Anomalies and Parity-Violating Interactions: From Conformal to Thermal Field TheoryChiral and conformal anomalies are fundamental phenomena that span multiple disciplines, including high-energy physics, condensed matter theory and cosmology. These anomalies play a crucial role in…Stefano Lionetti·Dec 18, 2025SaveLearn
The Use of Torsion in Supergravity Uplifts and Covariant FractonsThe aim of this Thesis is twofold. On the one hand, we find the necessary and sufficient conditions for a maximally supersymmetric supergravity theory in 3D to be a solution of 11D supergravity (but…Davide Rovere·Dec 18, 2025SaveLearn
Shockwaves and Time Delays in Einstein-Maxwell Effective Field TheoryWe derive the shockwave metric in four-dimensional Einstein-Maxwell effective field theory (EFT) by performing an ultra-relativistic boost of the charged black hole solution accompanied by a…Christophe Grojean, Minyuan Jiang, Pham Ngoc Hoa Vuong·Dec 17, 2025SaveLearn
Unleash Q! Cohomology, Localization, and Interpolation in Parisi-Sourlas SupersymmetryParisi-Sourlas supersymmetric models are known to undergo dimensional reduction; that is, their physics is captured by models in two fewer dimensions. In this work, we revisit dimensional reduction,…Bruno Le Floch, Gela Patashuri, Emilio Trevisani·Dec 17, 2025SaveLearn
Lanczos Meets Orthogonal PolynomialsWe establish a direct correspondence between the Lanczos approach and the orthogonal polynomials approach in random matrix theory. In the large-N and continuum limits, the average Lanczos…Le-Chen Qu·Dec 17, 2025SaveLearn
On Positive Celestial Geometry: ABHY in the SkyCelestial amplitudes are multiple Mellin transforms w.r.t. conformal dimensions. For arbitrary multiplicity n of massless states in sufficiently high space--time dimension D we perform all Mellin…Jin Dong, Stephan Stieberger·Dec 17, 2025SaveLearn
Scalar, vector and tensor fields on dS3 with arbitrary sources: harmonic analysis and antipodal mapsThe scalar, vector and tensor spherical harmonics on three-dimensional de Sitter spacetime are defined and analyzed. Each harmonic defines two sets of asymptotic data on the two-sphere in the…Geoffrey Compère, Sébastien Robert·Dec 17, 2025SaveLearn
Confinement by Monopole Loops in Inhomogeneous Magnetic FieldWe show that a generalized Polyakov mechanism can lead to confinement at weak coupling in 3+1 dimensions when the theory is placed in a non-trivial, spatially varying magnetic field background.…Stefano Bolognesi·Dec 17, 2025SaveLearn
3d Chern--Simons matter theories from generalized Argyres--Douglas theoriesWe study 3d N=2 Chern--Simons matter theories describing the R-twisted S1-reduction of Argyres--Douglas theories of (AM-1,AN-1) type with gcd(M,N)=1, via a…Takahiro Nishinaka, Yutaka Yoshida·Dec 17, 2025SaveLearn
Thermal spectral function asymptotics and black hole singularity in holographyWe investigate the analytic structure of thermal spectral function of holographic CFTs, synthesizing recent developments into a set of observations about its asymptotics. Specifically, for a class of…Hewei Frederic Jia, Mukund Rangamani·Dec 17, 2025SaveLearn
Nonlinearly Realised Defect Symmetries and AnomaliesConformal defects -- extended objects in conformal field theories -- carry localised excitations inherited from symmetry currents, known as the displacements and tilts. They capture the linear…Nadav Drukker, Ziwen Kong, Petr Kravchuk·Dec 17, 2025SaveLearn
Charged black holes in the 1/N expansionWe study some implications of SU(N)× U(1) theories coupled to gravity in the large-N limit. We find that in theories with quarks transforming as q (N,1), black holes (BH) with…Georges Obied, Mario Reig·Dec 17, 2025SaveLearn
