[1] ILIADIS C. Nuclear Physics of Stars[M]. Berlin:Wiley-VCH, 2007:536.
[2] SUESS H E, UREY H C. Rev Mod Phys, 1956, 28(1):53.
[3] FERMI E. Z Phys, 1934, 88(161):19.
[4] TAKAHASHI K, YAMADA M. Prog Theor Phys, 1969, 41(6):1470.
[5] TACHIBABA T, YAMADA M, YOSHIDA Y. Prog Theor Phys, 1990, 84(4), 641.
[6] KRATZ K L, HERRMANN G. Z Phys, 1973, 263(5):435.
[7] MÖLLER P, NIX J R, KRATZ K L. At Data Nucl Data Tables, 1997, 66(2):131.
[8] NI D D, REN Z Z, ZHI Q J. Sci China:Phys Mech Astron, 2012, 55(12):2397.
[9] ZHANG X P, REN Z Z, ZHI Q J, et al. J Phys G, 2007, 34(12):2611.
[10] SUZUKI T, YOSHIDA T, KAJINO T, et al. Phys Rev C, 2012, 85(1):015802.
[11] TULI J K. Nuclear Wallet Cards, National Nuclear Data Center. Brookhaven National Laboratory, 2005.
[12] SARGENT B W. Proc R Soc London Ser A, 1933, 139(839):659.
[13] HOLSTEIN B R. Phys Rev C, 1979, 19(4):1467.
[14] LOGUE L J, CHERN B. Phys Rev, 1968, 175(4):1367.
[15] WANG N, LIU M. Phys Lett B, 2014, 734:215.
[16] LORUSSO G, NISHIMURA S, XU Z Y, et al. Phys Rev Lett, 2015, 114(19):192501.
[17] FANG D L, BROWN B A, SUZUKI T. Phys Rev C, 2013, 88(2):024314.
[18] BORZOV I N. Nucl Phys A, 2006, 777:645.