A family of black-bounce spacetimes with new mass functions is shown to be regular, to have positive quasi-local mass, and to generally, though not monotonically, suppress Hawking temperature as the bounce and deformation parameters grow.
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Thermal Behavior of Generalized Black-Bounce Black Hole Model
A family of black-bounce spacetimes with new mass functions is shown to be regular, to have positive quasi-local mass, and to generally, though not monotonically, suppress Hawking temperature as the bounce and deformation parameters grow.