Thermal solutions of the MAD numerical simulation at r = 8 r_g for an XRB with M_BH = 10 M_⊙. In both panels, the gray line shows the hot, optically thin branch that extends up to ṁ ≈ 10⁻¹, while the gold line shows the cold, optically thick branch that only extends down to ṁ ≈ 10⁻³. The black lines show reference solutions for comparison with the dash-dotted, dotted, and dashed lines, which show the solutions for a standard Shakura-Sunyaev disk, a one-temperature ADAF analytical solution, and a two-temperature JED semi-analytical solution, respectively. The uniqueness of our MAD thermal solutions is that they have two stable thermal branches within the range 10⁻³ ≲ ṁ ≲ 10⁻¹.