Characteristic initial value problems for the Einstein-Maxwell-scalar field equations in spherical symmetry

Fuente: arXiv
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Main Authors: Mädler, Thomas, Gannouji, Radouane, Gallo, Emanuel
Format: Preprint
Published: 2025
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author Mädler, Thomas
Gannouji, Radouane
Gallo, Emanuel
author_facet Mädler, Thomas
Gannouji, Radouane
Gallo, Emanuel
contents The characteristic initial boundary problem is discussed in spherical symmetry for the Einstein-Maxwell-scalar field equations. It is formulated for an affine-null metric and the resulting field equations are cast into a hierarchical system of partial differential equations. The initial boundary value problem for a family of null hypersurfaces is specified for a timelike-null foliation at the central geodesic of spherical symmetry as well as for a double-null foliation where the corresponding boundary is a null hypersurface. For the latter, two distinct boundary value formulations arise -- one where the null boundary has zero Misner-Sharp mass and another one where the corresponding Misner-Sharp mass is nonzero. As an application, the nonextremal and the extremal Reissner-Nordström solution in null coordinates for a charged black hole and the Fisher-Janis-Newman-Winicour solution are derived.
format Preprint
id arxiv_https___arxiv_org_abs_2503_24162
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Characteristic initial value problems for the Einstein-Maxwell-scalar field equations in spherical symmetry
Mädler, Thomas
Gannouji, Radouane
Gallo, Emanuel
General Relativity and Quantum Cosmology
High Energy Physics - Theory
The characteristic initial boundary problem is discussed in spherical symmetry for the Einstein-Maxwell-scalar field equations. It is formulated for an affine-null metric and the resulting field equations are cast into a hierarchical system of partial differential equations. The initial boundary value problem for a family of null hypersurfaces is specified for a timelike-null foliation at the central geodesic of spherical symmetry as well as for a double-null foliation where the corresponding boundary is a null hypersurface. For the latter, two distinct boundary value formulations arise -- one where the null boundary has zero Misner-Sharp mass and another one where the corresponding Misner-Sharp mass is nonzero. As an application, the nonextremal and the extremal Reissner-Nordström solution in null coordinates for a charged black hole and the Fisher-Janis-Newman-Winicour solution are derived.
title Characteristic initial value problems for the Einstein-Maxwell-scalar field equations in spherical symmetry
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2503.24162