Bekenstein-Hawking temperature is completely determined from the projective structure on the Killing horizon because the Schwarzian of the affine parameter equals minus half the square of surface gravity.
Circular Orbits in Stationary Axisymmetric Spacetimes
2 Pith papers cite this work, alongside 16 external citations. Polarity classification is still indexing.
2
Pith papers citing it
16
external citations · OpenAlex
fields
gr-qc 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
External quadrupolar distortion imprints on orbital dynamics and accretion structure in thin disks around deformed compact objects, with the radiating region's outer edge tied to the radiation-to-gas pressure transition.
citing papers explorer
-
Bekenstein-Hawking temperature from the Schwarzian
Bekenstein-Hawking temperature is completely determined from the projective structure on the Killing horizon because the Schwarzian of the affine parameter equals minus half the square of surface gravity.
-
Analytic thin disks and rings in a class of nonasymptotically flat static spacetimes
External quadrupolar distortion imprints on orbital dynamics and accretion structure in thin disks around deformed compact objects, with the radiating region's outer edge tied to the radiation-to-gas pressure transition.