Radiating spherical collapse with shear and heat flow

DOI10.1007/BF00613196zbMath0766.76100OpenAlexW1966272935MaRDI QIDQ1209093

Nazira A. Tomimura, F. C. P. Nunes

Publication date: 16 May 1993

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00613196

zbMATH Keywords

geodesic motionspherical bodyVaidya's metric

Mathematics Subject Classification ID

Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (7)

Shear-free axial model in massive Brans-Dicke gravity ⋮ EXACT NONSPHERICAL RADIATING COLLAPSE ⋮ Geodesic models generated by Lie symmetries ⋮ Effects of some physical factors on the stability of collapsing stars ⋮ Gravitational collapse without a remnant ⋮ Radiating relativistic matter in geodesic motion ⋮ Mixed potentials in radiative stellar collapse

Cites Work

• Spherical gravitational collapse with energy transport by radiative diffusion
• On Continued Gravitational Contraction
• ‘Newtonian’ Time in General Relativity

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