Thermodynamics and phase transitions of galactic clustering in higher-order modified gravity

DOI10.1142/S0218271819500275zbMath1431.83152arXiv1809.03579MaRDI QIDQ5217811

Behnam Pourhassan, Sudhaker Upadhyay, Salvatore Capozziello

Publication date: 26 February 2020

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1809.03579

zbMATH Keywords

thermodynamicsdistribution functionlarge scale structuremodified gravity

Mathematics Subject Classification ID

Classical and relativistic thermodynamics (80A10) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar dynamics (85A05)

Related Items (6)

Large scale structure formation for conformal theory of gravity ⋮ Study of the large scale structure through modified gravity theory using statistical mechanics ⋮ \(f(R)\) gravity effects on charged accelerating AdS black holes using holographic tools ⋮ Galactic clustering under power-law modified Newtonian potential ⋮ Effect of thermal fluctuation on the thermodynamics of GMGHS black hole ⋮ Finite Tsallis gravitational partition function for a system of galaxies

Cites Work

• Clustering of galaxies in brane world models
• Reparametrization of the relativistic infinitely extended charged particle action
• The dark matter problem from f(R) gravity viewpoint
• A Relativistic Field Theory of an Extended Particle, I
• Low scale unification, Newton's law and extra dimensions

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