Crustal oscillations of slowly rotating relativistic stars
M. VavoulidisDepartment of Physics, Aristotle University of Thessaloniki, 54124 Thessaloniki, GreeceKostas D. KokkotasTheoretical Astrophysics, Eberhard-Karls University of Tbingen, 72076 Tbingen, GermanyA. StavridisDepartment of Physics, Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece
Ochiq kirishBronza
ABI
Annotatsiya
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.
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