Quasilocal mass in scalar-tensor gravity: spherical symmetry
arXiv:2005.04770 · doi:10.1088/1361-6382/aba845
Abstract
A recent generalization of the Hawking-Hayward quasilocal energy to scalar-tensor gravity is adapted to general spherically symmetric geometries. It is then applied to several black hole and other spherical solutions of scalar-tensor and gravity. The relations of this quasilocal energy with the Abreu-Nielsen-Visser gauge and the Kodama vector are discussed.
arXiv comment11 pages, no figures, to appear in Class.Quant.Grav
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