TypAmountVATCurrencyShareStatusCost centre
APC2767.4826.29EUR100.00 %(Zahlung erfolgt)9001010 / 476151
APC-700.000.00EUR-25.29 %(Storniert)9001010 / 476151
APC700.000.00EUR25.29 %(Zahlung erfolgt)28901 / 476151
Sum2767.4826.29EUR   
Total2793.77     
Journal Article PUBDB-2023-07884

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AM³: An Open-Source Tool for Time-Dependent Lepto-Hadronic Modeling of Astrophysical Sources

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2024
Institute of Physics Publ. London

The astrophysical journal / Supplement series 275(1), 4 () [10.3847/1538-4365/ad725c]
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Report No.: arXiv:2312.13371

Abstract: We present the Astrophysical Multimessenger Modeling (AM$^3$) software. AM$^3$ is a documented open-sourcesoftware (source code at https://gitlab.desy.de/am3/am3; user guide and documentation at https://am3.readthedocs.io/en/latest/) that efficiently solves the coupled integro-differential equations describing the temporalevolution of the spectral densities of particles interacting in astrophysical environments, including photons,electrons, positrons, protons, neutrons, pions, muons, and neutrinos. The software has been extensively used tosimulate the multiwavelength and neutrino emission from active galactic nuclei (including blazars), gamma-raybursts, and tidal disruption events. The simulations include all relevant nonthermal processes, namely synchrotronemission, inverse Compton scattering, photon–photon annihilation, proton–proton and proton–photon pionproduction, and photo-pair production. The software self-consistently calculates the full cascade of primary andsecondary particles, including nonlinear feedback processes and predictions in the time domain. It also allows theuser to track separately the particle densities produced by means of each distinct interaction process, including thedifferent hadronic channels. With its efficient hybrid solver combining analytical and numerical techniques, AM3combines efficiency and accuracy at a user-adjustable level. We describe the technical details of the numericalframework and present three examples of applications to different astrophysical environments.

Keyword(s): Compton scattering: inverse ; neutrino: spectrum ; particle: density ; photon photon: annihilation ; pi: production ; gamma ray: burst ; programming ; photon ; spectral ; AGN ; nonlinear ; feedback ; positron ; muon ; blazar ; hybrid ; tracks ; efficiency ; electron ; cascade ; time dependence ; synchrotron

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Note: Astrophys.J.Supp. 275 (2024) 1, 4. The BSD-licensed source code can be found under https://gitlab.desy.de/am3/am3, for the user guide and documentation see https://am3.readthedocs.io/en/latest/

Contributing Institute(s):
  1. Theoretische Astroteilchenphysik (Z_THAT)
Research Program(s):
  1. 613 - Matter and Radiation from the Universe (POF4-613) (POF4-613)
  2. DFG project G:(GEPRIS)390783311 - EXC 2094: ORIGINS: Vom Ursprung des Universums bis zu den ersten Bausteinen des Lebens (390783311) (390783311)
Experiment(s):
  1. No specific instrument

Appears in the scientific report 2024
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AM$^3$: An Open-Source Tool for Time-Dependent Lepto-Hadronic Modeling of Astrophysical Sources
[10.3204/PUBDB-2024-06535]  GO OpenAccess  Download fulltext Files  Download fulltextFulltext by arXiv.org BibTeX | EndNote: XML, Text | RIS


 Record created 2023-12-15, last modified 2025-07-23