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A hidden sector that kinetically mixes with the Minimal Supersymmetric Standard Model provides simple and well-motivated dark matter candidates that possess many of the properties of a traditional weakly interacting massive particle (WIMP).…

高能物理 - 唯象学 · 物理学 2020-10-21 Patrick Barnes , Zachary Johnson , Aaron Pierce , Bibhushan Shakya

It is often said that asymmetric dark matter is light compared to typical weakly interacting massive particles. Here we point out a simple scheme with a neutrino portal and $\mathcal{O}(60 \text{ GeV})$ asymmetric dark matter which may be…

高能物理 - 唯象学 · 物理学 2022-10-19 Eleanor Hall , Robert McGehee , Hitoshi Murayama , Bethany Suter

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

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

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

Baryon number violation in the visible sector induced by anti-baryonic dark matter provides a viable mechanism for low-scale baryogenesis. Two of the most sensitive probes of this scenario are neutron decay processes such as $n \to…

高能物理 - 唯象学 · 物理学 2025-09-30 Mathew Thomas Arun , Anuja Bandu Khadse

Low-scale baryogenesis and dark matter generation can occur via the production of neutral $B$ mesons at MeV temperatures in the early Universe, which undergo CP-violating oscillations and subsequently decay into a dark sector. In this work,…

高能物理 - 唯象学 · 物理学 2020-04-22 Gonzalo Alonso-Álvarez , Gilly Elor , Ann E. Nelson , Huangyu Xiao

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

The nonbaryonic dark matter of the Universe is assumed to consist of new stable forms of matter. Their stability reflects symmetry of micro world and mechanisms of its symmetry breaking. Particle candidates for cosmological dark matter are…

宇宙学与河外天体物理 · 物理学 2013-11-12 Maxim Yu. Khlopov

The similar densities of dark matter and baryons in the universe imply that they might arise from the same ultraviolet model. The B-Mesogenesis, which assumes dark matter is charged under the baryon number, attempts to simultaneously…

高能物理 - 唯象学 · 物理学 2024-08-20 Yong Zheng , Jian-Nan Ding , Dong-Hao Li , Lei-Yi Li , Cai-Dian Lü , Fu-Sheng Yu

Dark matter, baryonic matter and dark energy have different properties but contribute comparable energy density to the present Universe. We point out that they may have a common origin. As the dark energy has a scale far lower than all…

高能物理 - 唯象学 · 物理学 2010-04-06 Pei-Hong Gu , Utpal Sarkar

A ~5 GeV `dark baryon' with a cosmic asymmetry similar to that of baryons is a natural candidate for the dark matter. We study the possibility of generating such a state through dynamical electroweak symmetry breaking, and show that it can…

高能物理 - 唯象学 · 物理学 2011-09-28 Mads T. Frandsen , Subir Sarkar , Kai Schmidt-Hoberg

We perform a systematic analysis of models with GeV-scale dark matter coupled to baryons and leptons. Such theories provide a natural framework to explain the matter-antimatter asymmetry of the universe. We find that only a few baryonic…

高能物理 - 唯象学 · 物理学 2021-02-26 Bartosz Fornal , Alec Hewitt , Yue Zhao

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

We propose a new mechanism to understand the relation between the baryon and dark matter asymmetries in the universe in theories where the baryon number is a local symmetry. In these scenarios the B-L asymmetry generated through a mechanism…

高能物理 - 唯象学 · 物理学 2014-03-11 Pavel Fileviez Perez , Hiren H. Patel

The possible role of supersymmetry in our understanding of big bang baryogenesis and cosmological dark matter is explored. The discussion will be limited to the out-of equilibrium decay scenario in SUSY GUTs, the decay of scalar…

高能物理 - 唯象学 · 物理学 2016-09-01 Keith A. Olive

Ordinary baryonic particles (such as protons and neutrons) account for only one-sixth of the total matter in the Universe. The remainder is a mysterious "dark matter" component, which does not interact via electromagnetism and thus neither…

We introduce a new mechanism for the simultaneous generation of baryon and dark matter asymmetries through ultraviolet-dominated freeze-in scatterings. The mechanism relies on heavy Majorana neutrinos that connect the visible Standard Model…

高能物理 - 唯象学 · 物理学 2026-03-05 Pouya Asadi , Marianne Moore , David E. Morrissey , Michael Shamma

In the context of the relationship between physics of cosmological dark matter and symmetry of elementary particles a wide list of dark matter candidates is possible. New symmetries provide stability of different new particles and their…

高能物理 - 唯象学 · 物理学 2017-04-26 M. Yu. Khlopov

A comet-like, but magnitudes smaller, extremely low albedo interstellar meteoroid population of fragile aggregates with solar type composition, measured in space and terrestrially, is most probably the universal dark matter. Although…

天体物理学 · 物理学 2007-05-23 Robert K. Soberman , Maurice Dubin