General relativistic self-similar waves that induce an anomalous acceleration into the standard model of cosmology / [electronic resource] Joel Smoller, Blake Temple.

By: Smoller, JoelContributor(s): Temple, BlakeMaterial type: TextTextSeries: Memoirs of the American Mathematical Society ; v. 1025Publication details: Providence, R.I. : American Mathematical Society, 2012Description: 1 online resource (69 p. : ill.)ISBN: 9780821890127 (online)Subject(s): Einstein field equations | Shock waves -- Mathematical models | Relativistic quantum theory | General relativity (Physics)Additional physical formats: General relativistic self-similar waves that induce an anomalous acceleration into the standard model of cosmology /DDC classification: 531/.1133 LOC classification: QC173.6 | .S66 2012Online resources: Contents | Contents
Contents:
Chapter 1. Introduction Chapter 2. Self-similar coordinates for the $k=0$ FRW spacetime Chapter 3. The expanding wave equations Chapter 4. Canonical co-moving coordinates and comparison with the $k \ne 0$ FRW spacetimes Chapter 5. Leading order corrections to the standard model induced by the expanding waves Chapter 6. A foliation of the expanding wave spacetimes into flat spacelike hypersurfaces with modified scale factor $R(t) = t^a$. Chapter 7. Expanding wave corrections to the standard model in approximate co-moving coordinates Chapter 8. Redshift vs luminosity relations and the anomalous acceleration Chapter 9. Appendix: The mirror problem Chapter 10. Concluding remarks
Item type: E-BOOKS
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Link to resource Available EBK13478

"July 2012, volume 218, number 1025 (third of 5 numbers)."

Includes bibliographical references (p. 69) and index.

Chapter 1. Introduction Chapter 2. Self-similar coordinates for the $k=0$ FRW spacetime Chapter 3. The expanding wave equations Chapter 4. Canonical co-moving coordinates and comparison with the $k \ne 0$ FRW spacetimes Chapter 5. Leading order corrections to the standard model induced by the expanding waves Chapter 6. A foliation of the expanding wave spacetimes into flat spacelike hypersurfaces with modified scale factor $R(t) = t^a$. Chapter 7. Expanding wave corrections to the standard model in approximate co-moving coordinates Chapter 8. Redshift vs luminosity relations and the anomalous acceleration Chapter 9. Appendix: The mirror problem Chapter 10. Concluding remarks

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Electronic reproduction. Providence, Rhode Island : American Mathematical Society. 2012

Mode of access : World Wide Web

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