An analytical solution of stationary hydrodynamic equations of a main-sequence star

DOI10.1142/S0219887819501202zbMath1420.35420OpenAlexW2947488924MaRDI QIDQ5233064

Antonio Romano, Addolorata Marasco

Publication date: 13 September 2019

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/s0219887819501202

zbMATH Keywords

spherical symmetryhydrodynamic equationsperfect gasstationary conditionsmain-sequence starSchwarzschild's inequality and equation

Mathematics Subject Classification ID

PDEs in connection with fluid mechanics (35Q35) Galactic and stellar structure (85A15) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Exact solutions to problems in general relativity and gravitational theory (83C15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) PDEs in connection with astronomy and astrophysics (35Q85)

Cites Work

• Unnamed Item
• Continuum mechanics using Mathematica. Fundamentals, methods, and applications
• Hydrodynamics and Thermodynamics of Newtonian Stars
• On static stars in Newtonian gravity and Lane-Emden type equations

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