Book contents
- Frontmatter
- Contents
- The scope of this text
- Preface to the second edition
- Acknowledgments
- 1 How the theory of relativity came into being (a brief historical sketch)
- Part I Elements of differential geometry
- Part II The theory of gravitation
- 12 The Einstein equations and the sources of a gravitational field
- 13 The Maxwell and Einstein–Maxwell equations and the Kaluza–Klein theory
- 14 Spherically symmetric gravitational fields of isolated objects
- 15 Relativistic hydrodynamics and thermodynamics
- 16 Relativistic cosmology I: general geometry
- 17 Relativistic cosmology II: the Robertson–Walker geometry
- 18 Relativistic cosmology III: the LemaÎtre–Tolman geometry
- 19 Relativistic cosmology IV: simple generalisations of L–T and related geometries
- 20 Relativistic cosmology V: the Szekeres geometries
- 21 The Kerr metric
- 22 Relativity enters technology: the Global Positioning System
- 23 Subjects omitted from this book
- 24 Comments to selected exercises and calculations
- References
- Index
18 - Relativistic cosmology III: the LemaÎtre–Tolman geometry
from Part II - The theory of gravitation
Published online by Cambridge University Press: 30 May 2024
- Frontmatter
- Contents
- The scope of this text
- Preface to the second edition
- Acknowledgments
- 1 How the theory of relativity came into being (a brief historical sketch)
- Part I Elements of differential geometry
- Part II The theory of gravitation
- 12 The Einstein equations and the sources of a gravitational field
- 13 The Maxwell and Einstein–Maxwell equations and the Kaluza–Klein theory
- 14 Spherically symmetric gravitational fields of isolated objects
- 15 Relativistic hydrodynamics and thermodynamics
- 16 Relativistic cosmology I: general geometry
- 17 Relativistic cosmology II: the Robertson–Walker geometry
- 18 Relativistic cosmology III: the LemaÎtre–Tolman geometry
- 19 Relativistic cosmology IV: simple generalisations of L–T and related geometries
- 20 Relativistic cosmology V: the Szekeres geometries
- 21 The Kerr metric
- 22 Relativity enters technology: the Global Positioning System
- 23 Subjects omitted from this book
- 24 Comments to selected exercises and calculations
- References
- Index
Summary
The Lemaitre–Tolman class of cosmological models (spherically symmetric inhomogeneous metrics obeying the Einstein equations with a dust source) is derived and discussed in much detail, from the point of view of its geometry and its applications to cosmology. It is shown that these metrics can be used to describe the formation of cosmic voids and of galaxy clusters out of small perturbations of homogeneity at the time of emission of the cosmic microwave background radiation. Apparent horizons for central and noncentral observers, the formation of black holes, the existence and avoidance of shell crossings, the equations of redshift and the generation and meaning of blueshift are discussed. A simple example of a shell focussing singularity is derived. Among the cosmological applications are: solving the horizon problem without inflation, mimicking the accelerating expansion of the Universe by mass-density inhomogeneities in a decelerating model, drift of light rays, lagging cores of Big Bang, misleading conclusions drawn from observed mass distribution in redshift space.
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- An Introduction to General Relativity and Cosmology , pp. 289 - 365Publisher: Cambridge University PressPrint publication year: 2024