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arXiv · 1511.01948

Self-Trapping of Diskoseismic Corrugation Modes in Neutron Star Spacetimes

David Tsang·George Pappas
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Abstract

We examine the effects of higher-order multipole contributions of rotating neutron star (NS) spacetimes on the propagation of corrugation (c-)modes within a thin accretion disk. We find that the Lense-Thirring precession frequency, which determines the propagation region of the low-frequency fundamental corrugation modes, can experience a turnover allowing for c-modes to become self-trapped for sufficiently high dimensionless spin $j$ and quadrupole rotational deformability $α$. If such self-trapping c-modes can be detected, e.g. through phase-resolved spectroscopy of the iron line for a high-spin low-mass accreting neutron star, this could potentially constrain the spin-induced NS quadrupole and the NS equation of state.

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David Tsang, George Pappas. 2015-11-05. Self-Trapping of Diskoseismic Corrugation Modes in Neutron Star Spacetimes. https://doi.org/10.3847/2041-8205%2F818%2F1%2Fl11

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