4.7 Article

Dark matter profiles of SPARC galaxies: a challenge to fuzzy dark matter

相关参考文献

注意:仅列出部分参考文献,下载原文获取全部文献信息。
Article Astronomy & Astrophysics

Galaxy rotation favors prolate dark matter haloes

Adriana Bariego-Quintana et al.

Summary: The flattening rotation velocity v(r) -> constant discovered by Rubin and collaborators in the SPARC galaxy-rotation data is in line with Kepler's law in one less dimension. Elongated dark matter distributions, with their axis of prolateness perpendicular to the galactic plane, naturally reproduce this phenomenon. Detailed fits to the rotation data also support this theoretical understanding, showing that elongated distributions provide a better fit than purely spherical ones.

PHYSICAL REVIEW D (2023)

Article Astronomy & Astrophysics

Soliton formation and the core-halo mass relation: An eigenstate perspective

J. Luna Zagorac et al.

Summary: Ultralight dark matter (ULDM) is a dark matter candidate with a small particle mass. ULDM halos consist of a solitonic core and an NFW-like skirt. By simulating soliton mergers, we studied the core-halo mass relation and found no universal relationship for ULDM.

PHYSICAL REVIEW D (2023)

Article Astronomy & Astrophysics

Solitons in the dark: First approach to non-linear structure formation with fuzzy dark matter

Mattia Mina et al.

Summary: In this study, we present the results of a cosmological simulation using the new code SCALAR to study the formation and evolution of fuzzy dark matter. Despite limitations on large-scale resolution, the study provides detailed analysis of the formation and evolution of central solitonic cores. The results indicate a shallower halo mass function in the low-mass end due to the quantum nature of the scalar field.

ASTRONOMY & ASTROPHYSICS (2022)

Article Astronomy & Astrophysics

The diversity of core-halo structure in the fuzzy dark matter model

Hei Yin Jowett Chan et al.

Summary: In the fuzzy dark matter model, there is a significant dispersion in the core-halo mass relation, increasing with halo mass. A new empirical equation for the core-halo mass relation is provided, with uncertainties encompassing previously found relations. Any observational constraints on particle mass using a tight one-to-one core-halo mass relation should consider an additional uncertainty of about 50%.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2022)

Article Astronomy & Astrophysics

Constraining ultra light dark matter with the Galactic nuclear star cluster

Firat Toguz et al.

Summary: In this study, the existence of a dark matter "soliton core" predicted in the ultra-light dark matter (ULDM) model is tested using the nuclear star cluster (NSC) of the Milky Way. The results show that a soliton core for a single ULDM particle within a specific mass range is not supported by the observed data. Further dynamical modeling of a larger region of the Galactic center can provide tighter constraints on the mass of dark matter.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2022)

Article Astronomy & Astrophysics

Non-spherical dark matter structures detection

Nicolas Loizeau et al.

Summary: A rotation curve inequality for spherically symmetric mass distributions is derived and tested against the SPARC galaxy rotation curves dataset. Several galaxies, such as NGC7793 and UGC11557, are identified as potential hosts for non-spherical dark matter structures that could be detected through more precise measurements.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2022)

Article Physics, Multidisciplinary

Deep Zoom-In Simulation of a Fuzzy Dark Matter Galactic Halo

Bodo Schwabe et al.

Summary: Fuzzy dark matter (FDM) composed of ultralight bosonic particles is an alternative to cold dark matter with distinguishable features on small scales. While behaving gravitationally like cold dark matter on large scales, FDM exhibits unique wave interference effects near the de Broglie scale. Investigating these phenomena requires numerical integration of the Schrodinger equation, and the authors present an improved method for reconstructing the wave function inside previously collapsed structures.

PHYSICAL REVIEW LETTERS (2022)

Article Astronomy & Astrophysics

Excluding fuzzy dark matter with sizes and stellar kinematics of ultrafaint dwarf galaxies

Neal Dalal et al.

Summary: We use observations of ultrafaint dwarf galaxies to constrain the particle mass of ultralight dark matter. Based on simulations and measurements of UFDs, we derive a lower limit on the dark matter particle mass, which can potentially be strengthened in the future.

PHYSICAL REVIEW D (2022)

Article Astronomy & Astrophysics

Testing multiflavored ultralight dark matter models with SPARC

Lauren Street et al.

