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The similarity of the visible and dark matter abundances indicates that they may originate via the same mechanism. If both the dark and the visible matter are charged under a generalized baryon number which remains always conserved, then…

高能物理 - 唯象学 · 物理学 2011-12-09 Nicole F. Bell , Kalliopi Petraki , Ian M. Shoemaker , Raymond R. Volkas

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 study generation of baryon number asymmetry and both abundance of dark matter and dark energy on the basis of global symmetry and its associating flat directions in a supersymmetric model. We assume the existence of a model independent…

天体物理学 · 物理学 2009-11-13 Daijiro Suematsu

Low-scale supersymmetry breaking in string motivated theories implies the presence of O(100) TeV scale moduli, which generically lead to a significant modification of the history of the universe prior to Big Bang Nucleosynthesis. Such an…

高能物理 - 唯象学 · 物理学 2015-05-30 Gordon Kane , Jing Shao , Scott Watson , Hai-Bo Yu

We propose a new framework for explaining the proximity of the baryon and dark matter relic densities \Omega_{DM} \approx 5\Omega_B. The scenario assumes that the number density of the observed dark matter states is generated due to decays…

高能物理 - 唯象学 · 物理学 2015-06-12 James Unwin

Asymmetric Dark Matter (ADM) models relate the dark matter density to the baryon asymmetry, so that a natural mass scale for ADM is around a few GeV. In existing models of ADM, this mass scale is unexplained; here we generate this GeV scale…

高能物理 - 唯象学 · 物理学 2014-11-21 Timothy Cohen , Daniel J. Phalen , Aaron Pierce , Kathryn M. Zurek

We highlight that the observed concurrence between the baryon and dark matter relic densities can be explained via a parametric coincidence between two distinct production mechanisms: Affleck-Dine baryogenesis and dark matter UV freeze-in.…

高能物理 - 唯象学 · 物理学 2025-11-05 Jae Hyeok Chang , Chang Sub Shin , James Unwin

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

We consider the production of asymmetric dark matter during hidden sector baryogenesis. We consider a particular supersymmetric model where the dark matter candidate has a number density approximately equal to the baryon number density,…

高能物理 - 唯象学 · 物理学 2011-10-03 Bhaskar Dutta , Jason Kumar

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 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 class of `Asymmetric Dark Matter' scenarios relies on the existence of a primordial particle/anti-particle asymmetry in the dark sector related to the baryon asymmetry as a way to address the observed similarity between the baryonic and…

高能物理 - 唯象学 · 物理学 2013-01-01 Gabrijela Zaharijas

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 existence of dark matter (DM) and the origin of the baryon asymmetry are persistent indications that the SM is incomplete. More recently, the ATLAS and CMS experiments have observed an excess of diphoton events with invariant mass of…

高能物理 - 唯象学 · 物理学 2016-06-08 Mads T. Frandsen , Ian M. Shoemaker

Asymmetric Dark Matter (ADM) models invoke a particle-antiparticle asymmetry, similar to the one observed in the Baryon sector, to account for the Dark Matter (DM) abundance. Both asymmetries are usually generated by the same mechanism and…

高能物理 - 唯象学 · 物理学 2015-06-04 Mattias Blennow , Enrique Fernandez-Martinez , Olga Mena , Javier Redondo , Paolo Serra

The comparable abundances of dark matter and baryons imply a deep connection between the dark sector and the QCD sector. In models of asymmetric dark matter, the number densities of both sectors are ensured to be similar. However, a…

高能物理 - 唯象学 · 物理学 2025-12-09 Yi Chung

In standard models of baryogenesis and of dark matter, the mechanisms which generate the densities in both sectors are unrelated to each other. In this paper we explore models which generate the baryon asymmetry through the dark matter…

高能物理 - 唯象学 · 物理学 2010-12-24 Jessie Shelton , Kathryn M. Zurek

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

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

Pangenesis is the mechanism for jointly producing the visible and dark matter asymmetries via Affleck-Dine dynamics in a baryon-symmetric universe. The baryon-symmetric feature means that the dark asymmetry cancels the visible baryon…

高能物理 - 唯象学 · 物理学 2012-05-21 Benedict von Harling , Kalliopi Petraki , Raymond R. Volkas
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