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Celestial two-point functions and rectified dictionary

  • Hideo Furugori,
  • Naoki Ogawa,
  • Sotaro Sugishita,
  • Takahiro Waki

摘要

A naive celestial dictionary causes massless two-point functions to take the delta-function forms in the celestial conformal field theory (CCFT). We rectify the dictionary, involving the shadow transformation so that the two-point functions follow the standard power-law. In this new definition, we can smoothly take the massless limit of the massive dictionary. We also compute a three-point function using the new dictionary and discuss the OPE in CCFT.