“…The most common proton halo is the 8 B nuclei which has low break up threshold. The 8 B nuclei has a weakly bound proton with a proton separation energy Sp =0.137 MeV and its half-life is t1/2=770 ms. Nuclear reactions and densities involving short-lived 8 B nuclei have been extensively investigated by both nuclear astrophysicists, experimental and theoretical nuclear physicist (Aguilera et al, 2011;Aguilera, Martinez-Quiroz, Belyaeva, Kolata, & Leyte-Gonzalez, 2008;Aguilera et al, 2009;Aguilera, Martinez-Quiroz, Rosales, et al, 2008;Barioni et al, 2011;Camacho, Aguilera, Gomes, & Lubian, 2011;Camacho, Aguilera, Lubian, & Gomes, 2013;Carlson et al, 2015;Chandel, Dhiman, & Shyam, 2003;Horii, Takashina, Furumoto, Sakuragi, & Toki, 2010;Lubian et al, 2009;Lubian & Nunes, 2007;Mackintosh & Pang, 2013;Mitchell et al, 2010;Morcelle et al, 2017;Moro, Crespo, Nunes, & Thompson, 2002;Varga, Suzuki, & Tanihata, 1995;Yang et al, 2013). In the theoretical analysis microscopic and phenomenological potential approximations have been used in explaining the measured experimental data.…”