r-modes in the Tolman VII solution
classification
🌀 gr-qc
astro-ph
keywords
r-modesolutiontolmanapproximationcalculationscompactcorrectionestimated
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The r-mode frequencies of the Tolman VII solution for the slowly rotating non-barotropic approximation within the low frequency regime are estimated. The relativistic correction to Newtonian r-mode calculations is shown as function of the tenuity $\frac{R}{M}$ and is shown to be significant only for very compact neutron stars.
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