Solutions of Einstein’s equations relevant to the description of ‘‘bubbles’’ in the early universe

DOI10.1063/1.528086zbMath0659.53052OpenAlexW2106193783MaRDI QIDQ3808833

J. Ponce de Leon

Publication date: 1988

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1063/1.528086

zbMATH Keywords

Einstein field equationsspherically symmetric solutionsinflationary universe models

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Applications of local differential geometry to the sciences (53B50)

Related Items (4)

An extension of spherically symmetric self-similar inhomogeneous cosmological models ⋮ Inflation in a spatially closed anisotropic universe ⋮ The similarity hypothesis in general relativity ⋮ Self-similar symmetry in general relativity

Cites Work

• Plane symmetric self-gravitating fluids with pressure equal to energy density
• Partially Self-Similar Solutions in General Relativity
• Reduction of Partially Self-Similar Space-Times to Self-Similar Ones in General Relativity
• Inflationary universe: A possible solution to the horizon and flatness problems

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