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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

Scalar Field Dark Matter (SFDM), comprised of ultralight ($\gtrsim 10^{-22}$ eV) bosons, is distinguished from massive ($\gtrsim$ GeV), collisionless Cold Dark Matter (CDM) by its novel structure-formation dynamics as Bose-Einstein…

星系天体物理 · 物理学 2021-05-26 Sonja O. Schobesberger , Tanja Rindler-Daller , Paul R. Shapiro

(abridged) We present simulations of halo formation and evolution in scalar field dark matter (SFDM) cosmologies in the Thomas-Fermi regime, aka ``SFDM-TF", where a strong repulsive 2-particle self-interaction (SI) is included, being a…

星系天体物理 · 物理学 2023-08-21 Horst Foidl , Tanja Rindler-Daller , Werner Zeilinger

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

Scalar-field dark matter (SFDM) halos exhibit a core-envelope structure with soliton-like cores and CDM-like envelopes. Simulations without self-interaction (free-field case) report a core-halo mass relation $M_c\propto M_{h}^{\beta}$, with…

星系天体物理 · 物理学 2022-11-08 Luis E. Padilla , Tanja Rindler-Daller , Paul R. Shapiro , Tonatiuh Matos , J. Alberto Vázquez

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

Building upon results of cosmological simulations of ultra-light scalar field dark matter (SFDM), we present a comprehensive model for the density profiles of SFDM haloes as a function of halo virial mass $M_{\rm h}$ and scalar field mass…

宇宙学与河外天体物理 · 物理学 2018-12-12 Victor H. Robles , James S. Bullock , Michael Boylan-Kolchin

The scalar field endowed with a cosh scalar field potential, behaves exactly in the same way as cold dark matter (CDM) in the region where the scalar field oscillates around its minimum. Also, in the linear regime, the scalar field dark…

天体物理学 · 物理学 2021-02-09 Argelia Bernal , Tonatiuh Matos , Dario Nunez

In the last time the cold dark matter (CDM) model has suggested more and more that it is not able to describe all the properties of nearby galaxies that can be observed in great detail as well as that it has some problems in the mechanism…

宇宙学与河外天体物理 · 物理学 2015-06-04 Juan Magaña , Tonatiuh Matos , Victor Robles , Abril Suárez

In recent times, the Scalar Field Dark Matter (SFDM) model (also called Fuzzy, Wave, Ultralight dark matter model) has received much attention due to its success in describing dark matter on both cosmological and galactic scales. Several…

星系天体物理 · 物理学 2022-03-25 Tonatiuh Matos , Abdel Perez-Lorenzana , Jordi Solís-López

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), consisting of ultralight bosons, is an intriguing alternative to Cold Dark Matter. Numerical simulations solving the Schr\"odinger-Poisson (SP) equation, which governs FDM dynamics, show that FDM halos consist of a…

We have derived the first, fully-cosmological, similarity solutions for CDM halo formation in the presence of nongravitational collisionality, which provides an analytical theory of the effect of the self-interacting dark matter (SIDM)…

天体物理学 · 物理学 2009-11-10 Kyungjin Ahn , Paul R. Shapiro

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

Fuzzy dark matter (FDM) is a dark matter candidate consisting of ultra-light scalar particles with masses around $10^{-22} \mathrm{eV}/c^2$, a regime where cold bosonic matter behaves as a collective wave rather than individual particles.…

宇宙学与河外天体物理 · 物理学 2023-07-19 Simon May , Volker Springel

Recent observations of tidal debris around galaxies have revealed that the structural properties of the spheroidal components of tidally disturbed galaxies are similar to those found in non-interacting early-type galaxies(ETGs), likely due…

星系天体物理 · 物理学 2015-03-04 Victor H. Robles , L. A. Martinez-Medina , T. Matos

(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

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

Bose-Einstein-condensed dark matter, also called scalar-field dark matter (SFDM), has become a popular alternative to cold dark matter (CDM), because it predicts galactic cores, in contrast to the cusps of CDM halos ("cusp-core problem").…

星系天体物理 · 物理学 2022-06-08 Kevin Pils , Tanja Rindler-Daller

Self-interacting dark matter (SIDM) is an intriguing alternative to the standard cold dark matter (CDM) paradigm, which predicts that dark matter halos typically have large, isothermal cores. Numerical simulations have shown that dynamical…

星系天体物理 · 物理学 2026-02-16 Frank C. van den Bosch , Shashank Dattathri
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