English
Related papers

Related papers: Dark Matter as a weakly coupled Dark Baryon

200 papers

A component of the dark matter could consist of two darkly charged particles with a large mass ratio and a massless force carrier. This `atomic' dark sector could behave much like the baryonic sector, cooling and fragmenting down to…

Astrophysics of Galaxies · Physics 2018-07-04 Akshay Ghalsasi , Matthew McQuinn

Ordinary baryonic particles (such as protons and neutrons) account for only one-sixth of the total matter in the Universe. The remainder is a mysterious "dark matter" component, which does not interact via electromagnetism and thus neither…

Dark Matter constitutes most of the matter in the presently accepted cosmological model for our Universe. The extreme conditions of ordinary baryonic matter, namely high density and compactness, in Neutron Stars make these objects suitable…

High Energy Astrophysical Phenomena · Physics 2017-10-20 M. Cermeño , M. Ángeles Pérez-García , Joseph Silk

A baryonic bound state with a mass of O(100) TeV, which is composed of strongly interacting messenger quarks in the low scale gauge mediation, can naturally be the cold dark matter. Interestingly, we find that such a baryonic dark matter is…

High Energy Physics - Phenomenology · Physics 2010-01-15 Koichi Hamaguchi , Eita Nakamura , Satoshi Shirai , T. T. Yanagida

We propose a novel class of Dark Matter (DM) candidates in the form of a heavy composite Axion-Like Particle (ALP) with highly suppressed electromagnetic interactions populating vast yet unexplored domains in the ALP parameter space. This…

High Energy Physics - Phenomenology · Physics 2025-07-10 Pierluca Carenza , Roman Pasechnik , Zhi-Wei Wang

A new dark sector consisting of a pure non-abelian gauge theory has no renormalizable interaction with SM particles, and can thereby realise gravitational Dark Matter (DM). Gauge interactions confine at a scale $\Lambda_{\rm DM}$ giving…

High Energy Physics - Phenomenology · Physics 2021-03-22 Christian Gross , Sotirios Karamitsos , Giacomo Landini , Alessandro Strumia

Although well established observations on cosmological, cluster, and galactic scales strongly suggest the existence of dark matter (DM), our understanding of its non-gravitational properties is still lacking. I review basic aspects of…

High Energy Physics - Phenomenology · Physics 2010-08-04 Marco Regis

The minimal standard model of quarks and leptons is extended with a set of vectorlike fermions to allow baryon number $B$ to become a gauged $U(1)_B$ symmetry. The $B$ assignments of the new particles are determined by renormalizable…

High Energy Physics - Phenomenology · Physics 2021-01-13 Ernest Ma

The available data on large scale structures seem to favour models with mixed dark matter (MDM), i.e. with a hot and cold component in a rather well--defined amount, or with some form of ``warm" dark matter. I discuss some prospects for…

High Energy Physics - Phenomenology · Physics 2016-09-01 A. Masiero

The cosmological origin of both dark and baryonic matter can be explained through a unified mechanism called hylogenesis where baryon and antibaryon number are divided between the visible sector and a GeV-scale hidden sector, while the…

High Energy Physics - Phenomenology · Physics 2012-12-04 Nikita Blinov , David E. Morrissey , Kris Sigurdson , Sean Tulin

In gauge-mediated theories supersymmetry breaking originates in a strongly interacting sector and is communicated to the ordinary sparticles via SU(3)$\times$SU(2)$\times$U(1) carrying ``messenger'' particles. Stable baryons of the strongly…

High Energy Physics - Phenomenology · Physics 2009-10-28 S. Dimopoulos , G. F. Giudice , A. Pomarol

We investigate scenarios in which dark matter is stabilized by an abelian Z_N discrete gauge symmetry. Models are surveyed according to symmetries and matter content. Multi-component dark matter arises when N is not prime and Z_N contains…

High Energy Physics - Phenomenology · Physics 2011-02-18 Brian Batell

Dark matter could be a baryonic composite of strongly-coupled constituents transforming under SU(2)$_L$. We classify the SU(2)$_L$ representations of baryons in a class of simple confining dark sectors and find that the lightest state can…

High Energy Physics - Phenomenology · Physics 2024-12-20 Pouya Asadi , Austin Batz , Graham D. Kribs

We propose a simple theory for the idea that cosmological dark matter (DM) may be present today mainly in the form of stable neutral hadronic thermal relics. In our model neutrino masses arise radiatively from the exchange of colored DM…

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

As cosmology has entered a phase of precision experiments, the content of the universe has been established to contain interesting and not yet fully understood components, namely dark energy and dark matter. While the cause and exact nature…

High Energy Physics - Phenomenology · Physics 2015-06-25 Lars Bergstrom

It is conjectured that dark matter (DM) was produced before inflation from neutral particles present after the Big Bang and survived inflation due to a specific coupling with gravitation, while the charged particles existing after the Big…

High Energy Physics - Phenomenology · Physics 2017-03-07 Richard M. Weiner

Dark sector particles at the GeV scale carrying baryon number provide an attractive framework for understanding the origin of dark matter and the matter-antimatter asymmetry of the universe. We demonstrate that dark decays of hadronic…

High Energy Physics - Phenomenology · Physics 2022-06-08 Gonzalo Alonso-Álvarez , Gilly Elor , Miguel Escudero , Bartosz Fornal , Benjamín Grinstein , Jorge Martin Camalich

We study a scenario in which the baryon asymmetry is created through Hawking radiation from primordial black holes via a dynamically-generated chemical potential. This mechanism can also be used to generate the observed dark matter…

High Energy Physics - Phenomenology · Physics 2022-03-14 Nolan Smyth , Lillian Santos-Olmsted , Stefano Profumo

Dark matter (comprising a quarter of the Universe) is usually assumed to be due to one and only one weakly interacting particle which is neutral and absolutely stable. We consider the possibility that there are several coexisting…

High Energy Physics - Phenomenology · Physics 2007-12-03 Qing-Hong Cao , Ernest Ma , Jose Wudka , C. -P. Yuan

Well known scaling laws among the structural properties of the dark and the luminous matter in disc systems are too complex to be arisen by two inert components that just share the same gravitational field. This brings us to critically…

Cosmology and Nongalactic Astrophysics · Physics 2020-08-28 Paolo Salucci , Nicola Turini , Chiara Di Paolo