available models.

On the other hand, one of the oldest problems of nuclear physics is the nuclear binding energies: The interactions between nucleons are very strong, while the nuclear matter is not relativistic. Nuclear binding energies are experimentally known with high accuracy while they are not predicted with sufficient accuracy using different theoretical models. Since, prediction of nuclear binding energy is a useful tool to test the goodness of a theoretical nucleon-nucleon (NN) interaction model, we use our NN holography potential to obtain the light nuclei binding energies. We construct a nuclear holographic model \[50-53\] in the noncritical base and calculate the nuclei potentials as the sum of their NN interactions. The minimum of the ground state potential is considered as the binding energy. Also, difference between this energy and the minimum of the excited state potential presents the excited energy for each state. In order to compute the potentials, we use the values of nucleon-meson coupling constants obtained from both the critical and noncritical holography models.

This paper is organized as follows: In Sec. 2 we briefly review the AdS/CFT correspondence. The noncritical holographic model is introduced in Sec. 3 and NN potential is constructed in this section. In 