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Neutrino masses and mixings are analyzed in terms of left-handed fields and a 6x6 complex symmetric mass matrix whose singular values are the neutrino masses. An angle x_nu characterizes the kind of the neutrinos, with x_nu = 0 for Dirac…

High Energy Physics - Phenomenology · Physics 2007-05-23 Kevin Cahill

Neutrino masses could originate in seesaw models testable at colliders, with light mediators and an approximate lepton number symmetry. The minimal model of this type contains two quasi-degenerate Majorana fermions forming a pseudo-Dirac…

High Energy Physics - Phenomenology · Physics 2019-03-27 P. Hernández , J. Jones-Pérez , O. Suarez-Navarro

In a model with $B-L$ gauge symmetry, right-handed neutrinos may have exotic local $B-L$ charge assignment: two of them with $B-L=-4$ and the other one having $B-L=5$. Then, it is natural to accommodate the right-handed neutrinos with the…

High Energy Physics - Phenomenology · Physics 2013-02-22 A. C. B. Machado , V. Pleitez

We study leptogenesis in two seesaw models where maximal atmospheric neutrino mixing and $U_{e3} = 0$ result from symmetries. Salient features of those models are the existence of three Higgs doublets and a twofold degeneracy of the…

High Energy Physics - Phenomenology · Physics 2009-11-10 W. Grimus , L. Lavoura

We propose and study a novel extension of the Standard Model based on the B-L gauge symmetry that can account for dark matter and neutrino masses. In this model, right-handed neutrinos are absent and the gauge anomalies are canceled instead…

High Energy Physics - Phenomenology · Physics 2016-10-12 Sudhanwa Patra , Werner Rodejohann , Carlos E. Yaguna

We revisit a supersymmetric flavor model based on the symmetries $SU(2)_L \times A_4 \times Z_3 \times U(1)_R$, which extends the original Altarelli and Feruglio construction by introducing flavon and driving superfields responsible for the…

High Energy Physics - Phenomenology · Physics 2025-12-10 Takaaki Nomura , Yusuke Shimizu , Towa Takahashi

A large neutrino asymmetry is an interesting possibility for cosmology, which can have significant observable consequences for nucleosynthesis and the cosmic microwave background. However, although it is a possibility, there is no obvious…

High Energy Physics - Phenomenology · Physics 2009-10-31 John McDonald

We consider a dark electroweak phase transition, during which a baryon asymmetry in the dark neutrons and an equal lepton asymmetry in the dark Dirac neutrinos can be simultaneously induced by the CP-violating reflection of the dark…

High Energy Physics - Phenomenology · Physics 2017-10-04 Pei-Hong Gu

We extend the visible content of the standard model (SM) with a hidden sector composed of three right-handed singlet neutrinos and one singlet Higgs. These extra singlets are charged under a new U(1)_X gauge symmetry while the SM particles…

High Energy Physics - Phenomenology · Physics 2009-11-11 Pei-Hong Gu , Hong-Jian He

We investigate non-resonant thermal leptogenesis in the context of the $SU(5) \times \mathcal{T}_{13}$ "asymmetric texture", where both Dirac and Majorana ${CP}$ violation arise from a single phase in the tribimaximal seesaw mixing matrix.…

High Energy Physics - Phenomenology · Physics 2021-02-24 Moinul Hossain Rahat

The Dirac nature of the gauginos (and also the Higgsinos) can be realized in $R$-symmetric supersymmetry models. In this class of models, the Dirac bino (or wino) with a small mixture of the Dirac Higgsinos is a good dark matter candidate.…

High Energy Physics - Phenomenology · Physics 2011-03-22 Eung Jin Chun

We consider realizations of a gauged B-L symmetry in the context of the Dark Dimension scenario, where the SM lives on a codimension one brane in 5d spacetime. The B-L can naturally be a bulk gauge symmetery leading to a global symmetry on…

High Energy Physics - Theory · Physics 2026-03-04 Miguel Montero , Cumrun Vafa , Irene Valenzuela

Choosing how gauge $U(1)_\chi$ breaks in the context of $SO(10) \to SU(5) \times U(1)_\chi$, $Z_4$ lepton number may be obtained which maintains neutrinos as Dirac fermions. Choosing $\Delta(27)$ as the family symmetry of leptons,…

High Energy Physics - Phenomenology · Physics 2019-10-02 Ernest Ma

It is known that the cosmological baryon density (Omega(b)) and dark matter density (Omega(dm)) have strikingly similar values. However, in most theories of the early Universe, each density is explained by separate dynamics and consequently…

High Energy Physics - Phenomenology · Physics 2007-05-23 Stephen M. West

A light ($m_{\nu d} \lesssim $ MeV) dark fermion mixing with the Standard Model neutrinos can naturally equilibrate with the neutrinos via oscillations and scattering. In the presence of dark sector interactions, production of dark fermions…

Cosmology and Nongalactic Astrophysics · Physics 2024-02-02 Daniel Aloni , Melissa Joseph , Martin Schmaltz , Neal Weiner

Realization of the inverted hierarchy is studied in the radiative neutrino mass model with an additional doublet, in which neutrino masses and dark matter could be induced from a common particle. We show that the sufficient baryon number…

High Energy Physics - Phenomenology · Physics 2015-06-12 Shoichi Kashiwase , Daijiro Suematsu

We propose a gauged $U(1)_{B-L}$ extension of the standard model (SM) to explain simultaneously the light neutrino masses and dark matter (DM). The generation of neutrino masses occurs through a variant of type-II seesaw mechanism in which…

High Energy Physics - Phenomenology · Physics 2020-02-18 Satyabrata Mahapatra , Nimmala Narendra , Narendra Sahu

We entertain the possibility that neutrino masses and dark matter (DM) originate from a common composite dark sector. A minimal effective theory can be constructed based on a dark $SU(3)_D$ interaction with three flavors of massless dark…

High Energy Physics - Phenomenology · Physics 2017-12-13 Hooman Davoudiasl , Pier Paolo Giardino , Ethan T. Neil , Enrico Rinaldi

We explore a new mechanism for reproducing the Dark Matter (DM) abundance: scatterings of one DM particle on light Standard Model particles. Strong bounds on its decays can be satisfied if DM undergoes freeze-in and has a mass around or…

Recently there is a renewed interest in exploring the Dark sector of the universe in a more constrained way. Particularly in [1], the FIMP ( Feebly Interacting Massive Particle) scenario was shown to be realized with a minimal extension of…

High Energy Physics - Phenomenology · Physics 2023-05-12 Utkarsh Patel , Lekhika Malhotra , Sudhanwa Patra , Urjit A. Yajnik
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