We present a recently developed strategy [Nucl. Phys. A 785C, 142 (2005), Phys. Rev. C 69, 041307(R) (2004), Phys. Rev. C 67, 054309 (2003)] of calculating the spin and parity dependent shell model level density for application to astrophysics reaction rates. We also present an exact method for removing the spurious contribution to the nuclear level density in shell model spaces that are factorizable in center-of-mass (CoM) and intrinsic components.
|Journal||Proceedings of Science|
|State||Published - 2006|
|Event||9th International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos, NIC 2006 - Geneva, Switzerland|
Duration: Jun 25 2006 → Jun 30 2006