A particle of mass $m$ moves in a potential that is $V = \frac{1}{2}m(\omega_1^2 x^2 + \omega_2^2 y^2 + \omega_3^2 z^2)$ in the coordinates of a non-inertial frame $F$. The frame $F$ is rotating with respect to an inertial frame with an angular velocity $\hat{\mathbf{k}}\Omega$, where $\hat{\mathbf{k}}$ is the unit vector along their common $z$-axis. The motion of the particle is unstable for all angular frequencies satisfying
In the rotating frame with angular velocity $\vec{\Omega} = \Omega\hat{\mathbf{k}}$, the effective potential includes the centrifugal term:
$$V_{\text{eff}} = V - \frac{1}{2}m |\vec{\Omega} \times \vec{r}|^2 = \frac{1}{2}m [(\omega_1^2 - \Omega^2)x^2 + (\omega_2^2 - \Omega^2)y^2 + \omega_3^2 z^2]$$
The equations of motion including the Coriolis force $\vec{F}_{\text{cor}} = 2m(\vec{v} \times \vec{\Omega}) = 2m(\dot{y}\Omega \hat{\mathbf{i}} - \dot{x}\Omega \hat{\mathbf{j}})$ are:
$$\ddot{x} - 2\Omega \dot{y} + (\omega_1^2 - \Omega^2)x = 0$$
$$\ddot{y} + 2\Omega \dot{x} + (\omega_2^2 - \Omega^2)y = 0$$
$$\ddot{z} + \omega_3^2 z = 0$$
Assuming normal modes of the form $x, y \propto e^{i\omega t}$, the characteristic equation for the frequencies in the $xy$-plane is obtained from:
$$\begin{vmatrix} -\omega^2 + (\omega_1^2 - \Omega^2) & -2i\Omega\omega \\ 2i\Omega\omega & -\omega^2 + (\omega_2^2 - \Omega^2) \end{vmatrix} = 0$$
Expanding the determinant:
$$(\omega^2 - (\omega_1^2 - \Omega^2))(\omega^2 - (\omega_2^2 - \Omega^2)) - 4\Omega^2 \omega^2 = 0$$
$$\omega^4 - (\omega_1^2 + \omega_2^2 + 2\Omega^2)\omega^2 + (\omega_1^2 - \Omega^2)(\omega_2^2 - \Omega^2) = 0$$
Letting $\Lambda = \omega^2$, we have a quadratic equation:
$$\Lambda^2 - (\omega_1^2 + \omega_2^2 + 2\Omega^2)\Lambda + (\omega_1^2 - \Omega^2)(\omega_2^2 - \Omega^2) = 0$$
For stable oscillatory motion, all roots $\Lambda = \omega^2$ must be real and positive.
If the constant term of the quadratic equation is negative, i.e.,
$$(\omega_1^2 - \Omega^2)(\omega_2^2 - \Omega^2) = (\Omega^2 - \omega_1^2)(\Omega^2 - \omega_2^2) < 0$$
then the product of the two roots is negative. This guarantees that one root $\Lambda = \omega^2$ is strictly negative, which means $\omega = \pm i |\omega|$, leading to exponentially growing solutions $e^{|\omega| t}$, and thus the motion is definitively unstable. Hence, the motion is unstable for all angular frequencies satisfying $(\Omega^2 - \omega_1^2)(\Omega^2 - \omega_2^2) < 0$.
Q1mcq
The Hamiltonian of a particle of mass $m$ in one-dimension is $H = \frac{1}{2m} p^2 + \lambda |x|^3$; where $\lambda > 0$ is a constant. If $E_1$ and $E_2$, respectively, denote the ground-state energies of the particle for $\lambda = 1$ and $\lambda = 2$ (in appropriate units) the ratio $E_2 / E_1$ is best approximated by
a.
1.260
b.
1.414
c.
1.516
d.
1.320
Correct Answer
Step-by-Step AI Explanation
Verified Method
To find how the energy scales with the coupling constant $\lambda$, we can use a scaling argument on the time-independent Schrödinger equation:
$$-\frac{\hbar^2}{2m} \frac{d^2\psi}{dx^2} + \lambda |x|^k \psi = E \psi$$
Let $x = c y$. Then $\frac{d^2}{dx^2} = \frac{1}{c^2}\frac{d^2}{dy^2}$. The equation becomes:
$$-\frac{\hbar^2}{2m c^2} \frac{d^2\psi}{dy^2} + \lambda c^k |y|^k \psi = E \psi$$
To make the equation dimensionless or independent of $\lambda$, we set the scaling factor such that the coefficients of the kinetic and potential terms are proportional, meaning:
$$\frac{1}{c^2} \propto \lambda c^k \implies c^{k+2} \propto \lambda^{-1} \implies c \propto \lambda^{-1/(k+2)}$$
Then the energy eigenvalues scale as:
$$E \propto \frac{1}{c^2} \propto \lambda^{2/(k+2)}$$
Here, the potential has $k = 3$, so:
$$E \propto \lambda^{2/(3+2)} = \lambda^{2/5}$$
Therefore, the ratio of the ground-state energies for $\lambda_2 = 2$ and $\lambda_1 = 1$ is:
$$\frac{E_2}{E_1} = \left(\frac{\lambda_2}{\lambda_1}\right)^{2/5} = 2^{2/5} = 2^{0.4} = 4^{0.2} \approx 1.3195$$
Rounding to three decimal places gives $1.320$, which corresponds to Option D.