Quantum microstate counting from Brownian motion: from many-body systems to black holesWe introduce a new way to produce infinite families of bases of a quantum system's Hilbert space, as well as methods to find its dimension. These families are constructed via Brownian motions in…Enzo Bavaro, Javier M. Magan, Leandro Martinek·Dec 17, 2025SaveLearn
Revisiting the tensionless limit of pure-Ramond-Ramond AdS3/CFT2We revisit the numerical solution of the mirror TBA equations for pure--Ramond-Ramond strings on AdS3× S3× T4 in the tensionless limit. Our analysis uses the recently-proposed…Alberto Brollo, Dennis le Plat, Alessandro Sfondrini·Dec 17, 2025SaveLearn
Integrable models from 4d holomorphic BF theoryWe show how to construct 2d field theories with holomorphic integrability from defect setups in 4d holomorphic BF. In a simple example setup, we explicitly construct the 2d theory and perform an…Lewis T. Cole, Ben Hoare·Dec 17, 2025SaveLearn
Cosmology meets cluster algebraIn this paper we explore the mathematical properties of wavefunction coefficients in power-law FRW cosmologies, and establish their relation to cluster algebras. We focus on the particular…Mattia Capuano, Livia Ferro, Tomasz Lukowski et al.·Dec 16, 2025SaveLearn
Torsional Carroll GravityThe ultra-relativistic (Carrollian) regime of gravity has recently emerged as a fertile framework for exploring holography, non-Lorentzian symmetries, and geometric limit of General Relativity. In…P. Concha, N. Merino, L. Ravera et al.·Dec 16, 2025SaveLearn
A Compact Formula for Conserved Three-Point Tensor Structures in 4D CFTWe derive a compact analytic formula for a complete basis of conformally invariant tensor structures for three-point functions of conserved operators in arbitrary 4D Lorentz representations. The…Paul Heslop, Hector Puerta Ramisa·Dec 16, 2025SaveLearn
Cosmic Lockdown: When Decoherence Saves the Universe from TunnelingWe investigate how quantum decoherence influences the tunneling dynamics of quantum fields in cosmological spacetimes. Specifically, we study a scalar field in an asymmetric double-well potential…Robson Christie, Jaewoo Joo, Greg Kaplanek et al.·Dec 16, 2025SaveLearn
General Effective Theories of Black Holes in the Large D LimitWe derive the general form of the effective equations governing black hole dynamics in the limit of a large number of dimensions D. These split into a universal soap-bubble embedding…Roberto Emparan, Jordi Rafecas-Ventosa, Benson Way·Dec 16, 2025SaveLearn
Heisenberg-Euler and the Quantum DilogarithmA dispersion integral representation of the Heisenberg-Euler QED effective lagrangian is derived, with Faddeev's quantum dilogarithm as a generalized Borel kernel. The nonperturbative imaginary…Gerald V. Dunne·Dec 16, 2025SaveLearn
Exact formula for geometric quantum complexity of cosmological perturbationsNielsen's geometric approach offers a powerful framework for quantifying the complexity of unitary transformations. In this formulation, complexity is defined as the length of the minimal…Satyaki Chowdhury, Jakub Mielczarek·Dec 16, 2025SaveLearn
Quantizing non-projectable Hořava gravity with Lagrangian path integralWe formulate the quantum version of non-projectable Hořava gravity as a Lagrangian theory with a path integral in the configuration space with an ultra-local in time, but non-local in space,…D. Blas, F. Del Porro, M. Herrero-Valea et al.·Dec 16, 2025SaveLearn
Cluster algebras for cosmological correlatorsIn this paper, we explore the cluster algebras for symbol letters or singularities of cosmological correlators in a conformally coupled scalar field theory. We show that the symbol letters for…Pouria Mazloumi, Xiaofeng Xu·Dec 16, 2025SaveLearn
Holographic interpolations of defect CFTsWe propose a new class of holographic dualities between certain, generically non supersymmetric, defect conformal field theories (dCFTs) and their gravity duals. Our construction interpolates between…George Georgiou, Dimitrios Zoakos·Dec 16, 2025SaveLearn