An extension of spherically symmetric self-similar inhomogeneous cosmological models

DOI10.1023/A:1018875014930zbMath0900.53043OpenAlexW123248473MaRDI QIDQ1368709

Kenji Tomita

Publication date: 29 September 1997

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1023/a:1018875014930

zbMATH Keywords

inhomogeneous cosmological modelsobservational quantities

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Applications of differential geometry to physics (53Z05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20)

Cites Work

• Partially Self-Similar Solutions in General Relativity
• Reduction of Partially Self-Similar Space-Times to Self-Similar Ones in General Relativity
• Solutions of Einstein’s equations relevant to the description of ‘‘bubbles’’ in the early universe
• Kinematic self-similarity
• Effect of Inhomogeneity on Cosmological Models

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