2026 CMS Winter Meeting

Montreal, Dec 11 - 14, 2026

Abstracts        

Differential Geometry and Mathematical Physics
Org: Eric Bahuaud (Seattle University) and Frédéric Rochon (UQÀM)

ARAM ALYOUSEF, University of Alberta

ABDOU OUSSAMA BENABIDA, UBC

FACUNDO CAMANO, Waterloo

BENJAMIN FRIEDMAN, UQÀM

CHRISTINE GUENTHER, Pacific University

ROBERT HARRIS, UQÀM

CHRIS KOTTKE, Reed College

HARI KUNDURI, McMaster University

KUAN-HUI LEE, McGill

MAXENCE MAYRAND, University of Sherbrooke

RUXANDRA MORARU, University of Waterloo

TRISTAN OZUCH, MIT

ERIC WOOLGAR, University of Alberta
Spacetime conformal boundary causal rigidity  [PDF]

A well-known boundary rigidity problem for Riemannian geometry asks whether a manifold-with-boundary, such that all geodesic chords have the same length, is necessarily a round hemisphere. It is, and therefore any chord leaving a given boundary point passes through that point's antipode. For Lorentzian geometry, we pose the following conformal boundary rigidity problem. If all light rays leaving a point p in the distant past (Penrose's conformal infinity) refocus at the same point q in the distant future, and if the same is true for all such p, is the spacetime conformal to a maximally symmetric spacetime? For example, if the spacetime is also asymptotically anti-de Sitter, is it actually anti-de Sitter (up to conformal transformations that preserve the asymptotics)? I will answer this question, assuming that the spacetime is also stationary, based on joint work with Gabriel Paternain. Time permitting, I will discuss joint work with Alex Sandhu and Giulio Sanzeni on the positive cosmological constant version of this problem.

XUWEN ZHU, Northeastern University


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