In order to overcome the coulomb repulsion between nuclei as two lighter nuclei join to produce a heavier nucleus, high temperature, and high pressure are necessary.
To understand why fusion reactions require high temperatures, let's delve into the fundamental principles involved in nuclear fusion.
Nuclear fusion is a process where two light atomic nuclei combine to form a heavier nucleus. This process releases a significant amount of energy and is the principle that powers stars, including our sun.
At the atomic level, atomic nuclei are positively charged, which leads to repulsion due to the Coulomb force (electromagnetic repulsion between like charges). To initiate a fusion reaction, the following conditions are needed:
Among the options given, the reason fusion takes place at high temperatures is correctly described by:
In summary, high temperatures in fusion reactions provide the necessary kinetic energy to overcome the electrostatic repulsion between nuclei, allowing them to collide and fuse, releasing vast amounts of energy.
The electric potential at the surface of an atomic nucleus \( (z = 50) \) of radius \( 9 \times 10^{-13} \) cm is \(\_\_\_\_\_\_\_ \)\(\times 10^{6} V\).
In a nuclear fission reaction of an isotope of mass \( M \), three similar daughter nuclei of the same mass are formed. The speed of a daughter nuclei in terms of mass defect \( \Delta M \) will be: