Isotropic Coordinates for Generalized Schwarzschild-like Solutions

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Hauptverfasser: Zeng, Zeyu, Kopteva, Elena
Format: Preprint
Veröffentlicht: 2026
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author Zeng, Zeyu
Kopteva, Elena
author_facet Zeng, Zeyu
Kopteva, Elena
contents We consider a broad class of static, spherically symmetric generalized Schwarzschild-like solutions with multiple non-interacting anisotropic fluid sources and derive the coordinate transformation from Schwarzschild-like (curvature) to isotropic coordinates with conformally flat spatial slices. The isotropic form removes spatial-sector coordinate pathologies at the horizon, clarifies geometric quantities (e.g., ADM mass and curvature invariants), and enables the construction of well-posed initial data on t=const hypersurfaces, suitable for the Hamiltonian and conformal formulations of numerical relativity and for perturbation theory. The backgrounds in isotropic coordinates we develop make it straightforward to separate environmental effects from intrinsic strong-gravity signals and meet the growing interest in non-vacuum black hole phenomenology across scattering, lensing, and waveform modeling.
format Preprint
id arxiv_https___arxiv_org_abs_2603_21040
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Isotropic Coordinates for Generalized Schwarzschild-like Solutions
Zeng, Zeyu
Kopteva, Elena
General Relativity and Quantum Cosmology
Mathematical Physics
We consider a broad class of static, spherically symmetric generalized Schwarzschild-like solutions with multiple non-interacting anisotropic fluid sources and derive the coordinate transformation from Schwarzschild-like (curvature) to isotropic coordinates with conformally flat spatial slices. The isotropic form removes spatial-sector coordinate pathologies at the horizon, clarifies geometric quantities (e.g., ADM mass and curvature invariants), and enables the construction of well-posed initial data on t=const hypersurfaces, suitable for the Hamiltonian and conformal formulations of numerical relativity and for perturbation theory. The backgrounds in isotropic coordinates we develop make it straightforward to separate environmental effects from intrinsic strong-gravity signals and meet the growing interest in non-vacuum black hole phenomenology across scattering, lensing, and waveform modeling.
title Isotropic Coordinates for Generalized Schwarzschild-like Solutions
topic General Relativity and Quantum Cosmology
Mathematical Physics
url https://arxiv.org/abs/2603.21040