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Common Envelope Wind Tunnel: The Effects of Binary Mass Ratio and Implications for the Accretion-driven Growth of LIGO Binary Black Holes

  • Authors: Soumi De, Morgan MacLeod, Rosa Wallace Everson, Andrea Antoni, Ilya Mandel, and Enrico Ramirez-Ruiz

2020 The Astrophysical Journal 897 130.

  • Provider: AAS Journals

Caption: Figure 8.

Exponents of power-law relations of the accretion rate, ﹩{\alpha }_{\dot{M}}﹩, and drag force, αF, on the sink radius. Top panel: for each γ = 4/3 simulation in Table 1, an ﹩{\alpha }_{\dot{M}}﹩ (denoted by a cross) is derived from a linear least-squares fit of Equation (16) to the Ca value measured from that simulation of sink size Rs = 0.05 Ra, plus similar simulations with Rs = [0.025, 0.0125] Ra. The plot shows a largely positive ﹩{\alpha }_{\dot{M}}﹩, which indicates that accretion rates decrease as sink size decreases. The blue line shows a fit to the dependence of ﹩{\alpha }_{\dot{M}}﹩ on ﹩{{ \mathcal M }}_{\infty }﹩, using the piecewise fitting relation given by Equation (18). Bottom panel: Following the same procedure for calculating ﹩{\alpha }_{\dot{M}}﹩, each αF (denoted by a cross) value is derived from a linear least-squares fit of Equation (17) to Cd values from simulations of varying sink sizes. The plot shows values of αF ∼ 0, indicating little change in the overall drag force as the sink radius is modified. The blue line shows αF across ﹩{{ \mathcal M }}_{\infty }﹩ values using a constant least-squares fit, which gives αF ≈ 0.05.

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