The negativity core of a 1+1D massless scalar quantum fieldVacuum entanglement is a fundamental feature of quantum field theory exhibiting rich structure that is not completely understood. Here, we provide a complete characterization of the entanglement…Jason Pye, Atharva Hingane, Robert H. Jonsson·May 22, 2026SaveLearn
Compact structures in impurity-doped vacuumless systemsWe investigate novel structures which arise from the compactification of vacuumless kinks in scalar field models coupled to impurities that preserve half the BPS sectors, described by first-order…I. Andrade, D. Bazeia, M. A. Marques et al.·May 22, 2026SaveLearn
Brane-probes response to poly-vector deformationsWe probe poly-vector deformations of Type II backgrounds using the fundamental string, D0-brane and D3-brane, and of the 11D membrane background by the fundamental M2-brane. We show that the…Sergei Barakin, Angelina Kurenkova, Edvard T. Musaev·May 22, 2026SaveLearn
Counting Degrees of Freedom in Open Effective TheoriesOpen effective field theories provide a systematic framework for describing physical systems interacting with an environment whose microscopic details are unknown, unobservable, or uncalculable. A…Enrica Lausdei, Enrico Pajer·May 22, 2026SaveLearn
The Smarr Formula is Gauss's Law: A Kerr-Schild Single-Copy PerspectiveIn the Kerr-Schild double copy, static and spherically symmetric black hole solutions of general relativity are mapped to purely electric solutions of Maxwell's theory in flat spacetime. We…Gokhan Alkac·May 22, 2026SaveLearn
Schwinger-Keldysh Path Integral for Gauge theoriesWe develop the Schwinger-Keldysh path-integral formalism for open non-Abelian gauge theories that are gauge-fixed via the BRST method in covariant gauges. We focus on generic initial states, pure and…Greg Kaplanek, Maria Mylova, Andrew J. Tolley·May 22, 2026SaveLearn
Lecture Notes on Symmetry Reduction via the Dressing Field MethodThese notes - prepared for the conference school "Foundations of General-Relativistic Gauge Field Theory", held on March 17-19, 2026 at the Politecnico di Torino - present introductory…L. Ravera·May 22, 2026SaveLearn
Circular strings, magnons, plane waves and local quenches in BTZWe show that string theory on the geometry BTZ× S3× M supported with either Neveu-Schwarz flux or Ramond flux admits states which obey identical dispersion relations to those of…Justin R. David, Rahul Metya·May 22, 2026SaveLearn
Note on higher spins and holographic symmetry algebraIn this paper we discuss a higher spin extension of the holographic symmetry algebra for graviton and gluon. Our primary observation is that in the presence of higher spin particles the soft symmetry…Shamik Banerjee, Suman Guchait, Raju Mandal et al.·May 22, 2026SaveLearn
Central Charges and Vacuum Moduli of 2d N=(0,4) Theories from Class SWe investigate 2d N=(0,4) supersymmetric theories obtained from a topologically-twisted reduction of 4d N=2 class S theories on a Riemann surface. This study…Wei Cui, Junkang Huang, Zi-Xiao Huang et al.·May 22, 2026SaveLearn
Quantum Oscillons are Long-LivedAs the longest lived transient, oscillons play a critical role in classical field theory simulations of many phenomena. However, beyond the classical approximation, it is well-known that quantum…Jarah Evslin, Katarzyna Slawińska, Tomasz Romańczukiewicz et al.·May 22, 2026SaveLearn
Gauging Open EFTs from the top downWe present explicit top-down calculations of Open EFTs for gauged degrees of freedom with a focus on the effects of gauge fixing. Starting from the in-in contour with two copies of the action, we…Greg Kaplanek, Maria Mylova, Andrew J. Tolley·May 22, 2026SaveLearn
Klein Bottle CosmologyWe explore a higher-dimensional universe that is a product of Minkowski space and the nonorientable Klein bottle. The topology explicitly breaks important symmetries, such as translational invariance…Brian Greene, Daniel Kabat, Janna Levin et al.·May 22, 2026SaveLearn
