Growth rate of spherical voids with non-comoving dark matter and baryons
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Publication:6183709
DOI10.1088/1361-6382/AD0F4EarXiv2306.02668MaRDI QIDQ6183709
Ismael Delgado Gaspar, Juan Carlos Hidalgo, Fernando A. Pizaña, Roberto A. Sussman
Publication date: 4 January 2024
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2306.02668
Cites Work
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- On average properties of inhomogeneous fluids in general relativity: Dust cosmologies
- On average properties of inhomogeneous fluids in general relativity. III: General fluid cosmologies
- How well is our Universe described by an FLRW model?
- The covariant approach to LRS perfect fluid spacetime geometries
- Pancakes as opposed to Swiss cheese
- Relativistic Cosmology
- On average properties of inhomogeneous fluids in general relativity: Perfect fluid cosmologies
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