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Nuclear & Quantum Physics E.5 Stellar Properties & Processes (id: 43871a4ea)

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admin 发表于 2024-2-10 18:56:35 | 显示全部楼层 |阅读模式
本题目来源于试卷: Nuclear & Quantum Physics E.5 Stellar Properties & Processes,类别为 IB物理学

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1.A star X is burning carbo*id/y+ lupk7fy* :uau n u).b1zud5 ll jn)tk+pin its core. The reaction is given by:
$^{12}_{6}C$+$^{12}_{6}C$→$^{24}_{12}​Mg$
The following data are available for the reaction.
Rest mass of the$^{12}_{6}C$= 12.0111507u
Rest mass of the$^{24}_{12}​Mg$= 23.9909630u
Determine, in MeV, the energy released in the reaction. Be sure to express your answer to the correct number of significant figures. $ΔE$ =    MeV
2.The star Y is a red supergiant. State the next steps in the evolutionary sequence of the star Y.
3.Outline why the sun is not expected to undergo carbon fusion.




参考答案: 29.19±2%


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