Shock-wave cosmology inside a black hole

DOI10.1073/pnas.1833875100zbMath1064.83041arXivastro-ph/0210105OpenAlexW2146679943WikidataQ36160530 ScholiaQ36160530MaRDI QIDQ5460807

J. A. Smoller, J. Blake Temple

Publication date: 19 July 2005

Published in: Proceedings of the National Academy of Sciences (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0210105

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Black holes (83C57)

Related Items (11)

Noncommutative momentum and torsional regularization ⋮ Big bounce from spin and torsion ⋮ A valid finite bounded expanding Carmelian universe without dark matter ⋮ Absolute objects and counterexamples: Jones-geroch dust, torretti constant curvature, tetrad-spinor, and scalar density ⋮ General relativistic self-similar waves that induce an anomalous acceleration into the standard model of cosmology ⋮ An instability of the standard model of cosmology creates the anomalous acceleration without dark energy ⋮ Analysis of big bounce in Einstein–Cartan cosmology ⋮ SHOCK WAVE COSMOLOGY INSIDE A BLACK HOLE: THE CASE OF NON-CRITICAL EXPANSION ⋮ Expanding wave solutions of the Einstein equations that induce an anomalous acceleration into the Standard Model of Cosmology ⋮ A nonsingular, anisotropic universe in a black hole with torsion and particle production ⋮ HOW INFLATION IS USED TO RESOLVE THE FLATNESS PROBLEM

Cites Work

• General relativistic shock waves that extend the Oppenheimer-Snyder model
• Hyperbolic systems of conservation laws II
• Solutions in the large for nonlinear hyperbolic systems of equations
• Cosmology with a shock-wave

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