Magnetic effects on the viscous boundary layer damping of ther-modes in neutron stars
نویسندگان
چکیده
منابع مشابه
Viscous Boundary-Layer Damping of r-Modes in Neutron Stars.
Recent work has raised the exciting possibility that r-modes (Rossby waves) in rotating neutron star cores might be strong gravitational-wave sources. We estimate the effect of a solid crust on their viscous damping rate and show that the dissipation rate in the viscous boundary layer between the oscillating fluid and the nearly static crust is more than 105 times higher than that from the shea...
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ژورنال
عنوان ژورنال: Physical Review D
سال: 2001
ISSN: 0556-2821,1089-4918
DOI: 10.1103/physrevd.64.044009