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Introducing APERTURE: A GPU-based General Relativistic Particle-in-Cell Simulation Framework

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arxiv 2503.04558 v1 pith:J6XSLOLL submitted 2025-03-06 astro-ph.HE

classification astro-ph.HE
keywords aperturecodeparticle-in-cellblackframeworkgeneralgpu-basedrelativistic
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Low-luminosity Active Galactic Nuclei (AGN) are believed to be surrounded by a collisionless, highly magnetized accretion flow. As a result, Particle-in-Cell simulations are the best tools to study the immediate vicinity of the event horizons of these supermassive black holes. We present a GPU-based general relativistic particle-in-cell (GRPIC) code framework called Aperture. Aperture is developed in C++, with compute kernels written in CUDA and HIP to take advantage of the massive acceleration modern GPUs enable. The code is organized in a fully modular way, allowing easy extensions to new physics problems. In this paper, we describe in detail the particle pusher, field solver, and charge-conserving current deposition algorithms employed in Aperture, and present test cases to validate their correctness. Then, we apply the code to study spark gaps and plasma injection in black hole magnetospheres. We find that the apparent location and time-evolution of the gap depend on the observer. Our results reconcile the previous conflicting findings from 1D and 2D simulations in the literature.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. FPIC: a new Particle-In-Cell code for stationary and axisymmetric black-hole spacetimes

    astro-ph.HE 2026-02 conditional novelty 6.0 of 10

    A new general-relativistic particle-in-cell code, FPIC, is validated on black-hole magnetosphere tests and reproduces the Blandford–Znajek power with a one-parameter fit.

  2. CUDA Assisted Swampland and Black Hole Thermodynamics

    hep-th 2025-08 unverdicted novelty 4.0 of 10

    Charged black holes in a Gauss-Bonnet-modified theory are claimed to become unstable when Q/M > 2√π, linking black hole thermodynamics to swampland constraints.

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