STABLE INFLATIONARY DISSIPATIVE COSMOLOGIES
Copyright policy )STABLE INFLATIONARY DISSIPATIVE COSMOLOGIES
The stability of the de Sitter era of cosmic expansion in spatially curved homogeneous isotropic universes is studied. The source of the gravitational field is an imperfect fluid such that the parameters that characterize it may change with time. In this way we extend our previous analysis for spatially-flat spaces as well as the work of Barrow.
- University of Buenos Aires Argentina
- National Scientific and Technical Research Council Argentina
- Autonomous University of Barcelona Spain
https://purl.org/becyt/ford/1.3, FOS: Physical sciences, De Sitter Era, General Relativity and Quantum Cosmology (gr-qc), https://purl.org/becyt/ford/1, Stability, General Relativity and Quantum Cosmology, Imperfect Uid
https://purl.org/becyt/ford/1.3, FOS: Physical sciences, De Sitter Era, General Relativity and Quantum Cosmology (gr-qc), https://purl.org/becyt/ford/1, Stability, General Relativity and Quantum Cosmology, Imperfect Uid
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