Limits on the Energetics and other Astrophysics parameters of Pulsars from Gravitational Waves Limits from Advanced Interferometric Detectors

Details Limits on the Energetics and other Astrophysics parameters of Pulsars from Gravitational Waves Limits from Advanced Interferometric Detectors Limits on the Energetics and other Astrophysics parameters of Pulsars from Gravitational Waves Limits from Advanced Interferometric Detectors

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...21112001g&link_type=abstract

American Astronomical Society, AAS Meeting #211, #120.01; Bulletin of the American Astronomical Society, Vol. 39, p.949

Astronomy and Astrophysics

Astronomy

Scientific paper

We analyze different pulsar models with different braking mechanisms that include gravitational radiation braking. We show how possible null (or positive) detection of gravitational waves from known pulsars by proposed advanced detectors of gravitational waves (as advanced LIGO and VIRGO) can help us to understand better the braking mechanism and the energetics involved in the spin-down of the pulsars.

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