Effective density matrix for vacua in asymptotically flat gravityWe explicitly construct the density matrix associated to the vacuum state of a large spherically symmetric causal diamond of area A in four-dimensional asymptotically flat gravity. We achieve this…Temple He, Prahar Mitra, Kathryn M. Zurek·May 22, 2026SaveLearn
Evaporating universesRecent work by Headrick, Sasieta and myself provides an extension of the HRT formula for asymptotically flat spacetimes. I use this formula to construct a holographic model of black hole evaporation…Divij Gupta·May 22, 2026SaveLearn
Anatomy of the simplest renormalonPerhaps the simplest IR renormalon occurs in the ground state energy of a superrenormalizable model, the scalar O(N) theory in two dimensions with a quartic potential and negative squared mass. We…Marcos Marino·May 22, 2026SaveLearn
Proca-type Hair of Rotating Black Holes in Higher DimensionsWe show that spacetime symmetries on any background give rise to stealth vector fields obeying Proca-type equations supplemented by curvature terms. This observation, which is true for solutions of…David Kubiznak, Robert B. Mann, Marek Milička·May 21, 2026SaveLearn
Thermal effects and finite-temperature cosmology in perturbatively stabilized large volume scenariosWe analyze finite-temperature effects in the perturbative Large Volume Scenario (LVS), examining the dynamics of thermalized Kähler moduli and the stability of thermally induced vacua. We determine…Vasileios Basiouris·May 21, 2026SaveLearn
Cuspidal Singularities in Collapsing Domain WallsDomain wall networks have attracted renewed interest, particularly in relation to the dynamics of network collapse. Accurately describing this process is challenging and typically requires large…Jose J. Blanco-Pillado, Matthew Elley, Francesc Ferrer et al.·May 21, 2026SaveLearn
Sharpening the Supersymmetric Axion Weak Gravity ConjectureThe Axion Weak Gravity Conjecture provides one of the most effective quantum gravity tools for constraining particle physics and cosmology, but it has long been thought of as a slightly fuzzy…Muldrow Etheredge, Matthew Reece, Tom Rudelius et al.·May 21, 2026SaveLearn
Bottom-up open EFT for non-Abelian gauge theory with dynamical color environmentWe develop a bottom-up open effective field theory (EFT) for non-Abelian gauge theories within the Schwinger--Keldysh formalism. Instead of integrating out the environment completely and starting…Yoshihiko Abe, Kanji Nishii·May 21, 2026SaveLearn
Shading A-polynomials via huge representations of Uq(suN)Classical A-polynomials A(,m) define constraints on coordinates and m in SL(2,C) (a complexification of SU(2)) character varieties associated to knot complements…Dmitry Galakhov, Alexei Morozov·May 21, 2026SaveLearn
Entanglement viscosity to entropy density ratio for spin-3/2 theoryIt is known that the Minkowski vacuum appears as a thermal medium to an accelerated observer due to the renowned Unruh effect. More recently, it has been shown that at least for lower-spin fields…R. V. Khakimov, G. Yu. Prokhorov, O. V. Teryaev·May 21, 2026SaveLearn
New mechanism for fermion localization in f(T,TG)-braneWe investigate the localization of fermionic fields in a five-dimensional braneworld scenario within the framework of modified teleparallel gravity described by a general f(T,TG) function.…Allan R. P. Moreira, Fernando M. Belchior, Guo-Hua Sun et al.·May 21, 2026SaveLearn
Closed String Field Theory in 25.99 DimensionsWe return to and refine Zwiebach's formulation of closed string field theory (CSFT) built around non-critical backgrounds [1,2], restricting our attention to genus zero. The structure involves a…Amr Ahmadain, Alexander Frenkel, Xi Yin·May 21, 2026SaveLearn