Nordita-Uppsala samtliga seminarier
Möten organiseras omväxlande i Uppsala och Stockholm. När mötet hålls i Uppsala, sker det på onsdagar men, när den hålls i Stockholm flyttas det till på måndagar istället, det vill säga i enlighet med respektive lokala scheman. Detta möte kan kombineras med en kort informell presentation av en lokal talare. Lunch serveras vanligtvis klockan 12:30.
(1) Black hole bulk-cone singularities (2) The Higher Structure of Chiral Symmetry
Speakers: (1) Alexander Zhiboedov (CERN) (2) Michele Del Zotto (Uppsala)
Time: 16 March 2023 (1) 11:00-12:00 (2) 14:00-15:00
Abstract: (1) In theories with gravity duals Lorentzian correlators exhibit surprising singularities. These serve as the field-theoretic representation of the emergent bulk causal structure. In this talk we describe the singularity structure of the thermal two-point function which captures the causal structure of its dual black hole geometry. We explain how these singularities can be computed in the gravity approximation and discuss the effects of stringy corrections on the singular behavior. We argue that detecting traces of black hole bulk-cone singularities in future simulations of holographic systems can be likened to the black hole images recently captured by the Event Horizon Telescope. Based on an ongoing work with M. Dodelson, C. Iossa, R. Karlsson, A. Lupsasca.
(2) In presence of ABJ anomalies the familiar chiral symmetry of massless QED in 3+1 spacetime dimensions develops an interesting example of higher structure. In this talk we will explain that the higher structure of chiral symmetry is "physical", meaning that (1) it can be detected in specific correlators, and that (2) it implies selection rules and Ward-Takahashi identities for massless QED on curved spacetimes.
(1) The small-N expansion: a constructive approach to transseries (2) Gravitational Scattering at 4th Post-Minkowskian Order
Speakers: (1) Davide Lettera (Nordita) (2) Gregor Kälin (DESY)
Time: 16 March 2023 (1) 11:00-12:00 (2) 13:45-14:45
Location: Uppsala, Ångströmlaboratoriet 80121
Abstract: (1) Zero dimensional QFTs are much more manageable than fully fledged d > 0 QFT and they often provide us with a useful toy model that can be used to test their properties. This talk will be based on the recent work 2210.14776, in which we investigate a d = 0 quartic O(N) vector model and present a complete study of the partition function Z(g,N) and its logarithm, the free energy W (g, N ), seen as functions of the coupling g on a Riemann surface. Using constructive field theory techniques we prove that both Z(g,N) and W(g,N) are Borel summable functions along all the rays in the cut complex plane Cπ = C \ R−. Past the Stokes line at R− both Z(g,N) and W(g,N) cease to be Borel summable due to exponential (instanton) corrections. We describe the Stokes phenomenon and recover the transseries expansion of Z(g,N) using the intermediate field representation. We furthermore study the small-N expansions of Z(g,N) and W(g,N), and notice that the Taylor coefficients of these expansions, Zn(g) and Wn(g), exhibit analytic properties similar to Z(g,N) and W(g,N). The transseries expansion of Zn(g) is readily accessible, then the transseries of Wn(g) is obtained using Möbius inversion and allow us to derive the transseries expansion of W(g,N).
(2) The construction of gravitational waveform templates requires high-precision knowledge of the motion of a gravitationally interacting two-body system. In this talk I will present a complete, systematic, and efficient framework based on a world-line model to describe such a two-body system. I will discuss the tools and techniques -- many of them borrowed from high-energy particle physics -- that are being used for the state-of-the-art computation of the complete 4th Post-Minkowskian (NNNLO) scattering angle for a hyperbolic encounter. Our toolbox for the handling of Feynman integrals reaches from integration by part reduction, over canonical forms of differential equations, to machine-learning techniques for numerical evaluation. Furthermore, I will introduce a boundary-to-bound dictionary that allows us to analytically continue certain quantities to bound orbits which are directly relevant for the construction of gravitation waveforms.
(1) Kerr Black Holes Enjoy Massive Higher-Spin Gauge Symmetry (2) Machine code of holography
Speakers: (1) Lucile Cangemi (Uppsala) (2) Umut Gürsoy (Utrecht)
Time: 07 February 2023 (1) 11:00-12:00 (2) 14:00-15:00
Abstract: (1) In this talk, I will discuss the role gauge symmetry plays in constraining Kerr dynamics. I will introduce how we construct EFTs for Kerr black holes with Stückelberg fields and how to reproduce the known Kerr three point amplitudes using massive higher-spin gauge symmetry. In parallel, I will discuss EFTs for the closely related electromagnetic solution, root-Kerr, which are similarly constrained by the Ward identities that follow from the symmetry. I will also discuss aspects relevant to the analysis of the spin-s Compton amplitude and provide a prediction for the spin-2 root-Kerr Compton that follows from massive gauge symmetry.
