# On the non-radial oscillations of a star. V. A fully relativistic treatment of a Newtonian star

@article{Chandrasekhar1995OnTN, title={On the non-radial oscillations of a star. V. A fully relativistic treatment of a Newtonian star}, author={Subrahmanyan Chandrasekhar and Valeria Ferrari}, journal={Proceedings of the Royal Society of London. Series A: Mathematical and Physical Sciences}, year={1995}, volume={450}, pages={463 - 475} }

It is shown how the non-radial oscillations of a Newtonian star (i. e. a star built in the Newtonian framework) can be treated fully relativistically as the result of the scattering of gravitational radiation by its own, shallow, curved spacetime. It has the distinguishing characteristic that no gravitational radiation emerges.

## 3 Citations

### Quasinormal modes: the characteristic `sound' of black holes and neutron stars

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- 1999

Gravitational waves emitted by perturbed black holes or relativistic stars are dominated by `quasinormal ringing', damped oscillations at single frequencies which are characteristic of the underlying…

### High-frequency behavior of w-mode pulsations of compact stars

- Physics
- 2011

We study the asymptotic behavior of the quasinormal modes (QNMs) of $w$-mode pulsations of compact stars in the high-frequency regime. We observe that both the axial and polar $w$-mode QNMs attain…

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