[1] S. Wanajo, H.T. Janka, S. Kubono, Uncertaintiesin the νp-process: supernova dynamics versus nuclear physics, Astrophysical Journal (2011) 729-746.
[2] A. Tohsaki, H. Horiuchi, P. Schuck, G.R¨opke, Alpha cluster condensation in 12C and 16O, Physical Review Letters 87 (2001) 192501-192504.
[3] T. Kawabata, H. Akimune, H. Fujimura, H. Fujita, Y. Fujita, M. Fujiwara, K. Hara, K.Y. Hara, K. Hatanaka, T. Ishikawa, et al., Isovector and isoscalar spin-flip M1 strengths in 11B, Physical Review C 70 (2004) 034318-034327.
[4] T. Kawabata, H. Akimune, H. Fujita, Y. Fujita, M. Fujiwara, K. Hara, K. Hatanaka, M. Itoh, Y. Kanada-En’yo, S. Kishi, et al., 2α+t cluster structure in 11B, Physics Letters B 646 (2007) 6-11.
[5] G.M. Fuller, S.E. Woosley, T.A. Weaver. The evolution of radiation-dominated stars. I - Nonrotating supermassive stars.Astrophysical Journal 307 (1986)675-686.
[7] D. Thomas, D.N. Schramm, K.A. Olive, G.J. Mathews, B.S. Meyer, B.D. Fields, Production of lithium, beryllium, and boron from baryon inhomogeneous primordial nucleosynthesis, Astrophysical Journal 430 (1994) 291-299.
[8] A. Coc, S. Goriely, Y. Xu, M. Saimpert, E. Vangioni, standard Big Bang Nucleosynthesis up to CNO with an improved extended nuclear network, Astrophysical Journal 744 (2012) 158-190.
[9] M. Wiescher, J. G¨orres, S. Graff, L. Buchmann, F.K. Thielemann, The Hot Proton-Proton Chains in Low Metallicity Objects, Astrophysical Journal 343 (1989) 352-364.