UEICMSSeminar Room
FIRST seminar
SECOND seminar
We are piloting a hybrid seminar format. Speakers and attendees can opt to join in-person or remotely using Zoom.
Unless otherwise stated below, the bi-seminars will be held fortnightly on Wednesdays at 14:30-15:30 and 16:00-17:00, room 5.10 in the ICMS of the Bayes Centre. Instructions for Zoom attendees will be shared before each seminar.
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Appleton TowerAppleton Tower LT12022-06-01 Congkao Wen Queen MaryTBA TBA
Lydia Bieri U. Michigan TBATBA
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Appleton TowerAppleton Tower LT1 (please note the usual times)2022-05-18 Guilherme Pimentel SNS PisaDifferential equations for cosmological correlators The bootstrap approach to cosmological correlators relies on
the existence of differential equations in terms of boundary momenta. I
will describe a new method to efficiently characterize and (in some
sense) explain the existence of these differential equations. The method
is general, but I will focus on cosmological correlation functions of a
light scalar in power law FLRW cosmologies. It recasts the differential
equation in terms of a new (somewhat magical) object, a flat connection
in the boundary kinematic space. The mathematical theory of this flat
connection is beautiful on its own right, and not fully developed yet.
The physical information it carries - in particular, locality of the
correlator - is encoded in its structure in a way that I don’t understand.
Andrea Arduino Universita di TorinoBig-Bang type singularities in QFT and string theory on time-dependent orbifoldsTime-dependent orbifolds generated from Minkowski spacetime are very useful toy models to address the study of Big-Bang type singularities. After introducing their geometry, I will review some of the results presented in the literature when they have been considered as cosmological backgrounds of string theory. I will in particular discuss the most serious issue that has been encountered: the unusual divergences found in the computation of some tree-level string scattering amplitudes. I will then move to the study of an effective quantum field theory on these models, which shows where the real nature of their pathological behavior lies. Finally, in order to cure the divergences, I will introduce a noncommutative framework which seems promising both from the QFT and the string theory point of view.
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Appleton TowerAppleton Tower LT12022-05-04 Saso Grozdanov UoEUnivalence bounds on transport and effective field theories Bounds on transport represent a way of understanding allowable regimes of quantum and classical dynamics. Numerous such bounds have been proposed, either for classes of theories or (by using general heuristic arguments) universally for all theories. Few are exact and inviolable. In this talk, I will present new methods for deriving exact, rigorous, and sharp bounds on all coefficients of hydrodynamic dispersion relations, including diffusivity and the speed of sound. These general techniques combine analytic properties of hydrodynamics and the theory of univalent (complex holomorphic and injective) functions. Concrete examples will include bounds that relate transport to quantum chaos through 'pole-skipping' as well as bounds without relation to chaos, such as the conformal bound on the speed of sound. I will also outline a set of general observations regarding the univalence properties of diffusion and sound in holographic models. Finally, I will discuss how these ideas could be generally applicable to constraining any effective field theory, not only hydrodynamics.
Giandomenico Palumbo DIAS Non-Relativistic Supergeometry in the Moore-Read Fractional Quantum Hall
StateThe Moore-Read state is one the most well known non-Abelian fractional
quantum Hall states. It supports non-Abelian Ising anyons in the bulk
and a chiral boson and a chiral Majorana mode on the boundary. It has
been recently conjectured that these two boundary modes are
superpartners of each other and described by a supersymmetric conformal
field theory.
In this talk, I present a non-relativistic supergeometric theory that is
compatible with this picture and gives rise to an effective gravitino in
the bulk. After breaking supersymmetry through a goldstino (i.e. a
Nambu-Goldstone fermion), the gravitino becomes massive and can be seen
as the neutral spin-3/2 collective mode that characterises the
Moore-Read state in the bulk. After integrating out this massive fermion
field, I obtain a purely bosonic topological action that properly
encodes the Hall conductivity, Hall viscosity and gravitational anomaly,
which represent the physical observables of the fractional quantum Hall
effect.