Summary: By comparing maximum likelihood estimates for different cold dark matter (CDM) models, this study finds that the Burkert and Einasto models perform better than other commonly used CDM models. For ultralight dark matter (ULDM) models, most galaxies prefer particle masses in the range of 10-23 eV < m < 10-20 eV. In double flavor models, galaxies tend to prefer approximately equal particle masses.

PHYSICAL REVIEW D (2022)

Article Astronomy & Astrophysics

Galactic rotation curves versus ultralight dark matter: A systematic comparison with SPARC data

Nitsan Bar et al.

Summary: This study presents observational constraints on the imprint of ultralight dark matter (ULDM) soliton cores in rotation-dominated galaxies. It disfavors the soliton-host halo relation found in numerical simulations in a broad range of ULDM particle masses. Combining these constraints with theoretical arguments, the study argues against ULDM comprising 100% of the cosmological dark matter in a specific mass range. The constraints explore the ULDM fraction down to less than 0.3 of the total dark matter.

PHYSICAL REVIEW D (2022)

Article Astronomy & Astrophysics

Scaling relations of fuzzy dark matter haloes - I. Individual systems in their cosmological environment

Matteo Nori et al.

Summary: By utilizing the N-body code AX-GADGET, the study investigates the evolution of FDM structures in a cosmological framework, revealing the significant impact of the dynamical state, morphology, and merger history of individual systems on the scaling relations between solitonic cores and host haloes properties.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

Novel constraints on the particle nature of dark matter from stellar streams

Nilanjan Banik et al.

Summary: This paper provides constraints on alternative dark matter scenarios based on tidal streams analysis, deriving lower limits for warm dark matter and ultra-light dark matter masses using data from streams and dwarf satellite counts.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

Article Astronomy & Astrophysics

A cautionary tale in fitting galaxy rotation curves with Bayesian techniques: Does Newton's constant vary from galaxy to galaxy?

Pengfei Li et al.

Summary: The application of Bayesian techniques in astronomical data analysis faces challenges due to potential parameter degeneracies and uncertainties in error models. An analysis on rotation curves from the SPARC database shows that the inference of a variable G(N) is influenced by the combined effect of parameter degeneracies and uncertainties in error models.

ASTRONOMY & ASTROPHYSICS (2021)

Article Physics, Multidisciplinary

Constraints on Dark Matter Properties from Observations of Milky Way Satellite Galaxies

E. O. Nadler et al.

Summary: The study on Milky Way satellite galaxies provides strong cosmological constraints on various particle models of dark matter, supporting the cold, collisionless dark matter paradigm. Limits are reported on the mass of thermal relic warm dark matter, velocity-independent dark matter-proton scattering cross section, and the mass of fuzzy dark matter, complementing other observational and laboratory constraints on dark matter properties.

PHYSICAL REVIEW LETTERS (2021)

Article Physics, Multidisciplinary

Strong Bound on Canonical Ultralight Axion Dark Matter from the Lyman-Alpha Forest

Keir K. Rogers et al.

Summary: By using the Lyman-alpha forest to search for suppressed cosmic structure growth, we present a new lower limit on the ultralight axion (ULA) dark matter mass m(a): m(a) > 2 x 10(-20) eV. This study strongly disfavors the canonical ULA with mass within the range of 10(-22) eV to 10(-21) eV.

PHYSICAL REVIEW LETTERS (2021)

Article Astronomy & Astrophysics

Narrowing the Mass Range of Fuzzy Dark Matter with Ultrafaint Dwarfs

Kohei Hayashi et al.

Summary: Research has found that most of the ultrafaint dwarf galaxies prefer FDM particle masses heavier than 10(-21) eV, with Segue 1 providing the strongest constraint. Additionally, the constraints obtained in this study are compatible with various other independent cosmological and astrophysical bounds found in the literature, but are not compatible with the bounds from luminous dwarf galaxies.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Astronomy & Astrophysics

Don't cross the streams: caustics from fuzzy dark matter

Neal Dalal et al.