(2) Gauge-gravity duality plays a key role in understanding quantum gravity and strongly interacting gauge theories, however, lacks a satisfactory microscopic derivation. Fundamental questions such as, how does gravity emerge directly from quantum field theory observables and how to determine which QFTs are holographic, which are not, remain unanswered. In this talk, I propose a primitive form of gauge-string duality based on the worldline formulation of perturbative QFT. In particular we consider L loop quantum corrections to correlation functions in an holographic QFT where a Schwinger parameter is associated to each internal propagator in the corresponding Feynman diagrams. We argue that embedding of the holographic coordinate in string theory emerges from the collection of these Schwinger parameters in the continuum limit of the Feynman diagrams where L diverges. As a by product, we provide a novel Kallen-Lehmann representation of two-point functions as a sum over boundary-to-boundary propagators of massive bulk scalars in AdSd+1 with masses determined by L. This novel approach can be generalized to arbitrary N. Therefore it might have two potential uses: to provide i) a non-perturbative approach to quantum gravity in terms of perturbative QFT at finite N, ii) a true bottom-up holographic construction for confining gauge theories like QCD derived directly from QCD amplitudes.
(1) Non-Lorentzian Supergravity and Dualities (2) Geometry in Scattering Amplitudes
Speakers: (1) Johannes Lahnsteiner (Nordita) (2) Andreas Helset (Caltech)
Time: 09 November 2022 (1) 14:00-15:00 (2) 15:45-16:45
Location: Uppsala, Ångströmlaboratoriet Å4101
Abstract: (1) In this talk, I describe recent progress in understanding the background field dynamics of non-relativistic string theory. Building on earlier developments, I present a non-Lorentzian supergravity theory in ten dimensions and explain how it constrains the dynamics of the background fields. Special attention will be given to the exotic multiplet structures. Furthermore, I will show how string dualities are realized in this context. In the final part of this talk, I will present some results on non-Lorentzian supergravity in eleven dimensions and comment on possible applications.
(2) One central property of the S-matrix is its invariance under field redefinitions. I will discuss how the geometry of field space makes this invariance manifest. This geometric formulation also has practical consequences. Scattering amplitudes and the renormalization group equations for a theory of scalars and gauge bosons only depend on geometric quantities. Also, the scattering amplitudes satisfy a geometric soft theorem.
(1) Seven-dimensional super-Yang-Mills at negative coupling (2) A quick introduction to melonic CFTs
Speakers: (1) Charles Thull (Uppsala) (2) Sabine Harribey (Nordita)
Time: 11 October 2022 (1) 11:00-12:00 (2) 14:00-15:00
Abstract: (1) A stack of D6 branes in type IIA string theory admits two distinct low energy regimes. We show that these two regimes know about each other. We start from the weakly coupled seven-dimensional super-Yang-Mills theory and use supersymmetric localization to compute its sphere partition function. This admits a regime of negative effective 't Hooft coupling. Here, the non-perturbative contributions to the partition function become important and in the small negative coupling limit we find weakly tensioned instanton membranes. We understand these as part of a weakly coupled seven-dimensional supergravity theory, the second IR regime for the D6 brane stack.
(2) Random tensors exhibit a melonic large-$N$ limit, which is both richer than the large-$N$ limit of vector models and simpler than the planar limit of matrix models. They were first introduced in zero dimension in the context of random geometry and quantum gravity. They were then generalised in $d$ dimensions where they can be studied as proper quantum field theories. In this context, they give rise in the infrared to a new type of CFTs, analytically accessible, called melonic CFTs. After briefly reviewing the history of tensor models, I will present in particular the long-range $O(N)^3$ bosonic tensor model. In the large-N limit, but non-perturbatively in the coupling constants, we showed the existence of a stable, strongly-interacting line of fixed points. We also found strong hints of unitarity at large N. These results can then be used to study properties of QFTs in rigorous set-ups. For example, we recently showed that this model gives a new non-trivial example of the $F$-theorem.
(1) Understanding O(N) symmetry for non-integer N via Deligne categories (2) Localization of 4d N=1 theories on D2×T2
Speaker: (1) Slava Rychkov, (2) Antonio Pittelli
Department: (1) Institut des Hautes Études Scientifiques, (2) Uppsala University
Time: 2019-12-06 (1) 10:30-11:30, (2) 13:15-14:15
Abstract: (1) In QFT, we often analytically continue in the number of field components, or in the number of spatial dimensions. I always wished to know which rigorous mathematics underlies these computations. What replaces group symmetries and irreducible representations when one goes to non-integer dimensions? It turns out that the appropriate language is provided by symmetric tensor categories introduced by Pierre Deligne in 2004. They have since been studied by mathematicians, and their relevance to QFT and lattice models was pointed out in our recent work 1911.07895. This blackboard talk will expose relevant ideas, without assuming any prior familiarity with categories. (Joint work with Damon Binder.)
(2) We consider 4d N=1 gauge theories with R-symmetry on a hemisphere times a torus. We apply localization techniques to evaluate the exact partition function through a cohomological reformulation of the supersymmetry transformations. Our results represent the natural elliptic lifts of the lower dimensional analogs as well as a field theoretic derivation of the conjectured 4d holomorphic blocks, from which partition functions of compact spaces with diverse topology can be recovered through gluing. We also analyze the different boundary conditions which can naturally be imposed on the chiral multiplets, which turn out to be either Dirichlet or Robin-like. We show that different boundary conditions are related to each other by coupling the bulk to 3d N=1 degrees of freedom on the boundary three-torus, for which we derive explicit 1-loop determinants.
(1) Isolated zeros destroy segments of Fermi surface in holographic models with a lattice (2) Higher form symmetries and superfluids
Speaker: (1) Alexander Krikun, (2) Diego Hofman
Department: (1) Nordita, (2) Amsterdam
Time: 2019-10-09 (1) 10:45-12:00, (2) 13:45-15:00
Location: Uppsala, (1) Å10134, (2) Å4101
Abstract: (1) I will discuss the fermionic response of the holographic model of a strange metal in the non-homogeneous black hole background created by the periodically modulated chemical potential. Apart from the observation of the standard umklapp and the band formation, which is expected to occur in any system with the periodic potential, I will show that in the regimes of strong modulation the lines of zeros of the spectral function get pushed close to the lines of poles indicating the Fermi surface. This proximity destroys the full segments of the latter. The existence of zeros is the generic feature of the holographic fermionic response, which can be related to the alternatively quantized dual CFT. While the effect which we will see, relies substantially on the particularity of the holographic framework, it is quite similar to the Fermi arc formation in the pseudogap phase of the doped cuprates, observed experimentally. Based on: arXiv:1909.09394.
(2) I will describe superfluid hydrodynamics as the hydrodynamic theory of a system with an emergent anomalous higher-form symmetry. The higher-form charge counts the winding planes of the superfluid – its constitutive relation replaces the Josephson relation of conventional superfluid hydrodynamics. This formulation puts all hydrodynamic equations on equal footing. The anomalous Ward identity can be used as an alternative starting point to prove the existence of a Goldstone boson, without reference to spontaneous symmetry breaking. This provides an alternative characterization of Landau phase transitions in terms of higher-form symmetries and their anomalies instead of how the symmetries are realized. This treatment is more general and, in particular, includes the case of BKT transitions.
(1) CFT correlators, string theory scattering amplitudes, and supersymmetric localization (2) Bootstrapping Multiple Scattering Amplitudes
Speaker: (1) Silviu Pufu, (2) João Penedones
Department: (1) Princeton, (2) EPFL Lausanne
Time: 2019-05-08 (1) 10:45-12:00, (2) 13:45-15:00
Location: Uppsala, (1) Å4001, (2) Å4101
Abstract: (1) In this talk, I will discuss how a combination of supersymmetric localization, Mellin space, and string theory scattering amplitudes can be used to extract new information about the 4-point functions of single trace superconformal primaries in N=4 SYM theory. These computations also provide new precision tests of AdS/CFT beyond the supergravity approximation.
(2) The S-matrix Bootstrap approach can be used to derive bounds on the coupling constants on any Lorentz invariant quantum field theory due to analyticity, crossing symmetry and unitarity. In our previous work, constraints were derived by studying only the 2-to-2 scattering of the lightest particle of the theory. I will describe the extension of our techniques in order to include constraints stemming from 2-to-2 processes which involve the next-to-lightest particle of the theory. We test these techniques on a family of 1+1 dimensional theories inspired by (and including) the three state Potts field theory. We find that the inclusion of more 2-to-2 amplitudes significantly reduces the single amplitude bounds.
(1) Solving q-Virasoro constraints, (2) Integrable system constructed from the geometry of a spectral curve
Speaker: (1) Rebecca Lodin, (2) Bertrand Eynard
Department: (1) Uppsala, (2) IPhT Saclay
Time: 2019-03-25 (1) 10:45-11:45, (2) 13:15-14:15
Abstract: (1) The Virasoro constraints – arising from Ward identities – are a key component in understanding the relation between matrix models and conformal field theories; they provide the set of equations constraining the generating function which can then be solved using CFT methods. These Virasoro constraints can be derived either using differential operators or by using the so-called free field representation of the Virasoro algebra. In this talk I will discuss what happens when these constraints are q-deformed. In particular, I will outline how such q-Virasoro constraints can be derived for a large class of deformed eigenvalue matrix models by an elementary trick of inserting certain q-difference operators under the integral. These q-Virasoro constraints can then be solved recursively and they also have applications for gauge theories.
(2) One usual way of defining an integrable system is in terms of a Tau-function obeying Hirota equations.
The Tau-function (example KdV) is usually defined as a function of an infinite set of times t=(t0,t1,t2,t3,...).
Here instead we shall define Tau as a function on the moduli space of spectral curves (plane analytic curves with extra structure), and the “times” can be viewed as local coordinates (but not global in general). The tangent space (i.e. the span of all $\partial/\partial tk$, i.e. Hamiltonians) to the moduli space of spectral curves, is isomorphic to the space of meromorphic 1-forms on the curve, and by form-cycle duality is isomorphic to a Lagrangian in the space of cycles. In other words, we reinterpret Hamiltonians as cycles, and the symplectic Poisson structure as the intersection of cycles.
The topological recursion (TR) defines invariants of the spectral curve, and we show how to get a Tau-function from the TR-invariants. This is an efficient method, which gives new insights on integrable systems.
(1) Closed Strings and Moduli in AdS3 x S3, (2) Light ray operators, event shapes and Einstein gravity
Speaker: (1) Olof Ohlsson Sax, (2) Sacha Zhiboedov
Department: (1) Nordita, (2) CERN
Time: 2018-11-14 (1) 10:15-11:30, (2) 13:45-15:00
Location: Uppsala, (1) Å4001, (2) Å80101
Abstract: (1) String theory on AdS3 x S3 x T4 has 20 moduli. I will discuss how the perturbative closed string spectrum changes as we move around this moduli space in both the RR and NSNS flux backgrounds. At weak string coupling, only four of the moduli affect the energies. In the RR background the only effect of these moduli is to change the radius of curvature of the background. On the other hand, in the NSNS background, the moduli introduce worldsheet interactions which enable the use of integrability methods to solve the spectral problem. These results show that the worldsheet theory is integrable across the 20 dimensional moduli space.
(2) I will describe recent developments and new results in the understanding of light ray operators in CFTs. One application of these techniques is computation of event shapes that are used to describe collider experiments for generic CFTs. Another application is new constraints on low-energy gravitational theories that admit a UV completion.
(1) Local tree level BCJ numerators for all multiplicity, (2) Generalized Wilson loops in N=4 SYM and correlators on a line
Speaker: (1) Fei Teng, (2) Arkady Tseytlin
Department: (1) Uppsala, (2) Imperial C
Time: 2017-12-18 (1) 11:30-12:00, (2) 13:15-14:15
Abstract: (1) we investigate the expansion of tree level multitrace Einstein-Yang-Mills (EYM) amplitudes. First, we propose two types of recursive expansions of tree level EYM amplitudes with an arbitrary number of gluons, gravitons and traces by those amplitudes with fewer traces or/and gravitons. Then we give many support evidence, including proofs using the Cachazo-He-Yuan (CHY) formula and Britto-Cachazo-Feng-Witten (BCFW) recursive relation. As a byproduct, two types of generalized BCJ relations for multitrace EYM are further proposed, which will be useful in the BCFW proof. After one applies the recursive expansions repeatedly, any multitrace EYM amplitudes can be given in the Kleiss-Kuijf (KK) basis of tree level color ordered Yang-Mills (YM) amplitudes. Thus the Bern-Carrasco-Johansson (BCJ) numerators, as the expansion coefficients, for all multitrace EYM amplitudes are naturally constructed.
(2) We will discuss 1d CFT defined by correlators of operators inserted along BPS Wilson line following arXiv:1706.00756 and some ongoing work about generalizations to non-BPS Wilson loops.
