Mini-Symposium on Nuclear Physics: Sensitive Input for Understanding Nucleosynthesis I
FOCUS · J6 ·
Presentations
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The sensitivity of $r$-process nucleosynthesis to individual nuclear properties
COFFEE_KLATCH · Invited
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Authors
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Rebecca Surman
- Union College
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An astrophysical engine that stores gravitational work as nuclear Coulomb energy
ORAL
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Authors
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Donald Clayton
- Clemson Uiversity
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Benchmarks of results obtained in the new finite-range droplet model
ORAL
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Authors
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Peter Moller
- Los Alamos National Laboratory
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Effective Reaction Rates (ERR) for the Helium Burning Reactions
ORAL
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Authors
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Sam M. Austin
- National Superconducting Cyclotron Laboratory, Michigan State University
- MSU/NSCL
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Christopher West
- University of Minnesota
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Alexander Heger
- University of Minnesota, Monash University
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Sensitive r-process nuclei production at Notre Dame
ORAL
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Authors
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Maxime Brodeur
- University of Notre Dame
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$\beta$-decay studies of very neutron-rich Pd and Ag isotopes
ORAL
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Authors
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Karl Smith
- Univ. of Notre Dame, Joint Institute of Nuclear Astrophysics, National Superconducting Cyclotron Laboratory, Helmholtzzentrum fur Schwerionenforschung
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Validation of (d,p$\gamma$) as a Surrogate for (n,$\gamma$)
ORAL
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Authors
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A. Ratkiewicz
- Rutgers University
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J.A. Cizewski
- Rutgers University
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A. Adekola
- Rutgers University
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S. Burcher
- Rutgers University
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M.E. Howard
- Rutgers University
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B. Manning
- Rutgers University
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S.L. Rice
- Rutgers University
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C. Shand
- Rutgers University
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J.T. Burke
- LLNL
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R.J. Casperson
- LLNL
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N.D. Scielzo
- LLNL
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R.A.E. Austin
- St. Mary's University
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N. Fotiades
- LANL
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R.O. Hughes
- Richmond University
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T.J. Ross
- Richmond University
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M. McCleskey
- TAMU
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S.D. Pain
- ORNL
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W.A. Peters
- ORAU
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