A different approach to anisotropic spherical collapse with shear and heat radiation

DOI10.1142/S0218271816500498zbMath1341.83007arXiv1512.04072MaRDI QIDQ2809089

B. V. Ivanov

Publication date: 27 May 2016

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

Full work available at URL: https://arxiv.org/abs/1512.04072

zbMATH Keywords

geodesicRiccati equationshearhorizon functionheat radiationstar modelanisotropic collapsejunction equationstellar characteristics

Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Space-time singularities, cosmic censorship, etc. (83C75) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (13)

Lie symmetries, Painlevé analysis, and global dynamics for the temporal equation of radiating stars ⋮ Shearing, dissipative collapse influenced by an equation of state ⋮ Radiating stars with exponential Lie symmetries ⋮ Nonlinear equations in radiating stellar structures ⋮ Complexity of charged anisotropic spherically symmetric fluids in f() gravity ⋮ Analysis of the boundary condition and equation of state in radiating stars ⋮ Measure of complexity for dynamical self-gravitating structures ⋮ Evolution of the charged dynamical radiating spherical structures ⋮ Matching conditions in locally rotationally symmetric spacetimes and radiating stars ⋮ Junction conditions for composite matter in higher dimensions ⋮ A generating function and new exact solutions for geodesic matter ⋮ Embedding condition describing shearing, dissipative collapse ⋮ Riccati equations for bounded radiating systems

Cites Work

• Unnamed Item

This page was built for publication: A different approach to anisotropic spherical collapse with shear and heat radiation