2016/09/28 by Anne M. Green · 3 citations
Physics and Astronomy · #Astrophysics #Binary black hole #Black Holes and Theoretical Physics #Black hole (networking) #Cosmology and Gravitation Theories #Dark matter #Function (biology) #Galaxy #Gravitational microlensing #Gravitational wave #Particle physics #Physics #Primordial black hole #Pulsars and Gravitational Waves Research #Range (aeronautics) #astro-ph.CO #astro-ph.GA
paper · pdf · doi:10.1103/physrevd.94.063530
published as Phys. Rev. D 94, 063530 (2016) · 6 pages, 4 figures, v2: version published in Phys. Rev. D with additional references
openalex publication_date 2016/09/28 · arxiv created 2016/09/29 · arxiv updated 2016/10/05 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
The recent discovery of gravitational waves from mergers of \ensuremath∼10 M_\ensuremath\bigodot black hole binaries has stimulated interested in primordial black hole (PBH) dark matter in this mass range. Microlensing and dynamical constraints exclude all of the dark matter in compact objects with a delta function mass function in the range 10^\ensuremath-7\ensuremath\lesssimM/M_\ensuremath\bigodot\ensuremath\lesssim105. However it has been argued that all of the dark matter could be composed of compact objects in this range with an extended mass function. We explicitly recalculate the microlensing and dynamical constraints for compact objects with an extended mass function which replicates the PBH mass function produced by inflation models. We find that the microlensing and dynamical constraints place conflicting constraints on the width of the mass function, and do not find a mass function which satisfies both constraints.