@article{8a68e1cbf78745af9f59c7853e7438c8,
title = "NUGRID STELLAR DATA SET. I. STELLAR YIELDS from H to BI for STARS with METALLICITIES Z = 0.02 and Z = 0.01",
abstract = "We provide a set of stellar evolution and nucleosynthesis calculations that applies established physics assumptions simultaneously to low- and intermediate-mass and massive star models. Our goal is to provide an internally consistent and comprehensive nuclear production and yield database for applications in areas such as presolar grain studies. Our non-rotating models assume convective boundary mixing (CBM) where it has been adopted before. We include 8 (12) initial masses for Z = 0.01 (0.02). Models are followed either until the end of the asymptotic giant branch phase or the end of Si burning, complemented by simple analytic core-collapse supernova (SN) models with two options for fallback and shock velocities. The explosions show which pre-SN yields will most strongly be effected by the explosive nucleosynthesis. We discuss how these two explosion parameters impact the light elements and the s and p process. For low- and intermediate-mass models, our stellar yields from H to Bi include the effect of CBM at the He-intershell boundaries and the stellar evolution feedback of the mixing process that produces the pocket. All post-processing nucleosynthesis calculations use the same nuclear reaction rate network and nuclear physics input. We provide a discussion of the nuclear production across the entire mass range organized by element group. The entirety of our stellar nucleosynthesis profile and time evolution output are available electronically, and tools to explore the data on the NuGrid VOspace hosted by the Canadian Astronomical Data Centre are introduced.",
keywords = "nuclear reactions, nucleosynthesis, abundances, stars: abundances, stars: evolution, stars: interiors",
author = "M. Pignatari and F. Herwig and R. Hirschi and M. Bennett and G. Rockefeller and C. Fryer and Francis Timmes and C. Ritter and A. Heger and S. Jones and U. Battino and A. Dotter and R. Trappitsch and S. Diehl and U. Frischknecht and A. Hungerford and G. Magkotsios and C. Travaglio and Patrick Young",
note = "Funding Information: NuGrid acknowledges significant support from NSF grants PHY 02-16783 and PHY 09-22648 (Joint Institute for Nuclear Astrophysics, JINA), NSF grant PHY-1430152 (JINA Center for the Evolution of the Elements), and EU MIRG-CT-2006-046520. NuGrid computations are performed at the Arizona State Universitys Fulton High-performance Computing Center (USA) and the high-performance computer KHAOS at the EPSAM Institute at Keele University (UK). M. P. acknowledges an Ambizione grant of the SNSF, SNF (Switzerland), and support from the Lendulet-2014 Programme of the Hungarian Academy of Sciences. M.P., S.J., and R.H. thank the Eurocore project Eurogenesis for support. F.H. acknowledges NSERC Discovery Grant funding. R.H. and S.J. acknowledge support from the World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan. M.G.B.s research was carried out under the auspices of the National Nuclear Security Administration of the U.S. Department of Energy at the Los Alamos National Laboratory under Contract No. DEAC52-06NA25396. A.D. acknowledges support from the Australian Research Council under grant FL110100012. The research leading to these results has received funding from the European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013)/ERC grant agreement No. 306901. This work used the SE library (LA-CC-08-057) developed at the Los Alamos National Laboratory as part of the NuGrid collaboration; S.E. makes use of the HDF5 library, which was developed by The HDF Group and by the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign. M.P. acknowledges the support to the Milne Astrophysics Center granted by PRACE, through its Distributed Extreme Computing Initiative, for resource allocations on Sisu (CSC, Finland), Archer (EPCC, UK), and Beskow (KTH, Sweden), and by the STFC DiRAC High Performance Computing Facilities. Publisher Copyright: {\textcopyright} 2016. The American Astronomical Society. All rights reserved.",
year = "2016",
month = aug,
doi = "10.3847/0067-0049/225/2/24",
language = "English (US)",
volume = "225",
journal = "Astrophysical Journal, Supplement Series",
issn = "0067-0049",
publisher = "IOP Publishing Ltd.",
number = "2",
}