# Generating Kerr Amplitudes from Higher-Spin Theory

- Institution: CERN
- Department: Conferences, Workshops & Schools
- Speaker: Lucile Cangemi
- Year: 2023
- Language: English
- Source: [CERN](https://videos.cern.ch/record/2302754)
- Licence: [CERN](http://copyright.web.cern.ch)
- Who can watch: Teens profiles and older (sources give no ratings; placed by Invisible Network from the source's own words)

Higher-spin theory and massive gauge invariance can be used as input for constraining root-Kerr and Kerr amplitudes, relevant for calculating gravitational observables with spin. Elegant three-point spin-s amplitudes exist for Kerr black holes, however constructing the corresponding four-point Compton amplitudes is an open problem. In this talk, I will discuss the origin of the Kerr three-point amplitudes from a higher-spin theory perspective. Guided by higher-spin constraints and classical-limit analysis, I will propose quantum and classical tree-level Compton amplitudes relevant for root-Kerr and Kerr to all orders in spin..

0:00:00 Slide 1

0:01:39 Slide 2

0:04:09 Slide 3

0:05:27 Slide 4

0:07:25 Slide 5

0:09:10 Slide 6

0:10:30 Slide 7

0:12:18 Slide 8

0:13:22 Slide 9

0:14:59 Slide 10

0:16:49 Slide 11

0:18:23 Slide 12

0:19:51 Slide 13

0:23:54 Slide 14

0:25:20 Slide 15

0:26:33 Slide 16

0:28:29 Slide 17

0:30:51 Slide 18

0:33:42 Slide 19

0:35:10 Slide 20

## Lectures

1. [Generating Kerr Amplitudes from Higher-Spin Theory](https://invisiblenetwork.ai/learn/cern/2302754/516e7a20225e), 39 min (CERN's player)
