Gravitational Burst Radiation

This code calculates the waveforms and SNRs of gravitational burst radiation from a pulsar orbiting a massive BH. We use a numerical kludge method where the relativistic spin-orbital dynamics are specified by the Mathsisson Papetrou Dixon formulation. See also Gravitational burst radiation from pulsars in the Galactic centre and stellar clusters

Tom Kimpson
Tom Kimpson
Ph.D. Candidate, Theoretical Astrophysics

My research interests include high energy astrophysics and gravitational wave astronomy.

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