Gravitational waves from dynamical shape transition of protoneutron stars

DOI10.1142/S0218271821501042zbMath1490.83024OpenAlexW3197226105WikidataQ114820610 ScholiaQ114820610MaRDI QIDQ5068348

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Publication date: 6 April 2022

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0218271821501042

zbMATH Keywords

gravitational wavesrotating neutron starscompressible ellipsoids

Mathematics Subject Classification ID

Nuclear physics (81V35) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Weak interaction in quantum theory (81V15) Galactic and stellar structure (85A15) Celestial mechanics (70F15) Variants of convex sets (star-shaped, ((m, n))-convex, etc.) (52A30) Gravitational waves (83C35) Compressibility effects in hydrodynamic stability (76E19) Particle decays (81U90)

Cites Work

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