Evolution of hot bursts accreting models with Z = 0.0001, final masses of M_fin = 0.7 and 0.8 M_⊙, M_seed = 10 M_J, R_seed = 3 R_⊙, and ṁ = 10⁻⁵ M_⊙ yr⁻¹ (green line). Standard non-accreting models (grey lines), reference cold LLC (black line), and the hot (red line) accreting models with M_seed = 10 M_J, R_seed = 3 R_⊙, and ṁ = 10⁻⁵ M_⊙ yr⁻¹ are shown for comparison purposes. Left panel: HR diagram with the position of models at 1 Myr (filled triangles) and 10 Myr (filled squares), deuterium burning region (thick magenta line), and the end of the accretion phase (crosses) are marked. Right panel: evolution of the surface radius (in solar units) and central temperature (in units of 10⁶ K) as a function of the actual total mass. Hot and cold reference accretion cases (red and black lines) are only shown during the accretion phase for comparison purposes.