ON THE QUASI-ISOTROPIC INFLATIONARY SOLUTION

DOI10.1142/S0218271803003712zbMath1079.83564arXivgr-qc/0307048WikidataQ125292971 ScholiaQ125292971MaRDI QIDQ5699966

Giovanni Montani, Giovanni Imponente

Publication date: 27 October 2005

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0307048

zbMATH Keywords

inflationInhomogeneous cosmology

Mathematics Subject Classification ID

Relativistic cosmology (83F05)

Related Items (3)

CLASSICAL AND QUANTUM FEATURES OF THE MIXMASTER SINGULARITY ⋮ STUDY OF THE QUASI-ISOTROPIC SOLUTION NEAR THE COSMOLOGICAL SINGULARITY IN THE PRESENCE OF BULK VISCOSITY ⋮ INHOMOGENEOUS de SITTER SOLUTION WITH SCALAR FIELD AND PERTURBATIONS SPECTRUM

Cites Work

• A new type of isotropic cosmological models without singularity
• Comment about quasi-isotropic solution of Einstein equations near the cosmological singularity
• On the generic cosmological solution in the presence of ultrarelativistic matter and a scalar field
• On the quasi-isotropic solution in the presence of ultrarelativistic matter and a scalar field
• Semiclassicality and decoherence of cosmological perturbations
• Mixmaster Universe

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