Timing & geodetic precession in the double pulsar and two relativistic binaries

Details Timing & geodetic precession in the double pulsar and two relativistic binaries Timing & geodetic precession in the double pulsar and two relativistic binaries

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atnf.prop.1319b&link_type=abstract

ATNF proposal P455, Semester: April, 2008

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Stellar, Galactic, Parkes

Scientific paper

This project is to continue timing and profile monitoring of the first double-pulsar system and two other relativistic binaries discovered in our surveys. These systems provide unique laboratories for gravitational physics. In addition to the double pulsar we want to continue our studies of the double neutron star PSR J1756-2251, and the relativistic binary J1141-6545. We aim to provide the strongest tests to date for general relativity and to measure for the first time the moment-of-inertia of a neutron star. Additionally, we will determine the system geometries and map the pulsar beams via geodetic precession.

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