Effects of the Quantum Vacuum at a Cosmic Scale and of Dark Energy

The Einstein equation in a semiclassical approximation is applied to a spherical region of the universe, with the stress-energy tensor consisting of the mass density and pressure of the <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline">...

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Bibliographic Details
Main Author: Emilio Santos
Format: Article
Language:English
Published: MDPI AG 2024-11-01
Series:Entropy
Subjects:
Online Access:https://www.mdpi.com/1099-4300/26/12/1042
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