Chemical evolution and kilonova implications of post-merger accretion disk winds

Open Access

Table 1.

Simulation models and parameters.

Model	Resolution	r_in	r_max	β	a	M_BH	M_disk	S_disk	N_tr(t₀)	$N_{tr}^{out} (t_{f})$ $Mathematical equation: $ N_{\mathrm{tr}}^{\mathrm{out}} (t_{f}) $$	t_f
2D-Thick-s	288 × 256 × 1	4.0	9.0	100	0.9375	3.0	0.021	7	11072	186	20 000
2D-Thin-s	288 × 256 × 1	4.0	9.0	50	0.9375	3.0	0.002	10	11049	372	20 000
2D-Thick	288 × 256 × 1	4.0	9.78	100	0.9375	3.0	0.129	7	15998	1037	20 000
2D-Thin	288 × 256 × 1	4.0	9.78	50	0.9375	3.0	0.013	10	15988	554	18 200
2D-kn	288 × 256 × 1	4.0	12.6	50	0.6	8.2	0.785	10	20392	931	20 000

3D-Thick	256 × 128 × 64	4.0	9.78	100	0.9375	3.0	0.129	7	8131	1063	19 800
3D-Thin	256 × 128 × 64	4.0	9.78	50	0.9375	3.0	0.013	10	8124	544	18 300
3D-kn	288 × 128 × 64	4.0	12.6	50	0.6	8.2	0.781	10	10344	1000	20 000
3D-kn-p	288 × 128 × 64	4.0	12.6	50	0.6	8.2	0.834	10	9954	281	20 000

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