Cosmological density perturbations in Newtonian- and MONDian gravity scenario: a symmetry-based approach

DOI10.1007/s10701-018-00233-zzbMath1411.83144OpenAlexW2909866718MaRDI QIDQ1735917

Aritra Ganguly, Amitava Choudhuri

Publication date: 29 March 2019

Published in: Foundations of Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10701-018-00233-z

zbMATH Keywords

structure formationLie group symmetriescosmological density perturbationNewtonian- and MONDian gravity

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Astrophysical cosmology (85A40)

Related Items (1)

Cosmological density perturbations from matter domination to recombination in Newtonian and MONDian gravity scenarios

Cites Work

• Jeans' Formula for Gravitational Instability
• Scalar–tensor–vector gravity theory
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