Sensitivity of He Flames in X-Ray Bursts to Nuclear Physics

Through the use of axisymmetric 2D hydrodynamic simulations, we further investigate laterally propagating flames in X-ray bursts (XRBs). Our aim is to understand the sensitivity of a propagating helium flame to different nuclear physics. Using the Castro simulation code, we confirm the phenomenon of...

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Main Authors: Zhi Chen, Michael Zingale, Kiran Eiden
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/acec72
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author Zhi Chen
Michael Zingale
Kiran Eiden
author_facet Zhi Chen
Michael Zingale
Kiran Eiden
author_sort Zhi Chen
collection DOAJ
description Through the use of axisymmetric 2D hydrodynamic simulations, we further investigate laterally propagating flames in X-ray bursts (XRBs). Our aim is to understand the sensitivity of a propagating helium flame to different nuclear physics. Using the Castro simulation code, we confirm the phenomenon of enhanced energy generation shortly after a flame is established by adding ^12 C(p, γ ) ^13 N( α , p) ^16 O to the network, in agreement with the past literature. This sudden outburst of energy leads to a short accelerating phase, causing a drastic alteration in the overall dynamics of the flame in XRBs. Furthermore, we investigate the influence of different plasma screening routines on the propagation of the XRB flame. We finally examine the performance of simplified spectral deferred correction, a novel approach to hydrodynamics and reaction coupling incorporated in Castro, as an alternative to operator splitting.
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spelling doaj.art-5161489351c14a0a953e2503587809ae2023-09-26T17:14:16ZengIOP PublishingThe Astrophysical Journal1538-43572023-01-01955212810.3847/1538-4357/acec72Sensitivity of He Flames in X-Ray Bursts to Nuclear PhysicsZhi Chen0https://orcid.org/0000-0002-2839-107XMichael Zingale1https://orcid.org/0000-0001-8401-030XKiran Eiden2https://orcid.org/0000-0001-6191-4285Department of Physics and Astronomy, Stony Brook University , Stony Brook, NY 11794-3800, USA ; zhi.chen.3@stonybrook.eduDepartment of Physics and Astronomy, Stony Brook University , Stony Brook, NY 11794-3800, USA ; zhi.chen.3@stonybrook.eduDepartment of Astronomy, University of California , Berkeley, CA 94720-3411, USAThrough the use of axisymmetric 2D hydrodynamic simulations, we further investigate laterally propagating flames in X-ray bursts (XRBs). Our aim is to understand the sensitivity of a propagating helium flame to different nuclear physics. Using the Castro simulation code, we confirm the phenomenon of enhanced energy generation shortly after a flame is established by adding ^12 C(p, γ ) ^13 N( α , p) ^16 O to the network, in agreement with the past literature. This sudden outburst of energy leads to a short accelerating phase, causing a drastic alteration in the overall dynamics of the flame in XRBs. Furthermore, we investigate the influence of different plasma screening routines on the propagation of the XRB flame. We finally examine the performance of simplified spectral deferred correction, a novel approach to hydrodynamics and reaction coupling incorporated in Castro, as an alternative to operator splitting.https://doi.org/10.3847/1538-4357/acec72X-ray burstsNucleosynthesisExplosive nucleosynthesisComputational methodsHydrodynamics
spellingShingle Zhi Chen
Michael Zingale
Kiran Eiden
Sensitivity of He Flames in X-Ray Bursts to Nuclear Physics
The Astrophysical Journal
X-ray bursts
Nucleosynthesis
Explosive nucleosynthesis
Computational methods
Hydrodynamics
title Sensitivity of He Flames in X-Ray Bursts to Nuclear Physics
title_full Sensitivity of He Flames in X-Ray Bursts to Nuclear Physics
title_fullStr Sensitivity of He Flames in X-Ray Bursts to Nuclear Physics
title_full_unstemmed Sensitivity of He Flames in X-Ray Bursts to Nuclear Physics
title_short Sensitivity of He Flames in X-Ray Bursts to Nuclear Physics
title_sort sensitivity of he flames in x ray bursts to nuclear physics
topic X-ray bursts
Nucleosynthesis
Explosive nucleosynthesis
Computational methods
Hydrodynamics
url https://doi.org/10.3847/1538-4357/acec72
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