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相关论文: Asymmetric accidental composite dark matter

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The goal of this work is to find the simplest UV completions of Accidental Composite Dark Matter models that can dynamically generate an asymmetry for the Dark Matter candidate, the lightest dark baryon, and simultaneously annihilate the…

高能物理 - 唯象学 · 物理学 2022-05-19 Salvatore Bottaro , Marco Costa , Oleg Popov

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

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

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 investigate a novel type of asymmetric dark matter (ADM) model in which the dark matter asymmetry and the baryon asymmetry in our universe (BAU) are produced simultaneously via low-scale spontaneous leptogenesis, where the mass scale of…

高能物理 - 唯象学 · 物理学 2026-01-06 Hiroki Takahashi , Juntaro Wada

The asymmetric dark matter (ADM) scenario solves the baryon-dark matter coincidence problem when the dark matter (DM) mass is of $\mathcal{O}(1)$GeV. Composite ADM models based on QCD-like strong dynamics are particularly motivated since…

高能物理 - 唯象学 · 物理学 2021-08-18 Masahiro Ibe , Shin Kobayashi , Keiichi Watanabe

We study the possibility of generating dark matter (DM) and baryon asymmetry of the Universe (BAU) simultaneously in an asymmetric DM framework, which also alleviates the small-scale structure issues of cold DM. While the thermal relic of…

高能物理 - 唯象学 · 物理学 2024-08-29 Debasish Borah , Satyabrata Mahapatra , Partha Kumar Paul , Narendra Sahu , Prashant Shukla

We show that a general semi-annihilation scenario, in which a pair of dark matter (DM) particles annihilate to an anti-DM, and an unstable state that can mix with or decay to standard model states, can lead to particle anti-particle…

高能物理 - 唯象学 · 物理学 2020-10-21 Avirup Ghosh , Deep Ghosh , Satyanarayan Mukhopadhyay

We investigate, in the context of asymmetric dark matter (DM), a new mechanism of spontaneous co-genesis of linked DM and baryon asymmetries, explaining the observed relation between the baryon and DM densities, Omega_DM/Omega_B ~ 5. The…

高能物理 - 唯象学 · 物理学 2015-05-28 John March-Russell , Matthew McCullough

We propose a new mechanism where asymmetric dark matter (ADM) and the baryon asymmetry are both generated in the same decay chain of a metastable weakly interacting massive particle (WIMP) after its thermal freeze-out. Dark matter and…

高能物理 - 唯象学 · 物理学 2020-12-11 Yanou Cui , Michael Shamma

In this paper, we construct the first asymmetric strongly interacting massive particles (SIMP) dark matter (DM) model, where a new vector-like fermion and a new complex scalar both having nonzero chemical potentials can be asymmetric DM…

高能物理 - 唯象学 · 物理学 2022-10-31 Shu-Yu Ho

Asymmetric dark matter (ADM) is an attractive framework relating the observed baryon asymmetry of the Universe to the dark matter density. A composite particle in a new strong dynamics is a promising candidate for ADM as the strong dynamics…

高能物理 - 唯象学 · 物理学 2018-12-26 Masahiro Ibe , Ayuki Kamada , Shin Kobayashi , Wakutaka Nakano

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 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

Composite asymmetric dark matter (ADM) models provide a well-motivated paradigm that simultaneously explains dark matter (DM) relic density and matter-antimatter asymmetry. In these models, the mass of the DM candidate (the lightest dark…

高能物理 - 唯象学 · 物理学 2026-01-05 Chih-Ting Lu , Changbin Xi

Non-Abelian Vector Boson Dark Matter (VBDM), arising from an $SU(2)_N$ extension of the Standard Model (SM) has been studied. The Dark Matter (DM) is stabilized by imposing an additional discrete global symmetry $S^{'}$ with charges, such…

高能物理 - 唯象学 · 物理学 2019-07-05 Himadri Roy

We show that "accidental" supersymmetry is a beyond-the-Standard Model framework that naturally accommodates a thermal relic dark matter candidate and successful electroweak baryogenesis, including the needed strongly first-order character…

高能物理 - 唯象学 · 物理学 2015-06-11 Jonathan Kozaczuk , Stefano Profumo , Carroll L. Wainwright

In the early Universe, any particle carrying a conserved quantum number and in chemical equilibrium with the thermal bath will unavoidably inherit a particle-antiparticle asymmetry. A new particle of this type, if stable, would represent a…

高能物理 - 唯象学 · 物理学 2015-07-08 Sofiane M. Boucenna , Martin B. Krauss , Enrico Nardi

Almost commutative geometry offers a specific way to unify general relativity, quantum mechanics and gauge symmetries. The AC-model of elementary particles, arising on this way, naturally embeds the Standard model and predicts doubly…

天体物理学 · 物理学 2007-05-23 Maxim Yu. Khlopov , Christoph A. Stephan

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
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