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相关论文: Review of asymmetric dark matter

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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

We review the theoretical framework underlying models of asymmetric dark matter, describe astrophysical constraints which arise from observations of neutron stars, and discuss the prospects for detecting asymmetric dark matter.

高能物理 - 唯象学 · 物理学 2015-06-16 Jason Kumar

We review theories of Asymmetric Dark Matter (ADM), their cosmological implications and detection. While there are many models of ADM in the literature, our review of existing models will center on highlighting the few common features and…

高能物理 - 唯象学 · 物理学 2015-06-16 Kathryn M. Zurek

In existing dark matter models with global symmetries the relic abundance of dark matter is either equal to that of anti-dark matter (thermal WIMP), or vastly larger, with essentially no remaining anti-dark matter (asymmetric dark matter).…

高能物理 - 唯象学 · 物理学 2015-05-27 Michael L. Graesser , Ian M. Shoemaker , Luca Vecchi

The asymmetric dark matter (ADM) paradigm is motivated by the apparent coincidence between the cosmological 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 2023-02-15 Alexander C. Ritter , Raymond R. Volkas

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

A brief overview of our current understanding of abundance and properties of dark energy and dark matter is presented. A more focused discussion of supersymmetric dark matter follows. Included is a frequentist approach to the supersymmetric…

高能物理 - 唯象学 · 物理学 2010-01-28 Keith A. Olive

We investigate the relic abundance of asymmetric Dark Matter where the asymmetric Dark Matter is non--thermally produced from the decay of heavier particles in addition to the usual thermal production. We discuss the relic density of…

高能物理 - 唯象学 · 物理学 2023-08-02 Maqingshan , Hoernisa Iminniyaz

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

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

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

The observed dark matter relic abundance may be explained by different mechanisms, such as thermal freeze-out/freeze-in, with one or more symmetric/asymmetric components. In this work we investigate the role played by asymmetries in…

高能物理 - 唯象学 · 物理学 2023-05-15 Juan Herrero-Garcia , Giacomo Landini , Drona Vatsyayan

The pervasive presence in space of a flux of high-speed, electrically uncharged dark matter particles is examined here for potential consequences. Dark matter interactions with ordinary matter are considered, and a model of the dark matter…

综合物理 · 物理学 2009-08-25 C. L. Herzenberg

It is a puzzle why the densities of dark matter and dark energy are nearly equal today when they scale so differently during the expansion of the universe. This conundrum may be solved if there is a coupling between the two dark sectors. In…

高能物理 - 唯象学 · 物理学 2009-07-09 D. Comelli , M. Pietroni , A. Riotto

We study a mechanism where the dark matter number density today arises from asymmetries generated in the dark sector in the early universe, even though total dark matter number remains zero throughout the history of the universe. The dark…

高能物理 - 唯象学 · 物理学 2017-02-08 Prateek Agrawal , Can Kilic , Sivaramakrishnan Swaminathan , Cynthia Trendafilova

Why matter and dark matter contents of the universe are of the same order of magnitude, is one of the puzzles of modern cosmology. At the face of it, this would seem to point towards a basic similarity between matter and dark matter,…

高能物理 - 唯象学 · 物理学 2025-02-24 Rabindra N. Mohapatra , Nobuchika Okada

The existence of dark matter (DM) and the origin of the baryon asymmetry are persistent indications that the SM is incomplete. More recently, the ATLAS and CMS experiments have observed an excess of diphoton events with invariant mass of…

高能物理 - 唯象学 · 物理学 2016-06-08 Mads T. Frandsen , Ian M. Shoemaker

A model of cosmology, that arises from the hypothesis that ordinary matter, dark matter and dark energy are made of the same stuff, is studied. It is argued that this hypothesis is a consequence of considering space and time in the same…

天体物理学 · 物理学 2007-05-23 Isaac Cohen

Dark matter is a fundamental constituent of the universe, which is needed to explain a wide variety of astrophysical and cosmological observations. Although the existence of dark matter was first postulated nearly a century ago and its…

宇宙学与河外天体物理 · 物理学 2025-09-23 Csaba Balazs , Torsten Bringmann , Felix Kahlhoefer , Martin White

The paper suggests a left-right mirror symmetric model to account for the baryogenesis and asymmetric dark matter. The model can simultaneously accommodate the standard model, neutrino physics, matter-antimatter asymmetry and dark matter.…

高能物理 - 唯象学 · 物理学 2015-06-19 Wei-Min Yang
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