Star Clusters, Self-Interacting Dark Matter Halos, and Black Hole Cusps: The Fluid Conduction Model and Its Extension to General Relativity

Physical Review D - United States
doi 10.1103/physrevd.98.023021
Full Text
Abstract

Available in full text

Date
Authors
Publisher

American Physical Society (APS)

Related search

Black Hole Clusters: The Dark Matter

Journal of High Energy Physics, Gravitation and Cosmology
2019English

Testing General Relativity With Black Hole-Pulsar Binaries

Physical Review D
AstronomyPhysics
2018English

Testing General Relativity Using Golden Black-Hole Binaries

Physical Review D
AstronomyPhysics
2016English

Entropy and Gravitation—From Black Hole Computers to Dark Energy and Dark Matter

Entropy
Electronic EngineeringInformation SystemsMathematical PhysicsElectricalAstronomyPhysics
2019English

Vector Self-Interacting Dark Matter

Physical Review D
AstronomyPhysics
2020English

Self-Interacting Dark Matter and Monochromatic Lines

2016English

Decaying Dark Matter in Halos of Primordial Black Holes

European Physical Journal C
EngineeringAstronomyPhysics
2019English

Constraining the Star Formation Histories in Dark Matter Halos. I. Central Galaxies

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2013English

Self‐Consistent Massive Disks in Triaxial Dark Matter Halos

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2007English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy