Fig. A.1.

(a) Distribution of specific angular momentum (λ) and (b) heating in the system as a function of radius (log r), when viscosity assumed is relativistic (green, solid) and Newtonian (magenta, dotted). Panel b: we also compare the heating due to magnetic dissipation, QB (blue, dashed), assuming βd = 0.02. The flow parameters are E = 1.0005, αvis = 0.01, λ0 = 2.60, Ṁ = 0.01 ṀEdd, and MBH = 10 M⊙.
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