Published July 2018
| Published + Submitted
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A spacetime derivation of the Lorentzian OPE inversion formula
Abstract
Caron-Huot has recently given an interesting formula that determines OPE data in a conformal field theory in terms of a weighted integral of the four-point function over a Lorentzian region of cross-ratio space. We give a new derivation of this formula based on Wick rotation in spacetime rather than cross-ratio space. The derivation is simple in two dimensions but more involved in higher dimensions. We also derive a Lorentzian inversion formula in one dimension that sheds light on previous observations about the chaos regime in the SYK model.
Additional Information
© The Author(s) 2018. This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited. First Online: 12 July 2018. Article funded by SCOAP3. We thank Simon Caron-Huot, Abhijit Gadde, Denis Karateev, Petr Kravchuk, Eric Perlmutter, and Shu-Heng Shao for discussions. DS is supported by Simons Foundation grant 385600. DSD is supported by Simons Foundation grant 488657. EW is supported in part by NSF Grant PHY-1606531.Attached Files
Published - Simmons-Duffin2018_Article_ASpacetimeDerivationOfTheLoren.pdf
Submitted - 1711.03816
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Simmons-Duffin2018_Article_ASpacetimeDerivationOfTheLoren.pdf
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Additional details
- Eprint ID
- 87817
- Resolver ID
- CaltechAUTHORS:20180713-090329998
- Simons Foundation
- 385600
- Simons Foundation
- 488657
- NSF
- PHY-1606531
- SCOAP3
- Created
-
2018-07-13Created from EPrint's datestamp field
- Updated
-
2021-11-15Created from EPrint's last_modified field
- Caltech groups
- Walter Burke Institute for Theoretical Physics