Quasi-local energy in presence of gravitational radiation
arXiv:1603.08860 · doi:10.1142/S0218271816450012
Abstract
We discuss our recent work [4] in which gravitational radiation was studied by evaluating the Wang-Yau quasi-local mass of surfaces of fixed size at the infinity of both axial and polar perturbations of the Schwarzschild spacetime, à la Chandrasekhar [1].
5 pages and 2 figures