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Bayes CentreBayes Centre G.032022-04-20 Joan Elias Miro International Centre for Theoretical Physics, TriesteHamiltonian Truncation with Larger DimensionsHamiltonian Truncation (HT) is a numerical approach for calculating observables in a Quantum Field Theory non-perturbatively. This approach can be applied to theories constructed by deforming a conformal field theory with a relevant operator of scaling dimension N.
In this talk I will review the HT techniques and emphasise few key open problems.
I will also discuss the recent efforts to extend these ideas to higher dimensions and for UV divergent relevant operators.
Simon Pekar Universite de MonsCarrollian conformal higher-spin algebras in any dimensions -->
Bayes CentreBayes Centre 5.462022-04-06 Yannick Herfray Universite de MonsCartan geometry of null infinity A feature of General Relativity is the interplay between physics and geometry. An beautiful instance of this fact is realised at null infinity where asymptotic gravitational data are realised geometrically as a boundary "conformal Carrollian geometry", with the BMS group acting as a group of symmetry. The invariant meaning (and geometrical elegance) lying behind these however only fully appear in the language of Cartan geometry. I will explain this as well as relationship to other related construction such as local twistors.
Paolo Di Vecchia Nordic Institute for Theoretical Physics Universality at high energy in black hole scatteringSince in gravity theories the massless particle with the highest spin is the graviton, we expect that all observables have a universal behaviour at high energy. In this talk I will first consider the deflection angle in the elastic scattering and how that, in this case, universality is obtained by adding the radiation reaction contribution to the part obtained from the potential region. Then I will consider the inelastic processes in which gravitons are
emitted and, following the method of Bloch-Nordsieck, I will construct the eikonal operator for the emission of soft gravitons and I will use it to
compute the soft waveforms and the zero-frequency limit (ZFL) of the spectrum of emitted gravitons. I will show that the previous observables are also universal but, in these inelastic cases, universality is reached in a more non-trivial way.
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2022-03-23 Maciej Dunajski DAMTP, University of CambridgeQuasi-local mass, Kerr horizon, and causality I will discuss two approaches to mass in General Relativity. One quasi—local, and applicable to closed surfaces in space times (like that of the Kerr horizon), and one global, based on causal properties of space-times near space-like infinity.
Lionel Mason Mathematical Institute, University of Oxford Graviton scattering on curved self-dual backgrounds via integrabilityWe establish a framework for computing graviton scattering amplitudes on curved self-dual radiative space-times; these are chiral, source-free, and asymptotically flat spaces, determined by free characteristic data at null infinity. Such space-times admit an elegant twistor description via Penrose's non-linear graviton, which manifests their underlying integrability. The tree-level S-matrix is written in terms of an integral over the moduli space of holomorphic maps from the Riemann sphere to twistor space, with the degree of the map corresponding to the helicity configuration of the external gravitons. For the MHV sector, we derive the amplitudes directly from general relativity, while other helicity configurations arise from a natural family of generating functionals and pass several consistency checks. The amplitudes exhibit many novel features which are absent in Minkowski space, including tail effects. Although there are residual integrals due to the functional degrees of freedom in the background space-time, our formulae have fewer such integrals than expected from space-time perturbation theory. In highly symmetric special cases, such as self-dual plane waves, the number of residual integrals can be further reduced, resulting in even simpler expressions for the scattering amplitudes. If there is time I will discuss connections with celestial holography. This is joint work with Tim Adamo and Atul Sharma based on 2203.02238, 2110.06066, 2103.16984, 2010.14996.
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2022-03-09 Justin Vines Albert Einstein Institute, MPISpinning black hole probes in a Kerr background TBA
Neil Turok Higgs Chair of Theoretical Physics, UoE The puzzling path integral for gravityFeynman’s path integral is the most elegant known formulation of the quantum physics of continuous systems. It is particularly suited to relativistic theories, including gauge theories and gravity. However, it is an enduring embarrassment that path integrals have never been rigorously formulated except by ``Wick rotating'' to imaginary (``Euclidean'') time. Unfortunately, continuing back to real (Lorentzian) time, where observations are made, is usually impossible outside of perturbation theory. Moreover, the Euclidean path integral fails badly for gravity and therefore for cosmology. I will describe recent work with J. Feldbrugge aimed at defining and evaluating Lorentzian (i.e., real-time) path integrals, using new physical insights and an extension of Picard-Lefschetz (steepest descent) methods for finite-dimensional oscillatory integrals. Finally, I will summarise some exciting new work with L. Boyle using the path integral for cosmology to calculate the gravitational entropy of a semi-realistic universe. This calculation suggests a new, simpler explanation for the large scale geometry of space time.
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Appleton TowerAppleton Tower LT12022-02-23 Stephen Angus Asia Pacific Center for Theoretical PhysicsFractons, geometrically I will discuss how fracton physics can be studied systematically within the geometric framework of Double Field Theory (DFT). Following an introductory review of fractons, I will argue that their restricted mobility and large degeneracy of quantum states can be attributed to the generalized geodesics and infinite-dimensional isometries present in non-Riemannian backgrounds of DFT. Furthermore, we find that a doubled pure Yang-Mills or Maxwell theory reduces to an ordinary one interacting with a strain tensor theory, giving a unifying description of photons and phonons. I will show how this photon-phonon theory, when minimally coupled to a charged particle in a non-Riemannian background, lifts the particle immobility to a saturation velocity and gives a modified dispersion relation.
Tristan Orchard King's College Null Reduction of M5 branesI discuss the results from a series of papers on performing certain null reductions on coincident M5 branes. Starting with the most general result on curved backgrounds, before focusing on an interesting Omega-deformed spacetime. The latter is central to a construction that rebuilds the full 6d theory using instantons, I discuss this mechanism as well as the interesting symmetry groups at play.
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2022-02-09 Eric Sharpe Virginia Tech.An introduction to decompositionIn this talk I will review recent work on `decomposition,'
a property of 2d theories
with 1-form symmetries and, more generally, d-dim'l theories with (d-1)-form
symmetries. Decomposition is the observation that
such quantum field theories are equivalent to ('decompose into’)
disjoint unions of other QFTs, known in this context as "universes.”
Examples include two-dimensional gauge theories and
orbifolds with matter invariant under a subgroup of the gauge group.
Decomposition explains and relates several
physical properties of these theories -- for example,
restrictions on allowed instantons arise as a "multiverse
interference effect" between contributions from constituent universes.
First worked out in 2006 as part of efforts to understand string propagation
on stacks, decomposition has been the driver of a number of developments since.
In the first half of this talk, I will review decomposition; in the
second half, I will focus on the recent application to anomaly resolution of
Wang-Wen-Witten in two-dimensional orbifolds.
Praxitelis Ntokos University of EdinburghBlack hole superpotential as a unifying entropy function and BPS thermodynamicsIn the last few years, there has been enormous progress on the statistical description of the entropy of BPS black holes in AdS_D for 𝐷>3 in terms of states in the dual field theory. The success of such developments relies on the existence of an extremisation principle in the bulk which maps to the evaluation of the partition function in the field theory in the large charge limit. In this talk, I will describe an ''off-shell'' approach to the study of black hole thermodynamics in AdS_5 based on an effective superpotential. This approach offers a powerful tool to analyse the thermodynamics without resorting to explicit solutions and can be in principle implemented even to non-supersymmetric configurations. For BPS black holes, it provides the framework where the aforementioned (Hosseini-Hristov-Zaffaroni) extremisation principle emerges naturally in the bulk while it is also directly related to Sen’s entropy function for extremal black holes.
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2021-12-15 Jan Sbierski University of EdinburghThe strong cosmic censorship conjecture and singularities inside rotating black holesOne can paraphrase Penrose’s strong cosmic censorship conjecture as stating that general relativity is generically a deterministic theory. While the full conjecture remains wide open there has long been evidence pointing towards its validity at least for small perturbations of exact rotating Kerr black holes. In this talk I will give a brief historical account of this evidence, discuss the analytic as well as the geometric aspects of this conjecture, and conclude by presenting forthcoming work on the linear instability of the Kerr Cauchy horizon.
