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We consider the minimal extended seesaw model which can accommodate an eV scale sterile neutrino. The scenario also includes three heavy right handed neutrinos in addition to the light sterile neutrino. In this model, the active-sterile…

高能物理 - 唯象学 · 物理学 2022-06-08 Srubabati Goswami , Vishnudath K. N. , Ananya Mukherjee , Nimmala Narendra

We propose a realization of mass varying neutrino dark energy in two extensions of the Standard Model (SM) with a dynamical neutrino mass related to the acceleron field while satisfying the naturalness. In the first scenario the SM is…

高能物理 - 唯象学 · 物理学 2016-05-25 Chandan Hati , Utpal Sarkar

In the left-right symmetric models without bi-doublet Higgs scalars, the standard model fermions can obtain masses by integrating out heavy charged singlet fermions. We find the decays of heavy neutral singlet fermions, responsible for…

高能物理 - 唯象学 · 物理学 2010-05-19 Pei-Hong Gu

In this work we study a classically scale invariant extension of the Standard Model that can explain simultaneously dark matter and the baryon asymmetry in the universe. In our set-up we introduce a dark sector, namely a non-Abelian SU(2)…

高能物理 - 唯象学 · 物理学 2016-11-23 Valentin V. Khoze , Alexis D. Plascencia

We investigate a simple variant of type-II seesaw, responsible for neutrino mass generation, where the particle spectrum is extended with one singlet right-handed neutrino and an inert Higgs doublet, both odd under an additional $Z_2$…

高能物理 - 唯象学 · 物理学 2022-06-08 Arghyajit Datta , Rishav Roshan , Arunansu Sil

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 $Z_{2}$…

高能物理 - 唯象学 · 物理学 2026-02-24 Simran Arora , Debasish Borah , Arnab Dasgupta , P. S. Bhupal Dev , Devabrat Mahanta

It has been proposed that in a part of the parameter space of the Standard Model completed by three generations of keV...GeV right-handed neutrinos, neutrino masses, dark matter, and baryon asymmetry can be accounted for simultaneously.…

高能物理 - 唯象学 · 物理学 2019-07-25 J. Ghiglieri , M. Laine

The Standard Model (SM) is inadequate to explain the origin of tiny neutrino masses, the dark matter (DM) relic abundance and also the baryon asymmetry of the Universe. In this work to address all the three puzzles, we extend the SM by a…

高能物理 - 唯象学 · 物理学 2017-12-19 Anirban Biswas , Sandhya Choubey , Sarif Khan

Following a baryogenesis scenario proposed by Lazarides, Panagiotakopoulos and Shafi, we show how the observed baryon asymmetry can be explained via resonant leptogenesis in a class of supersymmetric models with an intermediate mass scale…

高能物理 - 唯象学 · 物理学 2008-11-26 S. Dar , S. Huber , V. N. Senoguz , Q. Shafi

We propose a novel scenario of generating lepton asymmetry via annihilation and coannihilation of dark sector particles including t-channel processes. In order to realistically implement this idea, we consider the scotogenic model having…

高能物理 - 唯象学 · 物理学 2020-05-19 Debasish Borah , Arnab Dasgupta , Sin Kyu Kang

We consider a left-right symmetric model with an $SU(2)_L$ and an $SU(2)_R$ scalar doublet but without the scalar bidoublet. The charged fermion masses in this model are generated via a universal seesaw mechanism. We add a set of three…

高能物理 - 唯象学 · 物理学 2025-05-01 Zafri A. Borboruah , Lekhika Malhotra , Utkarsh Patel , Sudhanwa Patra , S. Uma Sankar

We present a new realization of asymmetric dark matter in which the dark matter and lepton asymmetries are generated simultaneously through two-sector leptogenesis. The right-handed neutrinos couple both to the Standard Model and to a…

高能物理 - 唯象学 · 物理学 2011-05-26 Adam Falkowski , Joshua T. Ruderman , Tomer Volansky

We consider minimal $U(1)$ extensions of the Standard Model in which one of the right-handed neutrinos is charged under the new gauge symmetry and plays the role of dark matter. In particular, we perform a detailed phenomenological study…

高能物理 - 唯象学 · 物理学 2018-01-19 Peter Cox , Chengcheng Han , Tsutomu T. Yanagida

We discuss a 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 with imposed an exact…

高能物理 - 唯象学 · 物理学 2009-05-26 Mayumi Aoki , Shinya Kanemura , Osamu Seto

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 study a seesaw-type extension of the Standard Model in which the symmetry group is enlarged by a global U(1). We introduce adequate scalar and fermion representations which naturally explain the smallness of neutrino masses. With the…

高能物理 - 唯象学 · 物理学 2011-12-19 François-Xavier Josse-Michaux , Emiliano Molinaro

Models of leptogenesis often invoke the out-of-equilibrium decays of heavy right-handed neutrinos in order to create a baryon asymmetry of the universe through the electroweak phase transition. Their presumed existence argues strongly for…

高能物理 - 唯象学 · 物理学 2011-02-16 Ernest Ma , Subir Sarkar , Utpal Sarkar

We consider a generic model with four gauge singlets which generates successfully the right amount of baryon asymmetry through leptogenesis at the TeV scale. It also reproduces left-handed neutrino masses compatible with present data. In…

高能物理 - 唯象学 · 物理学 2007-05-23 Asmaa Abada , Habib Aissaoui , Marta Losada

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 implemented the neutrino dark energy proposal in a left-right symmetric model. Unlike earlier models of mass varying neutrinos, in the present model the mass parameter that depends on the scalar field (acceleron) remains very light…

高能物理 - 唯象学 · 物理学 2008-11-26 Jitesh R. Bhatt , Pei-Hong Gu , Utpal Sarkar , Santosh K. Singh