Ten new exact vacuum solutions, including black holes with zero entropy, arise in extended bumblebee gravity because varying the action and imposing the vector VEV constraint do not commute.
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An analytic semiclassical model produces closed-form first-order corrections to the Hawking temperature and horizon position for a Schwarzschild black hole in a finite cavity.
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New Exact Vacuum Solutions in Extended Bumblebee Gravity
Ten new exact vacuum solutions, including black holes with zero entropy, arise in extended bumblebee gravity because varying the action and imposing the vector VEV constraint do not commute.
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Analytic semiclassical backreaction of a Schwarzschild black hole in a finite cavity: horizon shift, temperature renormalization, and canonical stability in the Hartle-Hawking State
An analytic semiclassical model produces closed-form first-order corrections to the Hawking temperature and horizon position for a Schwarzschild black hole in a finite cavity.