Weak-field limits of Schwarzschild, Kerr, RN, and KN black hole metrics are reproduced from three-point amplitudes with exponential spin structure via the KMOC formula by extracting momentum impulses and matching to geodesics.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
citation-role summary
background 1
citation-polarity summary
fields
hep-th 1years
2026 1verdicts
CONDITIONAL 1roles
background 1polarities
background 1representative citing papers
citing papers explorer
-
Weak-Field Limits of Black Hole Metrics from the KMOC formalism: Schwarzschild, Kerr, Reissner-Nordstr\"om, and Kerr-Newman
Weak-field limits of Schwarzschild, Kerr, RN, and KN black hole metrics are reproduced from three-point amplitudes with exponential spin structure via the KMOC formula by extracting momentum impulses and matching to geodesics.