Nuclear reaction in which atomic nuclei combine.
Nuclear fusion is a process that powers the sun and the stars, and it holds the promise of providing a nearly limitless, clean source of energy for our planet. In this unit, we will explore the basic principles of fusion, the role of plasma in fusion reactions, and how fusion differs from fission.
Nuclear fusion is a process where two light atomic nuclei combine to form a heavier nucleus. This process releases a tremendous amount of energy, much more than that produced by nuclear fission, the process currently used in nuclear power plants. The fusion process is responsible for the energy produced by the sun and other stars.
In the core of the sun, fusion occurs when hydrogen nuclei (protons) come together under extreme temperature and pressure to form helium, releasing a large amount of energy in the process. On Earth, the most efficient fusion process combines deuterium and tritium, both isotopes of hydrogen, to form helium and a neutron. The energy released in this reaction is carried by the neutron and can be harnessed to produce electricity.
For fusion to occur, the atomic nuclei, which are all positively charged, must overcome their natural repulsion to each other, known as the Coulomb barrier. This requires extremely high temperatures and pressures. In the sun, this is achieved by the immense gravitational pressure at its core. On Earth, we need to create conditions of extreme temperature (over 100 million degrees Celsius) and pressure to achieve fusion.
Fusion and fission are both nuclear processes that release energy, but they are fundamentally different. Fission involves splitting a heavy atomic nucleus, such as uranium or plutonium, into two lighter nuclei. This process releases energy but also produces long-lived radioactive waste. Fusion, on the other hand, involves combining light nuclei to form a heavier nucleus, releasing energy. The primary byproduct of fusion is helium, a non-toxic and non-radioactive gas.
Plasma is often referred to as the fourth state of matter, alongside solids, liquids, and gases. It consists of a hot mix of charged particles – ions and electrons. In the extreme conditions required for fusion, the atoms of the fuel (usually isotopes of hydrogen) are stripped of their electrons, forming a plasma. The plasma must be confined and heated to temperatures high enough for the ions to overcome their mutual repulsion and collide, leading to fusion.
In conclusion, understanding the fundamentals of fusion is the first step towards appreciating the potential of this process as a future energy source. The next units will delve deeper into the history of fusion energy and the challenges faced in harnessing fusion energy.
Hi, any questions for me?