Giant planet formation via pebble accretion across different stellar masses

Open Access

Table 2

Parameters used in this study.

Parameter		Range	Result
Grain opacity factor	f_g	10⁻³–10⁰	Sect. 3.1
Turbulent viscosity	α_turb	10⁻⁵–10⁻³	Sect. 3.2
Core formation time	t₀	10⁵ –10⁷ yr	Sect. 3.3
Central star’s mass	M_s	0.1-1.5 M_⊙	Sect. 3.3

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