On the Non-Radial Oscillations of a Star: V. A Fully Relativistic Treatment of a Newtonian Star

Details On the Non-Radial Oscillations of a Star: V. A Fully Relativistic Treatment of a Newtonian Star On the Non-Radial Oscillations of a Star: V. A Fully Relativistic Treatment of a Newtonian Star

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995rspsa.450..463c&link_type=abstract

Proceedings: Mathematical and Physical Sciences, Volume 450, Issue 1939, pp. 463-475

Physics

5

Scientific paper

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.

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