Relativistic Common-envelope Dynamics of a Stellar-mass Black Hole II: Kerr Black Hole

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ID: 320243
2026
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Abstract
Abstract The common envelope phase plays a critical role in binary system evolution. In this study, we investigate the mass and momentum accretion rates during the interaction between a stellar-mass black hole and the envelope of a red supergiant using simplified two-dimensional simulations. We explore various Mach numbers and density gradients, finding that our simulations align with previous Bondi-Hoyle-Lyttleton accretion analyses. We observe the formation of a shock cone in the downstream flow, bow shocks in specific configurations, and subsonic regions within shocked flows. The shock cone is dragged when significant pressure gradients are present in the common envelope, with additional dragging near the black hole for highly rotating cases. We provide analytical fits for mass and momentum accretion rates, as well as bremsstrahlung luminosity, as functions of black hole spin, density gradients, and Mach number, offering first insights into general relativistic hydrodynamics modelling of the secular evolution of the common-envelope phase.
Reference Key
openalex_W7167795347 Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors Alejandro Cruz-Osorio, F. D. Lora-Clavijo
Journal monthly notices of the royal astronomical society
Year 2026
DOI
10.1093/mnras/stag1296
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