“…Another applicability of DF calculations with different types of NN interaction potentials are: density dependent CDM3Y6 [18,19], CDM3Y6-RT proposed by Khoa [20] which takes into account the effect of rearrangement term (RT), velocity dependent Sao Paulo potential (SPP), and independent Brazilian nuclear potential (BNP) given by Chammon et al [21,22] and presented in Refs. [23][24][25][26]. For 11 Li nucleus, Behairy et al [27] discussed the preferable density distribution forms among cluster-orbital shell model approximation (COSMA), Semi-phenomenological (SP), Hartree-Fock (HF) as well as M. Anwar et al examined the cluster model (CM) density for 8 B [28] and two parameters-Fermi (2pF), Gaussian-Oscillator (GO), Gaussian (G) for 6 Li [29] to produce the best fit for the experimental data.…”