Nuclear Level Density in the X(1266, 354) System

Single particle levels for the X(1266, 354) system as a function of energy are modeled using various functional forms. A power law form N(E) = a Eb for the total number of energy levels provides a better fit than the constant temperature and equidistant models. The number of energy levels/MeV is not well-fit by the commonly used constant temperature model. Model results are compared to existing systems as well as postulated theoretical superheavy nuclei. The comparison suggests that the level density characteristics of light systems and theoretical superheavy systems are different.