Work

Oscillatory Behaviors in General Relativistic Magnetohydrodynamical Simulations of Interacting Toroids

Year: 2025

Type: article

Abstract: Oscillatory behavior in the total flux emitted from both single and double torus structures was observed in our general relativistic magnetohydrodynamical simulations performed using the High-Accuracy Astrophysical Relativistic MHD code. These features became evident during a ray tracing conducted with the postprocessing tool IPOLE. Fast Fourier transform analysis of the resulting light curves revealed the presence of dominant frequency components. Two dominant frequencies are observed for interacting counterrotating tori, demonstrating a frequency ratio ∼3 : 2 that is generated during the most intensive interaction of the tori. For corotating tori, the situation is more complex. There are indications that increasing magnetic field intensity enlarges the number of observed oscillations.

Source: The Astrophysical Journal

DOI: 10.3847/1538-4357/ae1001

Authors: Dilshodbek Bardiev, Jan Schee, Zdeněk Stuchlík

Institution: Silesian University in Opava

Language: English

Topic: Astrophysical Phenomena and Observations

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: gold

Estimated APC paid: $4,499

Funders: Grantová Agentura České Republiky, Slezská Univerzita v Opavě