Spin-2 Green's Functions on Kerr in Radiation Gauge

Fuente: arXiv
Guardado en:
Detalles Bibliográficos
Autores principales: Casals, Marc, Hollands, Stefan, Pound, Adam, Toomani, Vahid
Formato: Preprint
Publicado: 2024
Materias:
Acceso en línea:
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
_version_ 1866915350279356416
author Casals, Marc
Hollands, Stefan
Pound, Adam
Toomani, Vahid
author_facet Casals, Marc
Hollands, Stefan
Pound, Adam
Toomani, Vahid
contents We construct retarded and advanced Green's functions for gravitational perturbations in Kerr in an ingoing radiation gauge. Our Green's functions have a frequency domain piece that has previously been obtained by Ori [Phys. Rev. D 67 (2003)] based on the Chrzanowski-Cohen-Kegeles metric reconstruction method. As is well known, this piece by itself is not sufficient to obtain an actual Green's function. We show how to complete it with a piece based on a method by Green et al. [Class. Quant. Grav. 37 (2020)]. The completion piece has a completely explicit form in the time-domain and is supported on pairs of points on the same outgoing principal null geodesic which are in the appropriate causal order. We expect our Green's functions to be useful for gravitational self-force calculations and other perturbation problems on Kerr spacetime.
format Preprint
id arxiv_https___arxiv_org_abs_2402_15468
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Spin-2 Green's Functions on Kerr in Radiation Gauge
Casals, Marc
Hollands, Stefan
Pound, Adam
Toomani, Vahid
General Relativity and Quantum Cosmology
High Energy Physics - Theory
We construct retarded and advanced Green's functions for gravitational perturbations in Kerr in an ingoing radiation gauge. Our Green's functions have a frequency domain piece that has previously been obtained by Ori [Phys. Rev. D 67 (2003)] based on the Chrzanowski-Cohen-Kegeles metric reconstruction method. As is well known, this piece by itself is not sufficient to obtain an actual Green's function. We show how to complete it with a piece based on a method by Green et al. [Class. Quant. Grav. 37 (2020)]. The completion piece has a completely explicit form in the time-domain and is supported on pairs of points on the same outgoing principal null geodesic which are in the appropriate causal order. We expect our Green's functions to be useful for gravitational self-force calculations and other perturbation problems on Kerr spacetime.
title Spin-2 Green's Functions on Kerr in Radiation Gauge
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2402.15468