h/2e Flux Trapping without SuperconductivityRecently, it was shown by Komargodski and Popov [arXiv:2601.09847] that ordinary metals threaded with an Aharonov-Bohm solenoid exclusively trap either 0 or h/2e flux. The latter value is familiar in…Will Lancer·Oct 29, 2026SaveLearn
Facets of Gravity: A journey exploring spacetime from Planckian to cosmological scalesWhat does it mean to quantize gravity, and what can a quantum theory of spacetime actually predict? This thesis explores these questions through complementary non-perturbative approaches, from the…Agustín Silva·Oct 29, 2026SaveLearn
Hilbert space in the flat limit of AdS/CFT. II. Massless particlesBuilding on Part I of this series, where we described the emergence of massive scattering states, we demonstrate how unitary lowest-weight representations D(Δ,s) of the conformal group…Kevin Nguyen·Oct 29, 2026SaveLearn
Proof of the entropic c-theoremWe prove an entropic c-theorem in two dimensions by constructing a c-function from the mutual information between spacelike separated wedges, defined through the relative entropy. The proof…Jonah Kudler-Flam·Oct 29, 2026SaveLearn
All Symmetries and Boundaries of the Two-Dimensional Free Scalar from Continuous Flat-GaugingWe propose a remote detectability criterion for two-dimensional conformal field theories, which asserts that any local operator outside of the product of the left- and right-moving Virasoro algebras…Yichul Choi, Ho Tat Lam, Brandon C. Rayhaun·Oct 29, 2026SaveLearn
Umbilic ObservatoriesWe study gravitational dynamics for the simplest example of an umbilic boundary in four-dimensional general relativity --- a three-dimensional de Sitter hypersurface embedded in a four-dimensional…Dionysios Anninos, Raúl Arias, Damián A Galante·Oct 29, 2026SaveLearn
Monopole-Fermion Scattering from Twisted Conformal Boundary StatesWe derive monopole-fermion scattering correlators from conformal boundary states in twisted sectors. The key ingredient is that symmetry-preserving boundary conditions contain sectors twisted by…Clay Córdova, Diego García-Sepúlveda, Lian-Tao Wang et al.·Oct 29, 2026SaveLearn
Conformal boundaries and the photon sphere of AdS black holesWe study linearized gravitational perturbations of four-dimensional Schwarzschild-AdS black holes with finite timelike boundaries subject to conformal boundary conditions. These fix the conformal…Raúl Arias, Valentino Di Pierro, Silvia Georgescu·Oct 29, 2026SaveLearn
On Boundary State Screening via SolitonsWe present a coarse classification scheme for the boundary data of massive QFTs based on transitions of boundary states via soliton / kink profiles. Starting from the lattice of boundary states, we…Vivek Chakrabhavi, Babak Haghighat, Jonathan J. Heckman·Oct 29, 2026SaveLearn
Giant Gravitons in AdS5×SE5 and the Superconformal Index of Toric Quiver Gauge TheoriesWe derive giant-graviton contributions to superconformal indices by quantizing probe D3-branes in type IIB backgrounds AdS5× SE5. For SE5=T1,1 and Yp,q, we…Evan Deddo, Sabarenath Jayaprakash, James T. Liu et al.·Oct 29, 2026SaveLearn
DiscKosky: Efficient Genealogical Constraints from Sector-By-Sector Critical Point CountingWe present DiscKosky, a new Mathematica package for efficiently generating genealogical constraints on the sequential discontinuities of Feynman integrals. DiscKosky works by tracking the solutions…Giulio Crisanti, Luke Lippstreu, Andrew J. McLeod et al.·Oct 29, 2026SaveLearn
The running of Weyl gauged gravity: asymptotic freedom, its obstruction, and a way outWe compute the one-loop beta functions of quadratic gravity in Weyl conformal geometry, the gauge theory of diffeomorphisms and dilatations with a dynamical Weyl gauge boson. The divergences are…Diego Buccio, Fabrizio Chicconi, Luca Parente et al.·Oct 29, 2026SaveLearn
