Supergravity 2025

Europe/Zurich
Turin

Turin

The address of the venue is: Via Nizza, 230, 10126 Torino TO
Anna Ceresole (INFN TORINO), Carlo Angelantonj (Turin University), Domenico Orlando (INFN TO), Laura Andrianopoli (Politecnico di Torino), Leonardo Castellani (UPO), Lucrezia Ravera (Politecnico), Mario Trigiante (Politecnico di Torino), Pietro Grassi (Universita del Piemonte Orientale (IT))
Description

 

Supergravity 2025 is the 6th edition in a series of workshops held biannually since 2015, where experts in supergravity and superstring theories gather to present their latest results and foster scientific collaboration. 

For information on the previous editions:

Supergravity 2023, Supergravity 2022, Supergravity 2019, Supergravity 2017, Supergravity 2015

The main topics covered in the present edition will include the gauge/gravity holographic correspondence and supergravity solutions to superstring and M-theory dynamics.

 

The present edition of the meeting will include extra talks by some of the main contributors to the construction of the theory, to celebrate the incoming 50th birthday of supergravity.

Invited Speakers

Erik Bergshoeff (Groningen Unv.) 
 

Nicolay Bobev (KU Leuven)

 Gianguido Dall’Agata (University of Padua)

Pietro Fré (Turin Univ.) 

Jerome Gauntlett (Imperial College London)

Adolfo Guarino (University of Oviedo)

Olaf Hohm (Humboldt University of Berlin)

Chris Hull (Imperial College London)

Bernard Julia (École Normale Supérieure)

Yolanda Lozano (University of Oviedo)

Carlos Nunez (Swansea University)

Jan Rosseel (Ruđer Bošković Institute)

Augusto Sagnotti (Scuola Normale Superiore di Pisa)

Henning Samtleben (ENS de Lyon)

Chiara Toldo (Harvard University)

Alessandro Tomasiello (University of Milano-Bicocca)

Stefan Vandoren (Utrecht University)

Antoine Van Proeyen (KU Leuven)

THE REGISTRATION DEADLINE WAS July 31st, 2025. 

Organizers

Laura Andrianopoli, Carlo Angelantonj, Leonardo Castellani, Anna Ceresole, Pietro Antonio Grassi, Ruggero Noris, Domenico Orlando, Lucrezia Ravera, Mario Trigiante

   

Participants
    • 09:00 09:25
      Registration 25m
    • 09:25 09:30
      Welcome 5m
    • 09:30 10:20
      Non-relativistic p-brane limits of supergravity 50m

      I will discuss so-called non-relativistic p-brane limits of (the bosonic part)
      of supergravity in diverse dimensions that lead to a generalized Newton-Cartan gravity
      with a Newton potential that satisfies a Poisson equation in the directions transverse to
      thep-brane. Iwilldiscussafewgeneralizationsthatmakecontactwithboth(thebosonic
      part of) eleven-dimensional supergravity and ten-dimensional heterotic supergravity.

      Speaker: Bergshoeff
    • 10:20 10:50
      Break with Coffee 30m
    • 10:50 11:40
      E8 families from exceptional invariants to Painlevé magics via supergravities 50m
      Speaker: Julia
    • 11:40 12:30
      N=2 Supergravity and the Swampland 50m

      We discuss N=2 supergravity theories in four dimensions and connect it with
      the swampland program and the distance conjectures. Examples with both vector mul-
      tiplets and hypermultiplets will be discussed. An interesting new class of models arises
      from freely acting orbifolds in string theory.

