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

DOI10.1134/S020228932003007XzbMath1454.83097OpenAlexW3089200732MaRDI QIDQ2215226

Aritra Ganguly, Amitava Choudhuri

Publication date: 11 December 2020

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1134/s020228932003007x

zbMATH Keywords

cosmological density perturbationsMONDian 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)

Related Items (2)

The minimally coupled and canonical scalar field inflationary cosmology with negative quadratic and modified Higgs-like potentials: a symmetry based approach ⋮ Cosmological density perturbation of cold dark matter in Newtonian gravity scenario after recombination: a symmetry-based approach

Cites Work

• Cosmological density perturbations in Newtonian- and MONDian gravity scenario: a symmetry-based approach
• Symmetries and differential equations
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