(A) Given $\lambda = \frac{m_p c}{\hbar} = \frac{2 \pi m_p c}{h}$. With $m_p = 10^{-6} m_e$,$\lambda = \frac{2 \pi (10^{-6} \times 9.1 \times 10^{-31} \text{ kg}) (3 \times 10^8 \text{ m/s})}{6.63 \times 10^{-34} \text{ J s}} \approx 2.58 \times 10^6 \text{ m}^{-1}$.
Since the Bohr radius $r_B \approx 5.3 \times 10^{-11} \text{ m}$,we have $\lambda r_B \approx 1.37 \times 10^{-4} \ll 1$.
Using the modified potential $U(r) = -\frac{e^2}{4\pi \epsilon_0} \frac{e^{-\lambda r}}{r}$,we expand the exponential for small $\lambda r$: $U(r) \approx -\frac{e^2}{4\pi \epsilon_0} \frac{1-\lambda r}{r} = -\frac{e^2}{4\pi \epsilon_0} (\frac{1}{r} - \lambda)$.
The change in potential energy is $\Delta U = U_{modified} - U_{coulomb} = \frac{e^2}{4\pi \epsilon_0} \lambda$.
Substituting $\frac{e^2}{4\pi \epsilon_0} = k e^2 \approx 1.44 \text{ eV nm} = 1.44 \times 10^{-9} \text{ eV m}$,the energy shift $\Delta E \approx \Delta U = (1.44 \times 10^{-9} \text{ eV m}) (2.58 \times 10^6 \text{ m}^{-1}) \approx 3.7 \times 10^{-3} \text{ eV}$.