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相关论文: Matter-Dark Matter Coincidence and Mirror World

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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 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

Our standard model of the Universe predicts the distribution of dark matter to $1\%$ at the scales needed for upcoming experiments, yet our predictions for how the luminous matter -- which has interactions besides gravity -- is distributed…

高能物理 - 理论 · 物理学 2025-03-03 Nora Elisa Chisari

We first suggested a scenario in which a generic, dark chiral gauge group undergoes a first order phase transition in order to generate the observed baryon asymmetry in the universe, provide a viable dark matter candidate and explain the…

高能物理 - 唯象学 · 物理学 2012-02-15 Devin G. E. Walker

If dark matter consists of hidden-sector photons which kinetically mix with regular photons, a tiny oscillating electric-field component is present wherever we have dark matter. In the surface of conducting materials this induces a small…

We suggest that recent neutrino puzzles that are the solar and atmospheric neutrino deficits as well as the possible neutrino oscillations reported by the LSND experiment and the possibility of massive neutrinos providing the hot component…

高能物理 - 唯象学 · 物理学 2009-10-28 Z. Berezhiani , R. N. Mohapatra

The cold dark matter model successfully explains both the emergence and evolution of cosmic structures on large scales and, when we include a cosmological constant, the properties of the homogeneous and isotropic Universe. However, the cold…

宇宙学与河外天体物理 · 物理学 2020-08-04 Ivan de Martino , Sankha S. Chakrabarty , Valentina Cesare , Arianna Gallo , Luisa Ostorero , Antonaldo Diaferio

Mirror dark matter provides a simple framework for which to explain the DAMA/Libra annual modulation signal consistently with the null results of the other direct detection experiments. The simplest possibility involves ordinary matter…

天体物理学 · 物理学 2010-04-21 Paolo Ciarcelluti , Robert Foot

Dark matter may be coupled to dark radiation: light degrees of freedom that mediate forces between dark sector particles. Cosmological constraints favor dark radiation that is colder than Standard Model radiation. In models with fixed…

高能物理 - 唯象学 · 物理学 2016-10-12 Matthew Reece , Thomas Roxlo

As cosmology has entered a phase of precision experiments, the content of the universe has been established to contain interesting and not yet fully understood components, namely dark energy and dark matter. While the cause and exact nature…

高能物理 - 唯象学 · 物理学 2015-06-25 Lars Bergstrom

It is now, generally, believed that the presence of some form of dark matter is essential to explain the flat rotation curves of galaxies, and anomalous large velocities of galaxies in the clusters and superclusters. This dark matter turns…

天体物理学 · 物理学 2007-05-23 Mofazzal Azam

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…

高能物理 - 唯象学 · 物理学 2009-07-09 David E. Kaplan , Markus A. Luty , Kathryn M. Zurek

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

Based on the results from numerous astrophysics experiments, it is currently believed that the majority of matter in the Universe is in some unknown form, known as dark matter. In the past it has been common to model dark matter as a…

高能物理 - 唯象学 · 物理学 2008-12-25 Chris Bird

A consequence of the evaporation of primordial black holes in the early universe may be the generation of mirror matter. This would have implications with regard to dark matter, and the number of light particle species in equilibrium at the…

天体物理学 · 物理学 2009-10-31 Nicole F. Bell , Raymond R. Volkas

The original mimetic model was proposed to take the role of dark matter. In this paper we consider possible direct interactions of the mimetic dark matter with other matter in the universe, especially the standard model particles such as…

广义相对论与量子宇宙学 · 物理学 2018-01-17 Liuyuan Shen , Yicen Mou , Yunlong Zheng , Mingzhe Li

According to the cosmological model without singularity, there are s-matter and v-matter which are symmetric and have oppose gravitational masses. In V-breaking s-matter is similar to dark energy to cause expansion of the universe with an…

综合物理 · 物理学 2010-01-26 Shi-Hao Chen

Mirror world, a parallel hidden sector with microphysics identical to ordinary particle physics, can have several interesting phenomenological and astrophysical implications and mirror matter can be a natural candidate for dark matter in…

高能物理 - 唯象学 · 物理学 2010-04-15 Zurab Berezhiani , Angela Lepidi

Composite asymmetric dark matter scenarios naturally explain why the dark matter mass density is comparable with the visible matter mass density. Such scenarios generically require some entropy transfer mechanism below the composite scale;…

高能物理 - 唯象学 · 物理学 2019-05-01 Masahiro Ibe , Ayuki Kamada , Shin Kobayashi , Takumi Kuwahara , Wakutaka Nakano

Dark matter is a vital component of the current best model of our universe, $\Lambda$CDM. There are leading candidates for what the dark matter could be (e.g. weakly-interacting massive particles, or axions), but no compelling observational…

宇宙学与河外天体物理 · 物理学 2015-07-06 David M. Jacobs , Glenn D. Starkman , Bryan W. Lynn