NASA NTRS · 19850042347
Gravitational radiation from a solid crust neutron star
Abstract
A rapidly rotating neutron star with a solid crust will have a rotationally induced oblateness that is constrained by the rigidity of the solid. It is shown that the effective triaxiality and the gravitational radiation output are small, in agreement with the very small change in period of PSR 1937 + 21.
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Ali Alpar, M., Pines, D.. 1984-06-01. Gravitational radiation from a solid crust neutron star. https://ntrs.nasa.gov/citations/19850042347
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