The binding energy per nucleon is a critical concept in nuclear physics that relates to the stability of a nucleus. It indicates how tightly the nucleons (protons and neutrons) are held together in the nucleus. Let's explore how the binding energy per nucleon changes as the mass number (the total number of protons and neutrons) increases.
This explanation shows that the correct answer is: "First increases and then decreases with increase in mass number". The other options can be ruled out because:
In summary, the variation in binding energy per nucleon first increases to a peak in stable middle-mass elements and then decreases as the nucleus becomes larger due to competing forces within the nucleus.
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: