Nuclear fusion is a process in which two light atomic nuclei combine to form a heavier nucleus, releasing a large amount of energy in the process. This process powers the sun and other stars, and has the potential to provide a clean and virtually limitless source of energy here on Earth.
In nuclear fusion, the nuclei of two light atoms, such as hydrogen isotopes deuterium and tritium, are forced together at extremely high temperatures and pressures. The strong nuclear force causes the nuclei to overcome their electrostatic repulsion and fuse together, forming a heavier nucleus and releasing a significant amount of energy in the form of gamma rays and kinetic energy of the newly formed nucleus.
Here are some key points to understand about nuclear fusion:
Understanding the process of nuclear fusion and its potential as a clean and abundant energy source is crucial for addressing future energy needs and environmental sustainability.
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