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Problem The CNO cycle is a series of nuclear fusion reactions taking place in massive stars. It consists of the reactions
1 1 H + 6 12 C → 7 13 N + γ {}_{1}^{1}\text{H} + {}_{6}^{12}\text{C} \rightarrow {}_{7}^{13}\text{N} + \gamma 1 1 H + 6 12 C → 7 13 N + γ
7 13 N → 6 13 C + 1 0 e + + ν {}_{7}^{13}\text{N} \rightarrow {}_{6}^{13}\text{C} + {}_{1}^{0}\text{e}^{+} + \nu 7 13 N → 6 13 C + 1 0 e + + ν
1 1 H + 6 13 C → 7 14 N + γ {}_{1}^{1}\text{H} + {}_{6}^{13}\text{C} \rightarrow {}_{7}^{14}\text{N} + \gamma 1 1 H + 6 13 C → 7 14 N + γ
1 1 H + 7 14 N → 8 15 O + γ {}_{1}^{1}\text{H} + {}_{7}^{14}\text{N} \rightarrow {}_{8}^{15}\text{O} + \gamma 1 1 H + 7 14 N → 8 15 O + γ
8 15 O → 7 15 N + 1 0 e + + ν {}_{8}^{15}\text{O} \rightarrow {}_{7}^{15}\text{N} + {}_{1}^{0}\text{e}^{+} + \nu 8 15 O → 7 15 N + 1 0 e + + ν
1 1 H + 7 15 N → 6 12 C + 2 4 He {}_{1}^{1}\text{H} + {}_{7}^{15}\text{N} \rightarrow {}_{6}^{12}\text{C} + {}_{2}^{4}\text{He} 1 1 H + 7 15 N → 6 12 C + 2 4 He
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