Parity-Dependence in the Nuclear Level Density

@article{Mocelj2005ParityDependenceIT,
  title={Parity-Dependence in the Nuclear Level Density},
  author={D. Mocelj and Thomas Rauscher and Gabriel Mart{\'i}nez-Pinedo and Karlheinz Langanke and Larisa Pacearescu and Amand Faessler and F. Thielemann},
  journal={Nuclear Physics},
  year={2005},
  volume={758},
  pages={154-157}
}
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References

SHOWING 1-10 OF 12 REFERENCES
Parity dependence of nuclear level densities
TLDR
A simple formula for the ratio of the number of odd- and even-parity states as a function of temperature is derived and describes well the transition from low excitation energies where a single parity dominates to high excitations where the two densities are equal.
Nuclear level density and the determination of thermonuclear rates for astrophysics
The prediction of cross sections for nuclei far off stability is crucial in the field of nuclear astrophysics. In recent calculations the nuclear level density{emdash}as an important ingredient to
M1 spin strength distribution in 154Sm
The effect of the residual spin-spin interaction on the M1 spin-flip strength distribution in 154Sm is studied within the quasi-particle random phase approximation. The double-peaked structure found
Phys. Rev. Lett
  • Phys. Rev. Lett
  • 2000
Nucl. Phys. A
  • Nucl. Phys. A
  • 1969
J. Phys. G
  • J. Phys. G
  • 1993
Phys. Lett. B
  • Phys. Lett. B
  • 1979
...
...