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r-modes in the Tolman VII solution

Nicholas Neary·Kayll Lake
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Abstract

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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Nicholas Neary, Kayll Lake. 2001-08-31. r-modes in the Tolman VII solution. https://arxiv.org/abs/gr-qc/0106056

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