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相关论文: A Dynamical Explanation of the Dark Matter-Baryon …

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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…

高能物理 - 唯象学 · 物理学 2015-06-12 John McDonald

A scalar field interacting differently with dark matter and baryons may explain why their ratio is of order unity today. We provide three working examples, checking them against the observations of CMB, Large Scale Structure, supernovae Ia,…

天体物理学 · 物理学 2010-12-09 R. Catena , M. Pietroni , L. Scarabello

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…

高能物理 - 唯象学 · 物理学 2026-05-15 Yang Bai , Ting-Kuo Chen

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…

高能物理 - 唯象学 · 物理学 2011-09-05 Pei-Hong Gu , Manfred Lindner , Utpal Sarkar , Xinmin Zhang

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…

高能物理 - 唯象学 · 物理学 2013-05-30 Kohei Kamada , Masahide Yamaguchi

The densities of dark and baryonic matter are comparable: \zeta = \rho_D / \rho_B ~ O(1). This is surprising because they are controlled by different combinations of low-energy physics parameters. Here we consider the probability…

高能物理 - 理论 · 物理学 2013-09-11 Raphael Bousso , Lawrence Hall

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…

高能物理 - 唯象学 · 物理学 2009-11-10 Ryuichiro Kitano , Ian Low

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 the possibility that dark matter is a baryon of a new strongly interacting gauge theory, which was introduced in the low energy theory of Cosmological SUSY Breaking (CSB). This particle can fit the observed dark matter density if…

高能物理 - 唯象学 · 物理学 2009-11-11 T. Banks , J. D. Mason , D. O'Neil

We investigate the possibility that both the baryon asymmetry of the universe and the observed cold dark matter density are generated by decays of a heavy scalar field which dominates the universe before nucleosynthesis. Since baryons and…

高能物理 - 唯象学 · 物理学 2008-11-26 Ryuichiro Kitano , Hitoshi Murayama , Michael Ratz

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…

高能物理 - 唯象学 · 物理学 2024-06-13 Arushi Bodas , Manuel A. Buen-Abad , Anson Hook , Raman Sundrum

We suggest the existence of a fundamental connection between baryonic and dark matter. This is motivated by both the stability of these two types of matter as well as the observed similarity of their present-day densities. A unified genesis…

高能物理 - 唯象学 · 物理学 2011-07-15 Michael L. Graesser , Ian M. Shoemaker , Luca Vecchi

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,…

高能物理 - 唯象学 · 物理学 2022-11-21 João G. Rosa , Duarte M. C. Silva

It is a puzzle why the densities of dark matter and dark energy are nearly equal today when they scale so differently during the expansion of the universe. This conundrum may be solved if there is a coupling between the two dark sectors. In…

高能物理 - 唯象学 · 物理学 2009-07-09 D. Comelli , M. Pietroni , A. Riotto

In this work we perform some studies related to dark energy. Firstly, we propose a dynamical approach to explain the dark energy content of the universe. We assume that a massless scalar field couples to the Hubble parameter with some…

高能物理 - 唯象学 · 物理学 2009-01-07 Fei Wang , Jin Min Yang

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…

高能物理 - 唯象学 · 物理学 2022-05-18 Clara Murgui , Kathryn M. Zurek

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

We present a new universal relation, satisfied by matter distributions at all observed scales, and show its amazingly good and detailed agreement with the predictions of the most up-to-date pure dark matter simulations of structure…

宇宙学与河外天体物理 · 物理学 2009-11-13 Alexey Boyarsky , Oleg Ruchayskiy , Dmytro Iakubovskyi , Andrea V. Maccio' , Denys Malyshev

The so called `cosmic coincidence' problem seems to suggest a coupling between dark energy and dark matter. A possibility could be given by dark matter particles with masses depending exponentially on the scalar field associated to dark…

高能物理 - 唯象学 · 物理学 2007-05-23 Massimo Pietroni

Recent studies point out that there exists some rough scaling relations for dark matter and some tight connections between dark matter and baryons. However, most of the relations and tight connections can only be found in galaxies, but not…

宇宙学与河外天体物理 · 物理学 2019-04-12 Man Ho Chan
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