Central Singularity of Three-Dimensional Kerr-de Sitter Black HolesFor three-dimensional Kerr-de Sitter space-time, we find the singular energy-momentum and spin tensor sources that generate the non-trivial geometry. The energy-momentum tensor is symmetric,…Mauro Carlone, Wolfgang Mück·Oct 29, 2025SaveLearn
Complex Saddles of Charged-AdS Gravitational partition functionIn this paper, we consider the Euclidean partition function of uncharged and charged AdSd+1 black hole geometries in canonical and grand canonical ensemble for d≥3. It is seen that the…Manishankar Ailiga, Shubhashis Mallik, Gaurav Narain·Oct 29, 2025SaveLearn
Group Representations of Lorentz Transformations Extended to Superluminal ObserversWe construct an extension of the proper orthochronous Lorentz group that includes space-time transformations for observers moving with superluminal relative velocities in arbitrary direction. This…Marco Zaopo·Oct 29, 2025SaveLearn
Interface line operators in N=4 SYM theories and supersymmetric indicesWe study configurations of two N=4 super Yang-Mills theories of unitary gauge groups connected by the BPS interfaces involving line operators. We find strong evidence of S-duality of the…Yasuyuki Hatsuda, Tadashi Okazaki·Oct 29, 2025SaveLearn
Constraints on the resolution of spacetime singularitiesWhat happens at spacetime singularities is poorly understood. The Penrose-Wall singularity theorem constrains possible scenarios, but until recently its key assumption--the generalized second law…Arvin Shahbazi-Moghaddam·Oct 29, 2025SaveLearn
Hadamard tails from flat-space perturbation theoryThe short-distance singular structure of the two-point function of a free scalar field in curved spacetime has a universal behavior that characterizes well-behaved states (called Hadamard states).…Ameya Chavda, Alberto Nicolis, Alessandro Podo et al.·Oct 29, 2025SaveLearn
λϕ4 as an Effective Theory in de SitterEffective field theories (EFTs) provide a powerful framework to parametrise unknown aspects of possible ultraviolet (UV) physics. For scalar fields in de Sitter space, however, new emergent phenomena…Sebastian Cespedes, Zhehan Qin, Dong-Gang Wang·Oct 29, 2025SaveLearn
The Geometry of BCFW for ABJM Loop IntegrandsIn this paper we investigate the loop-level geometry of ABJM theory from the perspective of lightcone geometries in dual space. This geometry admits a natural fibration, where one of the loop…Livia Ferro, Ross Glew, Tomasz Lukowski et al.·Oct 29, 2025SaveLearn
Hodge Structures of Complex Multiplication Type from Rational Conformal Field TheoriesUnder certain assumptions, we show that unitary rational N=(2,2) conformal field theories together with a certain generating set of Cardy boundary states in the associated boundary…Hans Jockers, Pyry Kuusela, Maik Sarve·Oct 29, 2025SaveLearn
Conformal Blocks in 2d Carrollian/Galilean CFTs and Excited State Entanglement EntropyWe advance the study of flat space holography by computing the entanglement entropy of highly excited states in two-dimensional Carrollian/Galilean Conformal Field Theories (C/G CFTs). Our approach…Peng-Xiang Hao, Shunta Takahashi·Oct 29, 2025SaveLearn
Matter Sourced Bubble Nucleation in the Asymmetron Scalar-Tensor TheoryWe investigate how matter density distributions affect thin-wall bubble formation in the asymmetron mechanism, a scalar-tensor theory with a universal coupling to matter and explicit…Usama Syed Aqeel, Clare Burrage, Oliver Gould et al.·Oct 29, 2025SaveLearn
NLIE formulations for the generalized Gibbs ensemble in the sine-Gordon modelIn this paper we propose two sets of nonlinear integral equations (NLIE) for describing the thermodynamics in the sine-Gordon model, when higher Lorentz spin conserved charges are also coupled to the…Arpad Hegedus·Oct 29, 2025SaveLearn