(1) Intersecting surface defects, instantons and 2d CFT, (2) Yang-Mills origin of gravitational symmetries
Speaker: (1) Yiwen Pan, (2) Leron Borsten
Department: (1) Uppsala, (2) Dublin
Time: 2017-04-10 (1) 11:30-12:00, (2) 13:15-14:15
Abstract: (1) we will introduce and study the intersection of multiple codimension two defects in 4d N=2 (and 5d N=1) gauge theories. These defects can be understood as 4d-2d-0d or 5d-3d-1d coupled systems. On the one hand, they naturally arise in the gauge theoretic operation called Higgsing, and on the other hand, they have 2d CFT interpretation via degeneration of the AGT correspondence. We will compute the partition functions of intersecting defects via the Higgsing procedure. We then discuss their exact relations to Liouville/Toda correlation functions with degenerate insertions. We will also present new Seiberg-like dualities between two simplest intersecting defect systems.
(2) A recurring theme in the attempts of understanding the quantum theory of gravity is the idea of “gravity as the square of Yang-Mills”. This involves the tensoring of the multiplet content of two super-Yang-Mills theories to obtain the multiplet content of a supergravity theory. A complete understanding of this correspondence requires studying how the gravitational symmetries originate from the corresponding Yang-Mills factors. In this talk I will show how both the global and local symmetries of linear supergravity arise from the corresponding super-Yang-Mills ones through a dictionary between both fields and transformation parameters. Finally, I will comment on how the dictionary seems to restrict the study of dynamics to particular gauge choices.
(1) Non-linear partially massless symmetry in an SO(1,5) continuation of conformal gravity, (2) The Nekrasov–Shatashvili Limit of the 5D Superconformal Index
Speaker: (1) Luis Apolo, (2) Costis Papageorgakis
Department: (1) Nordita, (2) Queen Mary
Time: 2016-11-23 (1) 11:30-12:00, (2) 13:45-14:45
Abstract: (1) Partially massless spin-2 fields in de Sitter space are characterized by a local symmetry that gauges away the helicity-0 mode of an otherwise massive graviton. Unlike massless or massive spin-2 fields, several “no-go” results exist that rule the existence of non-linear, interacting theories of partially massless fields. In this talk I will review some of these no-go results and describe a model that realizes the partially massless symmetry non-linearly.
(2) I will motivate and introduce the Nekrasov–Shatashvili (NS) limit of the five-dimensional N=1 superconformal index. I will then summarise recent results of Cordova and Shao, who related the so-called Schur limit of the four-dimensional N=2 index to the BPS spectrum of 4D theories on the Coulomb branch. Finally, I will describe how the technology of Cordova–Shao can also reproduce the NS index in 5D for simple examples of U(1) theories. In this picture, the 5D instanton solitons are interpreted as additional flavour nodes to an associated 5D BPS quiver.
(1) Background constraints in the infinite tension limit of the heterotic string, (2) S-matrix bootstrap and QFT in AdS
Speaker: (1) Thales Azevedo, (2) Jonathan Toledo
Department: (1) Uppsala, (2) EPFL
Time: 2016-10-24 (1) 11:30-12:00, (2) 13:15-14:15
Location: Nordita 132:028
Abstract: (1) Shortly after Mason & Skinner introduced the so-called Ambitwistor Strings, Berkovits came up with a pure-spinor analogue of the theory, which was later shown to provide the supersymmetric version of the Cachazo-He-Yuan amplitudes. In this talk, after briefly reviewing the infinite tension limit of the pure-spinor heterotic superstring in flat space, I will show how the model can be coupled to a general curved background, and then proceed to show that all the classical constraints on the supergravity and super Yang-Mills background superfields are elegantly obtained from the sole requirement that the BRST charge be nilpotent.
(2) We consider constraints on the S-matrix of any gapped, Lorentz invariant quantum field theory in 1+1 dimensions due to crossing symmetry and unitarity. In this way we establish rigorous bounds on the cubic couplings of a given theory with a fixed mass spectrum. In special cases we identify interesting integrable theories saturating these bounds. Our analytic bounds match precisely with numerical bounds obtained by considering massive QFT in an AdS box and studying the boundary correlators using the technology of the conformal bootstrap. The methods can be generalized to QFT in higher dimensions and I will comment on work underway in 3+1 dimensions. Talk based on 1607.06109 and 1607.06110 with Miguel Paulos, Joao Penedones, Balt van Rees and Pedro Vieira.
Supergravity and the cosmological constant
Speaker: Eric Bergshoeff
Department: Groningen University
Time: 2015-10-28 13:45-15:00
Location: Oseenska rummet (Å73121), Ångströmlaboratoriet
Abstract: I will discuss under which conditions a cosmological constant can be added to a given supergravity theory. In the case of a positive cosmological constant I will show how the results are related to brane supersymmetry breaking using an anti-D3-brane.