Summary: The study explores how tidal streams from globular clusters can be used to constrain the mass of ultra-light dark matter particles, with a focus on 'fuzzy' dark matter models. It is found that FDM perturbations impact tidal streams, with the possibility of determining FDM mass by analyzing fluctuations in quantities like angular momenta or actions.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

Article Astronomy & Astrophysics

On filaments, prolate halos and rotation curves

K. Zatrimaylov

Summary: This research proposes a simple geometric mechanism to explain the flattening of galactic rotation curves, suggesting that the presence of thin string-like objects or elongated dark matter halos induces local compression of field lines around their planes. By fitting 83 rotation curves and analyzing two galaxies in depth, it was found that the presence of a filament significantly improves the fit quality in many cases. This implies the existence of elongated mass distributions away from the galactic plane in several galaxies and could impact the ongoing debate between cold dark matter (CDM), self-interacting dark matter (SiDM), and modified Newtonian dynamics (MOND).

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

Review Astronomy & Astrophysics

Wave Dark Matter

Lam Hui

Summary: This paper reviews the physics and phenomenology of wave dark matter, outlining its particle physics motivations and rich phenomenology. Wave interference in dark matter leads to unique structures like vortices and solitons, with potential implications for observed astronomical phenomena. Detection experiments and theoretical predictions for wave dark matter are discussed, highlighting the importance of understanding the stochastic nature of waves in interpreting constraints and measurements.

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, VOL 59 (2021)

Article Astronomy & Astrophysics

The MUSE-Faint survey II. The dark-matter density profile of the ultra-faint dwarf galaxy Eridanus 2

Sebastiaan L. Zoutendijk et al.

Summary: Using stellar line-of-sight velocities, the study constrained the dark matter density profile of the ultra-faint dwarf galaxy Eridanus 2, deriving constraints on self-interacting and fuzzy dark matter scenarios. The results favored cold dark matter over self-interacting dark matter, and provided evidence for fuzzy dark matter. The study also found consistency with the literature regarding the mass-to-light ratio and set limits on core and soliton sizes. The constraints on self-interaction and fuzzy-dark matter particle mass offered complementary information and challenged previous results obtained for larger dwarf galaxies.

ASTRONOMY & ASTROPHYSICS (2021)

Review Astronomy & Astrophysics

Ultra-light dark matter

Elisa G. M. Ferreira

Summary: Ultra-light dark matter, composed of bosons with masses ranging from 10(-24)eV < m < eV, has garnered attention for its ability to form a Bose-Einstein condensate or superfluid on galactic scales. Various models have been proposed, including fuzzy dark matter, self-interacting fuzzy dark matter, and DM superfluid, with the potential to reconcile the cold DM picture with small-scale behavior. These models present a rich phenomenology and are being tested using astrophysical and cosmological observations.

ASTRONOMY AND ASTROPHYSICS REVIEW (2021)

Article Astronomy & Astrophysics

Soliton oscillations and revised constraints from Eridanus II of fuzzy dark matter

Barry T. Chiang et al.

Summary: The study demonstrates that soliton density oscillations persist even after significant tidal stripping of the outer halo. The central star cluster in Eridanus II has a characteristic timescale related to soliton density oscillations, but it significantly deviates from the timescale of the star cluster itself.

PHYSICAL REVIEW D (2021)

Article Astronomy & Astrophysics

Model-independent Constraints on Ultralight Dark Matter from the SPARC Data

Man Ho Chan et al.

Summary: In this study, a model-independent analysis using Spitzer Photometry and Accurate Rotation Curves data is conducted to constrain the mass range of Ultralight dark matter (ULDM). The results show that the ULDM proposal may not be able to alleviate the small-scale problems encountered in standard cold dark matter model. The most stringent constraint comes from the data of galaxy ESO563-G021, which excludes ULDM mass range m = (0.14-3.11) x 10^-22 eV.

ASTROPHYSICAL JOURNAL (2021)

Article Astronomy & Astrophysics

Fuzzy dark matter soliton cores around supermassive black holes

Elliot Y. Davies et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2020)

Article Astronomy & Astrophysics

DYNESTY: a dynamic nested sampling package for estimating Bayesian posteriors and evidences

Joshua S. Speagle

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2020)

Letter Astronomy & Astrophysics

Overconfidence in Bayesian analyses of galaxy rotation curves

Ewan Cameron et al.

