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相关论文: Leptogenesis and dark matter in minimal inverse se…

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In this paper, we construct a model with the help of modular symmetry in the framework of minimal inverse seesaw [ISS(2,3)]. We have used $\Gamma(3)$ modular group which is isomorphic to non-Abelian discrete symmetry group $A_4$. In this…

高能物理 - 唯象学 · 物理学 2023-05-03 Jotin Gogoi , Nayana Gautam , Mrinal Kumar Das

We study a model of neutrino and dark matter within the framework of a minimal extended seesaw. This framework is based on $A_4$ flavor symmetry along with the discrete $Z_4$ symmetry to stabilize the dark matter and construct desired mass…

高能物理 - 唯象学 · 物理学 2020-04-22 Pritam Das , Mrinal Kumar Das , Najimuddin Khan

A non-supersymmetric inverse seesaw model of neutrino mass based on the $A^{\prime}_5$ modular symmetry is presented. This framework provides a combined explanation for neutrino masses, mixing, and the cosmic baryon asymmetry through…

高能物理 - 唯象学 · 物理学 2026-03-20 Xianshuo Zhang , Yakefu Reyimuaji

We propose a minimal inverse seesaw framework based on $A_4$ modular symmetry. We have studied the neutrino oscillation parameters in our work and our model excludes some $3 \sigma$ values of the mixing angle $\theta_{23}$. Also, there is a…

高能物理 - 唯象学 · 物理学 2025-05-07 Gourab Pathak , Mrinal Kumar Das

Discrete symmetries being preferred to explain the neutrino phenomenology, we chose the simplest $S_3$ group and explore the implication of its modular form on neutrino masses and mixing. Non-trivial transformations of Yukawa couplings…

高能物理 - 唯象学 · 物理学 2020-08-06 Subhasmita Mishra

We study $S_{4}$ flavor symmetric inverse seesaw model which has the possibility of simultaneously addressing neutrino phenomenology, dark matter (DM) and baryon asymmetry of the universe (BAU) through leptogenesis. The model is the…

高能物理 - 唯象学 · 物理学 2021-09-01 Nayana Gautam , Mrinal Kumar Das

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 propose a model for leptons based on the smallest modular finite group $\Gamma_2\cong S_3$ that, for the first time, accounts for both the hints of large low-energy CP-violation in the lepton sector and the matter-antimatter asymmetry of…

高能物理 - 唯象学 · 物理学 2024-05-09 Simone Marciano , Davide Meloni , Matteo Parriciatu

In this present study, an extended Delta 54 flavor symmetry model incorporating two standard model Higgs doublets is investigated. This model generates neutrino masses through the triple inverse seesaw mechanism. It predicts deviations from…

高能物理 - 唯象学 · 物理学 2026-05-13 H. Bora , N. Bharali , R. Sarkar , S. K. Jha , A. Baruah , Ng. K. Francis

Describing neutrino masses using the inverse seesaw mechanism with discrete flavor symmetry imposed through modular forms provides a testable framework at TeV scales with fewer parameters. However, $S_3$, the smallest modular group, remains…

高能物理 - 唯象学 · 物理学 2025-05-01 Mitesh Kumar Behera , Pawin Ittisamai , Chakrit Pongkitivanichkul , Patipan Uttayarat

We consider the possibility of simultaneously addressing the baryon asymmetry of the Universe, the dark matter problem and the neutrino mass generation in minimal extensions of the Standard Model via sterile fermions with (small) total…

高能物理 - 唯象学 · 物理学 2018-03-20 Asmaa Abada , Giorgio Arcadi , Valerie Domcke , Michele Lucente

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…

高能物理 - 唯象学 · 物理学 2015-06-12 Shoichi Kashiwase , 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 2011-11-23 Francois-Xavier Josse-Michaux , Emiliano Molinaro

We introduce a lepton mass generation and flavor mixing model, realized through a (2,3) inverse seesaw structure based on modular \( S_4 \) symmetry. The model employs modular forms to construct the lepton Yukawa couplings, significantly…

高能物理 - 唯象学 · 物理学 2025-09-23 Abhishek , V. Suryanarayana Mummidi

We present a unified framework for neutrino masses, baryogenesis, and dark matter based on a modular $S_4$ symmetry combined with a type-III seesaw mechanism. All Yukawa couplings, CP phases, and flavor textures originate from a single…

高能物理 - 唯象学 · 物理学 2026-02-04 Abhishek , V. Suryanarayana Mummidi

Recently, Qu and Ding, have proposed a formalism where modular invariance is extended to non-supersymmetric scenario considering Yukawa couplings as non-holomorphic functions of modules field $\tau$. Adopting this formalism in this work, we…

高能物理 - 唯象学 · 物理学 2025-08-08 Priya , Labh Singh , B. C. Chauhan , Surender Verma

We present an S$_4$ flavour symmetric model within a minimal seesaw framework resulting in mass matrices that leads to TM$_1$ mixing. Minimal seesaw is realized by adding two right-handed neutrinos to the Standard Model. The model predicts…

高能物理 - 唯象学 · 物理学 2021-12-22 Bikash Thapa , Ng. K. Francis

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…

高能物理 - 唯象学 · 物理学 2009-11-10 W. Grimus , L. Lavoura

In this paper, we analyse resonant leptogenesis in a low scale inverse seesaw model with $A_4$ flavor symmetry, in a model we explored earlier to explain light neutrino masses and mixings, and also charged lepton flavor violating decay…

高能物理 - 唯象学 · 物理学 2023-05-04 Maibam Ricky Devi , Kalpana Bora

Current experimental data allow the zero value for one neutrino mass, either m_1 = 0 or m_3 = 0. This observation implies that a realistic neutrino mass texture can be established by starting from the limit (a) m_1 = m_2 = 0 and m_3 \neq 0…

高能物理 - 唯象学 · 物理学 2008-11-26 Aik Hui Chan , Harald Fritzsch , Shu Luo , Zhi-zhong Xing
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