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The near equality of the dark matter and baryon energy densities is a remarkable coincidence, especially when one realizes that the baryon mass is exponentially sensitive to UV parameters in the form of dimensional transmutation. We explore…

High Energy Physics - Phenomenology · Physics 2023-10-13 Dawid Brzeminski , Anson Hook

The dark energy, dark matter and baryon densities in the Universe are observed to be similar, with a factor of no more than 20 between the largest and smallest densities. We show that this coincidence can be understood via superhorizon…

High Energy Physics - Phenomenology · Physics 2015-06-12 John McDonald

The measured densities of dark and baryonic matter are surprisingly close to each other, even though the baryon asymmetry and the dark matter are usually explained by unrelated mechanisms. We consider a scenario where the dark matter S is…

High Energy Physics - Phenomenology · Physics 2009-11-10 Ryuichiro Kitano , Ian Low

We argue that the striking similarity between the cosmic abundances of baryons and dark matter, despite their very different astrophysical behavior, strongly motivates the scenario in which dark matter resides within a rich dark sector…

High Energy Physics - Phenomenology · Physics 2024-06-13 Arushi Bodas , Manuel A. Buen-Abad , Anson Hook , Raman Sundrum

The baryon-dark matter coincidence is a long-standing issue. Interestingly, the recent observations suggest the presence of dark radiation, which, if confirmed, would pose another coincidence problem of why the density of dark radiation is…

High Energy Physics - Phenomenology · Physics 2015-06-15 Tetsutaro Higaki , Kwang Sik Jeong , Fuminobu Takahashi

In a baryon-symmetric universe, the baryon asymmetry observed for visible matter is matched by an equal and opposite asymmetry for dark matter, thereby closely connecting the number densities of both types of matter. This is a necessary…

High Energy Physics - Phenomenology · Physics 2015-06-12 Raymond R. Volkas

The observational relation between the density of baryon and dark matter in the Universe, $\Omega_{\rm DM}/\Omega_B\simeq 5$, is one of the most difficult problems to solve in modern cosmology. We discuss a scenario that explains this…

High Energy Physics - Phenomenology · Physics 2013-05-30 Kohei Kamada , Masahide Yamaguchi

We propose a scenario that explains the comparable abundances of dark matter (DM) and baryons without any coincidence in the corresponding particle masses. Here, DM corresponds to heavy "dark baryons" in a hidden MSSM-like dark sector,…

High Energy Physics - Phenomenology · Physics 2022-11-21 João G. Rosa , Duarte M. C. Silva

We discuss relaxation solutions to the dark matter - baryon coincidence problem in the context of QCD axion dark matter. In relaxation solutions, a moduli dynamically adjusts the mass of dark matter and baryons until their energy densities…

High Energy Physics - Phenomenology · Physics 2024-10-31 Abhishek Banerjee , Dawid Brzeminski , Anson Hook

In the present universe visible and dark matter contribute comparable energy density although they have different properties. This coincidence can be elegantly explained if the dark matter relic density, originating from a dark matter…

High Energy Physics - Phenomenology · Physics 2011-09-05 Pei-Hong Gu , Manfred Lindner , Utpal Sarkar , Xinmin Zhang

Dark and baryonic matter contribute comparable energy density to the present Universe. The dark matter may also be responsible for the cosmic positron/electron excesses. We connect these phenomena with Dirac seesaw for neutrino masses. In…

High Energy Physics - Phenomenology · Physics 2009-10-29 Pei-Hong Gu , Utpal Sarkar , Xinmin Zhang

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,…

High Energy Physics - Phenomenology · Physics 2025-02-24 Rabindra N. Mohapatra , Nobuchika Okada

Motivated by the observed ratio of dark matter to baryon mass densities, $\rho_D/\rho_B \simeq 5$, we propose a theory of dark-color unification. In this theory, the dark to visible baryon masses are fixed by the ratio of dark to visible…

High Energy Physics - Phenomenology · Physics 2022-05-18 Clara Murgui , Kathryn M. Zurek

The observational fact that the present values of the densities of dark energy and dark matter are of the same order of magnitude, $\rho_{de0}/\rho_{dm0} \sim \mathcal{O}(1)$, seems to indicate that we are currently living in a very special…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-23 H. E. S. Velten , R. F. vom Marttens , W. Zimdahl

We propose an explanation for the dark matter-baryon coincidence based on collapsing $\mathbb{Z}_N$ domain walls, which form a novel compact baryonic state: the baryoid. A baryoid has an asteroid-scale mass and up-to-nuclear-scale energy…

High Energy Physics - Phenomenology · Physics 2026-05-15 Yang Bai , Ting-Kuo Chen

We investigate a theory of $SU(9)$ dark grand unification, where dark matter consists of asymmetric dark baryons from the $Sp(4)_D$ dark QCD sector. By unifying the dark color gauge group with the Standard Model gauge group, the asymmetry…

High Energy Physics - Phenomenology · Physics 2026-02-03 Yi Chung

It is known that the cosmological baryon density ($\Omega_{\rm{b}}$) and dark matter density ($\Omega_{\rm{dm}}$) have strikingly similar values. However, in most theories of the early Universe, each density is explained by separate…

High Energy Physics - Phenomenology · Physics 2008-11-26 Stephen M. West

We consider a simple class of models in which the relic density of dark matter is determined by the baryon asymmetry of the universe. In these models a $B - L$ asymmetry generated at high temperatures is transfered to the dark matter, which…

High Energy Physics - Phenomenology · Physics 2009-07-09 David E. Kaplan , Markus A. Luty , Kathryn M. Zurek

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…

High Energy Physics - Phenomenology · Physics 2019-10-23 Masahiro Ibe , Ayuki Kamada , Shin Kobayashi , Takumi Kuwahara , Wakutaka Nakano

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…

High Energy Physics - Phenomenology · Physics 2020-02-06 Masahiro Ibe , Shin Kobayashi , Ryo Nagai , Wakutaka Nakano
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