Mathematical Properties of Cosmological Models with Accelerated Expansion

@inproceedings{International2004MathematicalPO,
  title={Mathematical Properties of Cosmological Models with Accelerated Expansion},
  author={Erwin Schr{\"o}dinger International and Alan D. Rendall},
  year={2004}
}
An introduction to solutions of the Einstein equations defining cosmological models with accelerated expansion is given. Connections between mathematical and physical issues are explored. Theorems which have been proved for solutions with positive cosmological constant or nonlinear scalar fields are reviewed. Some remarks are made on more exotic models such as the Chaplygin gas, tachyons and k- 

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References

Publications referenced by this paper.
Showing 1-10 of 26 references

Asymptotic behaviour of homogeneous cosmological models with cosmological constant

R. M. Wald
Phys. Rev. D28, • 1983
View 4 Excerpts
Highly Influenced

Isotropization of arbitrary cosmological expansion given an effective cosmological constant

A. A. Starobinsky
JETP Lett. 37, • 1983
View 3 Excerpts
Highly Influenced

Brane-World Gravity

Living reviews in relativity • 2004

Brane-world gravity. Living Reviews in Relativity, 2004-7

R. Maartens
2004
View 1 Excerpt

The EinsteinVlasov system with a scalar field

H. Lee
2004

Asymptotic behaviour of the Einstein-Vlasov system with a positive cosmological constant. Preprint gr-qc/0308035

H. Lee
2003
View 2 Excerpts

Asymptotic behaviour of the EinsteinVlasov system with a positive cosmological constant

H. Lee
2003

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