Gravitational Waves from Wobbling Pulsars

Details Gravitational Waves from Wobbling Pulsars Gravitational Waves from Wobbling Pulsars

1994-10-14

arxiv.org/abs/astro-ph/9410047v1

Astronomy and Astrophysics

Astrophysics

PlainTex, 7 pp. , no figures, IAG/USP Rep. 67

Scientific paper

The prospects for detection of gravitational waves from precessing pulsars have been considered by constructing fully relativistic rotating neutron star models and evaluating the expected wave amplitude $h$ from a galactic source. For a "typical" neutron matter equation of state and observed rotation rates, it is shown that moderate wobble angles may render an observable signal from a nearby source once the present generation of interferometric antennas becomes operative.

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