Consistent cosmological structure formation on all scales in relativistic extensions of MOND
DOI10.1088/1475-7516/2023/06/006zbMath1528.83166arXiv2303.00038OpenAlexW4379534044MaRDI QIDQ6173856
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Publication date: 13 July 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2303.00038
Relativistic cosmology (83F05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar dynamics (85A05) (n)-body problems (70F10) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)
Cites Work
- The Acceleration Scale, Modified Newtonian Dynamics and Sterile Neutrinos
- A general theory of linear cosmological perturbations: stability conditions, the quasistatic limit and dynamics
- Parameterized post-Newtonian cosmology
- Scale invariance at low accelerations (aka MOND) and the dynamical anomalies in the Universe
- Unnamed Item
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