The carbon nitrogen oxygen cycle (carbon nitrogen oxygen), sometimes called the Bess Weitzzek cycle, isfixed startakehydrogenconvert toheliumOne of the two processes ofProton proton chainReaction.
In stars with masses like the sun or smaller,Proton proton chain reactionIs the main process of generating energy. The sun has only 1.7%fourThe He core is generated through the carbon nitrogen oxygen cycle, but the theoretical model shows thatHeavier stars generate energy mainly from the carbon nitrogen oxygen cycle。The process of carbon nitrogen oxygen cycle is composed ofCarl von WeizsäckerandHans BateThey were put forward independently in 1938 and 1939 respectively.
The reaction of carbon nitrogen oxygen cycle is as follows:
twelveC +oneH →thirteenN + γ +1.95 MeV
thirteenN →thirteenC + e++ νe+2.22 MeV
thirteenC +oneH →fourteenN + γ +7.54 MeV
fourteenN +oneH →fifteenO + γ +7.35 MeV
fifteenO →fifteenN + e++ νe+2.75 MeV
fifteenN +oneH →twelveC +fourHe +4.96 MeV
The net effect of this cycle is 4protonBecome aAlpha particle, 2positron(andElectronicsAnnihilation toGamma rayAnd two neutrinos carrying part of the energy escaped from the star.Carbon, nitrogen, and oxygen nuclei act as catalysts and regenerate in the cycle.
exceptional case
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In special cases, there is a small branch reaction, which only accounts for 0.04% of the total amount in the solar core. The final product is not 12 carbon and 4 helium, but 16 oxygen and a photon. The replacement process is as follows:
fifteenN +oneH →sixteenO + γ +12.13 MeV
sixteenO +oneH →seventeenF + γ +0.60 MeV
seventeenF →seventeenO +e++ νe+2.76 MeV
seventeenO +oneH →fourteenN +fourHe +1.19 MeV
Effect of fluorine
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Similarly, carbon, nitrogen, and oxygen are in the main branch, while in the smaller branchfluorineIt is only a catalyst in a stable state and will not accumulate in the star.
III Branch
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The main branch of the carbon nitrogen oxygen cycle is called carbon nitrogen oxygen I, and the small branch is called carbon nitrogen oxygen II. In the heavier stars, there are two secondary main branches, carbon nitrogen oxygen III and carbon nitrogen oxygen IV, which begin at the final stage of the carbon nitrogen oxygen II reaction, and result in the replacement of the original 14 nitrogen and helium nuclei with 18 oxygen and gamma rays
III Branch reaction:
seventeenO +oneH →eighteenF
eighteenF →eighteenO +e++ νe+ γ
IV Branch
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seventeenO +oneH →eighteenF + γ +5.61 MeV
eighteenF →eighteenO + e++ ve+1.656 MeV
eighteenO+oneH →nineteenF + γ +7.994 MeV
nineteenF +oneH →sixteenO +fourHe +8.114MeV
sixteenO+oneH →seventeenF + γ +0.6MeV
seventeenF →seventeenO + e++ ve+2.76MeV
Schematic diagram of carbon nitrogen oxygen cycle
Here, the number of all "catalysts" (carbon, nitrogen and oxygen nuclei) involved in the reaction is conserved, and the relative proportion of nuclei will change in the evolution of stars.No matter what the initial structure is, when the cycle is in equilibrium,twelveCarbon/thirteenThe proportion of carbon nuclei is 3.5, whilefourteenNitrogen became the most abundant nucleus.In the evolution of stars, convection will bring the products of carbon, nitrogen and oxygen cycle from the interior of stars to the surface and mix, changing the observed stellar composition.In red giant stars, compared withMain sequence star, a small amount oftwelveCarbon/thirteenCarbon andtwelveCarbon/fourteenNitrogen, all of which can prove that hydrogen fuses in the interior of stars for energy generation alternation.