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相关论文: Majorana Dark Matter

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We analyse how dark matter (DM) can be produced in the early universe, working in the framework of a hidden sector charged under a U(1)' gauge symmetry and interacting with the Standard Model through kinetic mixing. Depending on the masses…

高能物理 - 唯象学 · 物理学 2019-11-27 Thomas Hambye , Michel H. G. Tytgat , Jérôme Vandecasteele , Laurent Vanderheyden

We present a new model for radiatively generating Majorana active neutrino masses while incorporating a viable dark matter candidate. This is possible by extending the Standard Model with a single Majorana neutrino endowed with a dark…

高能物理 - 唯象学 · 物理学 2015-06-16 John N. Ng , Alejandro de la Puente

We consider the singlet Majoron model with softly broken lepton number. This model contains three right-handed neutrinos and a singlet scalar besides the standard model fields. The real part of the singlet scalar develops a vacuum…

高能物理 - 唯象学 · 物理学 2014-11-20 Pei-Hong Gu , Ernest Ma , Utpal Sarkar

The production rate of heavy Majorana neutrinos is relevant for models of thermal leptogenesis in the early Universe. In the high temperature limit the production can proceed via the 1 <-> 2 (inverse) decays which are allowed by the thermal…

高能物理 - 唯象学 · 物理学 2011-04-04 Alexey Anisimov , Denis Besak , Dietrich Bodeker

We present a realistic, simple and natural model of strongly-interacting dark matter based on the neutrino-portal paradigm. The strong interactions at small velocities are generated by the exchange of dark photons, and produce the observed…

高能物理 - 唯象学 · 物理学 2021-01-20 J. M. Lamprea , E. Peinado , S. Smolenski , J. Wudka

This work considers the following problem: what type (Dirac or Majorana) of neutrinos is produced in standard weak interactions? It is concluded that only Dirac neutrinos but not Majorana neutrinos can be produced in these interactions. It…

综合物理 · 物理学 2009-12-02 Kh. M. Beshtoev

A mechanism is presented, in which the mixing of right handed heavy Majorana neutrinos creates a $CP-$asymmetric universe. When these Majorana neutrinos subsequently decay more leptons than anti-leptons are produced. The lepton asymmetry…

高能物理 - 唯象学 · 物理学 2009-10-28 Marion Flanz , Emmanuel A. Paschos , Utpal Sarkar , Jan Weiss

In the introductory part we briefly consider basics of neutrino oscillations and convenient phenomenology of neutrino oscillations in vacuum. Main part of this report is dedicated to a discussion of a plausible BSM scenarios of neutrino…

高能物理 - 唯象学 · 物理学 2020-10-13 S. M. Bilenky

The nature of dark matter is one of the open problems of the Standard Model of particle physics. Despite the great experimental efforts, we have not yet found a positive signal of its interactions with ordinary matter. One possible…

高能物理 - 唯象学 · 物理学 2019-04-09 M. Blennow , E. Fernández-Martínez , A. Olivares-Del Campo , S. Pascoli , S. Rosauro-Alcaraz , A. V. Titov

We propose a new production mechanism for keV sterile neutrino dark matter which relies neither on the oscillations between sterile and active neutrinos nor on the decay of additional heavier particles. The dark matter neutrinos are instead…

高能物理 - 唯象学 · 物理学 2022-11-02 Carlos Jaramillo

Dark matter has been recognized as an essential part of matter for over 70 years now, and many suggestions have been made, what it could be. Most of these ideas have centered on Cold Dark Matter, particles that are predicted in extensions…

天体物理学 · 物理学 2016-11-15 Peter L. Biermann , Faustin Munyaneza

Standard Model predictions for Majorana neutrino transition magnetic moments (TMMs) are subject to severe chiral and GIM-like suppressions, rendering them vanishingly small. To dynamically generate a macroscopic TMM, we propose a dark…

高能物理 - 唯象学 · 物理学 2026-03-27 Haohao Zhang

We investigate the possibility that dark matter is made of heavy Dirac neutrinos with mass in the range [O(1) GeV- a few TeV] and with suppressed but non-zero coupling to the Standard Model Z as well as a coupling to an additional Z' gauge…

高能物理 - 唯象学 · 物理学 2009-01-06 Genevieve Belanger , Alexander Pukhov , Geraldine Servant

With the motivation of simultaneously explaining dark matter and neutrino masses, mixing angles, we have invoked the Type-II seesaw model extended by an extra $SU(2)$ doublet $\Phi$. Moreover, we have imposed a $\mathbb{Z}_2$ parity on…

高能物理 - 唯象学 · 物理学 2019-06-07 Anirban Biswas , Avirup Shaw

A sterile neutrino is a well-motivated and widely studied dark matter candidate. The most straightforward realization of sterile neutrino dark matter, through the Dodelson-Widrow mechanism, is now ruled out by a combination of X-ray and…

高能物理 - 唯象学 · 物理学 2016-03-16 Bibhushan Shakya

We propose a new mechanism to generate the neutrino Majorana mass in TeV-scale gravity models. The black hole violates all non-gauged symmetries and can become the origin of lepton number violating processes. The fluctuation of…

高能物理 - 唯象学 · 物理学 2007-05-23 Yosuke Uehara

Late decays of dark matter to a lighter, warm dark matter component are a known way to reduce the amplitude of the matter power spectrum on scales of $8$ Mpc. However, only very few particle physics models have been put forward that exhibit…

高能物理 - 唯象学 · 物理学 2025-12-01 María Dias Astros , Lukáš Gráf , Stefan Vogl

Minimal Dark Matter (MDM) stands as one of the simplest dark matter scenarios. In MDM models, annihilation and co-annihilation processes among the members of the MDM multiplet are usually very efficient, pushing the dark matter mass above…

高能物理 - 唯象学 · 物理学 2015-10-01 Mayumi Aoki , Takashi Toma , Avelino Vicente

We evaluate the predictive power of the neutrino mass matrices arising from seesaw mechanism with heavy Majorana mass matrices subject to texture zero and satisfy a cyclic permutation invariant form to the solar neutrino mixing phenomena.…

高能物理 - 唯象学 · 物理学 2010-09-21 Asan Damanik , Mirza Satriawan , Pramudita Anggraita , Arief Hermanto , Muslim

The simplest possibility to generate small Majorana neutrino masses is the seesaw mechanism. However, the smallness of the observed neutrino masses can also be understood, if neutrino masses are generated by higher-dimensional operators…

高能物理 - 唯象学 · 物理学 2020-05-20 Ricardo Cepedello , Renato Fonseca , Martin Hirsch