KPolaris: GPU-accelerated Polarized Radiative Transfer in General Relativity

arXiv:2609.26298 · astro-ph.HE, gr-qc · Submitted 2026-09-22 · Read on arXiv

astro-ph.HE, gr-qc

Submitted: 2026-09-22

Updated: 2026-09-22

Comments: 15 pages, 4 figures, 8 tables

Code: https://github.com/zelinzh/KPolaris

License: http://creativecommons.org/licenses/by/4.0/

The gist: Polarized black-hole images carry information about both the magnetized plasma and the curved spacetime through which the radiation propagates.

Terminology

Abstract

Polarized black-hole images carry information about both the magnetized plasma and the curved spacetime through which the radiation propagates. We present KPolaris, an open-source GPU-accelerated general-relativistic polarized radiative-transfer code built on the Kokkos framework. It supports analytic plasma models and GRMHD simulation data, with both fast-light and slow-light radiative transfer. The code also provides diagnostics that connect image structure to the emitting plasma and to propagation effects along the rays. These include emissivity-weighted plasma maps, emission contributions from selected regions, selected-ray histories, and sensitivities of the Stokes parameters to plasma parameters. Numerical convergence tests and comparisons with an independent radiative-transfer code assess the accuracy of the calculations. GPU acceleration reduces the computational cost of image generation, facilitating multi-frequency and time-dependent studies of polarized black-hole images.

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