A Unified Analytic Framework for Microlensing Caustics: Geode Solutions and Hyper--Catalan Signatures

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Autori principali: Berloff, Gleb, Berloff, Natalia G.
Natura: Preprint
Pubblicazione: 2025
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author Berloff, Gleb
Berloff, Natalia G.
author_facet Berloff, Gleb
Berloff, Natalia G.
contents We give a preparation-invariant analytic description of image formation near microlensing caustics. After a local Weierstrass preparation at any multiple image (order $d\ge2$), the lens mapping reduces to a single geode variable $m$ satisfying $m=U\,φ(m)$, where $U$ is a prepared source coordinate and $φ$ is an image-side kernel. The coefficients of $m(U)$ obey closed Hyper-Catalan (HC) recurrences, allowing termwise derivatives and truncation control from the characteristic system. We also use the same form for a short HC predictor-corrector: evaluate the series within its certified radius and apply a brief Newton polish near the boundary. We define an HC signature (first nonzero kernel coefficients) and an HC spectrum (branch points and analyticity radius $ρ_U$), which quantify sparsity, stiffness, and safe evaluation domains. The construction covers folds and cusps of any global degree. On a binary fold and cusp, an artificial decic with a resonant unit, and two triple-lens cusps of a challenging geometry, HC seeds plus a few Newton steps recover the exact images to machine precision within the certified domain and maintain continuity under continuation. The resulting single-series templates (with $(\mathrm{Sig}_R,ρ_U)$ metadata) are ready for photometric and astrometric modeling.
format Preprint
id arxiv_https___arxiv_org_abs_2511_15756
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle A Unified Analytic Framework for Microlensing Caustics: Geode Solutions and Hyper--Catalan Signatures
Berloff, Gleb
Berloff, Natalia G.
Instrumentation and Methods for Astrophysics
Astrophysics of Galaxies
We give a preparation-invariant analytic description of image formation near microlensing caustics. After a local Weierstrass preparation at any multiple image (order $d\ge2$), the lens mapping reduces to a single geode variable $m$ satisfying $m=U\,φ(m)$, where $U$ is a prepared source coordinate and $φ$ is an image-side kernel. The coefficients of $m(U)$ obey closed Hyper-Catalan (HC) recurrences, allowing termwise derivatives and truncation control from the characteristic system. We also use the same form for a short HC predictor-corrector: evaluate the series within its certified radius and apply a brief Newton polish near the boundary. We define an HC signature (first nonzero kernel coefficients) and an HC spectrum (branch points and analyticity radius $ρ_U$), which quantify sparsity, stiffness, and safe evaluation domains. The construction covers folds and cusps of any global degree. On a binary fold and cusp, an artificial decic with a resonant unit, and two triple-lens cusps of a challenging geometry, HC seeds plus a few Newton steps recover the exact images to machine precision within the certified domain and maintain continuity under continuation. The resulting single-series templates (with $(\mathrm{Sig}_R,ρ_U)$ metadata) are ready for photometric and astrometric modeling.
title A Unified Analytic Framework for Microlensing Caustics: Geode Solutions and Hyper--Catalan Signatures
topic Instrumentation and Methods for Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2511.15756