MG15 - Talk detail |
Participant |
Hackmann, Eva | |||||||
Institution |
ZARM, University of Bremen - Am Fallturm - Bremen - Bremen - Germany | |||||||
Session |
BH2 |
Accepted |
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Order |
Time |
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Talk |
Oral abstract |
Title |
The propagation delay for pulsars orbiting supermassive black holes | |||||
Coauthors | ||||||||
Abstract |
Pulsar timing offers the possibility to test the theory of gravity in the strong field regime. Particularly promising laboratories for such tests are pulsar--black hole binaries. In such a system it is therefore of paramount importance to accurately model the effects of General Relativity. We present an exact analytical calculation for the relativistic propagation delay of the signal of a pulsar orbiting a supermassive black hole. We use this result to test the accuracy of the usually employed post--Newtonian approximation methods. |
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Pdf file |
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