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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

We study the formation of solitons inside scalar-field dark matter halos with a non-polynomial self-interaction potential. We consider a self-interaction potential that is quartic in the scalar field in the low-density regime but saturates…

宇宙学与河外天体物理 · 物理学 2025-07-31 Raquel Galazo García , Philippe Brax , Patrick Valageas

We study cosmological structure formation with ultralight axion dark matter, or "fuzzy dark matter (FDM), using a particle-mesh scheme to account for the quantum pressure arising in the Madelung formulation of the Schr\"odinger-Poisson…

宇宙学与河外天体物理 · 物理学 2017-01-03 Jan Veltmaat , Jens C. Niemeyer

Scalar Field Dark Matter (SFDM) comprised of ultralight ($\gtrsim 10^{-22}$ eV) bosons is an alternative to standard, collisionless Cold Dark Matter (CDM) that is CDM-like on large scales but inhibits small-scale structure formation. As a…

宇宙学与河外天体物理 · 物理学 2021-11-04 Paul R. Shapiro , Taha Dawoodbhoy , Tanja Rindler-Daller

The Ultra-Light Axion (ULA) is a dark matter candidate with mass $\mathcal{O}(10^{-22})$eV and de Broglie wavelength of order kpc. Such an axion, also called the Fuzzy Dark Matter (FDM), thermalizes via the gravitational force and forms a…

宇宙学与河外天体物理 · 物理学 2018-01-30 Jiajun Zhang , Yue-Lin Sming Tsai , Jui-Lin Kuo , Kingman Cheung , Ming-Chung Chu

An ultra-light bosonic particle of mass around $10^{-22}\,\mathrm{eV}/c^2$ is of special interest as a dark matter candidate, as it both has particle physics motivations, and may give rise to notable differences in the structures on highly…

宇宙学与河外天体物理 · 物理学 2024-06-18 Simon May , Volker Springel

Fuzzy Dark Matter (FDM), motivated by string theory, has recently become a hot candidate for dark matter. The rest mass of FDM is believed to be $\sim 10^{-22}$eV and the corresponding de-Broglie wave length is $\sim 1$kpc. Therefore, the…

宇宙学与河外天体物理 · 物理学 2019-01-08 Jiajun Zhang , Hantao Liu , Ming-Chung Chu

Axion-like particle (ALP) dark matter shows distinctive behavior on scales where wavelike effects dominate over self-gravity. Ultralight axions are candidates for fuzzy dark matter (FDM) whose de Broglie wavelength in virialized halos…

宇宙学与河外天体物理 · 物理学 2020-07-15 Jens C. Niemeyer

We investigate the effect of self-interactions on the shape and oscillations of the solitonic core profile of condensed fuzzy dark matter systems without the backdrop of a halo, revealing universal features in terms of an appropriately…

宇宙学与河外天体物理 · 物理学 2025-02-26 Milos Indjin , I-Kang Liu , Nick P. Proukakis , Gerasimos Rigopoulos

Dark matter models involving a very light bosonic particle, generally known as Fuzzy Dark Matter (FDM), have been recently attracting great interest in the cosmology community, as their wave-like phenomenology would simultaneously explain…

宇宙学与河外天体物理 · 物理学 2020-12-23 Matteo Nori , Marco Baldi

(abridged)Scalar field dark matter (SFDM) made of bosons has become a popular alternative to the CDM paradigm, especially for its potential to cure the so-called "small-scale problems" of CDM. Cosmological simulations have determined that…

宇宙学与河外天体物理 · 物理学 2025-06-19 Matthias Stallovits , Tanja Rindler-Daller

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

Scalar Field Dark Matter (SFDM) comprised of ultralight bosons has attracted great interest as an alternative to standard, collisionless Cold Dark Matter (CDM) because of its novel structure-formation dynamics, described by the coupled…

宇宙学与河外天体物理 · 物理学 2021-08-03 Taha Dawoodbhoy , Paul R. Shapiro , Tanja Rindler-Daller

We investigate the role of contact interactions in the dynamics of fuzzy dark matter (FDM) modeled through the Schr\"odinger-Poisson equation in one spatial dimension. While the $\Lambda$CDM paradigm successfully explains structure…

宇宙学与河外天体物理 · 物理学 2026-02-27 Óscar Rodríguez-Villalba , Ivan Saychenko , Massimo Pietroni , Sandro Wimberger

(abridged) We continue the study of $\Lambda$SFDM cosmologies, which differ from $\Lambda$CDM in that CDM is replaced by scalar field dark matter (SFDM) by calculating the evolution of the background Universe, as well as linear…

宇宙学与河外天体物理 · 物理学 2023-06-16 Horst Foidl , Tanja Rindler-Daller

In the context of Fuzzy Dark Matter (FDM) we study the core formation in the presence of an Ideal Gas (IG). Our analysis is based on the solution of the Schr\"odinger-Poisson-Euler system of equations that drives the evolution of FDM…

宇宙学与河外天体物理 · 物理学 2025-11-17 Ivan Alvarez-Rios , Francisco S. Guzman , Jens Niemeyer

According to the Schr\"odinger-Poisson equations, fuzzy dark matter (FDM) can form a stable equilibrium configuration, the so-called FDM soliton. In principle, given the FDM particle mass, the profile of the FDM soliton is fixed. In…

高能物理 - 唯象学 · 物理学 2025-08-29 Chen Tan , M. Le Delliou , Ke Wang

It has been postulated that Fuzzy Dark Matter (FDM) could be a viable alternative to Cold Dark Matter (CDM). FDM is comprised of ultralight bosons which exist as a Bose-Einstein condensate. Due to the very low mass of FDM, the de Broglie…

宇宙学与河外天体物理 · 物理学 2019-02-28 V. Sreenath

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) made of ultra-light bosonic particles is a viable alternative to cold dark matter (CDM) with clearly distinguishable small-scale features in collapsed structures. On large scales, it behaves gravitationally like CDM…

宇宙学与河外天体物理 · 物理学 2022-05-11 Bodo Schwabe , Jens C. Niemeyer
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