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Conference contributions

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Proceedings paper and poster

Nuclei in the Cosmos XI
This folder contains contributions from NuGrid members to the 11th Symposium on Nuclei in the Cosmos, which was held in Heidelberg, Germany, from July 19 to July 23, 2010.
The convective-reactive flash in Sakuraiʼs object
Poster: F. Herwig, P. Woodward, M. Pignatari, C. Fryer, G. Rockefeller, D. Porter, M. Bennett and R. Hirschi; presented at the 2nd Halifax Meeting on Computational Astrophysics, held in Halifax, Nova Scotia, Canada, October 16-18, 2009 (http://www.smu.ca/partners/ICA/).
The eff ect of 12C + 12C rate uncertainties on s-process yields
M. E. Bennett, R. Hirschi, M. Pignatari, S. Diehl, C. Fryer, F. Herwig, A. Hungerford, G. Magkotsios, G. Rockefeller, F. Timmes, M. Wiescher and P. Young; published in the proceedings of Nuclear Physics in Astrophysics IV, held in Frascati, Italy, June 8-12, 2009 (http://npa4.lngs.infn.it/).
Nuclei in the Cosmos X
Many members of NuGrid attended the 10th Symposium on Nuclei in the Cosmos, held on Mackinac Island, Michigan, USA, from July 27 to August 1, 2008. The papers, posters, and talk collected in this folder were presented at the conference.
GCE JINA meeting presentation
An overview of the NuGrid project. F. Herwig at the Galactic Chemical Evolution meeting organized by JINA in the spring of 2010.
Post-DD merger evolution and RCB stars
Nucleosynthesis in long term evolution of merged low-mass WDs – Path to form R Coronae Borealis (RCB) stars & Hydrogen deficient Carbon (HdC) stars. Contributed presentation given by Athira Menon at the 2012 JINA Frontiers Meeting, Michigan State University, October 7, 2012.
Nova framework and presolar grains
Presentation about the nova framework paper (Denissenkov et al., 2013) at the Presolar Grain Workshop in January 2013 in Chicago. Talk given by Reto Trappitsch. Images of the workshop and the program available at http://meteorites.fieldmuseum.org/node/106
Nova Framework: A New Tool For Modeling of Nova Outbursts and Nucleosynthesis
We have combined the stellar evolution code MESA and post-processing nucleosynthesis tools of NuGrid into a framework that allows to produce up-to-date models of nova outbursts and compute detailed nucleosynthesis in novae occurring on CO and ONe WDs. In this preliminary report, we present the most interesting new results related to CO and ONe nova outbursts that have been obtained with the Nova Framework.
DPG 2013
Poster session of "DPG (Deutsche Physikalische Gesellschaft) Tagung" - Germany. Dresden, 4 - 8 of March 2013 Results are all preliminary! English version will be added soon.
New Lessons Learned About Stellar Nucleosynthesis from Barium Isotopic Composition of Presolar SiCs from the Murchison Meteorite
Liu et al., Pignatari, Herwig 2013, LPICo 1719, 2507
Presolar Graphite Grains from Post-AGB Stars
Jadhav, M.; Pignatari, M.; Herwig, F.; Zinner, E.; Gallino, R.; Huss, G. R. 2013 LPICo 1719, 1963
17O(α,γ)21Ne and 17O(α,n)20Ne for the weak s process
Best et al., Beard M., Pignatari M. 2013, AIPC 1498, 309
Nuclear Data 2013
Presentations and Posters from Nuclear Data 2013 featuring NuGrid.
CASCA 2013
Poster presentation of NuGrid yields at the annual meeting of the Canadian Astronomical Society (CASCA) at UBC in BC, Canada. (http://casca2013.phas.ubc.ca )
A Born-Again AGB Star Origin of Type AB Silicon Carbide Grains Inferred from Radiogenic Sulfur-32
Fujiya, W.; Hoppe, P.; Zinner, E.; Pignatari, M.; Herwig, F., LPI Contribution No. 1777, p.1515
Current quests in nucleosynthesis: present and future neutron-induced reaction measurements
Praena, J.; MP et al. 2014, EPJWC 66, id.07022
Evidence for Short-Lived ^32Si in Presolar SiC grains of Type C
Zinner, E.; Hoppe, P.; Pignatari, M., M&PSA 76, 5010
Nuclei in the Cosmos XIII
http://www.nic2014.org
Presolar SiC Type C Grain M7-D: Isotopic Fingerprints from Explosive He-Burning
Hoppe, P.; Pignatari, M.; Fujiya, W.; Zinner, E.; Publication: 77th Annual Meeting of the Meteoritical Society, held September 7--12, 2014 in Casablanca, Morocco. LPI Contribution No. 1800, id.5051
i process and CEMP-s+r stars
We discovered that single-exposure one-zone simulations of i-process conditions provide an alternative, direct nucleosynthesis pathway that can match all observed heavy element abundances of CS31062-050 from Y to Ir within the observational error.
Experiments with neutron beams for the astrophysical s process
Lederer et al. 2016, Journal of Physics: Conference Series, Volume 665, Issue 1, article id. 012020
Nuclear and stellar physics uncertainties in the modelling of the i-process nucleosynthesis in post-AGB and rapidly accreting white dwrf stars
Poster presented by P. Denisenkov at the JINA CEE Frontiers 2016 meeting
Uncertainties and Statistical Tools in Simple Galactic Chemical Evolution Models
Poster #1 presented by Benoit Cote at the 2016 JINA-CEE Frontiers meeting.
Connecting Nuclear Physics and Stellar Evolution to Galactic Chemical Evolution
Poster #2 presented by Benoit Cote at the 2016 JINA-CEE Frontiers meeting.
Convective-reactive nucleosynthesis in low-mass and massive stars
Poster #1, JINA CEE Frontiers meeting 2016
Nuclear sensitivity studies & data access techniques
Poster #2, JINA CEE Frontiers meeting 2016
Nuclei in the Cosmos XIV
http://nic2016.jp/
i-process nucleosynthesis and mass retention efficiency in He-shell flash evolution of rapidly accreting white dwarfs
Our first paper in which an i process on rapidly accreting white dwarfs is proposed. Accepted for publication in ApJ Letters.
Connecting Nuclear Physics and Massive Star Models to Galactic Chemical Evolution
IAUS 329 - New Zealand 2016 - B. Côté, C. Ritter, B. W. O'Shea, F. Herwig, K. Belczynski, C. L. Fryer

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