Non-Commutative Geometry for D-Branes in Large R-R Field BackgroundWe examine the role of non-commutative geometry in Dp-branes within large R-R field backgrounds. In this context, the background of a significant (p-1)-form R-R field can be effectively described…Chen-Te Ma·Oct 28, 2025SaveLearn
Covariance of Scattering Amplitudes from Counting CarefullyInvariance of on-shell scattering amplitudes under field redefinitions is a well known property in field theory that corresponds to covariance of on-shell amputated connected functions. In recent…Mohammad Alminawi·Oct 28, 2025SaveLearn
Large-N Free Energy of Chiral N=2 Chern-Simons-Matter TheoriesWe present the first successful large-N computation of the S3 free energy in chiral N=2 Chern-Simons-matter theories, long believed to evade the universal M2-brane scaling…Seyed Morteza Hosseini·Oct 28, 2025SaveLearn
Gravitational dressing: from the crossed product to more general algebraic and mathematical structureThe crossed product, and consequent transition from von Neumann algebras of type III to II, is recovered from a truncation of more general gravitational dressing constructions, about certain…Steven B. Giddings·Oct 28, 2025SaveLearn
On the Field Excursion BoundIn a recent work, Herderschee and Wall (HW) proved a bound on scalar field excursions in spatially flat FRW cosmologies. In this note, we give an alternate proof of their bound using the Friedmann…Tom Rudelius·Oct 28, 2025SaveLearn
Surprising one-loop finiteness of 6D half-maximal supergravitiesIn four dimensions, it has long been established that gravity coupled to matter exhibits ultraviolet divergences at one loop, irrespective of supersymmetry. Notably, the four-matter one-loop…Yu-tin Huang, Henrik Johansson, Michele Santagata et al.·Oct 28, 2025SaveLearn
From Quantum Relative Entropy to the Semiclassical Einstein EquationsWe provide arguments indicating that the semiclassical Einstein equations follow from quantum relative entropy and its proportionality to an area variation. Using modular theory, we establish that…Philipp Dorau, Albert Much·Oct 28, 2025SaveLearn
Penrose limits and TsT for fibered I-branesIn this paper we analyze a generalized "single-trace T T" deformation, defined by a TsT transformation, of the fibered I-brane solution from Nunez2023. We use the Penrose limit…Marcelo R. Barbosa, Horatiu Nastase, Lucas S. Sousa·Oct 28, 2025SaveLearn
Quasi-Characters for three-character Rational Conformal Field TheoriesWe revisit (3,0) and (3,3) admissible solutions obtained using the MLDE method. We show that all (3,0) solutions can be written in terms of a universal formula involving the 3F2…Suresh Govindarajan, Akhila Sadanandan, Jagannath Santara·Oct 28, 2025SaveLearn
Islands in Kerr-Newman Black HolesWe investigate the information paradox in the four-dimensional Kerr-Newman black hole by employing the recently proposed island paradigm. We first consider the quantum field in the four-dimensional…Ming-Hui Yu, Xian-Hui Ge·Oct 28, 2025SaveLearn
Revisiting zero modes and cluster decomposition at the late-time boundary of de SitterWe revisit the literature on locality on de Sitter with the goal to organize the main results with respect to the representation theory of the isometry group of four dimensional de Sitter. We make…Murat Onem, Gizem Sengor·Oct 28, 2025SaveLearn
The Weight of Spin(32)/Z2 Little Strings: T-duality and Hasse DiagramsWe study the worldvolume theories of stacks of Spin(32)/Z2 heterotic NS5-branes probing a transverse singularity g. We revisit and extend the original classification by Blum…Hamza Ahmed, Florent Baume, Paul-Konstantin Oehlmann·Oct 28, 2025SaveLearn
Bounds on CFT correlations from the thermal partition functionWe discuss upper bounds on the mutual information for disjoint spherical regions of the CFT vacuum. To prove our bounds, we utilize the modular nuclearity condition, which is in turn related to…Fikret Ceyhan, Thomas Faulkner·Oct 28, 2025SaveLearn