Abstract

Statistical level density ρ(E,A)ρ(E,A) is derived for nucleonic system with a given energy EE, particle number AA and other integrals of motion in the micro-macroscopic approximation beyond the standard saddle-point method of the Fermi gas model. This level density reaches the two limits; the well-known Fermi gas grand-canonical ensemble limit for a large entropy SS related to large excitation energies, and the finite micro-canonical limit for a small combinatorical entropy SS at low excitation energies. The inverse level density parameter KK as function of the particle number AA in the semiclassical periodic orbit theory, taking into account the extended Thomas-Fermi and Strutinsky shell corrections, is calculated and compared with experimental data.

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