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We describe cosmic gamma-ray and neutrino signals of dark matter annihilation, explaining how the complementarity of these signals provides additional information that, if observable, can enlighten the particle nature of dark matter. This…

High Energy Physics - Phenomenology · Physics 2013-05-30 Rouzbeh Allahverdi , Sheldon Campbell , Bhaskar Dutta

A dynamical mechanism, based on a confining non-abelian dark symmetry, which generates Majorana masses for hypercharge-less fermions, is proposed. We apply it to the inverse seesaw scenario, which allows to generate light neutrino masses…

High Energy Physics - Phenomenology · Physics 2024-08-08 Maximilian Berbig , Juan Herrero-Garcia , Giacomo Landini

We perform a detailed and quasi model-independent analysis of direct annihilation of Dark Matter into neutrinos. Considering different cases for scalar and fermionic Dark Matter, we identify several settings in which this annihilation is…

High Energy Physics - Phenomenology · Physics 2011-01-20 Manfred Lindner , Alexander Merle , Viviana Niro

We propose a scenario with a fermion dark matter, where the dark matter particle used to be the Dirac fermion, but it takes the form of the Majorana fermion at a late time. The relic number density of the dark matter is determined by the…

High Energy Physics - Phenomenology · Physics 2015-06-05 Nobuchika Okada , Osamu Seto

Although the standard {\Lambda}CDM model describes the cosmic microwave background radiation and the large scale structure of the Universe with great success, it has some tensions with observations in the effective number of neutrino…

High Energy Physics - Phenomenology · Physics 2012-11-26 Kiwoon Choi , Ki-Young Choi , Chang Sub Shin

Generating small sterile neutrino masses via the same seesaw mechanism that suppresses active neutrino masses requires a specific structure in the neutral fermion mass matrix. We present a model where this structure is enforced by a new…

High Energy Physics - Phenomenology · Physics 2013-06-03 Julian Heeck , He Zhang

Dark matter may be coupled to dark radiation: light degrees of freedom that mediate forces between dark sector particles. Cosmological constraints favor dark radiation that is colder than Standard Model radiation. In models with fixed…

High Energy Physics - Phenomenology · Physics 2016-10-12 Matthew Reece , Thomas Roxlo

We propose a simple scenario in which dark matter (DM) emerges as a stable neutral hadronic thermal relics, its stability following from an exact $\operatorname{U}(1)_D$ symmetry. Neutrinos pick up radiatively induced Majorana masses from…

High Energy Physics - Phenomenology · Physics 2018-06-27 M. Reig , D. Restrepo , J. W. F. Valle , O. Zapata

We study in detail the conditions to generate the baryon asymmetry of the universe from the annihilation of dark matter. This scenario requires a low energy mechanism for thermal baryogenesis, hence we first discuss some of these mechanisms…

High Energy Physics - Phenomenology · Physics 2015-06-16 Nicolas Bernal , Stefano Colucci , Francois-Xavier Josse-Michaux , J. Racker , Lorenzo Ubaldi

We present a simple mechanism which allows the simultaneous generation of the baryon asymmetry of the Universe along with its dark matter content. To this goal, we employ the out-of-equilibrium decays of heavy bath states into a feebly…

High Energy Physics - Phenomenology · Physics 2022-02-17 Andreas Goudelis , Pantelis Papachristou , Vassilis C. Spanos

We study neutrino and dark matter based on a gauged $U(1)_R$ symmetry in a framework of radiative seesaw scenario. Identifying dark matter as a bosoninc particle, it interacts with quark and lepton sectors through vector-like heavier quark…

High Energy Physics - Phenomenology · Physics 2021-05-27 Keiko I. Nagao , Hiroshi Okada

In this letter in the framework of a simple see-saw scenario with two (or three) quasi degenerate Majorana neutrinos we propose that one of these neutrinos can be very weakly coupled, yet there is a mechanism of the generation of the…

High Energy Physics - Phenomenology · Physics 2016-11-09 Alexey Anisimov

In some dark matter models, the coupling of the dark matter particle to the standard model Higgs determines the dark matter relic density while it is also consistent with dark matter direct detection experiments. On the other hand, the…

High Energy Physics - Phenomenology · Physics 2010-11-09 Adisorn Adulpravitchai , Pei-Hong Gu , Manfred Lindner

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

We review the annihilation of dark matter into neutrinos over a range of dark matter masses from MeV$/c^2$ to ZeV$/c^2$. Thermally-produced models of dark matter are expected to self-annihilate to standard model products. As no such signal…

High Energy Physics - Phenomenology · Physics 2021-09-22 Carlos A. Argüelles , Alejandro Diaz , Ali Kheirandish , Andrés Olivares-Del-Campo , Ibrahim Safa , Aaron C. Vincent

Self-Destructing Dark Matter (SDDM) is a class of dark sector models in which the collision of a dark sector particle with the earth induces its prompt decay into Standard Model particles, generating unique signals at neutrino detectors.…

High Energy Physics - Phenomenology · Physics 2021-08-18 Michael Geller , Ofri Telem

Antideuterons and antihelium nuclei in the cosmic-ray spectrum have long been considered a smoking gun signature of dark matter annihilation, making the tentative observation of several such events by AMS highly intriguing. Conventional…

High Energy Physics - Phenomenology · Physics 2026-03-16 Caleb Gemmell , Dan Hooper , Seth Koren , Fabrizio Vassallo

We investigate observable cosmological aspects of sterile neutrino dark matter produced via the freeze-in mechanism. The study is performed in a framework that admits many cosmologically interesting variations: high temperature production…

High Energy Physics - Phenomenology · Physics 2017-06-15 Samuel B. Roland , Bibhushan Shakya

We examine the cosmology of warm dark matter (WDM), both stable and decaying, from the point of view of structure formation. We compare the matter power spectrum associated to WDM masses of 1.5 keV and 0.158 keV, with that expected for the…

Cosmology and Nongalactic Astrophysics · Physics 2018-12-18 Jui-Lin Kuo , Massimiliano Lattanzi , Kingman Cheung , José W. F. Valle

The observations and research on the neutrinos provide a kind of indirect way of revealing the properties of dark matter particles. For the detection of muon neutrinos, the main issue is the large atmospheric background, which is caused by…

Cosmology and Nongalactic Astrophysics · Physics 2017-12-06 Yupeng Yang , Yan Qin