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相关论文: Pangenesis: a common origin for visible and dark m…

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The similarity of the visible and dark matter abundances indicates that they may originate via the same mechanism. If both the dark and the visible matter are charged under a generalized baryon number which remains always conserved, then…

高能物理 - 唯象学 · 物理学 2011-12-09 Nicole F. Bell , Kalliopi Petraki , Ian M. Shoemaker , Raymond R. Volkas

Pangenesis is the mechanism for jointly producing the visible and dark matter asymmetries via Affleck-Dine dynamics in a baryon-symmetric universe. The baryon-symmetric feature means that the dark asymmetry cancels the visible baryon…

高能物理 - 唯象学 · 物理学 2012-05-21 Benedict von Harling , Kalliopi Petraki , Raymond R. Volkas

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

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

Fragmentation of the Affleck-Dine condensate into Q-balls could fill the Universe with dark matter either in the form of stable baryonic balls, or LSP produced from the decay of unstable Q-balls. The dark matter and the ordinary matter in…

高能物理 - 唯象学 · 物理学 2009-10-31 Alexander Kusenko

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

We investigate the possibility that both the baryon asymmetry of the universe and the observed cold dark matter density are generated by decays of a heavy scalar field which dominates the universe before nucleosynthesis. Since baryons and…

高能物理 - 唯象学 · 物理学 2008-11-26 Ryuichiro Kitano , Hitoshi Murayama , Michael Ratz

We propose a novel framework in which the observed baryon and dark matter abundances are simultaneously generated via the Affleck-Dine mechanism. In its simplest realization, Affleck-Dine cogenesis is accomplished by a single superpotential…

高能物理 - 唯象学 · 物理学 2012-04-13 Clifford Cheung , Kathryn M. Zurek

The similar cosmological energy budgets in visible baryons and dark matter motivate one to consider a common origin for the generation of both. We outline the key features of scenarios that can accommodate a unified framework for the…

高能物理 - 唯象学 · 物理学 2015-06-04 Hooman Davoudiasl , Rabindra N. Mohapatra

The cosmological origin of both dark and baryonic matter can be explained through a unified mechanism called hylogenesis where baryon and antibaryon number are divided between the visible sector and a GeV-scale hidden sector, while the…

高能物理 - 唯象学 · 物理学 2012-12-04 Nikita Blinov , David E. Morrissey , Kris Sigurdson , Sean Tulin

Asymmetric dark matter models are based on the hypothesis that the present-day abundance of dark matter has the same origin as the abundance of ordinary or visible matter: an asymmetry in the number densities of particles and antiparticles.…

高能物理 - 唯象学 · 物理学 2013-08-02 Kalliopi Petraki , Raymond R. Volkas

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

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 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

Most of the mass of ordinary matter has its origin from quantum chromodynamics (QCD). A similar strong dynamics, dark QCD, could exist to explain the mass origin of dark matter. Using infrared fixed points of the two gauge couplings, we…

高能物理 - 唯象学 · 物理学 2014-03-27 Yang Bai , Pedro Schwaller

Combining one established idea with two recent ones, it is pointed out for the first time that three of the outstanding problems of particle physics and cosmology, i.e. neutrino mass, dark matter, and baryogenesis, may have a common…

高能物理 - 唯象学 · 物理学 2009-11-11 Ernest Ma

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

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

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

Low-scale supersymmetry breaking in string motivated theories implies the presence of O(100) TeV scale moduli, which generically lead to a significant modification of the history of the universe prior to Big Bang Nucleosynthesis. Such an…

高能物理 - 唯象学 · 物理学 2015-05-30 Gordon Kane , Jing Shao , Scott Watson , Hai-Bo Yu
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