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A novel mechanism for explaining the matter-antimatter asymmetry of the universe is considered. We assume that the universe starts from completely symmetric state and then, as it cools down, it undergoes a quantum-phase transition which in…

宇宙学与河外天体物理 · 物理学 2011-05-31 V. R. Shaginyan , G. S. Japaridze , M. Ya. Amusia , A. Z. Msezane , K. G. Popov

The asymmetry between matter and antimatter is key to the existence and nature of our Universe. A measure of the matter - antimatter asymmetry of the Universe is provided by the present value of the universal ratio of baryons (baryons minus…

宇宙学与河外天体物理 · 物理学 2018-01-31 Gary Steigman , Robert J. Scherrer

We present a mechanism to generate the baryon asymmetry of the Universe which preserves the net baryon number created in the Big Bang. If dark matter particles carry baryon number $B_X$, and $\sigma^{\rm annih}_{\bar{X}} < \sigma^{\rm…

高能物理 - 唯象学 · 物理学 2007-05-23 Glennys R. Farrar , Gabrijela Zaharijas

We present a mechanism to generate the baryon asymmetry of the Universe which preserves the net baryon number created in the Big Bang. If dark matter particles carry baryon number $B_X$, and $\sigma^{\rm annih}_{\bar{X}} < \sigma^{\rm…

高能物理 - 唯象学 · 物理学 2009-11-11 Glennys R. Farrar , Gabrijela Zaharijas

We review observational evidence for a matter-antimatter asymmetry in the early universe, which leads to the remnant matter density we observe today. We also discuss observational bounds on the presence of antimatter in the present day…

高能物理 - 唯象学 · 物理学 2012-11-06 Laurent Canetti , Marco Drewes , Mikhail Shaposhnikov

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

We propose a novel scenario to explain the observed cosmological asymmetry between matter and antimatter, based on nonperturbative QCD physics. This scenario relies on a mechanism of separation of quarks and antiquarks in two coexisting…

高能物理 - 唯象学 · 物理学 2009-11-10 David H. Oaknin , Ariel Zhitnitsky

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

The origin of the matter-antimatter asymmetry of the universe is one of the major unsolved problems in cosmology and particle physics. In this paper, we investigate the recently proposed possibility that split fermion models -- extra…

高能物理 - 唯象学 · 物理学 2009-11-11 Andrew Coulthurst

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 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

Baryon number violation, CP violation and non-equilibrium evolution of the early universe just after the big bang are proposed in the literature to be necessary conditions to explain the observed matter-antimatter asymmetry (baryon…

综合物理 · 物理学 2019-09-13 Gouranga C Nayak

The radiative neutrino mass model with an inert doublet scalar has been considered as a promising candidate which can explain neutrino masses, dark matter abundance and baryon number asymmetry if dark matter is identified with the lightest…

高能物理 - 唯象学 · 物理学 2015-06-05 Shoichi Kashiwase , Daijiro Suematsu

We propose a novel framework where baryon asymmetry can arise due to forbidden decay of dark matter (DM) enabled by finite temperature effects in the early universe. In order to implement it in a realistic setup, we consider the DM to be a…

高能物理 - 唯象学 · 物理学 2023-09-06 Debasish Borah , Suruj Jyoti Das , Rishav Roshan

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 put forward a new proposal for generating the baryon asymmetry of the universe by making use of the dynamics of a $\mathrm{U}(1)$ scalar field coupled to dark matter. High dark matter densities cause the $\mathrm{U}(1)$ symmetry to break…

高能物理 - 唯象学 · 物理学 2017-11-22 Jeremy Sakstein , Mark Trodden

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

The nature of dark matter and the origin of the baryon asymmetry are two of the deepest mysteries of modern particle physics. In the absence of hints regarding a possible solution to these mysteries, many approaches have been developed to…

高能物理 - 唯象学 · 物理学 2013-12-19 S. M. Boucenna , S. Morisi

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…

高能物理 - 唯象学 · 物理学 2015-06-12 Raymond R. Volkas

We entertain a new paradigm according to which the observed matter-antimatter asymmetry is generated as a large-scale quantum fluctuation over the baryon-symmetric state that occurred during the cosmic inflation.

高能物理 - 唯象学 · 物理学 2015-07-08 Archil Kobakhidze , Adrian Manning
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