téssio B. de Melo

Observational limits on the high-energy neutrino background have been used to place general constraints on dark matter that annihilates only into standard model particles. Dark matter particles that annihilate into neutrinos will also…

高能物理 - 唯象学 · 物理学 2009-02-20 James B. Dent , Robert J. Scherrer , Thomas J. Weiler

The generation of lepton asymmetry below the electroweak scale has a considerable impact on production of dark matter sterile neutrinos. Oscillations or decays of the heavier sterile neutrinos in the neutrino minimal standard model can give…

高能物理 - 唯象学 · 物理学 2010-11-09 Ananda Roy , 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

We discuss the possibility to find an upper bound on the seesaw scale using the cosmological bound on the cold dark matter relic density. We investigate a simple relation between the origin of neutrino masses and the properties of a dark…

高能物理 - 唯象学 · 物理学 2018-09-11 Pavel Fileviez Perez , Clara Murgui

We consider the leptonic asymmetry generation in the nuMSM via hadronic decays of sterile neutrinos at T<<T_{EW}, when the masses of two heavier sterile neutrinos are between pion mass and 2 GeV. The choice of upper mass bound is motivated…

高能物理 - 唯象学 · 物理学 2013-09-25 Volodymyr M. Gorkavenko , Igor Rudenok , Stanislav I. Vilchynskiy

We consider extensions of the standard model with fourth generation fermions (SM4) in which extra symmetries are introduced such that the transitions between the fourth generation fermions and the ones in the first three generations are…

高能物理 - 唯象学 · 物理学 2015-06-16 Shou-Shan Bao , Xue Gong , Zong-Guo Si , Yu-Feng Zhou

The minimal seesaw extension of the Standard SU(3) x SU(2) x U(1) 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…

高能物理 - 唯象学 · 物理学 2013-11-05 M. Hirsch , R. A. Lineros , S. Morisi , J. Palacio , N. Rojas , J. W. F. Valle

Small realistic Majorana neutrino masses can be generated via a Higgs triplet $(\xi^{++}, \xi^+, \xi^0)$ without having energy scales larger than $M_*={\cal O}(1)$ TeV in the theory. The large effective mass scale $\Lambda$ in the…

高能物理 - 唯象学 · 物理学 2009-10-31 Ernest Ma , Martti Raidal , Utpal Sarkar

We propose a Majoron-like extension of the Standard Model with an extra global $U(1)_X$-symmetry where neutrino masses are generated through an inverse seesaw mechanism at the 1-loop level. In contrast to the tree-level inverse seesaw, our…

We propose an extension of the minimal scotogenic model with a triplet fermion and a singlet scalar. An imposed $Z_{4}\times Z_{2}$ symmetry allows only diagonal Yukawa couplings among different generations of SM leptons and right-handed…

高能物理 - 唯象学 · 物理学 2025-02-13 Simran Arora , Devabrat Mahanta , B. C. Chauhan

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

Sterile neutrinos with keV masses can constitute all or part of the cosmological dark matter. The electroweak-singlet fermions, which are usually introduced to explain the masses of active neutrinos, need not be heavier than the electroweak…

天体物理学 · 物理学 2017-08-23 Alexander Kusenko