Impact of Anisotropic Cosmic-Ray Transport on the Gamma-Ray Signatures in the Galactic Center

The very high energy (VHE) emission of the central molecular zone (CMZ) is rarely modeled in 3D. Most approaches describe the morphology in 1D or simplify the diffusion to the isotropic case. In this work, we show the impact of a realistic 3D magnetic field configuration and gas distribution on the...

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Main Authors: J. Dörner, J. Becker Tjus, P. S. Blomenkamp, H. Fichtner, A. Franckowiak, E. M. Zaninger
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad2ea1
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author J. Dörner
J. Becker Tjus
P. S. Blomenkamp
H. Fichtner
A. Franckowiak
E. M. Zaninger
author_facet J. Dörner
J. Becker Tjus
P. S. Blomenkamp
H. Fichtner
A. Franckowiak
E. M. Zaninger
author_sort J. Dörner
collection DOAJ
description The very high energy (VHE) emission of the central molecular zone (CMZ) is rarely modeled in 3D. Most approaches describe the morphology in 1D or simplify the diffusion to the isotropic case. In this work, we show the impact of a realistic 3D magnetic field configuration and gas distribution on the VHE γ -ray distribution of the CMZ. We solve the 3D cosmic-ray transport equation with an anisotropic diffusion tensor using the approach of stochastic differential equations as implemented in the CRPropa framework. We test two different source distributions for five different anisotropies of the diffusion tensor, covering the range of effectively fieldline-parallel diffusion to isotropic diffusion. Within the tested magnetic field configuration, the anisotropy of the diffusion tensor is close to the isotropic case, and three point sources within the CMZ are favored. Future missions such as the upcoming CTA will reveal more small-scale structures that are not yet included in the model. Therefore, a more detailed 3D gas distribution and magnetic field structure will be needed.
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spelling doaj.art-f6dfd56cb7104c1cad86f880abbaaacc2024-04-18T08:56:07ZengIOP PublishingThe Astrophysical Journal1538-43572024-01-01965218010.3847/1538-4357/ad2ea1Impact of Anisotropic Cosmic-Ray Transport on the Gamma-Ray Signatures in the Galactic CenterJ. Dörner0https://orcid.org/0000-0001-6692-6293J. Becker Tjus1https://orcid.org/0000-0002-1748-7367P. S. Blomenkamp2https://orcid.org/0000-0002-5032-5896H. Fichtner3https://orcid.org/0000-0002-9151-5127A. Franckowiak4https://orcid.org/0000-0002-5605-2219E. M. Zaninger5Theoretische Physik IV, Fakultät für Physik & Astronomie, Ruhr-Universität Bochum , 44780 Bochum, Germany; Ruhr Astroparticle and Plasma Physics Center (RAPP Center), Ruhr-Universität Bochum , 44780 Bochum, GermanyTheoretische Physik IV, Fakultät für Physik & Astronomie, Ruhr-Universität Bochum , 44780 Bochum, Germany; Ruhr Astroparticle and Plasma Physics Center (RAPP Center), Ruhr-Universität Bochum , 44780 Bochum, Germany; Department of Space, Earth and Environment, Chalmers University of Technology , 412 96 Gothenburg, SwedenRuhr Astroparticle and Plasma Physics Center (RAPP Center), Ruhr-Universität Bochum , 44780 Bochum, Germany; Astronomisches Institut, Fakultät für Physik & Astronomie, Ruhr-Universität Bochum , 44780 Bochum, GermanyTheoretische Physik IV, Fakultät für Physik & Astronomie, Ruhr-Universität Bochum , 44780 Bochum, Germany; Ruhr Astroparticle and Plasma Physics Center (RAPP Center), Ruhr-Universität Bochum , 44780 Bochum, GermanyRuhr Astroparticle and Plasma Physics Center (RAPP Center), Ruhr-Universität Bochum , 44780 Bochum, Germany; Astronomisches Institut, Fakultät für Physik & Astronomie, Ruhr-Universität Bochum , 44780 Bochum, GermanyTheoretische Physik IV, Fakultät für Physik & Astronomie, Ruhr-Universität Bochum , 44780 Bochum, Germany; Ruhr Astroparticle and Plasma Physics Center (RAPP Center), Ruhr-Universität Bochum , 44780 Bochum, GermanyThe very high energy (VHE) emission of the central molecular zone (CMZ) is rarely modeled in 3D. Most approaches describe the morphology in 1D or simplify the diffusion to the isotropic case. In this work, we show the impact of a realistic 3D magnetic field configuration and gas distribution on the VHE γ -ray distribution of the CMZ. We solve the 3D cosmic-ray transport equation with an anisotropic diffusion tensor using the approach of stochastic differential equations as implemented in the CRPropa framework. We test two different source distributions for five different anisotropies of the diffusion tensor, covering the range of effectively fieldline-parallel diffusion to isotropic diffusion. Within the tested magnetic field configuration, the anisotropy of the diffusion tensor is close to the isotropic case, and three point sources within the CMZ are favored. Future missions such as the upcoming CTA will reveal more small-scale structures that are not yet included in the model. Therefore, a more detailed 3D gas distribution and magnetic field structure will be needed.https://doi.org/10.3847/1538-4357/ad2ea1Galactic cosmic raysGalactic centerGamma-rays
spellingShingle J. Dörner
J. Becker Tjus
P. S. Blomenkamp
H. Fichtner
A. Franckowiak
E. M. Zaninger
Impact of Anisotropic Cosmic-Ray Transport on the Gamma-Ray Signatures in the Galactic Center
The Astrophysical Journal
Galactic cosmic rays
Galactic center
Gamma-rays
title Impact of Anisotropic Cosmic-Ray Transport on the Gamma-Ray Signatures in the Galactic Center
title_full Impact of Anisotropic Cosmic-Ray Transport on the Gamma-Ray Signatures in the Galactic Center
title_fullStr Impact of Anisotropic Cosmic-Ray Transport on the Gamma-Ray Signatures in the Galactic Center
title_full_unstemmed Impact of Anisotropic Cosmic-Ray Transport on the Gamma-Ray Signatures in the Galactic Center
title_short Impact of Anisotropic Cosmic-Ray Transport on the Gamma-Ray Signatures in the Galactic Center
title_sort impact of anisotropic cosmic ray transport on the gamma ray signatures in the galactic center
topic Galactic cosmic rays
Galactic center
Gamma-rays
url https://doi.org/10.3847/1538-4357/ad2ea1
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