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相关论文: Hydrodynamics of Filtered Dark Matter: A Two-Compo…

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Motivated by current status of dark matter (DM) search, a new type of DM production mechanism is proposed based on thedynamical process of a strong first-order phase transition in the early universe, namely, the filtered DM mechanism. We…

高能物理 - 唯象学 · 物理学 2023-09-12 Siyu Jiang , Fa Peng Huang , Chong Sheng Li

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

Bubble columns are present in several applications, such as chemical and biochemical reactors and petrochemical and environmental engineering industries. This variety of applications is why understanding the bubble columns' dynamics is…

流体动力学 · 物理学 2023-04-20 Carlos Mendez , Fabio Santos , Gabriel Gonçalves

In this paper we present a novel mechanism for producing the observed Dark Matter(DM) relic abundance during the First Order Phase Transition (FOPT) in the early universe. We show that the bubble expansion with ultra-relativistic velocities…

高能物理 - 唯象学 · 物理学 2021-01-15 Aleksandr Azatov , Miguel Vanvlasselaer , Wen Yin

We consider a first order phase transition (FOPT) for a Vector Dark Matter (VDM) in the early universe in which its mass may partially arise from such mechanism in the hidden sector. We calculate the ratio of VDM that may enter the bubble…

高能物理 - 唯象学 · 物理学 2024-07-10 Mojtaba Hosseini , Seyed Yaser Ayazi , Ahmad Mohamadnejad

First-order phase transitions (FOPT) are ubiquitous in beyond the Standard Model physics and leave distinctive echoes in the history of early universe. We consider a FOPT serving the well-motivated role of dark matter mass generation and…

高能物理 - 唯象学 · 物理学 2026-02-13 Miha Nemevšek , Yue Zhang

Fuzzy Dark Matter (FDM) represents an alternative and intriguing description of the standard Cold Dark Matter (CDM) fluid, able to explain the lack of direct detection of dark matter particles in the GeV sector and to alleviate small scales…

宇宙学与河外天体物理 · 物理学 2018-11-30 Matteo Nori , Riccardo Murgia , Vid Iršič , Marco Baldi , Matteo Viel

We consider cosmology of the recently introduced mimetic matter with higher derivatives (HD). Without HD this system describes irrotational dust - Dark Matter (DM) as we see it on cosmologically large scales. DM particles correspond to the…

广义相对论与量子宇宙学 · 物理学 2015-06-22 Leila Mirzagholi , Alexander Vikman

In the so-called unified dark fluid models, the dark sector gets simplified because dark matter and dark energy are replaced by a single fluid that behaves as the former at early times and as the latter at late times. In this short paper we…

广义相对论与量子宇宙学 · 物理学 2015-06-19 Ninfa Radicella , Diego Pavon

Fuzzy Dark Matter (FDM), particularly in the $10^{-22}$ eV mass regime is frequently used to characterize wave-like interference effects. It exhibits macroscopic wave properties, which drive distinct baryonic dynamics within collapsed…

In this talk, we present a mechanism of Dark Matter production during first order phase transitions and happening via the collision of the bubble wall and plasma quanta. We will first study the possibility that the dark matter is produced…

高能物理 - 唯象学 · 物理学 2024-12-10 Miguel Vanvlasselaer

The interface between liquid water and the Pt(111) metal surface is characterized structurally and thermodynamically via reactive molecular dynamics (MD) simulations within the ReaxFF framework. The formation of a distinct buckled adsorbate…

化学物理 · 物理学 2021-03-19 Christoph Karsten Jung , Laura Braunwarth , Andrey Sinyavskiy , Timo Jacob

In cosmological first-order phase transitions, gravitational waves are generated by the collisions of bubble walls and by the bulk motions caused in the fluid. A sizeable signal may result from fast-moving walls. In this work we study the…

宇宙学与河外天体物理 · 物理学 2016-02-16 Leonardo Leitao , Ariel Megevand

If the mass of dark matter is generated from a cosmological phase transition involving the nucleation of bubbles, the corresponding bubble walls can filter out dark matter particles during the phase transition. Only particles with…

高能物理 - 唯象学 · 物理学 2020-05-20 Dongjin Chway , Tae Hyun Jung , Chang Sub Shin

We introduce new classes of hydrodynamic theories inspired by the recently discovered fracton phases of quantum matter. Fracton phases are characterized by elementary excitations (fractons) with restricted mobility. The hydrodynamic…

强关联电子 · 物理学 2020-07-29 Andrey Gromov , Andrew Lucas , Rahul M. Nandkishore

Mirroring their role in electrical and optical physics, two-dimensional crystals are emerging as novel platforms for fluid separations and water desalination, which are hydrodynamic processes that occur in nanoscale environments. For…

统计力学 · 物理学 2016-05-11 Steven E. Strong , Joel D. Eaves

The mass window of ultralight axion dark matter motivated by suppressing the growth of structure on subgalactic scales, $m\sim 10^{-22}\,\mathrm{eV}$, is now severely constrained by various observation data (e.g. Lyman-$\alpha$ forest). As…

宇宙学与河外天体物理 · 物理学 2025-06-26 Qi Yang , Bohua Li , Paul R. Shapiro

We investigate the dynamical friction (DF) acting on circularly-moving perturbers in fuzzy dark matter (FDM) backgrounds. After condensation, FDM is described by a single wave function satisfying a Schr\"odinger-Poisson equation. An…

宇宙学与河外天体物理 · 物理学 2023-01-25 Robin Buehler , Vincent Desjacques

A fundamental principle of chaotic quantum dynamics is that local subsystems eventually approach a thermal equilibrium state. Large subsystems thermalize slower: their approach to equilibrium is limited by the hydrodynamic build-up of…

Applications of metallic metamaterials have generated significant interest in recent years. Electromagnetic behavior of metamaterials in the optical range is usually characterized by a local-linear response. In this article, we develop a…

光学 · 物理学 2016-11-01 Ming Fang , Zhixiang Huang , Wei E. I. Sha , Xiaoyan Y. Z. Xiong , Xianliang Wu
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