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Asymmetric dark matter (ADM) is an attractive framework relating the observed baryon asymmetry of the Universe to the dark matter density. A composite particle in a new strong dynamics is a promising candidate for ADM as the strong dynamics…

高能物理 - 唯象学 · 物理学 2018-12-26 Masahiro Ibe , Ayuki Kamada , Shin Kobayashi , Wakutaka Nakano

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…

高能物理 - 唯象学 · 物理学 2025-08-07 Saikat Das , Ayuki Kamada , Takumi Kuwahara , Kohta Murase , Deheng Song

Asymmetric dark matter (ADM) is motivated by the similar cosmological mass densities measured for ordinary and dark matter. We present a comprehensive theory for ADM that addresses the mass density similarity, going beyond the usual ADM…

高能物理 - 唯象学 · 物理学 2018-05-23 Stephen J. Lonsdale , Raymond R. Volkas

We present a dynamical solution to the dark matter-baryon coincidence problem based on the neutron portal operator connecting the visible and dark sector asymmetries. This framework is motivated by the possibility that a strongly…

高能物理 - 唯象学 · 物理学 2026-04-24 Sudhakantha Girmohanta , Yuichiro Nakai , Yoshihiro Shigekami , Zhihao Zhang

The asymmetric dark matter (ADM) scenario can solve the coincidence problem between the baryon and the dark matter (DM) abundance when the DM mass is of ${\cal O}(1)\,$GeV. In the ADM scenarios, composite dark matter is particularly…

高能物理 - 唯象学 · 物理学 2020-02-06 Masahiro Ibe , Shin Kobayashi , Ryo Nagai , Wakutaka Nakano

The nature of dark matter (DM) and how it might interact with the particles of the Standard Model (SM) is an ever-growing mystery. It is possible that the existence of new `dark sector' forces, yet undiscovered, are the key to solving this…

高能物理 - 唯象学 · 物理学 2020-01-29 Thomas D. Rueter , Thomas G. Rizzo

The kinetic mixing (KM) portal, by which the Standard Model (SM) photon mixes with a light dark photon arising from a new $U(1)_D$ gauge group, allows for the possibility of viable scenarios of sub-GeV thermal dark matter (DM) with…

高能物理 - 唯象学 · 物理学 2025-03-28 Thomas G. Rizzo

A possible connection between the cosmological baryon asymmetry, dark matter and vector-like fermions is investigated. In this scenario an asymmetry generated through baryogenesis or leptogenesis (in the vector-like matter sector) connects…

高能物理 - 唯象学 · 物理学 2013-05-22 Pavel Fileviez Perez , Mark B. Wise

Models of asymmetric dark matter (ADM) seek to explain the apparent coincidence between the present-day mass densities of visible and dark matter, $\Omega_{\mathrm{DM}} \simeq 5\Omega_{\mathrm{VM}}$. However, most ADM models only relate the…

高能物理 - 唯象学 · 物理学 2021-09-02 Alexander C. Ritter , Raymond R. Volkas

We propose a new mechanism to simultaneously explain the observed dark matter abundance and the baryon asymmetry of the Universe. The mechanism is based on the Filtered Dark Matter scenario, where dark matter particles acquire a large mass…

高能物理 - 唯象学 · 物理学 2022-08-24 Michael J. Baker , Moritz Breitbach , Joachim Kopp , Lukas Mittnacht , Yotam Soreq

The kinetic mixing (KM) of a dark photon (DP) with the familiar one of the Standard Model (SM) requires the existence of a new set of fields, called portal matter (PM), which carry both SM and dark sector quantum numbers, some whose masses…

高能物理 - 唯象学 · 物理学 2023-05-24 Thomas G. Rizzo

About 80\% of the mass of the present Universe is made up of the unknown (dark matter), while the rest is made up of ordinary matter. It is a very intriguing question why the {\it mass} densities of dark matter and ordinary matter (mainly…

高能物理 - 唯象学 · 物理学 2019-10-23 Masahiro Ibe , Ayuki Kamada , Shin Kobayashi , Takumi Kuwahara , Wakutaka Nakano

We study a mechanism through which the cosmic dark matter density can be explained simultaneously with the observed baryon asymmetry of the Universe. At the core of our proposal lie the out-of-equilibrium scattering processes of bath…

高能物理 - 唯象学 · 物理学 2022-09-15 Andreas Goudelis , Dimitrios Karamitros , Pantelis Papachristou , Vassilis C. Spanos

Asymmetric symmetry breaking models dynamically break the G X G gauge symmetries of mirror models to distinct subgroups in the two sectors. The coincidental abundances of visible and dark matter, $\Omega_{DM} \simeq 5\Omega_{VM}$, motivates…

高能物理 - 唯象学 · 物理学 2015-07-08 Stephen J. Lonsdale

The goal of this work is to find the simplest UV completions of Accidental Composite Dark Matter models that can dynamically generate an asymmetry for the Dark Matter candidate, the lightest dark baryon, and simultaneously annihilate the…

高能物理 - 唯象学 · 物理学 2022-05-19 Salvatore Bottaro , Marco Costa , Oleg Popov

If dark matter (DM) interacts with the Standard Model (SM) via the $U(1)_D$ kinetic mixing (KM) portal at low energies, it necessitates not only the existence of portal matter (PM) particles which carry both dark and SM quantum numbers, but…

高能物理 - 唯象学 · 物理学 2022-10-31 Thomas G. Rizzo

Asymmetric dark matter is a well-motivated approach to explain the apparent coincidence between the relic densities of visible and dark matter, $\Omega_D \simeq 5.4\Omega_b$. A complete explanation requires two components, a relation…

高能物理 - 唯象学 · 物理学 2026-03-04 Peter Cox , Rafael E. Pérez , Raymond R. Volkas

Why matter and dark matter contents of the universe are of the same order of magnitude, is one of the puzzles of modern cosmology. At the face of it, this would seem to point towards a basic similarity between matter and dark matter,…

高能物理 - 唯象学 · 物理学 2025-02-24 Rabindra N. Mohapatra , Nobuchika Okada

The similar cosmological abundances observed for visible and dark matter suggest a common origin for both. By viewing the dark matter density as a dark-sector asymmetry, mirroring the situation in the visible sector, we show that the…

高能物理 - 唯象学 · 物理学 2012-03-01 Kalliopi Petraki , Mark Trodden , Raymond R. Volkas

Very light dark matter is usually taken to consist of uncharged bosons such as axion-like particles or dark photons. Here, we consider the prospect of very light, possibly even sub-eV dark matter carrying a net charge that is…

高能物理 - 唯象学 · 物理学 2019-09-11 Gonzalo Alonso-Álvarez , Julia Gehrlein , Joerg Jaeckel , Sebastian Schenk
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