Self-consistent solutions of the semi-classical back-reaction equations with cosmological constant spatial curvature and perfect fluid

DOI10.1007/BF00660080zbMath0811.76097OpenAlexW2039920648MaRDI QIDQ1338284

Norberto A. Zuccalá, Luis P. Chimento

Publication date: 29 November 1994

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00660080

zbMATH Keywords

Robertson-Walker metricconformally invariant free quantum fieldsEinstein universede Sitter solutionsemi-classical Einstein equations

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Cites Work

• Self-consistent solutions of the semi-classical Einstein equations with cosmological constant and perfect fluid
• Energy-momentum tensor of a massless scalar quantum field in a Robertson-Walker universe

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