The advanced evolution of massive stars - I. New reaction rates for carbon and oxygen nuclear reactions

Open Access

Table 4.

Peak neutron density $ρ_{n}^{\max}$ $\rm \rho_n^{max}$ (cm⁻³) and neutron exposure τ_n (mbarn⁻¹) during the first and second C-burning shell episodes for each of the three nuclear references: CF88, HIN(RES), and TDHF.

Model	$ρ_{n}^{\max, 1}$ $\rm \rho_n^{max, 1}$	$ρ_{n}^{\max, 2}$ $\rm \rho_n^{max, 2}$	$τ_{n}^{1}$ $\rm \tau_n^{1}$	$τ_{n}^{2}$ $\rm \tau_n^{2}$
CF88	1.4 × 10⁹	3.1 × 10¹⁰	7.4 × 10⁻²	4.5 × 10⁻²
HIN(RES)	9.8 × 10⁸	1.3 × 10¹⁰	8.9 × 10⁻²	3.0 × 10⁻²
TDHF	3.6 × 10⁹	5.3 × 10¹¹	8.1 × 10⁻²	8.3 × 10⁻²

Notes. Values are computed following the same method as in D24.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.