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Question

The spin-orbit interaction term of an electron moving in a central field is written as $f(r)\vec{l}\cdot\vec{s}$, where $r$ is the radial distance of the electron from the origin. If an electron moves inside a uniformly charged sphere, then

The correct answer is
$f(r) = \text{constant}$

Spin-Orbit Interaction Radial Dependence

The spin-orbit interaction energy ($H_{SO}$) for an electron in a central field is proportional to the dot product of orbital and spin angular momenta ($\vec{l}\cdot\vec{s}$) and depends on the radial part $f(r)$ as given: $H_{SO} = f(r)\vec{l}\cdot\vec{s}$.

The radial function $f(r)$ is determined by the potential $V(r)$ created by the charge distribution. The standard form is:

$f(r) \propto \frac{1}{r}\frac{dV(r)}{dr}$

Electric Field in Uniform Sphere

Consider an electron moving inside a uniformly charged sphere of radius $R$. The electric field $E(r)$ at a distance $r$ from the center ($r < R$) depends on the enclosed charge. Using Gauss's Law, the electric field is found to be proportional to the radius:

$E(r) \propto r$

Potential Gradient Calculation

The electric field is related to the potential $V(r)$ by $E(r) = -\frac{dV(r)}{dr}$. Therefore, the gradient of the potential has the following radial dependence:

$\frac{dV(r)}{dr} = -E(r) \propto -r$

Determining $f(r)$ Dependence

Now, substitute the radial dependence of the potential gradient into the expression for $f(r)$:

$f(r) \propto \frac{1}{r}\frac{dV(r)}{dr}$ $f(r) \propto \frac{1}{r}(-r)$ $f(r) \propto -1$

Conclusion

The result $f(r) \propto -1$ shows that $f(r)$ is a constant value, independent of the radial distance $r$. This corresponds to Option A.

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Important Questions from Angular Momentum Operators Eigenvalues Clebsch Gordan

  1. An electron in the Coulomb field of a proton is in the following state of coherent superposition of orthonormal states $\psi_{nlm}$ 
    $\Psi = \frac{1}{3}\psi_{100} + \frac{1}{\sqrt{3}}\psi_{210} - \frac{\sqrt{5}}{3}\psi_{320}$ 
    Let $E_1, E_2$, and $E_3$ represent the first three energy levels of the system. A sequence of measurements is done on the same system at different times. Energy is measured first at time $t_1$ and the outcome is $E_2$. Then total angular momentum is measured at time $t_2 > t_1$ and finally energy is measured again at $t_3 > t_2$. The probability of finding the system in a state with energy $E_2$ after the final measurement is $P/9$. The value of $P$ is ______________ (in integer).

  2. $H$ is the Hamiltonian, $\vec{L}$ the orbital angular momentum and $L_z$ is the $z$-component of $\vec{L}$. The $1s$ state of the hydrogen atom in the non-relativistic formalism is an eigen function of which one of the following sets of operators?
  3. An atom with non-zero magnetic moment has an angular momentum of magnitude $\sqrt{12}\hbar$. When a beam of such atoms is passed through a Stern-Gerlach apparatus, how many beams does it split into?
  4. In the vector model of angular momentum applied to atoms, what is the minimum angle in degrees (in integer) made by the orbital angular momentum vector and the positive $z$ axis for a $2p$ electron?
  5. A particle has wavefunction 
    $\psi(x,y,z) = N ze^{-\alpha(x^2+y^2+z^2)}$, 
    where $N$ is a normalization constant and $\alpha$ is a positive constant. In this state, which one of the following options represents the eigenvalues of $L^2$ and $L_z$ respectively? 
    Some values of $Y_l^m$ are: 
    $Y_0^0 = \sqrt{\frac{1}{4\pi}}$, $Y_1^0 = \sqrt{\frac{3}{4\pi}} \cos\theta$, $Y_1^{\pm 1} = \mp \sqrt{\frac{3}{8\pi}} \sin\theta e^{\pm i\phi}$

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