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Crustal oscillations of slowly rotating relativistic stars

M. VavoulidisDepartment of Physics, Aristotle University of Thessaloniki, 54124 Thessaloniki, GreeceKostas D. KokkotasDepartment of Physics, Aristotle University of Thessaloniki, 54124 Thessaloniki, GreeceA. StavridisDepartment of Physics, Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece
Monthly Notices of the Royal Astronomical Societyjournal2008en
ABI

Abstract

We study low-amplitude crustal oscillations of slowly rotating relativistic stars consisting of a central fluid core and an outer thin solid crust. We estimate the effect of rotation on the torsional toroidal modes and on the interfacial and shear spheroidal modes. The results compared against the Newtonian ones for wide range of neutron star models and equations of state.

Topics

Pulsars and Gravitational Waves ResearchAstrophysical Phenomena and ObservationsGamma-ray bursts and supernovae

Identifiers

DOI
10.1111/j.1365-2966.2007.12835.x

Citations and references

Cited by 246 references
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