Alfredo Guevara Harvard UniversityBlack Holes, Scattering Amplitudes and TwistorsScattering amplitudes are very natural in (2,2) signature, where the on-shell three-point functions do not vanish. Motivated by recent progress in celestial holography, we link (2,2) scattering amplitudes to Black Holes in (2,2) Klein space, and study their global structure. The link is very natural from the perspective of twistor theory. These black holes are a simple analytic continuation away from (1,3) solutions, but their (2,2) signature unveils new properties such as a direct diffeomorphism between Kerr Taub-NUT and Taub-NUT spacetimes.
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2021-12-08 Daniel Roggenkamp University of Mannheim Defects and affine Rozansky-Witten modelsIn this talk I will explain, in the example of Rozansky-Witten models with affine target spaces, how to reconstruct an (extended) TQFT from its identity defect. For illustration I will shoot a sparrow with a cannon and use defects to rederive the state spaces of affine RW models for arbitrary surfaces.
Lotte Hollands Heriot-Watt University Partition functions, BPS states and abelianizationIn this talk I will re-express the Nekrasov-Shatashvili free energy for a four-dimensional N=2 gauge theory as an integral of a ratio of Wronskians of solutions to the relevant oper equation, with the AD2 theory and the pure SU(2) theory as two main examples. This motivates the definition of a generalized Nekrasov-Shatashvili free energy for any four-dimensional N=2 theory of class S, and makes a connection with abelianization and exact WKB analysis. We will end with some remarks regarding the five-dimensional generalization and the relation to similar mathematical structures underlying the topological string partition function. This talk is based on 2109.14699 and work in progress.
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2021-11-17 Valentina Forini City, University of LondonConformal correlators and AdS_2/CFT_1Wilson lines are a prototypical example of defect in QFT. I will consider the defect CFT_1 defined by correlators of operator insertions on a supersymmetric Wilson line in the d=3 superconformal ABJM model, illustrating how superspace techniques, analytic bootstrap and direct Witten diagrammatics can be used, combined with holography, to find its CFT data. I will then present a nonperturbative definition of Mellin amplitude for more general CFT_1 four-point correlators, and describe the use of this formalism to derive new results.
Anthony Ashmore University of ChicagoMachine Learning for Calabi-Yau CompactificationsCalabi-Yau metrics and hermitian Yang-Mills connections have played a key role in both mathematics and physics in recent decades, and are particularly important for deriving semi-realistic models of particle physics from string theory. Unfortunately, explicit expressions for these objects are few and far between, leaving us unable, for example, to compute particle masses or couplings in string models. I will review recent progress on using machine learning techniques to compute these quantities numerically, with a particular focus on the example of computing gauge connections on line bundles.
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2021-11-03Pre-seminars for PhD students
Chris Heunen University of EdinburghAxioms for the category of Hilbert spacesWe provide axioms that guarantee a category is equivalent to that of continuous linear functions between Hilbert spaces. The axioms are purely categorical and do not presuppose any analytical structure such as probabilities, convexity, complex numbers, continuity, or dimension. We'll discuss the axioms, sketch the proof of the theorem, and survey open questions, further directions, and context. (Based on joint work with Andre Kornell arxiv:2109.07418.)
João Melo DAMTP, University of CambridgeThe Propagator Matrix ReloadedFor quantum fields in curved spacetimes there isn't a unique notion of vacuum state and the in and out vacua might be different, therefore, to perform calculations with interacting theories we require the use of the Schwinger-Keldysh formulation, very similar to undergraduate quantum mechanics. However, the usual assumption that the theory is free at past infinity isn't necessarily true and there is a need to modify the usual formalism to take this into account, resulting in a 3x3 matrix of propagators instead of the more familiar 2x2. In my talk I will describe this new formalism and test it in flat spacetime with the surprising conclusion that even in Minkowski spacetime it seems like the theory isn't free at past infinity at finite temperature as is commonly assumed.
