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相关论文: Cosmic Filament Spin from Dark Matter Vortices

200 篇论文

The halo spin flip refers to the phenomenon that the spin axes of dark matter halos with masses above a certain threshold tend to be preferentially aligned perpendicular to the hosting large-scale filaments, while low-mass halos tend to…

宇宙学与河外天体物理 · 物理学 2020-08-05 Jounghun Lee , Noam I Libeskind , Suho Ryu

The superfluid dark matter model offers an elegant solution to reconcile discrepancies between the predictions of the cold dark matter paradigm and observations on galactic scales. In this scenario, dark matter is composed of ultralight…

宇宙学与河外天体物理 · 物理学 2026-02-17 Lasha Berezhiani , Giordano Cintia , Valerio De Luca , Justin Khoury

Peculiar dynamics of a free surface of the superfluid 4He has been observed experimentally with a newly established technique utilizing a number of electrically charged fine metal particles trapped electrically at the surface by Moroshkin…

其他凝聚态物理 · 物理学 2019-01-30 S. Inui , M. Tsubota , P. Moroshkin , P. Leiderer , K. Kono

Galaxies and their dark-matter halos are commonly presupposed to spin. But it is an open question how this spin manifests in halos and soliton cores made of scalar dark matter (SDM, including fuzzy/wave/ultralight-axion dark matter). One…

宇宙学与河外天体物理 · 物理学 2023-12-14 Noah Glennon , Anthony E. Mirasola , Nathan Musoke , Mark C. Neyrinck , Chanda Prescod-Weinstein

Vorticity is ubiquitous in nature however, to date, studies of vorticity in cosmology and the early universe have been quite rare. In this paper, based on a talk in session CM1 of the 13th Marcel Grossmann Meeting, we consider vorticity…

宇宙学与河外天体物理 · 物理学 2012-10-09 Adam J. Christopherson , Karim A. Malik

We develop a theory of dark matter based on a previously proposed picture, in which a complex vacuum scalar field makes the universe a superfluid, with the energy density of the superfluid giving rise to dark energy, and variations from…

广义相对论与量子宇宙学 · 物理学 2014-04-30 Kerson Huang , Chi Xiong , Xiaofei Zhao

We derive oscillating gravitational potential caused by an ultralight axion as the cosmic dark matter, assuming the Compton wavelength smaller than the horizon scale. A new oscillatory term is found which dominates the previously known one…

宇宙学与河外天体物理 · 物理学 2021-12-08 Jai-chan Hwang , Hyerim Noh

An axion rotating in field space can produce dark photons in the early universe via tachyonic instability. This explosive particle production creates a background of stochastic gravitational waves that may be visible at pulsar timing arrays…

高能物理 - 唯象学 · 物理学 2022-01-05 Raymond T. Co , Keisuke Harigaya , Aaron Pierce

Both simulations and observations have found that the spin of halo/galaxy is correlated with the large scale environment, and particularly the spin of halo flips in filament. A consistent picture of halo spin evolution in different…

宇宙学与河外天体物理 · 物理学 2017-04-19 Peng Wang , Xi Kang

Dark photon dark matter may be produced by the cosmic strings in association with the dark U(1) gauge symmetry breaking. We perform three-dimensional lattice simulations of the Abelian-Higgs model and follow the evolution of cosmic strings.…

高能物理 - 唯象学 · 物理学 2023-08-04 Naoya Kitajima , Kazunori Nakayama

A new scenario for creation of galactic magnetic fields is proposed which is operative at the cosmological epoch of the galaxy formation, and which relies on unconventional properties of dark matter. Namely, it requires existence of feeble…

宇宙学与河外天体物理 · 物理学 2013-12-09 Zurab Berezhiani , A. D. Dolgov , I. I. Tkachev

We present a minimal model of fermionic dark matter (DM), where a singlet Dirac fermion can interact with the Standard Model (SM) particles via the torsion field of gravitational origin. In general, torsion can be realized as an…

高能物理 - 唯象学 · 物理学 2020-04-15 Basabendu Barman , Tapobroto Bhanja , Debottam Das , Debaprasad Maity

The recent WMAP data have confirmed that exotic dark matter together with the vacuum energy (cosmological constant) dominate in the flat Universe. The nature of the dark matter constituents cannot be determined till they are directly…

高能物理 - 唯象学 · 物理学 2010-01-21 J. D. Vergados

Matter in the Universe is arranged in a cosmic web, with a filament of matter typically connecting each neighbouring galaxy pair, separated by tens of millions of light-years. A quadrupolar pattern of the spin field around filaments is…

宇宙学与河外天体物理 · 物理学 2021-09-01 Qianli Xia , Mark C. Neyrinck , Yan-Chuan Cai , Miguel A. Aragón-Calvo

In this paper we propose a dark matter model and study aspects of its phenomenology. Our model is based on a new dark matter sector with a U(1)' gauge symmetry plus a discrete symmetry added to the Standard Model of particle physics. The…

高能物理 - 唯象学 · 物理学 2010-04-15 Xiao-Jun Bi , Robert Brandenberger , Paolo Gondolo , Tianjun Li , Qiang Yuan , Xinmin Zhang

Fuzzy (wave) dark matter (FDM), the dynamical model underlying an ultralight bosonic dark matter species, produces a rich set of non-gravitational signatures that distinguishes it markedly from the phenomenologically related warm (particle)…

宇宙学与河外天体物理 · 物理学 2025-04-22 Tim Zimmermann , David J. E. Marsh , Keir K. Rogers , Hans A. Winther , Sijing Shen

This document is on considerations and findings on modelling of spinning beams. Spinning has been proposed for stabilizing beams against perturbations notably risen by non-linear space charge forces, see [Y.-L. Cheon et al., Effects of beam…

加速器物理 · 物理学 2024-08-16 L. Groening

The existence of a scaling network of current-carrying cosmic strings in our Universe is expected to continuously create loops endowed with a conserved current during the cosmological expansion. These loops radiate gravitational waves and…

宇宙学与河外天体物理 · 物理学 2021-04-30 Pierre Auclair , Patrick Peter , Christophe Ringeval , Daniele Steer

We revisit the question of what mechanism is responsible for the spins of halos of dark matter. The answer to this question is of high importance for modeling galaxy intrinsic alignment, which can potentially contaminate current and future…

宇宙学与河外天体物理 · 物理学 2021-05-12 E. Ebrahimian , A. A. Abolhasani