g-modes of non-radially pulsating relativistic stars: the slow-motion formalism

DOI10.1093/mnras/222.3.393zbMath0633.76138OpenAlexW2037934374MaRDI QIDQ3771931

Lee Samuel Finn

Publication date: 1986

Published in: Monthly Notices of the Royal Astronomical Society (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1093/mnras/222.3.393

zbMATH Keywords

boundary conditionpolytropic equation of stategravitational radiationenergy principleperturbation variablesg-modesinstantaneous-gravity approximationlow-frequency g-mode pulsationsNewtonian- like boundary conditionnon-rotating, perfect-fluid, relativistic stars

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

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