Dynamics of Laterally Propagating Flames in X-ray Bursts. II. Realistic Burning & Rotation

Abstract

We continue to investigate two-dimensional laterally propagating flames in type I X-ray bursts using fully compressible hydrodynamics simulations. In the current study we relax previous approximations where we artificially boosted the flames. We now use more physically realistic reaction rates, thermal conductivities, and rotation rates, exploring the effects of neutron star rotation rate and thermal structure on the flame. We find that at lower rotation rates the flame becomes harder to ignite, whereas at higher rotation rates the nuclear burning is enhanced by increased confinement from the Coriolis force and the flame propagates steadily. At higher crustal temperatures, the flame moves more quickly and accelerates as it propagates through the atmosphere. If the temperature is too high, instead of a flame propagating across the surface the entire atmosphere burns steadily. All of the software used for these simulations is freely available.

arXiv comment19 pages, 19 figures, accepted for publication in ApJ

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• Horizons: Nuclear Astrophysics in the 2020s and Beyond
• Comparing Early Evolution of Flames in X-ray Bursts in Two and Three Dimensions
• Simulating Lateral H/He Flame Propagation in Type I X-ray Bursts
• AMReX-Astrophysics Microphysics: A set of microphysics routines for astrophysical simulation codes based on the AMReX library