      Speaker: Vandoren
    • 12:30 14:00
      Lunch 1h 30m
    • 14:00 14:50
      The surprising structure of non-relativistic 11D supergravity 50m

      In this talk, I will outline the construction of a non-relativistic limit of 11-
      dimensional supergravity that leads to a theory with an underlying membrane Newton-
      Cartan geometry. I will argue that consistency of the non-relativistic limit requires the
      imposition of constraints, requiring that certain bosonic and fermionic torsions and cur-
      vatures vanish. I will show that in one version of these constraints only 16 supersymme-
      try transformations are kept, leading to a simple constraint structure in which however
      the supersymmetry algebra does not close into diffeomorphisms. Keeping all 32 su-
      persymmetry transformations requires a complicated sequence of bosonic and fermionic
      constraints, eventually involving three derivatives of bosonic fields. Finally, I will dis-
      cuss a family of supersymmetric solutions that satisfy all constraints and that contains
      a non-relativistic limit of the M2 supergravity solution that was obtained by Lambert
      and Smith as a background relevant for non-relativistic holography

      Speaker: Rosseel
    • 14:50 15:40
      Aspects of gauge-strings duality 50m

      I will discuss recent progress in the duality between gauge fields and strings,
      with an emphasis on the Supergravity side of things. The material is taken from the
      papers I wrote in the last year. I hope to make the presentation accessible to members
      of the audience with different technical expertise.

      Speaker: Nunez
    • 15:40 16:10
      Break with Tea 30m
    • 16:10 18:00
      Gong Show and Poster Session 1h 50m
    • 09:30 10:20
      Surprises from Non-Supersymmetric Strings 50m
      Speaker: Sagnotti
    • 10:20 10:50
      Coffee at the break 30m
    • 10:50 11:40
      AdS3/CFT2 and defect CFTs 50m

      I will discuss recent interpretations of AdS3 solutions as holographic duals
      of surface defect CFTs. One solution will be interpreted as an extension of ABJM
      to the massive case, in which one of the external directions becomes an energy scale
      and generates a flow towards an AdS3 space. A second solution will be related to
      surface defects embedded in 6d (1,0) CFTs living in D6-NS5-D8 brane intersections.
      In this second example we will find an interesting connection with the phenomenon of
      deconstruction.

      Speaker: Lozano
    • 11:40 12:30
      Thermodynamics of near-extreme rotating black holes 50m

      From the perspective of classical gravity, a black hole is the simplest object
      we know of. At the same time, it possesses huge entropy, hinting at an incredibly com-
      plex microstructure: understanding this fact falls in the realm of quantum gravity. In
      this talk I will review recent results concerning the microscopics and the thermody-
      namics of near-extreme black holes in asymptotically flat and Anti-de Sitter space. In
      the first part, I will describe how recently developed techniques allow to compute the
      quantum corrections to the entropy of fast spinning Kerr black holes. I will show that
      the quantum-corrected near-extremal entropy exhibits 3/2logT behavior characteristic
      of the Schwarzian model, and predicts a lifting of the ground state degeneracy for the
      extremal Kerr black hole. In the second part, I will show the computation for the den-
      sity of states for fast spinning AdS4 black holes in theories of gauged supergravity. The
      solutions admit a supersymmetric limit: I will comment on the spectrum of near-BPS
      states and on the interpretation in terms of the dual 3d field theory.

      Speaker: Toldo
    • 12:30 14:00
      Lunch 1h 30m
    • 14:00 14:50
      On non-supersymmetric vacua in string theory 50m

      I will discuss new classes of supersymmetry-breaking AdS vacua in string
      theory. In the first part, using calibrations, I will obtain type II vacua that enjoy partial
      or total protection from decays mediated by D-brane bubbles. In the second, I will work
      in non-supersymmetric heterotic theory; I will outline a method to obtain solutions on
      G/H coset spaces, with H-valued gauge field, and describe several examples.

      Speaker: Tomasiello
    • 14:50 15:40
      Supergravity in one dimension 50m

      A particularly interesting corner of the holographic dualities is the corre-
      spondence between the backgrounds of Dp-branes and their non-conformal field theory
      duals. Extrapolating this correspondence to the extremal case of p=-1, suggests a holo-
      graphic duality for the IKKT matrix model. The dual D-instanton background is a
      half-supersymmetric BPS solution of Euclidean IIB supergravity. I describe the relevant
      maximallysupersymmetricone-dimensionalsupergravitytheoryaroundthisbackground
      and the match of its fields to the lowest BPS multiplet of gauge invariant operators of
      the IKKT model.

