Quasi-Einstein equations and a Myers-Perry rigidity problem
APA
Woolgar, E. (2025). Quasi-Einstein equations and a Myers-Perry rigidity problem. Perimeter Institute. https://pirsa.org/25020038
MLA
Woolgar, Eric. Quasi-Einstein equations and a Myers-Perry rigidity problem. Perimeter Institute, Feb. 18, 2025, https://pirsa.org/25020038
BibTex
@misc{ pirsa_PIRSA:25020038, doi = {10.48660/25020038}, url = {https://pirsa.org/25020038}, author = {Woolgar, Eric}, keywords = {Cosmology}, language = {en}, title = {Quasi-Einstein equations and a Myers-Perry rigidity problem}, publisher = {Perimeter Institute}, year = {2025}, month = {feb}, note = {PIRSA:25020038 see, \url{https://pirsa.org}} }
Quasi-Einstein equations are generalizations of the Einstein equation. They arise from warped product Einstein metrics (Kaluza-Klein reductions), Ricci solitons, cosmology, near-horizon geometries, and smooth measured Lorentzian length spaces. Despite their apparent generality, they often have a surprising rigidity. I will review some recent developments in the area, focusing on near-horizon geometries, including Dunajski and Lucietti's near-horizon version of the Hawking rigidity theorem. I will discuss an application to 5-dimensional extreme (Myers-Perry type) black holes whose horizons admit the structure of the group SU(2).