Table 2.
Overview of the methodology employed to obtain the quantities of interest presented in the last column.
| Accretion disk model |
Reaction network |
Quantity of interest | ||||
|---|---|---|---|---|---|---|
| Input | Range explored | Output | Input | Range explored | Output | |
| m | [10−4, 108] M⊙ | T = f(m,ṁ,R,α) | T | > 2 × 106 K | MX = f(MX0, T, t) |
 |
| ṁ | [10−4,105] ṀEdd | ρ = f(m,ṁ,R,α) | t | [10−6, 1014] s | τe = f(MX) | |
| R | [3, 300] Rsch | vR = f(m,ṁ,R,α) | ||||
| α | [10−4, 1] | |||||
Notes. The first three columns provide the input parameters, the ranges explored, and the outputs of the accretion disk model. The three next columns present the inputs, their range, and the outputs of the reaction network used. Two steps lead to the computation of the important timescales: the viscous timescale only depends on the accretion disk model, while the burning/enriched timescale depends on the evolution of the mass ratio of chemical element X (dependent on the temperature, thus, on the disk model and on the reaction network).
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