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[ascl:2404.022] jetsimpy: Hydrodynamic model of gamma-ray burst jet and afterglow

jetsimpy creates hydrodynamic simulations of relativistic blastwaves with tabulated angular energy and Lorentz factor profiles and efficiently models Gamma-Ray Burst afterglows. It supports tabulated angular energy and tabulated angular Lorentz factor profiles. jetsimpy also supports ISM, wind, and mixed external density profile, including synthetic afterglow light curves, apparent superluminal motion, and sky map and Gaussian equivalent image sizes. Additionally, you can add your own emissivity model by defining a lambda function in a c++ source file, allowing the package to be used for more complicated models such as Synchrotron self-absorption.

Code site:
https://github.com/haowang-astro/jetsimpy
Described in:
https://ui.adsabs.harvard.edu/abs/2024arXiv240219359W
Bibcode:
2024ascl.soft04022W

Views: 289

ascl:2404.022
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