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A scenario that relates the abundance of dark matter to the baryon asymmetry of the Universe is presented. In this scenario, based on a left-right extension of the Standard Model, dark matter is made of light, ~ 1 GeV, right-handed Majorana…

High Energy Physics - Phenomenology · Physics 2007-05-23 Michel H. G. Tytgat

The nature of dark matter is one of the most pressing questions in modern cosmology. Much work has been focussed in the past upon probing potential particle dark matter via gamma-rays resulting from its annihilation or decay. These processs…

High Energy Astrophysical Phenomena · Physics 2019-12-09 Geoff Beck

Recent observations of a large excess of cosmic-ray positrons at high energies have raised a lot of interest in leptonic decay modes of dark matter particles. Nevertheless, dark matter particles in the Milky Way halo could also decay…

High Energy Physics - Phenomenology · Physics 2009-11-19 Alejandro Ibarra , David Tran

Dark matter annihilation is one of the leading explanations for the recently observed $e^\pm$ excesses in cosmic rays by PAMELA, ATIC, FERMI-LAT and HESS. Any dark matter annihilation model proposed to explain these data must also explain…

High Energy Physics - Phenomenology · Physics 2010-04-29 Xiao-Jun Bi , Xiao-Gang He , Ernest Ma , Juan Zhang

It is possible that the strongest interactions between dark matter and the Standard Model occur via the neutrino sector. Unlike gamma rays and charged particles, neutrinos provide a unique avenue to probe for astrophysical sources of dark…

High Energy Physics - Phenomenology · Physics 2023-11-07 Carlos A. Argüelles , Diyaselis Delgado , Avi Friedlander , Ali Kheirandish , Ibrahim Safa , Aaron C. Vincent , Henry White

We consider supersymmetric models in which the right-handed sneutrino is a viable WIMP dark matter candidate. These are either simple extensions of the Minimal Supersymmetric Standard Model or models with the addition of an extra U(1)…

High Energy Physics - Phenomenology · Physics 2012-09-10 Valentina De Romeri

We discuss the possibility of light scalar dark matter generated by right-handed neutrino in a $L_{\mu}-L_{\tau}$ model, in which the dark matter $\phi_{dm}$ carries $U(1)_{L_{\mu}-L_{\tau}}$ charge but it is a singlet in the Standard…

High Energy Physics - Phenomenology · Physics 2023-09-12 XinXin Qi , Hao Sun

It has been pointed out in ref.[1] that in the nuMSM (Standard Model extended by three right-handed neutrinos with masses smaller than the electroweak scale), there is a corner in the parameter space where CP-violating resonant oscillations…

High Energy Physics - Phenomenology · Physics 2009-01-06 M. Laine , M. Shaposhnikov

The decay of dark matter particles which are coupled predominantly to charged leptons has been proposed as a possible origin of excess high-energy positrons and electrons observed by cosmic-ray telescopes PAMELA and Fermi LAT. Even though…

High Energy Physics - Phenomenology · Physics 2015-03-17 Mathias Garny , Alejandro Ibarra , David Tran , Christoph Weniger

We consider supersymmetric models with right-handed neutrinos where neutrino masses are purely Dirac-type. In this model, right-handed sneutrino can be the lightest supersymmetric particle and can be a viable candidate of cold dark matter…

High Energy Physics - Phenomenology · Physics 2009-11-11 Takehiko Asaka , Koji Ishiwata , Takeo Moroi

We study a scenario that a hidden gaugino dark matter decays into the standard-model particles (and their supersymmetric partners) through a kinetic mixing with the gaugino of a U(1)B-L broken at a scale close to the grand unification…

High Energy Physics - Phenomenology · Physics 2010-02-02 Satoshi Shirai , Fuminobu Takahashi , T. T. Yanagida

Recent observations of lepton cosmic rays, coming from the PAMELA and FERMI experiments, have pushed our understanding of the interstellar medium and cosmic rays sources to unprecedented levels. The imprint of dark matter on lepton cosmic…

High Energy Astrophysical Phenomena · Physics 2011-01-27 Roberto A. Lineros

A triplet dark matter candidate from thermal leptogenesis is considered with building a model. The model is based on the standard two Higgs doublet model and seesaw mechanism with Higgs triplets. The parameters (couplings and masses) are…

High Energy Physics - Phenomenology · Physics 2014-04-24 Jae Ho Heo , C. S. Kim

We have shown that inflatons with a mass which is calculated to be of the order of $10^{10}\GeV$ can constitute a dominant part of dark matter. They can decay uniquely into a neutrino and antineutrino with a lifetime calculated to be…

Astrophysics · Physics 2007-05-23 Saul Barshay , Georg Kreyerhoff

We discuss asymmetric or symmetric dark matter candidate in the supersymmetric Dirac leptogenesis scenario. By introducing a singlet superfield coupling to right-handed neutrinos, the overabundance problem of dark matter can be evaded and…

High Energy Physics - Phenomenology · Physics 2015-06-12 Ki-Young Choi , Eung Jin Chun , Chang Sub Shin

A right-handed neutrino is a promising candidate for dark matter (DM) which has no interaction with nuclei. Since two right-handed neutrinos explain neutrino oscillation data and baryon number asymmetry through both the seesaw mechanism and…

High Energy Physics - Phenomenology · Physics 2026-02-17 Daijiro Suematsu

We study the properties of the right-handed sneutrino and its viability as a WIMP dark matter candidate in an extended version of the NMSSM in which a right-handed neutrino superfield is included with a coupling to the singlet Higgs in…

High Energy Physics - Phenomenology · Physics 2009-09-28 David G. Cerdeno , Osamu Seto

We investigate the possibility that dark matter and the baryon asymmetry of the Universe are generated by the same mechanism, following an idea initially proposed by V.A. Kuzmin and recently discussed by R. Kitano and I. Low. In our model,…

High Energy Physics - Phenomenology · Physics 2009-11-11 Nicolas Cosme , Laura Lopez Honorez , Michel H. G. Tytgat

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…

High Energy Physics - Phenomenology · Physics 2014-11-20 Pei-Hong Gu , Ernest Ma , Utpal Sarkar

The Galactic positrons, as observed by their annihilation gamma-ray line at 0.511 MeV, are difficult to account for with astrophysical sources. It has been proposed that they are produced instead by dark matter annihilation or decay in the…

Astrophysics · Physics 2009-07-09 John F. Beacom , Nicole F. Bell , Gianfranco Bertone