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