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相关论文: Minimal dark matter models with radiative neutrino…

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We analyze the prospects for light neutralino dark matter in the minimal supersymmetric model extended by a $U(1)$ gauge group. We allow the neutralino to be an arbitrary admixture of singlet and doublet higgsinos, as well as of the three…

高能物理 - 唯象学 · 物理学 2014-10-22 Mariana Frank , Subhadeep Mondal

We study a gauged $B-L$ extension of the standard model where the new fermions with fractional $B-L$ charges that play the role of keeping the model anomaly free can also explain the origin of neutrino mass at one loop level as well as dark…

高能物理 - 唯象学 · 物理学 2017-12-27 Dibyendu Nanda , Debasish Borah

With the advent of new and more sensitive direct detection experiments, scope for a thermal WIMP explanation of dark matter (DM) has become extremely constricted. The non-observation of thermal WIMP in these experiments has put a strong…

高能物理 - 唯象学 · 物理学 2016-09-28 Anirban Biswas , Aritra Gupta

It is well known that the differences between the lepton numbers can be gauged with the Standard Model matter content. Such extended gauge theories, dubbed as the gauged U(1)$_{L_\alpha - L_\beta}$ models, have been widely discussed so far…

高能物理 - 唯象学 · 物理学 2019-03-29 Kento Asai , Koichi Hamaguchi , Natsumi Nagata , Shih-Yen Tseng , Koji Tsumura

Little Higgs models are formulated as effective theories with a cut-off of up to 100 times the electroweak scale. Neutrino masses are then a puzzle, since the usual see-saw mechanism involves a much higher scale that would introduce…

高能物理 - 唯象学 · 物理学 2009-11-11 F. del Aguila , M. Masip , J. L. Padilla

Knowledge of the mechanism of neutrino mass generation would help understand a lot more about Lepton Number Violation (LNV), the cosmological evolution of the Universe, or the evolu tion of astronomical objects. Here we propose a verifiable…

高能物理 - 唯象学 · 物理学 2020-03-18 Claudio Dib , Sergey Kovalenko , Ivan Schmidt , Adam Smetana

In this work, we interpret the 3-3-1-1 model when the B-L and 3-3-1 breaking scales behave simultaneously as the inflation scale. This setup not only realizes the previously-achieved consequences of inflation and leptogenesis, but also…

高能物理 - 唯象学 · 物理学 2017-04-04 D. T. Huong , P. V. Dong

Standard Model with right handed neutrinos charged under additional $U(1)_{B-L}$ gauge symmetry offer solutions to both dark matter (DM) problem and neutrino mass generation, although constrained severely from relic density, direct search…

高能物理 - 唯象学 · 物理学 2020-04-15 Subhaditya Bhattacharya , Nabarun Chakrabarty , Rishav Roshan , Arunansu Sil

The type-I seesaw Lagrangian yields a non-generic set of active-sterile oscillation parameters - the neutrino mass eigenvalues and the physical elements of the full mixing matrix are entwined. For this reason one is able to, in principle,…

高能物理 - 唯象学 · 物理学 2013-05-30 Andre de Gouvea , Wei-Chih Huang

We investigate the sensitivity of relic neutrino detection methods within the Standard Model, extended to include right-chiral neutrino singlets with Majorana mass terms. In particular, we study neutrino capture on unstable nuclei, the…

高能物理 - 唯象学 · 物理学 2025-09-08 Yuber F. Perez-Gonzalez , Jack D. Shergold

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 propose a model with an $U(1)_{B-L}$ gauge symmetry, in which small neutrino masses, dark matter and the matter-antimatter asymmetry in the Universe can be simultaneously explained. In particular, the neutrino masses are generated…

高能物理 - 唯象学 · 物理学 2018-02-19 Chao-Qiang Geng , Hiroshi Okada

We propose a model where neutrino masses are generated at three loop order but neutrinoless double beta decay occurs at one loop. Thus we can have large neutrinoless double beta decay observable in the future experiments even when the…

高能物理 - 唯象学 · 物理学 2018-06-21 Julien Alcaide , Dipankar Das , Arcadi Santamaria

We propose a minimal predictive scenario for dark matter and radiative neutrino mass where the relic abundance of dark matter is generated from a hybrid setup comprising of both thermal freeze-out as well as non-thermal freeze-in…

高能物理 - 唯象学 · 物理学 2018-09-11 Anirban Biswas , Debasish Borah , Dibyendu Nanda

We consider the possibility of neutrinos being Dirac particles and study minimal mass matrices with as much zero entries as possible. We find that up to 5 zero entries are allowed. Those matrices predict one vanishing mass state, CP…

高能物理 - 唯象学 · 物理学 2010-02-03 C. Hagedorn , W. Rodejohann

We present a class of models with radiative neutrino mass and stable dark-matter candidates. Neutrino mass is generated by a one-loop diagram with the same topography as Ma's 2006 proposal (which used an inert scalar-doublet and singlet…

高能物理 - 唯象学 · 物理学 2015-06-16 Sandy S. C. Law , Kristian L. McDonald

The minimal seesaw extension of the Standard SU(3) x SU(2) x U(1) Model requires two electroweak singlet fermions in order to accommodate the neutrino oscillation parameters at tree level. Here we consider a next to minimal extension where…

高能物理 - 唯象学 · 物理学 2013-11-05 M. Hirsch , R. A. Lineros , S. Morisi , J. Palacio , N. Rojas , J. W. F. Valle

We present a model that generates small neutrino masses at three-loop level due to the existence of Majorana fermionic dark matter, which is stabilized by a Z2 symmetry. The model predicts that the lightest neutrino is massless. We show a…

高能物理 - 唯象学 · 物理学 2018-05-09 Li-Gang Jin , Rui Tang , Fei Zhang

We look for predictive flavour patterns of the effective Majorana neutrino mass matrix that are compatible with current neutrino oscillation data. Our search is based on the assumption that the neutrino mass matrix contains equal elements…

高能物理 - 唯象学 · 物理学 2016-04-20 Luis M. Cebola , David Emmanuel-Costa , Ricardo Gonzalez Felipe

After discovery of the Higgs boson at CERN the Standard Model acquired a status of the theory of the elementary particles in the electroweak range (up to about 300 GeV). What general conclusions can be inferred from the Standard Model? It…

高能物理 - 唯象学 · 物理学 2015-01-05 S. M. Bilenky