Turnaround radius in scalar-tensor gravity with quasilocal mass
arXiv:2003.13935 · doi:10.1103/PhysRevD.102.044002
Abstract
Following an existing procedure in general relativity, the turnaround radius of a spherical structure is studied in scalar-tensor gravity using a new prescription for the analog of the Hawking-Hayward quasilocal mass in this class of theories.
arXiv comment10 pages, no figures, to appear in Phys.Rev.D
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