The propagation delay in the timing of a pulsar orbiting a supermassive black hole
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Publication:1730007
DOI10.1007/S10714-019-2517-2zbMath1414.83032arXiv1806.02547OpenAlexW3104403082MaRDI QIDQ1730007
Publication date: 7 March 2019
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1806.02547
Black holes (83C57) Equations of motion in general relativity and gravitational theory (83C10) Radiative transfer in astronomy and astrophysics (85A25)
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Cites Work
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- The post-Newtonian approximation for relativistic compact binaries
- Comparing timelike geodesics around a Kerr black hole and a boson star
- The second post-Newtonian motion of compact binary-star systems with spin
- Complete conservative dynamics for inspiralling compact binaries with spins at the fourth post-Newtonian order
- Next‐to‐next‐to‐leading order post‐Newtonian linear‐in‐spin binary Hamiltonians
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