
- ✓$(1, n),\left(2, p^{+}\right),\left(3, e^{-}\right)$
- B$\left(1, p^{+}\right),\left(2, e^{-}\right),(3, n)$
- C$\left(1, e^{-}\right),\left(2, p^{+}\right),(3, n)$
- D$\left(1, p^{+}\right),(2, n),\left(3, e^{-}\right)$

For an electron and nucleus pair, Potential energy $=\frac{K(-e)(+Z e)}{r}$
$=\frac{-K Z e^2}{r}$
So, potential energy of electron is negative and it tends to zero as separation $r$ increases.
Hence, correct variation of potential energy with $r$ is as shown in graph $(3)$. For a neutron, force outside nucleus is zero.
Hence, potential energy of neutron is zero as $r > r_0$.
So, correct variation of potential energy with $r$ for a neutron is as shown in graph $(1)$.
For a proton, as $r > r_0$, force is repulsive. Hence, potential energy is positive.
So, correct variation of potential energy with $r$ is as shown in graph $(2)$.
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Reason : The stars are much bigger in size than the planets.
Which of the following statement($s$) is(are) correct?
$(A)$ $E_b^p-E_b^n$ is proportional to $Z(Z-1)$ where $Z$ is the atomic number of the nucleus.
$(B)$ $E_b^p-E_b^n$ is proportional to $A^{-\frac{1}{3}}$ where $A$ is the mass number of the nucleus.
$(C)$ $E_b^p-E_b^n$ is positive.
$(D)$ $E_b^p$ increases if the nucleus undergoes a beta decay emitting a positron.
