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相关论文: Diversity of Fuzzy Dark Matter Solitons

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Fuzzy dark matter (FDM) is a compelling candidate for dark matter, offering a natural explanation for the structure of diffuse low-mass haloes. However, the canonical FDM model with a mass of $10^{-22}~{\rm eV}$ encounters challenges in…

Dark matter may be composed of ultra-light bosons whose de Broglie wavelength in galaxies is of order 1 kpc. The standard model for this fuzzy dark matter (FDM) is a complex scalar field that obeys the Schr\"odinger-Poisson equations. The…

宇宙学与河外天体物理 · 物理学 2023-11-23 Boris Zupancic , Lawrence M. Widrow

Fuzzy Dark Matter (FDM) has recently gained attention as a motivated candidate for the dark matter (DM) content of the Universe, as opposed to the commonly assumed cold DM (CDM), since the soliton profile intrinsic to FDM models was found…

宇宙学与河外天体物理 · 物理学 2024-08-01 Tatyana Shevchuk , Ely D. Kovetz , Adi Zitrin

According to the Schr\"odinger-Poisson (SP) equations, fuzzy dark matter (FDM) can form a stable equilibrium configuration, the so-called FDM soliton. The SP system can also determine the evolution of FDM solitons, such as head-on…

宇宙学与河外天体物理 · 物理学 2024-12-30 Chen Tan , Jing-Kang Bin , Ke Wang

Fuzzy dark matter (FDM) is composed of ultra-light bosons having a de Broglie wavelength that is comparable to the size of the stellar component of galaxies at typical galactic velocities. FDM behaves like cold dark matter on large scales.…

星系天体物理 · 物理学 2021-07-07 Ben Bar-Or , Jean-Baptiste Fouvry , Scott Tremaine

An intriguing alternative to cold dark matter (CDM) is that the dark matter is a light ( $m \sim 10^{-22}$ eV) boson having a de Broglie wavelength $\lambda \sim 1$ kpc, often called fuzzy dark matter (FDM). We describe the arguments from…

宇宙学与河外天体物理 · 物理学 2017-03-08 Lam Hui , Jeremiah P. Ostriker , Scott Tremaine , Edward Witten

Fuzzy Dark Matter (FDM), consisting of ultralight bosons ($m_{\rm b} \sim 10^{-22}\ \rm eV$), is an intriguing alternative to Cold Dark Matter. Numerical simulations that solve the Schr\"odinger-Poisson (SP) equation show that FDM halos…

Stability properties of gravitationally bound condensates composed of ultralight axionic Fuzzy Dark Matter (FDM) are studied. Previous work has shown that astrophysical collisions could make self-gravitating condensates structurally…

宇宙学与河外天体物理 · 物理学 2018-12-11 Joshua Eby , Madelyn Leembruggen , Peter Suranyi , L. C. R. Wijewardhana

The fuzzy dark matter model (FDM, also known as quantum wave dark matter model) argues that light bosons with a mass of $\sim10^{-22}{\;{\rm eV}}$ are a possible candidate for dark matter in the Universe. One of the most important…

星系天体物理 · 物理学 2020-02-12 Zhi Li , Juntai Shen , Hsi-Yu Schive

Fuzzy dark matter (FDM), composed of ultralight bosons, exhibits intricate wave phenomena on galactic scales. Compared to cold dark matter, FDM simulations are significantly more computationally demanding due to the need to resolve the de…

宇宙学与河外天体物理 · 物理学 2026-04-07 Hsi-Yu Schive

Dark matter may be composed of light bosons, ${m_b \sim 10^{-22}\, \mathrm{eV}}$, with a de Broglie wavelength $\lambda \sim 1 \,\mathrm{kpc}$ in typical galactic potentials. Such `fuzzy' dark matter (FDM) behaves like cold dark matter…

星系天体物理 · 物理学 2019-01-28 Ben Bar-Or , Jean-Baptiste Fouvry , Scott Tremaine

Fuzzy dark matter (FDM) is an attractive dark matter candidate composed of ultralight particles. In this paper, toward a clear understanding of the core-halo relation in the FDM halos, we consider a simple model of the soliton-halo system,…

宇宙学与河外天体物理 · 物理学 2024-11-25 Yusuke Manita , Takuya Takahashi , Atsushi Taruya

We investigate cosmological structure formation in Fuzzy Dark Matter (FDM) with an attractive self-interaction (SI) with numerical simulations. Such a SI would arise if the FDM boson were an ultra-light axion, which has a strong CP…

The era of precision cosmology allows us to test the composition of the dark matter. Mixed ultralight or fuzzy dark matter (FDM) is a cosmological model with dark matter composed of a combination of particles of mass $m\leq…

宇宙学与河外天体物理 · 物理学 2023-12-11 Alex Laguë , Bodo Schwabe , Renée Hložek , David J. E. Marsh , Keir K. Rogers

Dark matter as scalar particles consisting of multiple species is well motivated in string theory where axion fields are ubiquitous. A two-field fuzzy dark matter (FDM) model features two species of ultralight axion particles with different…

宇宙学与河外天体物理 · 物理学 2024-02-01 Hoang Nhan Luu , Philip Mocz , Mark Vogelsberger , Simon May , Josh Borrow , S. -H. Henry Tye , Tom Broadhurst

The axion-like particles with ultralight mass ($\sim10^{-22}$eV) can be a possible candidate of dark matter, known as the fuzzy dark matter (FDM). These particles form Bose-Einstein condensate in the early Universe which can explain the…

广义相对论与量子宇宙学 · 物理学 2022-01-14 Shreyansh S. Dave , Sanatan Digal

Ultralight bosonic dark matter called fuzzy dark matter (FDM) has attracted much attention as an alternative to the cold dark matter. An intriguing feature of the FDM model is the presence of a soliton core, a stable dense core formed at…

宇宙学与河外天体物理 · 物理学 2022-12-07 Atsushi Taruya , Shohei Saga

We investigate phenomenologically the viability of fuzzy dark matter (FDM). We do this by confronting the predictions of the model, in particular, the formation of a solitonic core at the center of dark matter halos, with a homogeneous and…

星系天体物理 · 物理学 2024-03-15 Andrés Bañares-Hernández , Andrés Castillo , Jorge Martin Camalich , Giuliano Iorio

Fuzzy Dark Matter (FDM) comprised of ultralight ($m \sim 10^{-22}~\rm{eV}$) boson particles has received significant attention as a viable alternative to Cold Dark Matter (CDM), as it approximates CDM on large scales ($\gtrsim 1$ Mpc) while…

宇宙学与河外天体物理 · 物理学 2024-02-28 Connor A. Painter , Michael Boylan-Kolchin , Philip Mocz , Mark Vogelsberger

Fuzzy Dark Matter (FDM) is one of the recent models for dark matter. According to this model, dark matter is made of very light scalar particles with considerable quantum mechanical effects on the galactic scale, which solves many problems…

星系天体物理 · 物理学 2020-05-13 Alireza Maleki , Shant Baghram , Sohrab Rahvar
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