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Majorons are the Goldstone bosons of spontaneously broken lepton number and hence intimately connected to Majorana neutrino masses. Since all majoron couplings are heavily suppressed by the seesaw scale they are interesting candidates for…

High Energy Physics - Phenomenology · Physics 2018-09-26 Julian Heeck

We revisit the decaying wino dark matter scenario in the light of the updated positron fraction, electron and positron fluxes in cosmic ray recently reported by the AMS-02 collaboration. We show the AMS-02 results favor the mass of the wino…

High Energy Physics - Phenomenology · Physics 2018-05-09 Masahiro Ibe , Shigeki Matsumoto , Satoshi Shirai , Tsutomu T. Yanagida

Brown dwarfs, being transitional objects between giant planets and low-mass stars, possess dense, cool interiors that provide optimal conditions to explore non-standard physics. Capture and accumulation of dark-matter particles can alter…

Solar and Stellar Astrophysics · Physics 2026-05-15 A. Pérez-Garrido

Wherever one talks of dark matter, one does so where there is an observable matter and an associated unsolved dynamical issue to be settled. We promote this observation to the status of an axiom and conjecture that there is a dark companion…

General Relativity and Quantum Cosmology · Physics 2009-03-31 Yousef Sobouti

Dark matter could decay into Standard Model particles producing neutrinos directly or indirectly. The resulting flux of neutrinos from these decays could be detectable at neutrino telescopes and would be associated with massive celestial…

High Energy Astrophysical Phenomena · Physics 2023-08-10 Minjin Jeong , Carsten Rott

From data recently reported from the IceCube telescope, we derive new bounds on the monochromatic neutrino signal produced from dark matter particle decays. In the few TeV to tens of TeV energy range, these bounds turn out to be better than…

High Energy Physics - Phenomenology · Physics 2015-12-23 Chaïmae El Aisati , Michael Gustafsson , Thomas Hambye

We discuss dark matter decay mediated by exotically charged particles ("exotics") in a supersymmetric model with two dark matter (DM) components: One is the (bino-like) lightest supersymmetric particle (LSP) \chi, and the other is a newly…

High Energy Physics - Phenomenology · Physics 2009-05-29 Kyu Jung Bae , Bumseok Kyae

We explore a scenario that the dark matter is a boson condensate created by the misalignment mechanism, in which a spin 0 boson (an axion-like particle) and a spin 1 boson (the dark photon) are considered, respectively. We find that…

High Energy Physics - Phenomenology · Physics 2018-09-25 Qiaoli Yang , Haoran Di

This paper investigates the parameter space of theories with gauge mediated supersymmetry breaking leading to gravitino (cold) dark matter with mass m_{3/2}= 1keV - 10MeV. We pay particular attention to the cosmological role of messenger…

High Energy Physics - Phenomenology · Physics 2009-11-11 Karsten Jedamzik , Martin Lemoine , Gilbert Moultaka

We briefly review the general insight into the indirect searches of dark matter. We discuss the primary equation in a three-level multimessenger approach (gamma rays, neutrinos and antiprotons), and we introduce the reader to the main…

High Energy Astrophysical Phenomena · Physics 2021-04-05 Viviana Gammaldi

WIMPless dark matter offers an attractive framework in which dark matter can be very light. We investigate the implications of such scenarios on invisible decays of bottomonium states for dark matter with a mass less than around $5 {\rm…

High Energy Physics - Phenomenology · Physics 2009-12-06 David McKeen

The recent observation by the PAMELA satellite of a rising positron fraction up to $\sim$ 100 GeV has triggered a considerable amount of putative interpretations in terms of dark matter (DM) annihilation or decay. Here, we make a critical…

Astrophysics of Galaxies · Physics 2014-11-20 Julien Lavalle

I point out that the sterile neutrinos suggested as candidates of "cool" Dark Matter will decay through their mixing with light neutrinos. This leads to an upper bound of about 200 keV on the mass of the sterile neutrinos, but might…

High Energy Physics - Phenomenology · Physics 2007-05-23 Manuel Drees

We have recently proposed a new candidate for baryonic dark matter: very cold molecular gas, in near-isothermal equilibrium with the cosmic background radiation at 2.73 K. The cold gas, of quasi-primordial abundances, is condensed in a…

Astrophysics · Physics 2016-01-27 F. Combes , D. Pfenniger

Composite asymmetric dark matter (ADM) is the framework that naturally explains the coincidence of the baryon density and the dark matter density of the Universe. Through a portal interaction sharing particle-antiparticle asymmetries in the…

High Energy Physics - Phenomenology · Physics 2025-08-07 Saikat Das , Ayuki Kamada , Takumi Kuwahara , Kohta Murase , Deheng Song

The lightest electroweak baryon as a topological object is investigated by using a general effective Lagrangian of composite electroweak symmetry breaking and the spin-independent electroweak baryon-nucleon scattering cross section is…

High Energy Physics - Phenomenology · Physics 2017-02-17 Yong-Liang Ma

In the context of Twin Higgs models, we study a simple mechanism that simultaneously generates asymmetries in the dark and visible sector through the out-of-equilibrium decay of a TeV scale particle charged under a combination of baryon and…

High Energy Physics - Phenomenology · Physics 2016-08-24 Marco Farina , Angelo Monteux , Chang Sub Shin

The cold dark matter may be in a meta-stable state and decays to other particles with a very long lifetime. If the decaying products of the dark matter are weakly interacting, e.g. neutrinos, then it would have little impact on…

Astrophysics · Physics 2008-11-26 Yan Gong , Xuelei Chen

We propose a simple model in which the baryon asymmetry and dark matter are created via the decays and inverse decays of QCD-triplet scalars, at least one of which must be in the TeV mass range. Singlet fermions produced in these decays…

High Energy Physics - Phenomenology · Physics 2020-07-01 Brian Shuve , David Tucker-Smith

We confront a non-relativistic Bose--Einstein Condensate (BEC) model of light bosons interacting gravitationally either through a Newtonian or a Yukawa potential with the observed rotational curves of $12$ dwarf galaxies. The baryonic…

Cosmology and Nongalactic Astrophysics · Physics 2019-05-14 Emma Kun , Zoltán Keresztes , Saurya Das , László Á. Gergely
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