Tolman mass of spherical fluids with electromagnetic field
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Publication:4615541
DOI10.1142/S0217732319500123zbMath1405.83046WikidataQ128634563 ScholiaQ128634563MaRDI QIDQ4615541
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Publication date: 29 January 2019
Published in: Modern Physics Letters A (Search for Journal in Brave)
Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15) Equations of motion in general relativity and gravitational theory (83C10)
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Cites Work
- Dynamical instability and the expansion-free condition
- Dynamics and stability of charged spherical star with tilted and non-tilted congruences
- Dynamical variables and evolution of the universe
- Collapse of a radiating star
- Some anisotropic planar stellar models
- On the active gravitational mass of a non-spherical source leaving hydrostatic equilibrium
- PHYSICAL CAUSES OF ENERGY DENSITY INHOMOGENIZATION AND STABILITY OF ENERGY DENSITY HOMOGENEITY IN RELATIVISTIC SELF-GRAVITATING FLUIDS
- The contraction of gravitating spheres
- On Continued Gravitational Contraction
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