Primordial black hole formation with full numerical relativity

DOI10.1088/1475-7516/2022/03/029zbMath1504.83019arXiv2109.04896OpenAlexW3200218131MaRDI QIDQ5099198

Eugene A. Lim, Eloy de Jong, Josu C. Aurrekoetxea

Publication date: 31 August 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2109.04896

zbMATH Keywords

gravityprimordial black holesphysics of the early universe

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Black holes (83C57) Geometrodynamics and the holographic principle (83E05) Perturbations in context of PDEs (35B20) Numerical radial basis function approximation (65D12) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)

Related Items (4)

CTTK: a new method to solve the initial data constraints in numerical relativity ⋮ Primordial black holes from strong first-order phase transitions ⋮ Primordial stochastic gravitational wave backgrounds from a sharp feature in three-field inflation. Part I. The radiation era ⋮ Lessons for adaptive mesh refinement in numerical relativity

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