M(N, Z) = NMn + ZMP + Bc2
M(N, Z) = NMn + ZMP – \(\frac{B}{c^2}\)
M(N, Z) = NMn + ZMP +\(\frac{B}{c^2}\)
M(N, Z) = NMn + ZMP – Bc2
To solve this problem, we need to understand the concept of nuclear binding energy and its relation to the mass of a nucleus.
The binding energy \( B \) of a nucleus is the energy required to disassemble the nucleus into its constituent protons and neutrons. It is a measure of the stability of the nucleus. According to Einstein's mass-energy equivalence principle, the binding energy can be expressed in terms of mass as:
E = \frac{B}{c^2}
Here, \( c \) is the speed of light in a vacuum.
The mass of a nucleus \( M(N, Z) \) can be calculated by subtracting the equivalent mass of the binding energy from the total mass of its individual protons and neutrons. Therefore, this is given by:
Hence, the total mass of protons and neutrons (without considering binding energy) is:
\( Total\_mass = N M_n + Z M_p \)
The actual mass of the nucleus is less than this total mass by the amount corresponding to the binding energy. Therefore, the correct formula for the mass of the nucleus is:
\( M(N, Z) = N M_n + Z M_p - \frac{B}{c^2} \)
Thus, among the given options, the correct answer is:
\( M(N, Z) = N M_n + Z M_p - \frac{B}{c^2} \)
This choice reflects the fact that the binding energy reduces the total mass of the nucleus compared to the isolated nucleons.
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: