Quasi-local mass at the null infinity of the Vaidya spacetime
Differential Geometry
2016-08-23 v1 General Relativity and Quantum Cosmology
Abstract
There are two important statements regarding the Trautman-Bondi mass [1,8,5] at null infinity: one is the positivity [7,6], and the other is the Bondi mass loss formula [1], which are both global in nature. The positivity of the quasi-local mass can potentially lead to a local description at null infinity. This is confirmed for the Vaidya spacetime in this note. We study the Wang-Yau quasi-local mass on surfaces of fixed size at the null infinity of the Vaidya spacetime. The optimal embedding equation is solved explicitly and the quasi-local mass is evaluated in terms of the mass aspect function of the Vaidya spacetime.
Keywords
Cite
@article{arxiv.1608.06165,
title = {Quasi-local mass at the null infinity of the Vaidya spacetime},
author = {Po-Ning Chen and Mu-Tao Wang and Shing-Tung Yau},
journal= {arXiv preprint arXiv:1608.06165},
year = {2016}
}
Comments
15 pages