Gravitational waves from neutron stars

dc.creatorBonazzola, S.
dc.creatorGourgoulhon, E.
dc.date1996-05-30
dc.date.accessioned2026-07-07T06:32:44Z
dc.date.available2026-07-07T06:32:44Z
dc.descriptionContents: 1. Introduction 2. Spontaneous symmetry breaking 2.1 Review of classical results about Maclaurin/Jacobi ellipsoids 2.2 Spontaneous breaking of symmetry: a general phenomenom 2.3 Previous results for compressible Newtonian stars 2.4 Generation of gravitational waves 2.5 Finding the equilibrium configurations of a rotating star in the Newtonian regime 2.6 Extension to general relativity 2.7 First integral of fluid motion in general relativity 2.8 Gravitational field equations 2.9 Numerical results 3. CW emission from pulsars 4. Discussion and conclusion Appendix: Relativistic hydrodynamics in an accelerated frame
dc.description33 pages, LaTeX, 6 PostScript figures. Lecture delivered at Les Houches School ``Astrophysical Sources of Gravitational Radiation'' (Les Houches, France, Sept. 26 - Oct. 6, 1995). To be published in the Proceedings (eds. J.-A. Marck and J.-P. Lasota)
dc.identifierhttps://arxiv.org/abs/astro-ph/9605187
dc.identifierhttp://arxiv.org/abs/astro-ph/9605187
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/98960
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational waves from neutron stars
dc.typetext

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