Chandrasekhar, Subrahmanyan ; Ferrari, Valeria (1995) On the non-radial oscillations of a star. V. A fully relativistic treatment of a Newtonian star Proceedings of the Royal Society A: Mathematical, Physical & Engineering Sciences, 450 (1939). pp. 463-475. ISSN 1364-5021
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Official URL: http://rspa.royalsocietypublishing.org/content/450...
Related URL: http://dx.doi.org/10.1098/rspa.1995.0094
Abstract
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.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to The Royal Society. |
| ID Code: | 70303 |
| Deposited On: | 16 Nov 2011 04:21 |
| Last Modified: | 16 Nov 2011 04:21 |
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