Convective overshooting and production of s-nuclei in massive stars during their core He-burning phase

Abstract

With the "post-processing" technique we explore the role of the convective overshooting on the production of s-nuclei in stellar models of different initial mass and metallicity ($15\le M_{ZAMS}/M_{\odot }\le 25$; $10^{-4}\le Z\le 0.02$), considering a range of values for the parameter $f$, which determines the overall efficiency of convective overshooting.We find enhancements in the production of s-nuclei until a factor $\sim 6$ (measured as the average overproduction factor of the 6 s-only nuclear species with $60\lesssim A\lesssim 90$) in all our models of different initial mass and metallicity with $f$ in the range $0.01-0.035$ (i.e. models with overshooting) compared to the production obtained with "no-overshooting" models (i.e. models with the same initial mass and metallicity, but $f=10^{-5}$). Moreover the results indicate that the link between the overshooting parameter $f$ and the s-process efficiency is essentially monotonic in all our models of different initial mass and metallicity. Also evident is the higher s-process efficiency when we progressively increase for a given f value both the mass of the models from 15 M${}_{\odot }$ to 25 M${}_{\odot }$ and the Z value from 10${}^{-4}$ to 0.02. We also briefly discuss the possible consequences of these results for some open questions linked to the s-process weak component efficiency, as well as a "rule of thumb" to evaluate the impact of the convective overshooting on the yields of a generation of stars.

12 pages, 6 figures, A&A accepted (corrected typos plus minor changes in order to fulfill the guidelines for A&A manuscripts)

References in corpus (6)

• The nucleosynthesis of Al26 and Fe60 in solar metallicity stars extending in mass from 11 to 120 Msun: the hydrostatic and explosive contributions
• The s process in massive stars at low metallicity. Effect of primary N14 from fast rotating stars
• s-Process Nucleosynthesis in Advanced Burning Phases of Massive Stars
• On the Sensitivity of Massive Star Nucleosynthesis and Evolution to Solar Abundances and to Uncertainties in Helium Burning Reaction Rates
• Dependence of S-Process Nucleosynthesis in Massive Stars on Triple-Alpha and 12C(a,g)16O Reaction Rate Uncertainties
• How to define the boundaries of a convective zone and how extended is overshooting?

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• The oxygen vs. sodium (anti)correlation(s) in omega Cen
• Chemical Signature Indicating A Lack of Massive Stars in Dwarf Galaxies
• Impact of the latest 22Ne+α reaction rates on nucleosynthesis in massive stars and galactic chemical evolution