Primordial black holes in linear and non-linear regimes
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Publication:5024213
DOI10.1088/1475-7516/2017/06/041OpenAlexW3105727440MaRDI QIDQ5024213
No author found.
Publication date: 28 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1608.00591
Cites Work
- Asymptotically FRW black holes
- Cosmic matter flux may turn Hawking radiation off
- Isolated and dynamical horizons and their applications
- Cosmological and black hole apparent horizons
- Do we know the mass of a black hole? Mass of some cosmological black hole models
- Primordial black hole formation in the early universe: critical behaviour and self-similarity
- Hamilton–Jacobi tunneling method for dynamical horizons in different coordinate gauges
- Curvature profiles as initial conditions for primordial black hole formation
- Cosmological black holes: the spherical perfect fluid collapse with pressure in a FRW background
- Computations of primordial black-hole formation
- THE SPHERICAL SYMMETRY BLACK HOLE COLLAPSE IN EXPANDING UNIVERSE
- A general proof of the conservation of the curvature perturbation
- A Relativist's Toolkit
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