Role of modified scalar variables in the modeling of spherical fluids
DOI10.1142/S0219887818501402zbMath1393.83019OpenAlexW2801664610WikidataQ129934262 ScholiaQ129934262MaRDI QIDQ4566470
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Publication date: 27 June 2018
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1142/s0219887818501402
celestial mechanics\(f(R)\) gravityunified field theoriesrelativistic gravitational theories other than Einstein'sdissipative anisotropic viscous fluid distributionsrelativistic sphere
Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Relativistic dynamics for problems in Hamiltonian and Lagrangian mechanics (70H40) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Celestial mechanics (70F15) Einstein-Maxwell equations (83C22)
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