Toward a realistic description of dark matter overdensities around black holes
- 28 August 2025
- journal article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 112 (4)
Abstract
No abstract availableAll Related Versions
Funding Information
- Instituto Nazionale di Fisica Nucleare
- Ministerio de Ciencia e Innovación (CNS2023-144071)
- Agencia Estatal de Investigación
- European Commission
- NextGenerationEU
- PRTR
This publication has 53 references indexed in Scilit:
- Distinguishing environmental effects on binary black hole gravitational waveformsNature Astronomy, 2023
- The origins of massive black holesNature Reviews Physics, 2021
- Planck 2018 resultsAstronomy & Astrophysics, 2021
- Constraints on the astrophysical environment of binaries with gravitational-wave observationsAstronomy & Astrophysics, 2020
- Planck2018 resultsAstronomy & Astrophysics, 2020
- Particle dark matter: evidence, candidates and constraintsPhysics Reports, 2005
- Formation of massive black holes through runaway collisions in dense young star clustersNature, 2004
- Massive Black Holes as Population III RemnantsThe Astrophysical Journal, 2001
- The Structure of Cold Dark Matter HalosThe Astrophysical Journal, 1996
- Models of Galaxies with Central Black Holes: Adiabatic Growth in Spherical GalaxiesThe Astrophysical Journal, 1995