      Speaker: Samtleben
    • 15:40 16:10
      Tea and Coffee, this time 30m
    • 16:10 17:00
      Precision Holography for Dp-branes 50m
      Speaker: Bobev
    • 17:00 17:50
      Localization in Supergravity 50m

      Important BPS quantities, including central charges, black hole entropy and
      the on-shell action, can be computed for supersymmetric solutions of supergravity with-
      out ever solving the Einstein equations or the Killing spinor equations. Instead one
      exploits the fact that the solutions have a Killing vector and a set of equivariantly closed
      forms. This allows one to compute just by inputting some global data and utilising
      the Berligne-Verne-Atiyah-Bott localisation theorem. We explain the formalism and
      illustrate with some examples.

      Speaker: Gauntlett
    • 09:30 10:20
      Supergravities I and II and their (enhanced) dualities 50m

      Combinations of dimensional reduction and dualities will be discussed leading
      to type I and type II supergravities in D=4 and D=6 with maximal supersymmetry.
      The relations between the different types of supergravity are also connected to choices
      of gauge fixing for the representatives of the coset spaces. The preserved manifest global
      symmetries differ and this raises questions on gauge equivalence of these theories. (In
      collaboration with R. Kallosh and H. Samtleben).

      Speaker: Van Proeyen
    • 10:20 10:50
      Coffee, Tea, and Milk break 30m
    • 10:50 11:40
      Casimir energy and the stability of supergravity vacua 50m

      We discuss the perturbative stability of susy breaking Minkowski vacua in
      supergravity compactifications on Riemann-flat manifolds.

      Speaker: Dall'Agata
    • 11:40 12:30
      Supergravity from Superstring Field Theory 50m

      A new superstring field theory gives a background independent 2nd-quantised formulation of superstring theory. In particular, it gives a novel formulation of the supergravity action with a democratic action for the RR gauge fields. This involves some novel gravitational couplings and the geometry behind these will be discussed.

      Speaker: Hull
    • 12:30 14:00
      Lunch 1h 30m
    • 14:00 14:50
      Scale-separated AdS3 flux vacua of type IIB 50m

      The existence of AdS/CFT pairs with scale separation remains an open question, with no explicit examples known to date and doubts raised about their very possibility. In this talk, I will present the first examples of type IIB AdS3​ flux vacua that exhibit parametrically-controlled scale separation. Remarkably, these solutions come equipped with integer-valued conformal dimensions for the would-be dual CFT2 operators, making the task of identifying and understanding the corresponding CFT2s particularly compelling. I will also comment on the implications of our results in light of the Swampland program.

      Speaker: Guarino
    • 14:50 15:40
      Supergravity, String Theory and Homotopy Algebras 50m

      I give an overview of homotopy algebras such as L∞ algebras as a tool for su-
      pergravity and other theories. Possible applications include: i)a first-principle derivation
      of “double copy", which relates, for instance, N=4 super-Yang-Mills to N=8 supergrav-
      ity in D=4; ii) the use of homotopy transfer to transport the Kaluza-Klein spectrum of
      exceptional field theory or supergravity on AdS to its boundary; iii) as new foundations
      for quantum field theory via factorization algebras.

      Speaker: Hohm
    • 15:40 16:10
      Coffee, Tea, Milk and, some juice, too. 30m
    • 16:10 17:00
      From Supergravity to Machine Learning: a Mathematical Adventure 50m

      In this talk starting from a critical analysis of the existing Neural Networks we illustrate their geometrical reformulation that cures their original sin, namely the use of ad-hoc point-wise activation functions, that are contradictory with covariance and with the supposedly vector space structure of the hidden layers. Starting from first principles, namely the need of a distance function and homogeneity, we identify the hidden layers with non-compact symmetric spaces and show that their characterization as normal Alekseevsky Riemannian spaces is crucial. Non-linearity is provided by the exponential map from solvable Lie algebras to solvable Lie groups and the general form of the map between adjacent hidden layers is reduced to an isometric map, whose core is a solvable Lie algebra homomorphism (the true mathematical nature of the learnable weights) followed by a generic isometry of the next layer (the true mathematical nature of the bias vectors). The implications and the on going developments are briefly outlined.

      Speaker: Frè