NATURE ASTRONOMY (2020)

Review Physics, Nuclear

Small-scale structure of fuzzy and axion-like dark matter

Jens C. Niemeyer

PROGRESS IN PARTICLE AND NUCLEAR PHYSICS (2020)

Article Astronomy & Astrophysics

Dynamical evidence of a dark solitonic core of 109M⊙ in the milky way

Ivan De Martino et al.

PHYSICS OF THE DARK UNIVERSE (2020)

Article Astronomy & Astrophysics

Ultra-light Dark Matter Is Incompatible with the Milky Way's Dwarf Satellites

Mohammadtaher Safarzadeh et al.

ASTROPHYSICAL JOURNAL (2020)

Article Astronomy & Astrophysics

Fuzzy Dark Matter and Dark Matter Halo Cores

A. Burkert

ASTROPHYSICAL JOURNAL (2020)

Article Astronomy & Astrophysics

Simulating mixed fuzzy and cold dark matter

Bodo Schwabe et al.

PHYSICAL REVIEW D (2020)

Article Astronomy & Astrophysics

Subhalo mass function and ultralight bosonic dark matter

Katelin Schutz

PHYSICAL REVIEW D (2020)

Article Astronomy & Astrophysics

Baryon-driven growth of solitonic cores in fuzzy dark matter halos

Jan Veltmaat et al.

PHYSICAL REVIEW D (2020)

Article Astronomy & Astrophysics

Testing the Prediction of Fuzzy Dark Matter Theory in the Milky Way Center

Zhi Li et al.

ASTROPHYSICAL JOURNAL (2020)

Article Astronomy & Astrophysics

A Comprehensive Catalog of Dark Matter Halo Models for SPARC Galaxies

Pengfei Li et al.

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2020)

Article Astronomy & Astrophysics

New mass bound on fermionic dark matter from a combined analysis of classical dSphs

D. Savchenko et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2019)

Article Physics, Multidisciplinary

Strong Constraints on Fuzzy Dark Matter from Ultrafaint Dwarf Galaxy Eridanus II

David J. E. Marsh et al.

PHYSICAL REVIEW LETTERS (2019)

Article Astronomy & Astrophysics

Predictions for the abundance of high-redshift galaxies in a fuzzy dark matter universe

Yueying Ni et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2019)

Article Physics, Multidisciplinary

First Star-Forming Structures in Fuzzy Cosmic Filaments

Philip Moco et al.

PHYSICAL REVIEW LETTERS (2019)

Article Astronomy & Astrophysics

Scalar field dark matter: helping or hurting small-scale problems in cosmology?

Victor H. Robles et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2019)

Article Astronomy & Astrophysics

Lyman α forest and non-linear structure characterization in Fuzzy Dark Matter cosmologies

Matteo Nori et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2019)

Article Computer Science, Theory & Methods

Dynamic nested sampling: an improved algorithm for parameter estimation and evidence calculation

Edward Higson et al.

STATISTICS AND COMPUTING (2019)

Article Astronomy & Astrophysics

Rotation curves of high-resolution LSB and SPARC galaxies with fuzzy and multistate (ultralight boson) scalar field dark matter

T. Bernal et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2018)

Article Astronomy & Astrophysics

Fitting the radial acceleration relation to individual SPARC galaxies

Pengfei Li et al.

ASTRONOMY & ASTROPHYSICS (2018)

Review Physics, Multidisciplinary

Dark matter self-interactions and small scale structure

Sean Tulin et al.

PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS (2018)

Article Astronomy & Astrophysics

Fitting the radial acceleration relation to individual SPARC galaxies

Pengfei Li et al.

ASTRONOMY & ASTROPHYSICS (2018)

Article Astronomy & Astrophysics

Absence of a fundamental acceleration scale in galaxies

Davi C. Rodrigues et al.

NATURE ASTRONOMY (2018)

Letter Astronomy & Astrophysics

Presence of a fundamental acceleration scale in galaxies

Stacy S. McGaugh et al.

NATURE ASTRONOMY (2018)

Article Astronomy & Astrophysics

Can light dark matter solve the core-cusp problem?

Heling Deng et al.

