Book contents
- Frontmatter
- Contents
- List of illustrations
- Preface
- Acknowledgements
- 1 Preliminaries
- 2 The Szekeres–Szafron family of solutions
- 3 Physics and cosmology in an inhomogeneous Universe
- 4 The Stephani–Barnes family of solutions
- 5 Solutions with null radiation
- 6 Solutions with a “stiff fluid”/scalar field source
- 7 Other solutions
- 8 Averaging out inhomogeneities of geometry and matter in cosmological models
- 9 Comments
- Appendix A Dictionary of abbreviations used in the text and in the diagrams
- Appendix B Why should one consider inhomogeneous models of the Universe?
- Appendix C Memorable statements about the cosmological principle
- Appendix D How was this review compiled?
- Appendix E Historical milestones
- Notes added in proof
- Bibliography
- Index
4 - The Stephani–Barnes family of solutions
Published online by Cambridge University Press: 03 May 2010
- Frontmatter
- Contents
- List of illustrations
- Preface
- Acknowledgements
- 1 Preliminaries
- 2 The Szekeres–Szafron family of solutions
- 3 Physics and cosmology in an inhomogeneous Universe
- 4 The Stephani–Barnes family of solutions
- 5 Solutions with null radiation
- 6 Solutions with a “stiff fluid”/scalar field source
- 7 Other solutions
- 8 Averaging out inhomogeneities of geometry and matter in cosmological models
- 9 Comments
- Appendix A Dictionary of abbreviations used in the text and in the diagrams
- Appendix B Why should one consider inhomogeneous models of the Universe?
- Appendix C Memorable statements about the cosmological principle
- Appendix D How was this review compiled?
- Appendix E Historical milestones
- Notes added in proof
- Bibliography
- Index
- Type
- Chapter
- Information
- Inhomogeneous Cosmological Models , pp. 142 - 194Publisher: Cambridge University PressPrint publication year: 1997