Stability analysis of stellar radiating filaments

DOI10.1088/1361-6382/AA73B9zbMath1373.83091arXiv1709.04365OpenAlexW3098482582MaRDI QIDQ4592640

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Publication date: 7 November 2017

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1709.04365

zbMATH Keywords

stabilitygravitationrelativistic systemsdynamical instabilityhydrodynamical equationcylindrical systemsparticular cosmological modelstellar radiating filaments

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (23)

Influence of f(G) gravity on the complexity of relativistic self-gravitating fluids ⋮ Role of modified scalar variables in the modeling of spherical fluids ⋮ Quasi static evolution of compact objects in modified gravity ⋮ Models of collapsing and expanding cylindrical source in \(f(R, T)\) theory ⋮ Energy conditions in higher derivative f(R,□R,T) gravity ⋮ Some anisotropic planar stellar models ⋮ Role of Strong Matter‐Field Coupling on Axial Complex Systems ⋮ Influence of modification of gravity on spherical wormhole models ⋮ Dynamical analysis for cylindrical geometry in non-minimally coupled f(R,T) gravity ⋮ Electromagnetic effects on cylindrical gravastar-like strings in f(R, T, R_σηT^ση) gravity ⋮ Measure of complexity for dynamical self-gravitating structures ⋮ Evolution of the charged dynamical radiating spherical structures ⋮ A view of compact configurations from the R + γe ^χT scenario ⋮ Axially and reflection symmetric systems and structure scalars in \(f(R,T)\) gravity ⋮ Compact stars ⋮ Propagation of polar gravitational waves in \(f(R, T)\) scenario ⋮ Dynamical instability of charged self-gravitating stars in modified gravity ⋮ Structure scalars with charged dissipative systems in \(f(G, T)\) gravity ⋮ Effects of non-minimally coupled \(f(R, T)\) gravity on the stability of a self-gravitating spherically symmetric fluid ⋮ Role of f(G,T) gravity on the evolution of relativistic stars ⋮ Hydrodynamic properties of dissipative fluids associated with tilted observers ⋮ Quasi-homologous evolution of relativistic stars ⋮ Dissipative self-gravitating systems in modified gravity

Cites Work

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