Astrophysics Program, Oak Ridge National
Laboratory |
 |
Activities
The Nuclear Astrophysics Program at Oak Ridge National Laboratory
includes efforts in Experimental Measurements, Nuclear Data Evaluation,
and Theoretical Nuclear Astrophysics.
- Experimental Measurements
- Measurements of reactions with proton-rich accelerated radioactive ion
beams at the
Holifield Radioactive
Ion Beam Facility (HRIBF). These measurements will improve our
understanding of stellar explosions.
- Measurements of neutron capture and transmission cross sections
at the
Oak Ridge Electron
Linear Accelerator (ORELA) pulsed white neutron
source. These measurements are important for studies of heavy element
nucleosynthesis through the s-, r-, and p-processes.
- Nuclear Data Evaluation
- Systematic calculations of stellar-averaged neutron capture reaction
rates for heavy element nucleosynthesis, utilizing neutron resonance
parameters extracted from standard online data files.
- Evaluation of thermonuclear reaction rates important for
nucleosynthesis occurring in stellar explosions.
- Contributions toward establishing a
coordinated
U.S. effort in nuclear astrophysics data evaluation.
- Theoretical
Nuclear Astrophysics
- Simulations of Stellar Explosions:
Type II Supernovae and Novae,
via numerical solution of the coupled equations of radiation transport,
multidimensional hydrodynamics, and the synthesis of nuclei;
Type I Supernovae, via lattice Boltzmann techniques.
- Calculation of Gamow-Teller strength functions and electron capture rates
in fp-shell nuclei with Monte Carlo Shell Model techniques.
Research sponsored by the Oak Ridge National Laboratory, managed by
Lockheed Martin Energy Research Corp. for the U.S. Department of
Energy under contract number DE-AC05-96OR22464.
Contact
| Michael Smith |
| Oak Ridge National Laboratory | | Phone:
| | +1-423-576-5037 |
| Physics Division | | Fax: | |
+1-423-576-8746 |
| Bldg. 6010, MS-6354 | | Email: |
| msmith@orph01.phy.ornl.gov |
| P.O. Box 2008 |
| Oak Ridge, TN 37831-6354 |
Electronic Access
Translated into HTML by
TWB (February
1, 1996); Last updated on September 20, 2000.