Non-standard s process in low metallicity massive rotating stars
arXiv:1112.5548 · doi:10.1051/0004-6361/201117794
Abstract
Context. Rotation is known to affect the nucleosynthesis of light elements in massive stars, mainly by rotation-induced mixing. In particular, rotation boosts the primary nitrogen production. Models of rotating stars are able to reproduce the nitrogen observed in low-Z halo stars. Aims. Here we present the first grid of stellar models for rotating massive stars at low Z, where a full s-process network is used to study the impact of rotation-induced mixing on the nucleosynthesis of heavy elements. Methods. We used the Geneva stellar evolution code that includes an enlarged reaction network with nuclear species up to bismuth to calculate 25 M models at three different Z and with different initial rotation rates. Results. First, we confirm that rotation-induced mixing leads to a production of primary Ne, which is the main neutron source for the s process in massive stars. Therefore rotation boosts the s process in massive stars at all Z. Second, the neutron-to-seed ratio increases with decreasing Z in models including rotation, which leads to the complete consumption of all iron seeds at Z < 1e-3 by the end of core He-burning. Thus at low Z, the iron seeds are the main limitation for this boosted s process. Third, as Z decreases, the production of elements up to the Ba peak increases at the expense of the elements of the Sr peak. We studied the impact of the initial rotation rate and of the uncertain O rate (which strongly affects the neutron poison strength of O) on our results. This study shows that rotating models can produce significant amounts of elements up to Ba over a wide range of Z. Fourth, compared to the He-core, the primary Ne production in the He-shell is even higher (> 1% in mass fraction at all Z), which could open the door for an explosive neutron capture nucleosynthesis in the He-shell, with a primary neutron source.
4 pages, 1 figure, accepted by A&A, language edited
References in corpus (12)
- First stars VI - Abundances of C, N, O, Li, and mixing in extremely metal-poor giants. Galactic evolution of the light elements
- Very low metallicity massive star models: Pre-SN evolution and primary nitrogen production
- A strong case for fast stellar rotation at very low metallicities
- The s process in massive stars at low metallicity. Effect of primary N14 from fast rotating stars
- The VLT-FLAMES survey of massive stars: atmospheric parameters and rotational velocity distributions for B-type stars in the Magellanic Clouds
- Stellar Archaeology -- Exploring the Universe with Metal-Poor Stars
- The VLT-FLAMES Survey of Massive Stars: Stellar parameters and rotational velocities in NGC3293, NGC4755 and NGC6611
- Dependence of S-Process Nucleosynthesis in Massive Stars on Triple-Alpha and 12C(a,g)16O Reaction Rate Uncertainties
- Be stars and binaries in the field of the SMC open cluster NGC330 with VLT-FLAMES
- Constraints on rotational mixing from surface evolution of light elements in massive stars
- First direct measurement of resonance strengths in 17O(α, γ)21Ne
- Stellar Evolution in the Early Universe
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