The intermediate neutron capture process - I. Development of the i-process in low-metallicity low-mass AGB stars

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Volume 648 (April 2021)

A&A, 648 (2021) A119

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This article has an erratum: [https://doi.org/10.1051/0004-6361/202040170e]

Table 1.

Characteristics of the models used to assess the impact of temporal and spatial discretization on the resulting nucleosynthesis.

Model	ϵ_max	α	log(N_n, max)	N_shell
label
Mϵ8α10	0.08	0.01	14.64	2085
Mϵ8α8	0.08	0.008	14.63	2085
Mϵ8α6	0.08	0.006	14.63	2085
Mϵ8α4	0.08	0.004	14.74	2091

Mϵ6α10	0.06	0.01	14.65	2324
Mϵ6α8	0.06	0.008	14.65	2321
Mϵ6α6	0.06	0.006	14.49	2321
Mϵ6α4	0.06	0.004	14.71	2341

Mϵ4α10	0.04	0.01	14.45	3096
Mϵ4α8	0.04	0.008	14.45	3104
Mϵ4α6	0.04	0.006	14.41	3102
Mϵ4α4	0.04	0.004	14.70	3111

Notes. Columns 2 and 3 are the discretization parameters defined in Sects. 4.1 and 4.2. Column 4 reports the maximum neutron density and column 5 indicates the mesh number when the neutron density reaches its peak value. Our reference model (described in Sect. 3) is Mϵ8α10.

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