The Clustering Dynamics of Primordial Black Boles in <em>N</em>-Body Simulations
We explore the possibility that Dark Matter (DM) may be explained by a nonuniform background of approximately stellar mass clusters of Primordial Black Holes (PBHs) by simulating the evolution from recombination to the present with over 5000 realisations using a Newtonian \({ N }\)-body code. We com...
Main Authors: | Manuel Trashorras, Juan García-Bellido, Savvas Nesseris |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2021-01-01
|
Series: | Universe |
Subjects: | |
Online Access: | https://www.mdpi.com/2218-1997/7/1/18 |
Similar Items
-
The Merger Rate of Black Holes in a Primordial Black Hole Cluster
by: Viktor D. Stasenko, et al.
Published: (2021-05-01) -
Origin and growth of primordial black holes
by: Krzysztof A. Meissner, et al.
Published: (2021-08-01) -
Multi-Field versus Single-Field in the Supergravity Models of Inflation and Primordial Black Holes
by: Sergei V. Ketov
Published: (2021-04-01) -
Primordial Regular Black Holes: Thermodynamics and Dark Matter
by: José Antonio de Freitas Pacheco
Published: (2018-05-01) -
PRIMORDIAL BLACK HOLES, DIFFUSE GAMMA RADIATION OF THE UNIVERSE AND POSSIBLE NATURE OF DARK MATTER
by: Чаругин Виктор Максимович
Published: (2020-02-01)