Turbulent perfect fluid analogy for an inflationary nonsingular vacuum bubble and the strong energy condition within a string derived cosmology

DOI10.1023/A:1001938319441zbMath0977.83127OpenAlexW1568773613MaRDI QIDQ5931069

Steven David Miller

Publication date: 2 May 2001

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1023/a:1001938319441

zbMATH Keywords

cosmologycosmological constantdilation-Einstein field equationsRobertson-Walker universe

Mathematics Subject Classification ID

Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30) Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory (83-02)

Cites Work

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• STRING DILATON FLUID COSMOLOGY
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• Primary state diffusion
• Quantum Mechanics, Stochasticity and Space-Time
• The coherence of primordial fluctuations produced during inflation
• Semiclassicality and decoherence of cosmological perturbations
• Inflationary universe: A possible solution to the horizon and flatness problems
• The cosmological constant problem
• The Large Scale Structure of Space-Time
• General Relativity
• Thermodynamics and cosmology
• Effective field theory from quantized strings

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