paper

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.

11 pages, no figures, to appear in Class.Quant.Grav

References in corpus (32)

Cited by in corpus (3)