中文
相关论文

相关论文: The Inert Zee Model

200 篇论文

A minimal extension of the standard model to naturally generate small neutrino masses and provide a dark matter candidate is proposed. The dark matter particle is part of a new scalar doublet field that plays a crucial role in radiatively…

高能物理 - 唯象学 · 物理学 2014-07-03 Michael Gustafsson , Jose Miguel No , Maximiliano A. Rivera

Here we study the pattern of neutrino oscillations emerging from a previously proposed warped model construction incorporating $\Delta(27)$ flavor symmetry. In addition to a complete description of fermion masses, the model predicts the…

高能物理 - 唯象学 · 物理学 2017-06-07 Pedro Pasquini , S. C. Chuliá , J. W. F. Valle

Baryon asymmetry of the Universe is evaluated in the model originally proposed in Phys. Rev. Lett. 102 (2009) 051805, where Majorana masses of neutrinos are generated via three-loop diagrams composed of additional scalar bosons including…

高能物理 - 唯象学 · 物理学 2023-06-19 Mayumi Aoki , Kazuki Enomoto , Shinya Kanemura

We establish a hybrid seesaw mechanism to explain small neutrino masses and predict cold dark matter candidate in the context of the B-L gauge symmetry extension of the Standard Model. In this model a new scalar doublet and two new fermion…

高能物理 - 唯象学 · 物理学 2015-03-13 Tong Li , Wei Chao

In this review we discuss how the models of neutrino masses can accommodate solutions to the problem of matter-antimatter asymmetry in the universe, dark energy or cosmological constant problem and dark matter candidates. The…

高能物理 - 唯象学 · 物理学 2009-11-13 Utpal Sarkar

We construct a radiative inverse seesaw model with local B-L symmetry, and investigate the flavor structure of the lepton sector and the fermionic Dark Matter. Neutrino masses are radiatively generated through a kind of inverse seesaw…

高能物理 - 唯象学 · 物理学 2015-06-05 Hiroshi Okada , Takashi Toma

We propose a model with radiatively induced neutrino mass at two-loop level, applying modular $A_4$ symmetry. The neutrino mass matrix is formulated where the structure of associated couplings are restricted by the symmetry. Then we show…

高能物理 - 唯象学 · 物理学 2021-03-09 Takaaki Nomura , Hiroshi Okada

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

In this paper, we present a systematic investigation on simple inverse seesaw models for neutrino masses and flavor mixing based on the modular $S^{}_4$ symmetry. Two right-handed neutrinos and three extra fermion singlets are introduced to…

高能物理 - 唯象学 · 物理学 2021-10-01 Xinyi Zhang , Shun Zhou

We present a Majorana scotogenic-like loop framework in which neutrino mass generation and dark matter stability are intrinsically connected to the breaking of the discrete flavor symmetry $A_4$. This breaking leads to the emergence of the…

高能物理 - 唯象学 · 物理学 2025-11-25 Ranjeet Kumar , Hemant Kumar Prajapati , Rahul Srivastava , Sushant Yadav

After confirmation of massiveness and mixing of neutrinos, by neutrino oscillation data, the origin of neutrino mass and the occurrence of charged-lepton-flavor non-conservation in nature have become two main objectives for the physics of…

高能物理 - 唯象学 · 物理学 2026-02-05 Adrián González-Quiterio , Héctor Novales-Sánchez

By extending the lepton sector of standard model to include one sterile neutrino and two sets of new Higgs doublets and right-handed neutrinos, denoted by $(\eta_1, N_1, N_3)$ and $(\eta_2, N_2, N_4)$, with two $Z_2$ symmetries, the puzzles…

高能物理 - 唯象学 · 物理学 2009-05-26 Chuan-Hung Chen

We propose a new motivation for the stability of dark matter (DM). We suggest that the same non-abelian discrete flavor symmetry which accounts for the observed pattern of neutrino oscillations, spontaneously breaks to a Z2 subgroup which…

高能物理 - 唯象学 · 物理学 2010-12-24 M. Hirsch , S. Morisi , E. Peinado , J. W. F. Valle

We demonstrate that the extension of the Zee-Babu model can generate not only the small neutrino masses but also the baryon number asymmetry in the universe. In particular, we show that the scale of the singlet scalar responsible for the…

高能物理 - 唯象学 · 物理学 2008-12-30 C. S. Chen , C. Q. Geng , D. V. Zhuridov

We propose a model with two Higgs doublet where quark and charged-lepton masses in the first and second families are induced at one-loop level, and neutrino masses are induced at the two-loop level. In our model we introduce an extra…

高能物理 - 唯象学 · 物理学 2017-07-19 Takaaki Nomura , Hiroshi Okada

We study a one-loop induced neutrino mass model with an inert isospin triplet scalar field of $Y=0$ and heavier isospin doublet vector-like leptons and singlet Majorana right-handed fermions. In addition to the neutrino mass matrix, We…

高能物理 - 唯象学 · 物理学 2024-09-18 Shilpa Jangid , Keiko I. Nagao , Hiroshi Okada

The lepton sector is studied within a flavored non-renormalizable model where the $\mathbf{S}_{3}\otimes \mathbf{Z}_{2}$ flavor symmetry drives the Yukawa couplings. In this framework, the effective neutrino mass, that comes from the type…

高能物理 - 唯象学 · 物理学 2022-06-17 J. D. García-Aguilar , Juan Carlos Gómez-Izquierdo

We present a model which employs $CP\times Z_3$ symmetries where quark mixing and charged leptons masses are explained by following some texture. To achieve neutrino mass and mixing, we write a non-renormalizable Lagrangian using type-II…

高能物理 - 唯象学 · 物理学 2022-07-13 Joy Ganguly

We discuss the possibility of flavor symmetries to explain the pattern of charged lepton and neutrino masses and mixing angles. We emphasize what are the obstacles for the generation of an almost maximal atmospheric mixing and what are the…

高能物理 - 唯象学 · 物理学 2014-11-17 Shao-Long Chen , Michele Frigerio , Ernest Ma

A new S3 flavor model based on $\mathrm{SU}(3)_C \otimes \mathrm{SU}(3)_L \otimes \mathrm{U}(1)_X$ gauge symmetry responsible for fermion masses and mixings different from our previous work is constructed. The new feature is a two -…

高能物理 - 唯象学 · 物理学 2014-07-11 V. V. Vien , H. N. Long