Propagation time delay and frame dragging effects of lightlike geodesics in the timing of a pulsar orbiting SgrA∗

authored by: Bilel Ben-Salem, Eva Hackmann
Abstract: Timing a pulsar in a close orbit around the supermassive black hole SgrA∗ at the centre of the Milky Way would open the window for an accurate determination of the black hole parameters and for new tests of general relativity and alternative modified gravity theories. An important relativistic effect which has to be taken into account in the timing model is the propagation delay of the pulses in the gravitational field of the black hole. Due to the extreme mass ratio of the pulsar and the supermassive back hole we use the test particle limit to derive an exact analytical formula for the propagation delay of lightlike geodesics in a Kerr space-Time, and deduce a relativistic formula for the corresponding frame dragging effect on the arrival time. As an illustration, we treat an edge-on orbit in which the frame dragging effect on the emitted lightlike geodesics is expected to be maximal. We compare our formula for the propagation time delay with Post-Newtonian approaches, and in particular with the frame dragging terms derived in previous works by Wex & Kopeikin and Rafikov & Lai. Our approach correctly identifies the asymmetry of the frame dragging delay with respect to superior conjunction, avoids singularities in the time delay, and indicates that in the Post-Newtonian approach frame dragging effects on the lightlike pulses are generally slightly overestimated.
Organisation(s): QuantumFrontiers
External Organisation(s): Bielefeld University
Center of Applied Space Technology and Microgravity (ZARM)
University of Bremen
Type: Article
Journal: Monthly Notices of the Royal Astronomical Society
Volume: 516
Pages: 1768-1780
No. of pages: 13
ISSN: 0035-8711
Publication date: 01.10.2022
Publication status: Published
Peer reviewed: Yes
ASJC Scopus subject areas: Astronomy and Astrophysics, Space and Planetary Science
Electronic version(s): https://doi.org/10.1093/mnras/stac2337 (Access: Open)

BibTeX

@article{1229770e5fbf418ab3ea1d8fb39c3272,
title = "Propagation time delay and frame dragging effects of lightlike geodesics in the timing of a pulsar orbiting SgrA∗",
abstract = "Timing a pulsar in a close orbit around the supermassive black hole SgrA∗ at the centre of the Milky Way would open the window for an accurate determination of the black hole parameters and for new tests of general relativity and alternative modified gravity theories. An important relativistic effect which has to be taken into account in the timing model is the propagation delay of the pulses in the gravitational field of the black hole. Due to the extreme mass ratio of the pulsar and the supermassive back hole we use the test particle limit to derive an exact analytical formula for the propagation delay of lightlike geodesics in a Kerr space-Time, and deduce a relativistic formula for the corresponding frame dragging effect on the arrival time. As an illustration, we treat an edge-on orbit in which the frame dragging effect on the emitted lightlike geodesics is expected to be maximal. We compare our formula for the propagation time delay with Post-Newtonian approaches, and in particular with the frame dragging terms derived in previous works by Wex & Kopeikin and Rafikov & Lai. Our approach correctly identifies the asymmetry of the frame dragging delay with respect to superior conjunction, avoids singularities in the time delay, and indicates that in the Post-Newtonian approach frame dragging effects on the lightlike pulses are generally slightly overestimated.",
keywords = "black hole physics, gravitation, pulsars: general, relativistic processes",
author = "Bilel Ben-Salem and Eva Hackmann",
note = "Publisher Copyright: {\textcopyright} 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.",
year = "2022",
month = oct,
day = "1",
doi = "10.1093/mnras/stac2337",
language = "English",
volume = "516",
pages = "1768--1780",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "2",
}