Speaker
Mr
Bevan Tucker
(University of the Witwatersrand)
Description
The advent of the MeerKAT and SKA radio telescope projects will allow for vastly improved precision in the measurement of pulsar radio frequency emissions. Thus, the propagation of a pulsar’s conical radio beam through the strong gravitational field region in the vicinity of a compact object, i.e. black-hole or another neutron star, will probe the metric of spacetime in the high-field regime. This talk outlines the theoretical and associated numerical predictions of General Relativistic effects, such as the Lense-Thirring effect, on such a pulsar signal.
| Would you like to <br> submit a short paper <br> for the Conference <br> Proceedings (Yes / No)? | Yes |
|---|---|
| Level (Hons, MSc, <br> PhD, other)? | MSc |
| Consider for a student <br> award (Yes / No)? | Yes |
Primary author
Mr
Bevan Tucker
(University of the Witwatersrand)
