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The observed density of dark matter is of the magnitude expected for a thermal relic weakly-interacting massive particle (WIMP). In addition, the observed baryon density is within an order of magnitude of the dark matter density. This…

高能物理 - 唯象学 · 物理学 2012-01-17 John McDonald

In the present universe visible and dark matter contribute comparable energy density although they have different properties. This coincidence can be elegantly explained if the dark matter relic density, originating from a dark matter…

高能物理 - 唯象学 · 物理学 2011-09-05 Pei-Hong Gu , Manfred Lindner , Utpal Sarkar , Xinmin Zhang

The observed density of dark matter is of the magnitude expected for a thermal relic weakly-interacting massive particle (WIMP). In addition, the observed baryon density is within an order of magnitude of the dark matter density. This…

高能物理 - 唯象学 · 物理学 2015-03-06 John McDonald

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

We study the possibility of generating baryon asymmetry of the universe from dark matter (DM) annihilations during non-standard cosmological epochs. Considering the DM to be of weakly interacting massive particle (WIMP) type, the generation…

高能物理 - 唯象学 · 物理学 2023-03-29 Devabrat Mahanta , Debasish Borah

We propose a robust, unified framework, in which the similar baryon and dark matter cosmic abundances both arise from the physics of weakly interacting massive particles (WIMPs), with the rough quantitative success of the so-called "WIMP…

高能物理 - 唯象学 · 物理学 2015-06-12 Yanou Cui , Raman Sundrum

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 explore models in which weakly interacting massive particle (WIMP) dark matter annihilation is directly responsible for baryogenesis, thereby connecting dark matter with baryogenesis. We call this process "WIMPy baryogenesis". The dark…

高能物理 - 唯象学 · 物理学 2015-06-03 Yanou Cui , Lisa Randall , Brian Shuve

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 formation of baryon asymmetry in the Universe is considered in the left-right asymmetry model of weak interaction. In this model, the nature of CP violation is associated with the presence of a right vector boson admixture, with a…

高能物理 - 唯象学 · 物理学 2026-05-22 A. P. Serebrov , O. M. Zherebtsov , A. K. Fomin , R. M. Samoilov , N. S. Budanov

The Minimal Supersymmetric Standard Model has a candidate dark matter particle in its spectrum and may be able to generate the baryon asymmetry of the Universe (BAU) at the electroweak phase transition. In the Constrained MSSM, we find the…

高能物理 - 唯象学 · 物理学 2009-10-31 Sacha Davidson , Toby Falk , Marta Losada

The possibility that both the baryon asymmetry and dark matter arise from the late decay of a population of supersymmetric particles is considered. If the decay takes place below the LSP freeze out temperature, a nonthermal distribution of…

高能物理 - 唯象学 · 物理学 2009-10-28 Scott Thomas

We investigate the possibility that dark matter and the baryon asymmetry of the Universe are generated by the same mechanism, following an idea initially proposed by V.A. Kuzmin and recently discussed by R. Kitano and I. Low. In our model,…

高能物理 - 唯象学 · 物理学 2009-11-11 Nicolas Cosme , Laura Lopez Honorez , Michel H. G. Tytgat

Baryogenesis appears to require lepton number violation. This is naturally realized in extensions of the standard model containing right-handed neutrinos. We discuss the generation of a baryon asymmetry by the out-of-equilibrium decay of…

高能物理 - 唯象学 · 物理学 2007-05-23 W. Buchmuller , M. Plumacher

The experimental fact that the energy density in Dark Matter and in Baryons is of the same order is one of the most puzzling in cosmology. In this letter we suggest a new mechanism able to explain this coincidence in the context of…

高能物理 - 唯象学 · 物理学 2014-05-28 Giorgio Arcadi , Laura Covi , Marco Nardecchia

In a baryon-symmetric universe, the baryon asymmetry observed for visible matter is matched by an equal and opposite asymmetry for dark matter, thereby closely connecting the number densities of both types of matter. This is a necessary…

高能物理 - 唯象学 · 物理学 2015-06-12 Raymond R. Volkas

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

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 2009-11-11 Glennys R. Farrar , Gabrijela Zaharijas

We will review the main aspects of a mechanism for the contemporary generation of the baryon and Dark Matter abundances from the out-of-equilibrium decay of a Wimp-like mother particle and briefly discuss a concrete realization in a…

高能物理 - 唯象学 · 物理学 2016-03-23 Giorgio Arcadi

We present a generic framework, "baryomorphosis", which modifies the baryon asymmetry to be naturally of the order of a typical thermal relic WIMP density. We consider a simple scalar-based model to show how this is possible. This model…

高能物理 - 唯象学 · 物理学 2015-05-20 John McDonald
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