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Minimal atomic dark matter with its distinctive cooling mechanisms offers an instructive framework for understanding the potential impact of dark matter on small-scale structure formation and early cosmology. The model consists of two…

高能物理 - 唯象学 · 物理学 2026-02-12 Jared Barron , Rouven Essig , Megan H. McDuffie , Jesús Pérez-Ríos , Gregory Suczewski

We review current cosmological constraints on the axion. We describe the basic mechanisms by which axions are created in the early universe, focussing on the standard thermal scenario where the dominant process is through axion radiation by…

天体物理学 · 物理学 2016-08-30 R. A. Battye , E. P. S. Shellard

Dark matter axions form a rethermalizing Bose-Einstein condensate. This provides an opportunity to distinguish axions from other forms of dark matter on observational grounds. I show that if the dark matter is axions, tidal torque theory…

星系天体物理 · 物理学 2015-05-18 Pierre Sikivie

If dark matter (DM) acquires mass during a first order phase transition, there will be a filtering-out effect when DM enters the expanding bubble. In this paper we study the filtering-out effect for a pseudo-scalar DM, whose mass may…

高能物理 - 唯象学 · 物理学 2021-06-30 Wei Chao , Xiu-Fei Li , Lei Wang

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 2007-05-23 Glennys R. Farrar , Gabrijela Zaharijas

We study the dynamics of axions at first-order phase transitions in non-Abelian gauge theories. When the duration of the phase transition is short compared to the timescale of the axion oscillations, the axion dynamics is similar to the…

高能物理 - 唯象学 · 物理学 2024-03-19 Junseok Lee , Kai Murai , Fuminobu Takahashi , Wen Yin

We propose a new theory of dark matter based on axion physics and cosmological phase transitions. We show that theories in which a gauge coupling increases through a first-order phase transition naturally result in `axion relic pockets':…

高能物理 - 唯象学 · 物理学 2024-08-23 Pierluca Carenza , Joshua Eby , Oksana Iarygina , M. C. David Marsh

We demonstrate a novel mechanism for the formation of topological defects in a first order phase transition for theories in the presence of small explicit symmetry breaking terms. We carry out numerical simulations of collisions of two…

高能物理 - 唯象学 · 物理学 2009-10-28 Sanatan Digal , Ajit M. Srivastava

We demonstrate that dark matter axion production is enhanced through a natural and unavoidable mechanism: primordial temperature fluctuations periodically modulate the axion mass during the QCD phase transition, thereby triggering…

高能物理 - 唯象学 · 物理学 2026-02-09 Pirzada , Yu Gao , Qiaoli Yang

We analyze the effect of primordial density perturbations on the cosmic QCD phase transition. According to our results hadron bubbles nucleate at the cold perturbations. We call this mechanism inhomogeneous nucleation. We find the typical…

天体物理学 · 物理学 2007-05-23 J. Ignatius , Dominik J. Schwarz

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 give an estimation of the masses of light dark matter particle and dark energy quasiparticle which can be extracted from the astrophysical data about the contributions of baryon, dark matter, and dark energy densities to the total…

宇宙学与河外天体物理 · 物理学 2010-05-12 V. E. Kuzmichev , V. V. Kuzmichev

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 demonstrate that B-ball decay in the MSSM can naturally solve the puzzle of why the densities of baryons and dark matter in the Universe are similar. This requires that the B-balls survive thermalization and decay below the freeze-out…

高能物理 - 唯象学 · 物理学 2009-10-31 Kari Enqvist , John McDonald

We point out that dark matter which is produced non-adiabatically in a phase transition (PT) with fast bubble walls receives a boost in velocity which leads to long free-streaming lengths. We find that this could be observed via the…

高能物理 - 唯象学 · 物理学 2023-03-16 Iason Baldes , Yann Gouttenoire , Filippo Sala

First order phase transitions in the early universe naturally lead to the production of a stochastic background of gravitational waves and to the generation of a matter-antimatter asymmetry. The dynamics of the phase transition is affected…

高能物理 - 唯象学 · 物理学 2022-11-30 Stefania De Curtis , Luigi Delle Rose , Andrea Guiggiani , Ángel Gil Muyor , Giuliano Panico

We consider the formation and evolution of Axion Quark Nugget dark matter particles in the early universe. The goal of this work is to estimate the mass distribution of these objects and assess their ability to form and survive to the…

高能物理 - 唯象学 · 物理学 2019-07-03 Shuailiang Ge , Kyle Lawson , Ariel Zhitnitsky

We extend the standard model fermions by a mirror copy to realize a left-right symmetry. During a strongly first order phase transition of the spontaneous left-right symmetry breaking, the CP-violating reflections of the mirror fermions off…

高能物理 - 唯象学 · 物理学 2020-01-09 Pei-Hong Gu

We have analyzed baryogenesis in the MSSM for the light stop scenario, where the phase transition is strong enough first order. We have found that enough baryon asymmetry can be generated provided that the phase of $\mu$ be $\simgt$ 0.01.…

高能物理 - 唯象学 · 物理学 2007-05-23 Mariano Quiros

We present a new mechanism for transferring a pre-existing lepton or baryon asymmetry to a dark matter asymmetry that relies on mass mixing which is dynamically induced in the early universe. Such mixing can succeed with only generic scales…

高能物理 - 唯象学 · 物理学 2011-12-14 Yanou Cui , Lisa Randall , Brian Shuve
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