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2021-10-20 PhD Student talks University of Edinburgh and Heriot-Watt UniversityTBATBA
Justin Vines Albert Einstein Institute, MPISpinning black holes meeting gravitonsClassical gravitational interactions of spinning black holes (BHs) can be usefully described by certain limits of certain quantum scattering amplitudes, for massive higher-spin fields "minimally coupled" to gravity. Tree-level interactions between two BHs are determined by 3-point amplitudes (BH in, BH out, meeting one graviton) which are arguably well understood -- on the quantum side, for arbitrary-spin massive particles; classically, to all orders in the BH spin. Two-BH (conservative) interactions at the classical 1-loop level (and other processes) are argued to be determined by the additional 4-point "Compton" amplitude (BH in, BH out, meeting two gravitons), which is more poorly understood -- on the quantum side, up to spin-2 (or 5/2?); classically, up to 4th (or 5th?) order in the BH spin. In this talk, we'll discuss efforts to better understand the BH-graviton Compton amplitude for higher spins, and its applications, including directly interpreting its classical limit as the o
utgoing amplitude for an incoming gravitational plane wave scattering off a Kerr BH.
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2021-10-06 Andrea Cristofoli University of EdinburghThe On-Shell Highway to WaveformsA particle physics approach to describing black hole interactions is opening new avenues for understanding gravitational-wave observations. In this talk, we will review this paradigm change showing how general relativity naturally emerges from scattering amplitudes. Applications for deriving solutions to Einstein field equations, the bending of light and waveforms - directly from quantum field theory - are explained.
Chiara Toldo University of AmsterdamThe Updates on the search for multicenter AdS black holesWhile multicenter black holes in asymptotically flat space have long been object of study, the construction of multi black holes geometries in Anti-de Sitter spacetimes remains so far elusive. In this talk I will discuss recent progress on the search for these solutions. Working in the probe approximation, I will show that there exist stable ad metastable black hole bound states in compactifications of M-theory on 7-dimensional Sasaki-Einstein manifolds with Betti multiplets and AdS4 vacua. I will map out their thermodynamic landscape and discuss the relevance of these setups for describing glassy systems via holography. I will finally discuss their supersymmetric limits, in light of recent developments regarding the entropy matching for stationary AdS4 black holes via localization in the dual 3d CFT.
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2021-09-29 Gabriel Larios IFT Madrid and University of MichiganLessons and surprises from Kaluza-Klein spectraInfinite towers of massive modes arise for every compactification of higher dimensional theories. Understanding the properties of these Kaluza-Klein towers on non-trivial solutions with an AdS factor has been a longstanding issue with clear holographic interest, as they describe the spectrum of single-trace operators of the dual CFTs at strong coupling and large N. In this talk, I will focus on two classes of solutions of such kind. The first class consists of AdS4 solutions of D=11 and Type II supergravity that can be obtained from maximal gauged supergravities in D=4. For the later part, I will describe new families of solutions in N=(1,1) supergravity in D=6 which uplift from half-maximal supergravity in D=3. In both cases, the spectra can be computed using recent techniques from Exceptional Field Theory, and the information thus obtained leads to several unexpected conclusions.
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2022-01-26 Minhyong Kim ICMSOn some infinities in arithmetic geometryThis will be a mostly expository talk to introduce mathematical physicists to some difficult problems of arithmetic geometry involving infinities that are conjectured to be 'regularizable.' The overall hope is that the maths/physics expertise can be of help in making progress on them.
Edward Witten IAS Gravity and the Crossed ProductRecently Leutheusser and Liu identified an emergent algebra of Type III1 in the operator algebra of N=4 super Yang-Mills theory for large N. Here we describe some 1/N corrections to this picture and show that the emergent Type III1 algebra becomes an algebra of Type II∞. The Type II∞ algebra is the crossed product of the Type III1 algebra by its modular automorphism group. In the context of the emergent Type II∞ algebra, the entropy of a black hole state is well-defined up to an additive constant, independent of the state. This is somewhat analogous to entropy in classical physics.