Solid interiors of neutron stars and gravitational radiation

dc.creatorHaensel, P.
dc.date1996-05-27
dc.date.accessioned2026-07-07T06:32:00Z
dc.date.available2026-07-07T06:32:00Z
dc.descriptionContents: 1.Introduction 2. Formation and composition of the solid crust 3. The bottom layers of the crust: exotic nuclear shapes and topologies 4. Crust contribution to stellar mass and moment of inertia 5. Solid cores 6. Deformation, elastic strain and mountains 7. Shape and energy of rotating, partially solid neutron star 8. Oblateness and precession 9. Gravitational radiation from precessing pulsars 10. Gravitational radiation from precessing pulsars and pulsar timing 11. Detectability
dc.description26 pages, Latex, uses l-school.sty, epsf.tex. Four figures. Lectures delivered at Les Houches Summer School 1995 ``Astrophysical Sources of Gravitational Radiation''. To be published in the Proceedings (eds. J.-A.Marck and J.-P.Lasota)
dc.identifierhttps://arxiv.org/abs/astro-ph/9605164
dc.identifierhttp://arxiv.org/abs/astro-ph/9605164
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/98777
dc.subjectAstrophysics
dc.titleSolid interiors of neutron stars and gravitational radiation
dc.typetext

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