Guaranteed Slater Conditions for the Numerical Conformal Bootstrap: Fixing Instabilities in SDPB, Navigator Methods, and SkydivingThe semidefinite programs (SDPs) of the numerical conformal bootstrap, and of S-matrix and quantum-mechanics bootstraps, are solved with primal-dual interior-point methods whose convergence…Marten Reehorst·Oct 29, 2026SaveLearn
Quantum Cosmology at the CuspIn top-down quantum gravity constructions, saxionic directions typically lead to cusps in moduli space, where the scalar potential and the axion decay constant asymptotically behave as $V…Luis A. Anchordoqui, Alek Bedroya, Muldrow Etheredge et al.·Oct 29, 2026SaveLearn
On Geometric Observables in GravityMeasures of geometry like distance and time are staples of classical gravity. While geometric quantities arise broadly in quantum gravity, their graviton corrections are less explored. In this paper,…Manthos Karydas, Murat Kologlu, Allic Sivaramakrishnan·Oct 29, 2026SaveLearn
Thermodynamics of Swirling Black Holes and Kerr-Taub-NUTWe establish the first law of black hole thermodynamics for the recently discovered Kerr swirling (KS) and accelerated Kerr swirling (AKS) black hole solutions. We also revisit the first law for the…Ernesto Frodden, Diego Hidalgo, Francisco Manzano·Oct 29, 2026SaveLearn
Localization in Seven-Dimensional SupergravitySeven-dimensional supergravity provides holographic access to strongly coupled six-dimensional superconformal theories through its highest-dimensional supersymmetric AdS vacua. Its unique…Florian Gaar, Michèle Levi·Oct 29, 2026SaveLearn
Generalised Ω-backgrounds in twisted N=4 super Yang-MillsWe introduce rigid supergravity backgrounds for 4d N=4 super Yang-Mills which deform its topological twists and generalise the Ω-deformation of N=2 gauge theories. We derive…Elisa Iris Marieni, Itamar Yaakov·Oct 29, 2026SaveLearn
Gravity between two masses beyond Newton's lawNewton's law of universal gravitation describes the attraction between two masses through an inverse-distance potential. In Einstein's theory gravity gravitates: each mass reshapes the…Zhengwen Liu, Xing-Bo Yuan·Oct 29, 2026SaveLearn
A Simplified Born Rule for Cosmological CorrelatorsCosmological correlators are natural observables of the primordial universe and are related to wavefunction coefficients by the Born rule. For equal-time in-in correlators in flat spacetime, we prove…Fan Zhu·Oct 29, 2026SaveLearn
Holographic duals of JT gravity at finite cutoff: the classical caseWe formulate JT gravity with finite-cutoff boundaries and end-of-the-world branes in the first-order BF formulation. We dynamically reduce the BF model into a one-dimensional system living at the…Andreas Belaey, Thomas G. Mertens, Lorenzo Russo et al.·Oct 29, 2026SaveLearn
Breaking of integrability in elliptic deformations of AdS3 strings with mixed fluxWe construct elliptic deformations of the AdS3 × S3 × T4 superstring supported by mixed NSNS and RR fluxes in type IIB supergravity and investigate their integrability. The NSNS sector…Ian Le Meur, Fiona K. Seibold·Oct 29, 2026SaveLearn
Exact holographic superfluid at the Bogomolny point: transport, large charge, and Rényi entropiesThe Abelian Higgs model in AdS5, in the probe limit, is a standard holographic model of a strongly coupled superfluid, usually solved numerically. When the scalar mass saturates the…Siqing Yu·Oct 29, 2026SaveLearn
Bounds on the Diagonal Degree of the Biadjoint Scalar Amplitude MatrixBiadjoint scalar theory partial amplitudes, mn(α,β), define an (n-1)!/2× (n-1)!/2 matrix, Mn, with rows and columns labeled by orderings. The CHY construction of Mn implies that its…Freddy Cachazo, Rajbir Longia·Oct 29, 2026SaveLearn
N=2 conformal higher-spin actions in harmonic superspaceWe construct linearized 4D, N=2 Weyl-type off-shell actions in harmonic superspace for the superconformal higher-spin gauge multiplets introduced in arXiv:2404.19016. This work is a…Evgeny Ivanov, Nikita Zaigraev·Oct 29, 2026SaveLearn