Here are the essential concepts you must grasp in order to answer the question correctly.
Nuclear Fusion
Nuclear fusion is the process where two light atomic nuclei combine to form a heavier nucleus, releasing energy in the process. This energy release occurs because the mass of the resulting nucleus is less than the sum of the masses of the original nuclei, with the mass difference converted into energy according to Einstein's equation, E=mc². Understanding fusion is crucial for analyzing energy changes in nuclear reactions.
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Energy Release in Fusion Reactions
The energy released during fusion reactions varies depending on the specific isotopes involved and the reaction pathway. In the given question, the fusion of deuterons produces different products with distinct energy outputs, which can be quantified in MeV (mega-electronvolts). This energy difference is essential for calculating the energy change in subsequent reactions, such as the one involving
3He and a neutron.
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Gibbs Free Energy of Reactions
Temperature and Reaction Rates
Temperature plays a critical role in nuclear fusion, as it affects the kinetic energy of the particles involved. Higher temperatures provide the necessary energy to overcome the electrostatic repulsion between positively charged nuclei. The process involving
3He and a neutron occurs at lower temperatures because it has a lower Coulomb barrier compared to the fusion of deuterons, allowing the reaction to proceed more readily under less extreme conditions.
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