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Title: NuGrid stellar data set – II. Stellar yields from H to Bi for stellar models with MZAMS = 1–25 M⊙ and Z = 0.0001–0.02

Journal Article · · Monthly Notices of the Royal Astronomical Society
 [1]; ORCiD logo [2];  [3];  [4];  [5];  [6]
  1. Univ. of Victoria, BC (Canada). Dept. of Physics & Astronomy; Keele Univ. (United Kingdom); Joint Inst. for Nuclear Astrophysics (JINA), East Lansing, MI (United States); Michigan State Univ., East Lansing, MI (United States)
  2. Univ. of Victoria, BC (Canada). Dept. of Physics & Astronomy; Joint Inst. for Nuclear Astrophysics (JINA), East Lansing, MI (United States); Michigan State Univ., East Lansing, MI (United States)
  3. Heidelberg Inst. for Theoretical Studies, Heidelberg (Germany); Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
  4. Univ. of Hull, Hull (United Kingdom). E. A. Milne Centre for Astrophysics, Dept. of Physics & Mathematics
  5. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
  6. Keele Univ. (United Kingdom)
+ Show Author Affiliations

We provide here a significant extension of the NuGrid Set 1 models in mass coverage and towards lower metallicity, adopting the same physics assumptions. The combined data set now includes the initial masses MZAMS/M⊙ = 1, 1.65, 2, 3, 4, 5, 6, 7, 12, 15, 20, 25 for Z = 0.02, 0.01, 0.006, 0.001, 0.0001 with α-enhanced composition for the lowest three metallicities. These models are computed with the MESA stellar evolution code and are evolved up to the AGB, the white dwarf stage, or until core collapse. The nucleosynthesis was calculated for all isotopes in post-processing with the NuGrid MPPNP code. Explosive nucleosynthesis is based on semi-analytic 1D shock models. Metallicity-dependent mass-loss, convective boundary mixing in low- and intermediate-mass models and H and He core burning massive star models are included. Convective O-C shell mergers in some stellar models lead to the strong production of odd-Z elements P, Cl, K, and Sc. In AGB models with hot dredge-up, the convective boundary mixing efficiency is reduced to accommodate for its energetic feedback. In both low-mass and massive star models at the lowest metallicity, H-ingestion events are observed and lead to i-process nucleosynthesis and substantial 15N production. Finally, complete yield data tables, derived data products and online analytic data access are provided.

Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE Laboratory Directed Research and Development (LDRD) Program
Grant/Contract Number:
89233218CNA000001
OSTI ID:
1492606
Report Number(s):
LA-UR--17-25747
Journal Information:
Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 1 Vol. 480; ISSN 0035-8711
Publisher:
Royal Astronomical SocietyCopyright Statement
Country of Publication:
United States
Language:
English

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Can Extra Mixing in RGB and AGB Stars Be Attributed to Magnetic Mechanisms? text January 2007
Nucleosynthesis and Evolution of Massive Metal-Free Stars text January 2008
New Asymptotic Giant Branch models for a range of metallicities text January 2009
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Updated stellar yields from Asymptotic Giant Branch models text January 2009
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Evolution and nucleosynthesis of extremely metal-poor and metal-free low- and intermediate-mass stars II. s-process nucleosynthesis during the core He flash text January 2010
Heavy Element Nucleosynthesis in the Brightest Galactic Asymptotic Giant Branch stars text January 2012
Production and evolution of Li, Be and B isotopes in the Galaxy text January 2012
The C-flame Quenching by Convective Boundary Mixing in Super-AGB Stars and the Formation of Hybrid C/O/Ne White Dwarfs and SN Progenitors text January 2013
Hot bottom burning and s-process nucleosynthesis in massive AGB stars at the beginning of the thermally-pulsing phase text January 2013
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Explosive yields of massive stars from Z=0 to Z=Zsun text January 2004
Stellar evolution with rotation XII: Pre-supernova models text January 2004
Yields of rotating stars at solar metallicity text January 2004
An empirical formula for the mass-loss rates of dust-enshrouded red supergiants and oxygen-rich Asymptotic Giant Branch stars text January 2005
Nucleosynthesis Yields of Core-Collapse Supernovae and Hypernovae, and Galactic Chemical Evolution text January 2006
Galactic chemical evolution: Carbon through Zinc text January 2006
Anelastic and Compressible Simulations of Stellar Oxygen Burning text January 2006
Nucleosynthesis of Elements in Low to Intermediate Mass Stars through the AGB Phase text January 1997
RAMSES-CH: a new chemodynamical code for cosmological simulations text January 2012
Application of a Theory and Simulation-based Convective Boundary Mixing Model for AGB Star Evolution and Nucleosynthesis text January 2016
s-process production in rotating massive stars at solar and low metallicities text January 2016

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r -process nucleosynthesis: connecting rare-isotope beam facilities with the cosmos journal July 2019
Missing red supergiants and carbon burning journal January 2020
Low-metallicity CO + He WD post-merger models for RCB stars as a source of pre-solar graphite grains journal September 2018
Simulating an isolated dwarf galaxy with multichannel feedback and chemical yields from individual stars journal October 2018
Convective boundary mixing in a post-He core burning massive star model journal December 2018
NuGrid stellar data set – III. Updated low-mass AGB models and s-process nucleosynthesis with metallicities Z= 0.01, Z = 0.02, and Z = 0.03 journal August 2019
Tentative detection of the circumgalactic medium of the isolated low-mass dwarf galaxy WLM journal September 2019
Nucleosynthetic yields from neutron stars accreting in binary common envelopes journal February 2019
60Fe in core-collapse supernovae and prospects for X-ray and gamma-ray detection in supernova remnants journal February 2019
Metal Mixing and Ejection in Dwarf Galaxies Are Dependent on Nucleosynthetic Source journal December 2018
Neutron Star Mergers Might Not Be the Only Source of r -process Elements in the Milky Way journal April 2019
Aluminium-26 from Massive Binary Stars. I. Nonrotating Models journal October 2019
Abundance Ratios in GALAH DR2 and Their Implications for Nucleosynthesis journal November 2019
Remnants and ejecta of thermonuclear electron-capture supernovae: Constraining oxygen-neon deflagrations in high-density white dwarfs text January 2018
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79 ASTRONOMY AND ASTROPHYSICS
stars: abundances — evolution — interiors