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We perform no-core full configuration calculations for a set of light nuclei including $^{16}$O with a realistic NN interaction, JISP16.
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P. Sternberg, E. G. Ng, C. Yang, P. Maris, J. P. Vary, M. Sosonkina and H. V. Le, ÒAccelerating Configuration Interaction Calculations for Nuclear StructureÓ, In Proceedings of the 2008 ACM/IEEE Conference on Supercomputing (Austin, Texas, November 15 - 21, 2008). Conference on High Performance Networking and Computing. IEEE Press, Piscataway, NJ, 1-12. DOI= http://doi.acm.org/10.1145/1413370.1413386
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This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of its employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof. The views and opinions of the authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof
Cited in the paper.
By “bare”, we mean that we have not performed renormalization by means of a Lee–Suzuki–Okamoto or other effective interaction approach
Cited in the paper.
P. Navrátil, private communication
Cited in the paper.
A Fortran program for the JISP16 interaction matrix elements is available at http://nuclear.physics.iastate.edu
Cited in the paper.
Y. Alhassid, G. F. Bertsch, and L. Fang, Phys. Rev. Lett. 100
2008
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