Numerical simulations of dynamics and emission from relativistic astrophysical jets

24th IUPAP Conference on Computational Physics

物理学;计算机科学

Mimica, Petar^1 ; Aloy, Miguel Angel^1 ; Rueda-Becerril, Jesus M.^1 ; Tabik, Siham^2 ; Aloy, Carmen^1

Departamento de Astronomía y Astrofísica, Universidad de Valencia, 46100, Burjassot, Spain^1

Department Computer Architecture, University of Malaga, 29080 Málaga, Spain^2

关键词: Active galactic nuclei;    Astrophysical plasma;    Gamma-ray bursts (GRBs);    Magneto-hydrodynamics simulations;    Nonthermal emission;    Radiative transfer codes;    Relativistic hydrodynamics;    Relativistic outflow;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/454/1/012001/pdf
DOI  :  10.1088/1742-6596/454/1/012001

学科分类：计算机科学（综合）

来源: IOP

【 摘 要 】

Broadband emission from relativistic outflows (jets) of active galactic nuclei (AGN) and gamma-ray bursts (GRBs) contains valuable information about the nature of the jet itself and about the central engine which launches it. Using special relativistic hydrodynamics and magnetohydrodynamics simulations we study the dynamics of the jet and its interaction with the surrounding medium. The observational signature of the simulated jets is computed using a radiative transfer code developed specifically for the purpose of computing multi-wavelength, time-dependent, non-thermal emission from astrophysical plasmas. We present results of a series of long-term projects devoted to understanding the dynamics and emission of jets in parsec-scale AGN jets, blazars and the afterglow phase of the GRBs.