A preferred mass range for primordial black hole formation and black holes as dark matter revisited

DOI10.1007/JHEP09(2017)138zbMath1382.83133arXiv1703.04825OpenAlexW3102471445MaRDI QIDQ1706012

Julian Georg, Scott Watson

Publication date: 19 March 2018

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1703.04825

zbMATH Keywords

cosmology of theories beyond the SMstring theory and cosmic strings

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Black holes (83C57) String and superstring theories in gravitational theory (83E30) Supersymmetric field theories in quantum mechanics (81T60) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Astrophysical cosmology (85A40)

Related Items (5)

Analytic description of primordial black hole formation from scalar field fragmentation ⋮ Simulation of primordial black holes with large negative non-Gaussianity ⋮ Black hole thermodynamics with dynamical lambda ⋮ Curved spacetime effective field theory (cEFT) -- construction with the heat kernel method ⋮ Effects of the shape of curvature peaks on the size of primordial black holes

Cites Work

• Aspects of split supersymmetry
• Inhomogeneous baryogenesis, cosmic antimatter, and dark matter
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