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在恒星演化的过程中,CNO反应链是其能量的重要来源之一。当温度高于10^8K时,高温CNO反应链会取代CNO反应链,成为主要反应。高温链中入射道包含放射性核的重要反应有^13N(p,γ)^14O,^17F(p,γ)^18Ne,^18F(p,α)^15O和^18F(p,γ)^19Ne等。 相似文献
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The radiative capture reaction plays an important role in nuclear astrophysics. We have indirectly measured the astrophysical S(E) factors for some proton capture reactions and reaction rates for several neutron capture reactions with one nucleon transfer reactions at HI-13 tandem accelerator in recent years. Some of them are compiled into IAEA EXFOR database and JINA REACLIB project, and used in the network calculations of Big Bang nucleosynthesis and type-I X-ray bursts. 相似文献
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