Abstract
We present a new geometric approach to the study of static isolated general relativistic systems for which we suggest the name geometrostatics. After describing the setup, we introduce localized formulas for the ADM-mass and ADM/CMC-center of mass of geometrostatic systems. We then explain the pseudo-Newtonian character of these formulas and show that they converge to Newtonian mass and center of mass in the Newtonian limit, respectively, using Ehlers’ frame theory. Moreover, we present a novel physical interpretation of the level sets of the canonical lapse function and apply it to prove uniqueness results. Finally, we suggest a notion of force on test particles in geometrostatic space-times.
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Notes
- 1.
Here, time-like curves and the time functional are taken with respect to the static space-time metric \(ds^2=-N^2c^2dt^2+g\) induced by \((M^3,g,N)\).
- 2.
This assumes that the lapse function exists in the first place.
- 3.
Albeit without explicit reference to the speed of light.
- 4.
We note that our discussion of center of mass only applies to systems with non-vanishing mass.
- 5.
Under precise fall-off conditions at spacelike infinity that are satisfied here.
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Cederbaum, C. (2014). Geometrostatics: The Geometry of Static Space-Times. In: Bičák, J., Ledvinka, T. (eds) Relativity and Gravitation. Springer Proceedings in Physics, vol 157. Springer, Cham. https://doi.org/10.1007/978-3-319-06761-2_5
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