Spins of primordial black holes formed with a soft equation of state
DOI10.1088/1475-7516/2023/07/030zbMath1528.83084arXiv2305.13830MaRDI QIDQ6116516
Chul-Moon Yoo, Unnamed Author, Tomohiro Harada, Unnamed Author
Publication date: 18 July 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2305.13830
Black holes (83C57) Gravitational energy and conservation laws; groups of motions (83C40) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Spinor and twistor methods in general relativity and gravitational theory; Newman-Penrose formalism (83C60) Methods of global Riemannian geometry, including PDE methods; curvature restrictions (53C21) Motion of the gyroscope (70E05)
Cites Work
- Computations of primordial black-hole formation
- Analytical thresholds for black hole formation in general cosmological backgrounds
- Gravitational waves induced from primordial black hole fluctuations: the effect of an extended mass function
- Spin of primordial black holes
- Primordial black hole abundance from random Gaussian curvature perturbations and a local density threshold
- The initial spin probability distribution of primordial black holes
This page was built for publication: Spins of primordial black holes formed with a soft equation of state