Search arXiv⌕ Search

arXiv · 2610.27420

Pfaffian solutions to the Ernst equation

Abstract

We show that the Yamazaki-Hori solution to the Ernst equation can be represented in the Pfaffian form. We also discuss the consequences of this result for Nakamura's conjecture on the relation between the Ernst equation and the 2D Toda model.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Arsen Melikyan, Aleksandr Pinzul. 2026-10-20. Pfaffian solutions to the Ernst equation. https://arxiv.org/abs/2610.27420

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

The JLMS formula in a large code with approximate error correction

Gauge/gravity duality is often described as a quantum error correcting code. However, as seen in the Jafferis-Lewkowycz-Maldacena-Suh (JLMS) formula, exact quantum error correction with complementary recovery (and thus entanglement wedge reconstruction) emerges only in the limit $G \to 0$. As a result, precise arguments controlling error terms have focused on what we call `small' codes which, as $G \to 0$, describe only perturbative excitations near a given classical solution. Such settings are quite restrictive and, in particular, they prohibit discussion of any modular flow that would change the classical background. As a result, they forbid consideration of modular flows generated by semiclassical bulk states at order-one modular parameters. In contrast, we present a single `large' code for the bulk theory that can accommodate such flows and, in particular, in the $G \to 0$ limit includes superpositions of states associated with distinct classical backgrounds. This large code is assembled from small codes that each satisfy an approximate Faulkner-Lewkowycz-Maldacena formula. In this extended setting we clarify the meaning of the (approximate) JLMS relation between bulk and boundary modular Hamiltonians and quantify its validity in an appropriate class of states.

hep-th↗

Magic and Wormholes in the Sachdev-Ye-Kitaev Model

Any quantum state is fully specified by the expectation values of a complete set of Hermitian operators. For a system of Majorana fermions, such as the Sachdev-Ye-Kitaev (SYK) model, this set of observables can be taken to be all possible strings of Majorana fermion operators. The expectation values of these fermion strings in a thermal state depend erratically on the microscopic couplings that specify the SYK Hamiltonian, and we study their statistical properties directly in the thermodynamic limit using path integral techniques. When the underlying SYK Hamiltonian is chaotic, we find that these expectation values are well-modeled as real Gaussian random variables with zero mean and a variance that we compute. In contrast, for the integrable variant of SYK, we find that the expectation values are actually non-Gaussian. We then use these results to study measures of magic in the SYK thermal state, including the robustness of magic and the stabilizer Rényi entropy. We also show that our results can be quantitatively reproduced with a dual gravity calculation in the chaotic case at sufficiently low temperature. In this dual gravity model the variance of a given microscopic operator string is related to a wormhole geometry stabilized by a massive particle which is dual to the operator string. Our results thus provide a concrete and quantitative setting in which to study the relationship between randomness, wormholes and closed universes, as well as a holographic dual of quantum magic.

hep-th↗

Holographic Reconstruction from Broken Conformal Gauge Symmetry

We investigate bulk--boundary structures in $\AdS_4/\CFT_3$ from the viewpoint of gravity as a broken phase of conformal gauge symmetry. A crucial distinction is made between the Euler and Pontryagin characteristic classes. The gauge-theoretic gravitational action contains an Euler sector, whose total-derivative representation gives a boundary form depending on both intrinsic and extrinsic geometry. This structure is different from the Pontryagin descent to the three-dimensional gravitational Chern--Simons functional, whose metric variation gives the Cotton tensor and underlies the mixed boundary conditions studied by de Haro. We perform a Fefferman--Graham expansion of the Euler boundary form in asymptotically $\AdS_4$ spacetime. The normalizable coefficient $g_{(3)ij}$ does not contribute linearly to the finite Euler boundary term: its contribution from the cubic extrinsic- curvature sector vanishes by $\mathrm{Tr}\,g_{(3)}=0$, while curvature-- extrinsic-curvature terms containing $g_{(3)}$ vanish at the conformal boundary. A direct Codazzi analysis additionally shows that the Cotton tensor appears in the asymptotic mixed curvature but its contribution through the tangential-connection boundary variation vanishes for standard Dirichlet data. This indicates two distinct types of bulk--boundary structure: a global/topological Euler relation and a local Pontryagin--Cotton relation. We distinguish this kinematic Cotton appearance from a finite Cotton boundary response and discuss the implications for holographic reconstruction.

hep-th↗