Equality of ADM mass and generalized Komar energy in asymptotically-flat dynamical spacetimes

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Auteurs principaux: Wang, Zhi-Wei, Braunstein, Samuel L.
Format: Preprint
Publié: 2025
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author Wang, Zhi-Wei
Braunstein, Samuel L.
author_facet Wang, Zhi-Wei
Braunstein, Samuel L.
contents We find a relation between the ADM mass and a generalized Komar energy in asymptotically-flat spacetime. We do not need to assume the existence of either a Killing or even asymptotically-Killing vector field. Instead, our generalized Komar energy is constructed from the normal evolution vector (the lapse function times the future-directed unit normal to the spacelike hypersurfaces on which the ADM mass is measured). We find equality between the ADM mass and this generalized Komar energy even for dynamical asymptotically-flat spacetimes provided the 3-dimensional Einstein tensor drops off quickly enough at spatial infinity, in particular, whenever ${}^{(3)}G_{ij}=o(r^{-3})$. No additional assumptions are required for equality. As this generalized energy is fully covariant, it may provide a powerful tool for analyzing energy content in dynamical spacetimes containing compact objects.
format Preprint
id arxiv_https___arxiv_org_abs_2509_05928
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Equality of ADM mass and generalized Komar energy in asymptotically-flat dynamical spacetimes
Wang, Zhi-Wei
Braunstein, Samuel L.
General Relativity and Quantum Cosmology
Instrumentation and Methods for Astrophysics
High Energy Physics - Theory
Mathematical Physics
Differential Geometry
We find a relation between the ADM mass and a generalized Komar energy in asymptotically-flat spacetime. We do not need to assume the existence of either a Killing or even asymptotically-Killing vector field. Instead, our generalized Komar energy is constructed from the normal evolution vector (the lapse function times the future-directed unit normal to the spacelike hypersurfaces on which the ADM mass is measured). We find equality between the ADM mass and this generalized Komar energy even for dynamical asymptotically-flat spacetimes provided the 3-dimensional Einstein tensor drops off quickly enough at spatial infinity, in particular, whenever ${}^{(3)}G_{ij}=o(r^{-3})$. No additional assumptions are required for equality. As this generalized energy is fully covariant, it may provide a powerful tool for analyzing energy content in dynamical spacetimes containing compact objects.
title Equality of ADM mass and generalized Komar energy in asymptotically-flat dynamical spacetimes
topic General Relativity and Quantum Cosmology
Instrumentation and Methods for Astrophysics
High Energy Physics - Theory
Mathematical Physics
Differential Geometry
url https://arxiv.org/abs/2509.05928