Tue, 03 Mar 2026
13:00
L2

Beyond Wigner - How Non-Invertible Symmetries Preserve Probabilities

Thomas Bartsch
(Oxford )
Abstract

Recent years have seen the expansion of the traditional notion of symmetry in quantum theory to so-called generalised or categorical symmetries, which may in particular be non-invertible. This seems to be at odds with Wigner's theorem, which asserts that quantum symmetries ought to be implemented by (anti)unitary -- and hence invertible -- operators on the Hilbert space. In this talk, we will try to resolve this puzzle for generalised symmetries that are described by (higher) fusion categories. After giving a gentle introduction to the latter, we will discuss how one can associate an inner-product-preserving operator to (possibly non-invertible) symmetry defects and illustrate our construction through concrete examples. Based on the recent work 2602.07110 with Gai and Schäfer-Nameki.

Tue, 24 Feb 2026
13:00
L2

The Geometry of Gravitational Radiation

Jelle Hartong
(Edinburgh)
Abstract
Future null infinity of an asymptotically flat spacetime is a conformal Carroll manifold. I will not assume any familiarity with Carroll geometry and explain the relevant geometrical notions as we go along. We will consider asymptotic solutions to the 4D vacuum Einstein equations where future null infinity is endowed with the most general Carroll metric data that is allowed by the Einstein equations. This can be used to define an energy-momentum tensor (EMT) at future null infinity by varying a suitably renormalised action with respect to the boundary Carroll metric data. It is shown that the Ward identities obeyed by this boundary EMT agree with the Bondi loss equations that describe the loss of energy and momentum due to the emission of gravitational waves. The metric near future null infinity can be formulated in terms of a Cartan geometry based on the conformal Carroll algebra. The non-vanishing curvatures of said algebra dictate how radiative the spacetime is. For example, the vacuum degeneracy is described by a flat conformal Carroll connection. We will see that the Bondi loss equations can be rewritten as flux-balance laws where the fluxes are determined by the Cartan geometry for the conformal Carroll algebra.


 

Tue, 10 Feb 2026
13:00
L2

Dynamics of the Fermion-Rotor System

Vazha Loladze
(Oxford )
Abstract

In this talk, I will examine the dynamics of the fermion–rotor system, originally introduced by Polchinski as a toy model for monopole–fermion scattering. Despite its simplicity, the system is surprisingly subtle, with ingoing and outgoing fermion fields carrying different quantum numbers. I will show that the rotor acts as a twist operator in the low-energy theory, changing the quantum numbers of excitations that have previously passed through the origin to ensure scattering consistent with all symmetries, thereby resolving the long-standing Unitarity puzzle. I will then discuss generalizations of this setup with multiple rotors and unequal charges, and demonstrate how the system can be viewed as a UV-completion of boundary states for chiral theories, establishing a connection to the proposed resolution of the puzzle using boundary conformal field theory.

Tue, 17 Feb 2026
13:00
L2

A universal sum over topologies in 3d gravity

Boris Post
(Oxford )
Abstract

In this seminar, I will explore how the sum over topologies in pure AdS_3​ quantum gravity furnishes a consistent statistical interpretation of the boundary CFT_2. By formulating a statistical version of the conformal bootstrap, which combines crossing symmetry with typicality at high energies, we will discover a large set of non-handlebody topologies in the bulk (of which I will give some examples) that are needed for consistency of the boundary description. Interestingly, this set contains only on-shell (i.e. hyperbolic) 3-manifolds, but not all of them. This suggests that the full sum over all on-shell saddles in 3d gravity may be a highly non-minimal solution of the statistical bootstrap. Based on the recent work 2601.07906 with Belin, Collier, Eberhardt and Liska.

Tue, 18 Nov 2025
13:00
L2

An N=4 SYM Collider at Finite Rank and Finite Coupling

Robin Karlsson
(Oxford )
Abstract

Energy correlations characterise the energy flux through detectors at infinity produced in a collision event. In CFTs, these detectors are examples of light-ray operators and, in particular, the stress tensor operator integrated over future null infinity. In N=4 SU(N_c) SYM, we combine perturbation theory, holography, integrability, supersymmetric localisation, and modern conformal bootstrap techniques to obtain predictions for such a collider experiment at finite coupling, both at finite number of colours, and in the planar limit. In QCD, the coupling runs with the angle between detectors, and there is a transition from perturbative to non-perturbative QCD. In N=4 SYM, a similar transition occurs when the coupling is varied, which we explore quantitatively. I will describe the physics underlying this observable and some of the methods used, particularly in regimes with analytical control.


 

Tue, 28 Oct 2025
13:00
L2

Periods, the Hodge structure and the arithmetic of Calabi-Yau manifolds

Xenia de la Ossa
(Oxford )
Abstract

It is well known to mathematicians that there is a deep relationship between the arithmetic of algebraic varieties and their geometry.  

These areas of mathematics have a fascinating connection with physical theories and vice versa.  Examples include Feynman graphs and black hole physics.  There are very many relationships however I will focus on the structure of black hole solutions of superstring theories on Calabi-Yau manifolds. 

 
The main quantities of interest in the arithmetic context are the numbers of points of the variety, considered as varieties over finite fields, and how these numbers vary with the parameters of the varieties. The generating function for these numbers is the zeta function, about which much is known in virtue of the Weil conjectures. The first surprise, for a physicist, is that the numbers of these points, and so the zeta function, are given by expressions that involve the periods of the manifold.  These same periods determine also many aspects of the physical theory, including the properties of black hole solutions. 

 
I will discuss a number of interesting topics related to the zeta function, the corresponding L-function, and the appearance of modularity for one parameter families of Calabi-Yau manifolds. I will focus on an example for which the quartic numerator of the zeta function of a one parameter family factorises into two quadrics at special values of the parameter. These special values, for which the underlying manifold is smooth, satisfy an algebraic equation with coefficients in Q, so independent of any particular prime.  The significance of these factorisations is that they are due to the existence of black hole attractor points in the sense of type II supergravity which predict the splitting of the Hodge structure over Q at these special values of the parameter.  Modular groups and modular forms arise in relation to these attractor points, in a way that is familiar to mathematicians as a consequence of the Langland’s Program, but which is a surprise to a physicist.  To our knowledge, the rank two attractor points that were  found together with Mohamed  Elmi and Duco van Straten by the application of  number theoretic techniques, provide the first explicit examples of such attractor points for Calabi-Yau manifolds.  
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