
ProblemTesting whether real black holes deviate from Kerr requires modeling their photon rings pixel by pixel.
ApproachSelected for the BHEX (5 interns) and AstroAI (6 interns) cohorts. Implemented the beyond-Kerr KRZ spacetime metric in a JAX-based relativistic ray tracer and built a configurable pipeline generating photon-ring image libraries across ~10 spacetime and accretion parameters.
ResultTrained a CNN-based simulation-based inference pipeline that recovers black-hole spin and inclination with sub-percent error (R² = 0.999); ongoing normalizing-flow work quantifies the precision BHEX needs to detect deviations from General Relativity around Sgr A*.
R² = 0.999spin & inclination recovery




