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.
Homothetic Killing horizons in generic Vaidya spacetimes
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abstract
We study the conformal Killing equation for generic Vaidya-like spacetimes, including those with rotation. We show that these spacetimes admit a unique class of conformal Killing vectors that are homothetic for mass, charge, or rotation parameters being linear functions of the advanced null-time. For the Kerr-Vaidya metric, the solution to the conformal Killing equation exists iff both mass and rotation parameters become dynamic. The presence of a homothetic Killing vector (HKV) for such a spacetime enables one to conformally map the original dynamical spacetime to a stationary spacetime, enabling access to the standard methods pertaining to a Killing horizon. The surface where an HKV becomes null is termed the homothetic Killing horizon. We discuss the thermodynamic properties of such homothetic Killing horizons and formulate a version of the first law (or flux balance law) for spherically symmetric Vaidya spacetimes. We further study the maximal analytic extension of a charged Vaidya metric and indicate its implications for studying particle creation in such backgrounds.
fields
gr-qc 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
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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.