{ "id": "1403.2697", "version": "v2", "published": "2014-03-11T19:14:00.000Z", "updated": "2014-05-24T09:58:49.000Z", "title": "Gravitational-wave flux for a particle orbiting a Kerr black hole to 20th post-Newtonian order: a numerical approach", "authors": [ "Abhay G Shah" ], "categories": [ "gr-qc" ], "abstract": "In this article we present the post-Newtonian (pN) coefficients of the energy flux (and angular momentum flux) at infinity and event horizon for a particle in circular, equatorial orbits about a Kerr black hole (of mass $M$ and spin-parameter $a$) up to 20-pN order. When a pN term is not a polynomial in $a/M$ and includes irrational functions (like polygamma functions), it is written as a power series of $a/M$. This is achieved by calculating the fluxes numerically with an accuracy greater than 1 part in $10^{600}$. Such high accuracy allows us to extract analytical values of pN coefficients that are linear combinations of transcendentals like the Euler constant, logarithms of prime numbers and powers of $\\pi$. We also present the 22-pN expansion (spin-independent pN expansion) of the ingoing energy flux at the event horizon for a particle in circular orbit about a Schwarzschild black hole.", "revisions": [ { "version": "v2", "updated": "2014-05-24T09:58:49.000Z" } ], "analyses": { "subjects": [ "04.25.Nx", "04.30.Db", "04.70.Bw" ], "keywords": [ "kerr black hole", "20th post-newtonian order", "gravitational-wave flux", "numerical approach", "particle orbiting" ], "tags": [ "journal article" ], "publication": { "doi": "10.1103/PhysRevD.90.044025", "journal": "Physical Review D", "year": 2014, "month": "Aug", "volume": 90, "number": 4, "pages": "044025" }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1285355, "adsabs": "2014PhRvD..90d4025S" } } }