PHYSICAL REVIEW D (2018)

Article Astronomy & Astrophysics

Jeans analysis for dwarf spheroidal galaxies in wave dark matter

Shu-Rong Chen et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2017)

Article Astronomy & Astrophysics

Unbiased constraints on ultralight axion mass from dwarf spheroidal galaxies

Alma X. Gonzalez-Morales et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2017)

Article Astronomy & Astrophysics

Galaxy formation with BECDM - I. Turbulence and relaxation of idealized haloes

Philip Mocz et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2017)

Article Physics, Multidisciplinary

First Constraints on Fuzzy Dark Matter from Lyman-α Forest Data and Hydrodynamical Simulations

Vid Irsic et al.

PHYSICAL REVIEW LETTERS (2017)

Review Astronomy & Astrophysics

Small Scale Problems of the ΛCDM Model: A Short Review

Antonino Del Popolo et al.

GALAXIES (2017)

Article Astronomy & Astrophysics

Ultralight scalars as cosmological dark matter

Lam Hui et al.

PHYSICAL REVIEW D (2017)

Article Astronomy & Astrophysics

Understanding the shape and diversity of dwarf galaxy rotation curves in ΛCDM

J. I. Read et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2016)

Article Astronomy & Astrophysics

Dark matter cores all the way down

J. I. Read et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2016)

Article Astronomy & Astrophysics

CONTRASTING GALAXY FORMATION FROM QUANTUM WAVE DARK MATTER, ψDM, WITH ΛCDM, USING PLANCK AND HUBBLE DATA

Hsi-Yu Schive et al.

ASTROPHYSICAL JOURNAL (2016)

Article Astronomy & Astrophysics

SCALING LAWS FOR DARK MATTER HALOS IN LATE-TYPE AND DWARF SPHEROIDAL GALAXIES

John Kormendy et al.

ASTROPHYSICAL JOURNAL (2016)

Article Astronomy & Astrophysics

Cosmological particle-in-cell simulations with ultralight axion dark matter

Jan Veltmaat et al.

PHYSICAL REVIEW D (2016)

Article Astronomy & Astrophysics

SPARC: MASS MODELS FOR 175 DISK GALAXIES WITH SPITZER PHOTOMETRY AND ACCURATE ROTATION CURVES

Federico Lelli et al.

ASTRONOMICAL JOURNAL (2016)

Article Astronomy & Astrophysics

Galaxy UV-luminosity function and reionization constraints on axion dark matter

Brandon Bozek et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2015)

Article Astronomy & Astrophysics

A search for ultralight axions using precision cosmological data

Renee Hlozek et al.

PHYSICAL REVIEW D (2015)

Article Multidisciplinary Sciences

Cold dark matter: Controversies on small scales

David H. Weinberg et al.

PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA (2015)

Article Physics, Multidisciplinary

Cosmic structure as the quantum interference of a coherent dark wave

Hsi-Yu Schive et al.

NATURE PHYSICS (2014)

Article Physics, Multidisciplinary

Understanding the Core-Halo Relation of Quantum Wave Dark Matter from 3D Simulations

Hsi-Yu Schive et al.

PHYSICAL REVIEW LETTERS (2014)

Article Astronomy & Astrophysics

The inner structure of haloes in cold plus warm dark matter models

Andrea V. Maccio et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2013)

Article Astronomy & Astrophysics

The phase-space density of fermionic dark matter haloes

Shi Shao et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2013)

Article Physics, Multidisciplinary

Bayesian inference in physics

Udo von Toussaint

REVIEWS OF MODERN PHYSICS (2011)

Review Astronomy & Astrophysics

Molecular Clouds in Nearby Galaxies

Yasuo Fukui et al.

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, VOL 48 (2010)

Article Astronomy & Astrophysics

String axiverse

Asimina Arvanitaki et al.

PHYSICAL REVIEW D (2010)

Article Astronomy & Astrophysics

A constant dark matter halo surface density in galaxies

F. Donato et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2009)

Article Physics, Multidisciplinary

Bayes in the sky: Bayesian inference and model selection in cosmology

Roberto Trotta

CONTEMPORARY PHYSICS (2008)

Article Astronomy & Astrophysics

New cosmological model of quintessence and dark matter

V Sahni et al.

PHYSICAL REVIEW D (2000)

Article Physics, Multidisciplinary

Fuzzy cold dark matter: The wave properties of ultralight particles

W Hu et al.

PHYSICAL REVIEW LETTERS (2000)

Article Astronomy & Astrophysics

Dark matter scaling relations

P Salucci et al.

ASTROPHYSICAL JOURNAL (2000)