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In this work, we report on recent analyses of a class of models that generate neutrino mass at the three-loop level. We argue that these models offer a viable solution to both the neutrino mass and dark matter problems, without being in…

High Energy Physics - Phenomenology · Physics 2015-05-19 Amine Ahriche , Kristian L. McDonald , Salah Nasri

Right-handed neutrinos with MeV to GeV mass are very promising candidates for dark matter (DM). Not only can they solve the missing satellite puzzle, the cusp-core problem of inner DM density profiles, and the too-big-to fail problem, {\it…

High Energy Physics - Phenomenology · Physics 2020-01-29 J. Fiaschi , M. Klasen , M. Vargas , C. Weinheimer , S. Zeinstra

We investigate a radiative seesaw model with two leptoquarks under non-holomorphic modular $A_4$ symmetry. The leptons and quarks belong to non-trivial representations of the modular $A_4$ and the structures of their mass matrices are…

High Energy Physics - Phenomenology · Physics 2025-05-14 Takaaki Nomura , Hiroshi Okada , Xing-Yu Wang

We propose a simple scenario that directly connects the dark matter (DM) and neutrino mass scales. Based on an interaction between the DM particle $\chi$ and the neutrino $\nu$ of the form $\chi\chi\nu\nu/\Lambda^2$, the DM annihilation…

High Energy Physics - Phenomenology · Physics 2015-06-03 Wei-Chih Huang , Frank F. Deppisch

We propose a minimal extension of the type-I seesaw model to realise leptogenesis from the co-annihilation of dark sector particles. The type-I seesaw model is extended with a singlet fermion and two singlet scalars charged under a $Z_{2}$…

High Energy Physics - Phenomenology · Physics 2026-02-24 Simran Arora , Debasish Borah , Arnab Dasgupta , P. S. Bhupal Dev , Devabrat Mahanta

We demonstrate that TeV-scale heavy neutral leptons (HNLs) responsible for inverse-seesaw neutrino mass generation can simultaneously fix the cosmological abundance and decay properties of dark matter (DM). The spontaneous breaking of…

High Energy Physics - Phenomenology · Physics 2026-04-03 Cheng-Wei Chiang , Shu-Yu Ho , Van Que Tran

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…

High Energy Physics - Phenomenology · Physics 2009-02-27 Mayumi Aoki , Shinya Kanemura , Osamu Seto

We derive the lower bound on absolute scale of lightest neutrino mass for normal hierarchy and inverted hierarchy pattern of light neutrinos by studying the new physics contributions to charged lepton flavour violating decays and…

High Energy Physics - Phenomenology · Physics 2022-07-25 Prativa Pritimita , Urjit A. Yajnik , Nitali Dash , Sudhanwa Patra

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…

High Energy Physics - Phenomenology · Physics 2022-07-20 Purusottam Ghosh , Satyabrata Mahapatra , Nimmala Narendra , Narendra Sahu

We show that models with exotic leptons transforming as E ~ (1,3,-1) under the standard model gauge symmetry are well suited for generating neutrino mass via a radiative inverse seesaw. This approach realizes natural neutrino masses and…

High Energy Physics - Phenomenology · Physics 2015-06-04 Sandy S. C. Law , Kristian L. McDonald

We propose a model to explain tiny masses of neutrinos with the lepton number conservation, where neither too heavy particles beyond the TeV-scale nor tiny coupling constants are required. Assignments of conserving lepton numbers to new…

High Energy Physics - Phenomenology · Physics 2017-11-29 Shinya Kanemura , Kodai Sakurai , Hiroaki Sugiyama

We study neutrino mass generation and dark matter in a left-right symmetric model. The model is based on an $SU(3)_c\times SU(2)_L \times SU(2)_R \times U(1)_{B-L}$ gauge theory with a softly broken parity symmetry. Masses of the charged…

High Energy Physics - Phenomenology · Physics 2025-10-07 Shohei Okawa , Yuji Omura , Keyun Wu

We consider a two loop radiative seesaw model with an exact $Z_2 \times Z'_2$ symmetry, which can stabilize two or three dark matter particles. The model is a simple extension of the inert scalar model of Ma, where the lepton-number…

High Energy Physics - Phenomenology · Physics 2014-11-11 Mayumi Aoki , Jisuke Kubo , Hiroshi Takano

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…

High Energy Physics - Phenomenology · Physics 2011-08-08 Shinya Kanemura , Osamu Seto , Takashi Shimomura

We discuss phenomenology in a new TeV scale model which would explain neutrino oscillation, dark matter, and baryon asymmetry of the Universe simultaneously by the dynamics of the extended Higgs sector and TeV-scale right-handed neutrinos.…

High Energy Physics - Phenomenology · Physics 2010-08-17 Mayumi Aoki , Shinya Kanemura , Osamu Seto

In this talk, we discuss the phenomenology of radiative 3-loop seesaw models. The 3-loop suppression allows the new particles to have masses at the TeV scale, along with relatively large Yukawa couplings, while retaining consistency with…

High Energy Physics - Phenomenology · Physics 2024-11-04 Asmaa Abada , Nicolás Bernal , Antonio E. Cárcamo Hernández , Sergey Kovalenko , Téssio B. de Melo , Takashi Toma

We study a model with $U(1)$ gauged lepton number symmetry in which the active neutrino masses are generated at two-loop level through the spontaneous breaking of the lepton number symmetry. To cancel gauge anomalies some exotic leptons are…

High Energy Physics - Phenomenology · Physics 2017-06-06 Takaaki Nomura , Hiroshi Okada

Radiative neutrino mass models have interesting features, which make it possible to relate neutrino masses to the existence of dark matter. However, the explanation of the baryon number asymmetry in the universe seems to be generally…

High Energy Physics - Phenomenology · Physics 2015-03-17 H. Higashi , T. Ishima , D. Suematsu

Radiative seesaw models are examples of interesting and testable extensions of the Standard Model to explain the light neutrino masses. In radiative models at 1-loop level, such as the popular scotogenic model, in order to successfully…

High Energy Physics - Phenomenology · Physics 2024-05-22 Asmaa Abada , Nicolás Bernal , Antonio E. Cárcamo Hernández , Sergey Kovalenko , Téssio B. de Melo , Takashi Toma

Various mechanisms have been developed to explain the origin of Majorana neutrino masses. One of them is radiative mass generation. Two-loop mass generation is of particular interest because the masses and couplings of new particles…

High Energy Physics - Phenomenology · Physics 2014-12-22 Yasaman Farzan