High-Performance Computing for Astrophysical Simulations and Astroparticle Observations
摘要
Simulations in astrophysics play a crucial role in testing models and comparing them with observational data, for which High-Performance Computing has become indispensable for handling complex scenarios. In this paper, we present two important applications in astrophysical simulations. First, we explore the adaptation of the Pencil Code to study the evolution of magnetic field configurations in stratified stars. Second, we highlight the ARTI framework developed to estimate signals at the Latin American Giant Observatory. In addition, we discuss the importance of reproducibility in scientific analysis.