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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

Most of the matter in the universe is invisible. I review the status of dark matter and describe how both the theory of galaxy formation and novel types of experimental searches are revitalizing attempts to find non-baryonic dark matter.

天体物理学 · 物理学 2010-12-09 Joseph Silk

The distribution of the non-luminous matter in galaxies of different luminosity and Hubble type is much more than a proof of the existence of dark particles governing the structures of the Universe. Here, we will review the complex but…

星系天体物理 · 物理学 2019-02-25 Paolo Salucci

We illustrate, via a simplified model, a scenario in which the baryon-asymmetry and, possibly the dark matter component of the Universe are simultaneously generated by the decay of a WIMP-like mother particle, in turn produced non-thermally…

高能物理 - 唯象学 · 物理学 2026-04-15 Giorgio Arcadi , Sarif Khan , Agnese Mariotti

We provide an up to date account of progress in understanding the origin of the observed baryon asymmetry of the universe. While our primary goal is to be current, we have attempted to give a pedagogical introduction to the primary areas of…

高能物理 - 唯象学 · 物理学 2009-07-09 Antonio Riotto , Mark Trodden

I give a review of the development of the concept of dark matter. The dark matter story passed through several stages from a minor observational puzzle to a major challenge for theory of elementary particles. Modern data suggest that dark…

宇宙学与河外天体物理 · 物理学 2018-03-14 J. Einasto

The evidence is that the mass of the universe is dominated by an exotic nonbaryonic form of matter largely draped around the galaxies. It approximates an initially low pressure gas of particles that interact only with gravity, but we know…

宇宙学与河外天体物理 · 物理学 2017-01-23 P. J. E. Peebles

The origin of the asymmetry between matter and anti-matter of the Universe has been one of the great challenges in particle physics and cosmology. Leptogenesis as a mechanism for generating the cosmological baryon asymmetry of the Universe…

高能物理 - 唯象学 · 物理学 2007-05-23 Mu-Chun Chen

Affleck-Dine baryogenesis in models where the gravitino is both the lightest supersymmetric particle and the dark matter candidate is investigated. For a high enough reheating temperature to produce sufficient gravitinos by thermal…

高能物理 - 唯象学 · 物理学 2009-11-11 Osamu Seto

(Abridged) Present cosmological constraints and the absence of a direct detection and identification of any dark matter particle candidate leave room to the possibility that the dark sector of the Universe be actually more complex than it…

宇宙学与河外天体物理 · 物理学 2015-06-04 Marco Baldi

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

The Universe is modeled as consisting of pressureless baryonic matter and a bulk viscous fluid which is supposed to represent a unified description of the dark sector. In the homogeneous and isotropic background the \textit{total} energy…

宇宙学与河外天体物理 · 物理学 2011-11-22 W. Zimdahl , H. E. S. Velten , W. S. Hipólito-Ricaldi

We argue that neutrino mass and dark matter can arise from an approximate $B-L$ symmetry. This idea can be realized in a minimal setup of the flipped 3-3-1 model, which discriminates lepton families while keeping universal quark families…

高能物理 - 唯象学 · 物理学 2020-05-22 Duong Van Loi , Phung Van Dong , Dang Van Soa

Asymmetric dark matter is a well-motivated approach to explain the apparent coincidence between the relic densities of visible and dark matter, $\Omega_D \simeq 5.4\Omega_b$. A complete explanation requires two components, a relation…

高能物理 - 唯象学 · 物理学 2026-03-04 Peter Cox , Rafael E. Pérez , Raymond R. Volkas

We propose a simple theory for the idea that cosmological dark matter (DM) may be present today mainly in the form of stable neutral hadronic thermal relics. In our model neutrino masses arise radiatively from the exchange of colored DM…

高能物理 - 唯象学 · 物理学 2018-06-27 M. Reig , D. Restrepo , J. W. F. Valle , O. Zapata

We study the origin of dark matter based on the ghost-free bigravity theory with twin matter fluids. The present cosmic acceleration can be explained by the existence of graviton mass, while dark matter is required in several cosmological…

广义相对论与量子宇宙学 · 物理学 2015-01-07 Katsuki Aoki , Kei-ichi Maeda

The origin of dark matter in the universe may be scalar particles produced by amplification of quantum fluctuations during a period of dilaton-driven inflation. We show, for the first time, that a single species of particles, depending on…

高能物理 - 唯象学 · 物理学 2009-10-31 Ram Brustein , Merav Hadad

We propose a new mechanism for generating both luminous and dark matter during cosmic inflation. According to this mechanism, ordinary and dark matter carry common charge which is associated with an anomalous $ U(1)_{X} $ group. Anomaly…

高能物理 - 唯象学 · 物理学 2015-03-10 Neil D. Barrie , Archil Kobakhidze

A simple and well-motivated explanation for the origin of dark matter is that it consists of thermal relic particles that get their mass entirely through electroweak symmetry breaking. The simplest models implementing this possibility…

高能物理 - 唯象学 · 物理学 2007-05-23 Philip C. Schuster , Natalia Toro

A scenario that relates the abundance of dark matter to the baryon asymmetry of the Universe is presented. In this scenario, based on a left-right extension of the Standard Model, dark matter is made of light, ~ 1 GeV, right-handed Majorana…

高能物理 - 唯象学 · 物理学 2007-05-23 Michel H. G. Tytgat