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相关论文: Neutrino Masses from Loop-Induced Dirac Yukawa Cou…

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In a recent Letter we presented a systematic way of testing the seesaw origin of neutrino mass in the context of the Minimal Left-Right Symmetric Model. The essence of the program is to exploit lepton number violating decays of doubly…

高能物理 - 唯象学 · 物理学 2019-12-25 Goran Senjanovic , Vladimir Tello

The seesaw mechanism explains the exclusive smallness of neutrino masses by the presence of very heavy Majorana masses and leads to the appearance of Majorana particles and to the direct lepton number violation. The author proposes a seesaw…

高能物理 - 唯象学 · 物理学 2020-04-07 Igor T. Dyatlov

We prove in this paper that the electro-weak SU(4)L x U(1)X gauge models with spontaneous symmetry breaking can offer a natural framework for generating neutrino masses by simply exploiting the tree level realization of dimension-five…

高能物理 - 唯象学 · 物理学 2015-06-03 Adrian Palcu

In the context of Standard Model (SM) extensions, the seesaw mechanism provides the most natural explanation for the smallness of neutrino masses. In this work we consider the most economical type-I seesaw realization in which two…

高能物理 - 唯象学 · 物理学 2018-06-20 D. M. Barreiros , R. G. Felipe , F. R. Joaquim

The neutrinophilic two Higgs doublet model is one of the simplest models to explain the origin of tiny Dirac neutrino masses. This model introduces a new Higgs doublet with eV scale VEV to naturally generate the tiny neutrino masses.…

高能物理 - 唯象学 · 物理学 2023-11-14 Wan-Lun Xu , Zhi-Long Han , Yi Jin , Honglei Li , Zongyang Lu , Zhao-Xia Meng

The Dirac masses of neutrinos can exhibit a strong hierarchy even if the Majorana masses of the right-handed neutrinos are degenerate and the hierarchy of the mass scales governing the oscillations of solar and atmospheric neutrinos is…

高能物理 - 唯象学 · 物理学 2009-11-07 M. Jezabek , P. Urban

The small neutrino mass observed in neutrino oscillations is nicely explained by the seesaw mechanism. Rich phenomenology is generally expected if the heavy neutrinos are not much heavier than the electroweak scale. A model with this…

高能物理 - 唯象学 · 物理学 2008-11-26 Jian-Ping Bu , Yi Liao , Ji-Yuan Liu

We study sterile neutrino dark matter in a minimal Type-I Dirac seesaw framework where the states responsible for generating Dirac neutrino masses at tree level can be viable dark matter candidates. A $\mathcal{Z}_6$ symmetry, spontaneously…

高能物理 - 唯象学 · 物理学 2026-03-23 J. Adhikary , A. Batra , K. Deka , F. R. Joaquim

We propose a new scenario where neutrino masses are generated via operators with the mass dimension higher than five, which are induced at the loop level. The scenario is demonstrated with concrete models where neutrino masses are generated…

高能物理 - 唯象学 · 物理学 2010-11-22 Shinya Kanemura , Toshihiko Ota

We implement Dirac neutrinos in the minimal custodial Randall-Sundrum setting via the Krauss-Wilczek mechanism. We demonstrate by giving explicit lepton mass matrices that with neutrinos in the normal hierarchy, lepton mass and mixing…

高能物理 - 唯象学 · 物理学 2010-01-07 We-Fu Chang , John N. Ng , Jackson M. S. Wu

Minimal Flavour Violation can be realized in several ways in the lepton sector due to the possibility of Majorana neutrino mass terms. We derive the scalar potential for the fields whose background values are the Yukawa couplings, for the…

高能物理 - 唯象学 · 物理学 2015-06-05 R. Alonso , M. B. Gavela , D. Hernández , L. Merlo

Mixing between light and heavy neutrino states has been proposed as an explanation (or partial explanation) for the 3-sigma NuTeV anomaly and the 2-sigma departure of the $Z^0$ invisible width from its expected value. I assume herein that…

高能物理 - 唯象学 · 物理学 2016-09-06 Sheldon Lee Glashow

A new solution to the strong CP problem with distinct experimental signatures at the LHC is proposed. It is based on the Yukawa interactions between mirror quarks, Standard Model (SM) quarks and Higgs singlets. (Mirror quarks and leptons…

高能物理 - 唯象学 · 物理学 2017-04-28 P. Q. Hung

We study the correlation between the neutrino oscillation and the production/decay of the lightest supersymmetric particle(LSP) in the context of the minimal supergravity model(mSUGRA) without R-parity. We show how the neutrino masses and…

高能物理 - 唯象学 · 物理学 2007-05-23 Eung Jin Chun , Dong-Won Jung , Sin Kyu Kang , Jong Dae Park

We study neutrino masses and mixing in Supersymmetric Models without $R$ parity and with generic soft Supersymmetry breaking terms. Neutrinos acquire mass from various sources: tree level neutrino--neutralino mixing, loop effects and…

高能物理 - 唯象学 · 物理学 2009-10-28 Francesca M. Borzumati , Yuval Grossman , Enrico Nardi , Yosef Nir

We investigate the neutrino masses and mixing patten in a version of the $SU(3)_c\otimes SU(3)_L\otimes U(1)_X$ model with one extra exotic charged lepton per family as introduced by Ozer. It is shown that an extended scalar sector,…

高能物理 - 唯象学 · 物理学 2008-11-26 William A. Ponce , Oscar Zapata

The notion of U(1) lepton number (which may only be softly broken) is applied to models of dark matter which interacts with leptons. Previous scotogenic models of Majorana or Dirac neutrino mass are shown to be derivable in this framework…

高能物理 - 唯象学 · 物理学 2020-09-02 Ernest Ma

We show a TeV-scale seesaw model where Majorana neutrino masses, the dark matter mass, and stability of the dark matter can be all originated from the U(1)_{B-L} gauge symmetry. Dirac mass terms for neutrinos are forbidden at the tree level…

高能物理 - 唯象学 · 物理学 2013-05-30 Shinya Kanemura , Takehiro Nabeshima , Hiroaki Sugiyama

Tiny neutrino masses can arise naturally via loop diagrams. After a brief review of the radiative mass generation mechanism, I present a new model wherein TeV scale leptoquark scalars induce neutrino masses via two--loop diagrams. This…

高能物理 - 唯象学 · 物理学 2015-03-19 K. S. Babu

Weak bases of flavors (u, c), (d,s), (e, \mu), (\nu_e,\nu_\mu) are assumed as the S_3 doublet and t, b, \tau, {\nu_\tau} are the S_3 singlet and further there are assumed S_3 doublet Higgs (H_1, H_2) and S_3 singlet Higgs H_S. We suggest an…

高能物理 - 唯象学 · 物理学 2011-08-08 Tadayuki Teshima , Yoshitaka Okumura
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