Q2mcq
Potassium chloride forms an FCC lattice, in which K and Cl occupy alternating sites. The density of KCl is $1.98\text{ g/cm}^3$ and the atomic weights of K and Cl are $39.1$ and $35.5$, respectively. The angles of incidence (in degrees) for which Bragg peaks will appear when X-ray of wavelength $0.4\text{ nm}$ is shone on a KCl crystal are
a.
$18.5$, $39.4$ and $72.2$
Correct Answer
b.
$19.5$ and $41.9$
c.
$12.5$, $25.7$, $40.5$ and $60.0$
d.
$13.5$, $27.8$, $44.5$ and $69.0$
Step-by-Step AI Explanation
Verified Method
Potassium chloride has the rock-salt (NaCl-type) structure, with 4 formula units per conventional cubic unit cell.
The mass of a unit cell is:
$$M_{\text{cell}} = \frac{4 \times (39.1 + 35.5)\text{ g/mol}}{6.022 \times 10^{23}\text{ mol}^{-1}} = \frac{4 \times 74.6}{6.022 \times 10^{23}}\text{ g} \approx 4.955 \times 10^{-22}\text{ g}$$
The volume of the unit cell is $a^3 = \frac{M_{\text{cell}}}{\rho} = \frac{4.955 \times 10^{-22}}{1.98}\text{ cm}^3 \approx 2.503 \times 10^{-22}\text{ cm}^3 = 2.503 \times 10^{-28}\text{ m}^3$.
Thus, the lattice parameter is:
$$a = (2.503 \times 10^{-28})^{1/3}\text{ m} \approx 0.630\text{ nm} = 6.30\text{ \AA}$$
However, since $\text{K}^+$ and $\text{Cl}^-$ have nearly identical numbers of electrons ($18$ electrons each), they scatter X-rays almost identically ($f_{\text{K}^+} \approx f_{\text{Cl}^-}$). Thus, the crystal behaves like a simple cubic lattice with lattice parameter $a' = a/2 \approx 0.315\text{ nm}$, or systematically reflections appear when all indices are even, etc.
Let us check Bragg's law $2d\sin\theta = \lambda = 0.4\text{ nm}$:
For (200), $d_{200} = a/2 = 0.315\text{ nm}$, $\sin\theta = \frac{\lambda}{2d} = \frac{0.4}{2 \times 0.315} = 0.6349 \implies \theta = 39.4^\circ$.
Wait, if (111) is considered: with $f_K \approx f_{Cl}$, (111) is very weak or absent. If we consider all FCC reflections:
For $d_{111} = a/\sqrt{3} = 0.630/\sqrt{3} = 0.364\text{ nm}$, $\sin\theta = 0.4/(2 \times 0.364) = 0.550 \implies \theta = 33.3^\circ$.
For (110) of simple cubic with $a' = 0.315\text{ nm}$, $d = 0.315/\sqrt{2} = 0.223\text{ nm}$, $\sin\theta = 0.4 / (2 \times 0.223) = 0.898 \implies \theta = 63.9^\circ$.
Wait, let's look at Option A: $18.5^\circ, 39.4^\circ, 72.2^\circ$.
$\sin(18.5^\circ) = 0.3173 \approx 0.4 / (2 \times 0.630) = 0.3175$, which corresponds to $d = 0.630\text{ nm}$, i.e., the $(100)$ plane with lattice parameter $a = 0.63\text{ nm}$!
$\sin(39.4^\circ) = 0.6347 \approx 2 \times 0.3175$, corresponding to $(200)$!
$\sin(72.2^\circ) = 0.952 \approx 3 \times 0.3175$, corresponding to $(300)$!
So these are successive orders of reflection from the (100) family with $d = a = 0.630\text{ nm}$ (or $n = 1, 2, 3$ in $2d\sin\theta = n\lambda$).
Thus, option A matches precisely.
Q2mcq
A particle of mass $1\text{ GeV}/c^2$ and its antiparticle, both moving with the same speed $v$, produce a new particle $X$ of mass $10\text{ GeV}/c^2$ in a head-on collision. The minimum value of '$v$' required for this process is closest to
a.
$0.83\ c$
b.
$0.93\ c$
c.
$0.98\ c$
Correct Answer
d.
$0.88\ c$
Step-by-Step AI Explanation
Verified Method
Let the particle and antiparticle have rest mass $m = 1\text{ GeV}/c^2$. They move head-on with equal speed $v$, so the total momentum in the lab frame is zero. The new particle $X$ can be produced at rest with mass $M = 10\text{ GeV}/c^2$.
From conservation of energy:
$$2\gamma m c^2 = M c^2 \implies \gamma = \frac{M}{2m} = \frac{10}{2\times 1} = 5$$
Since $\gamma = \frac{1}{\sqrt{1 - v^2/c^2}} = 5$:
$$1 - \frac{v^2}{c^2} = \frac{1}{25} = 0.04$$
$$\frac{v}{c} = \sqrt{1 - 0.04} = \sqrt{0.96} \approx 0.9798 \approx 0.98$$
Thus, the required speed is closest to $0.98\ c$.
Q3mcq
A particle of mass $m$ is in a one-dimensional infinite potential well of length $L$, extending from $x = 0$ to $x = L$. When it is in the energy eigenstate labelled by $n, (n = 1, 2, 3, ....)$ the probability of finding it in the interval $0 \le x \le (L/8)$ is $1/8$. The minimum value of $n$ for which this is possible is
a.
4
Correct Answer
b.
2
c.
6
d.
8
Step-by-Step AI Explanation
Verified Method
The wavefunctions in an infinite square well of length $L$ are $\psi_n(x) = \sqrt{\frac{2}{L}}\sin\left(\frac{n\pi x}{L}\right)$.
The probability $P$ of finding the particle in $[0, L/8]$ is:
$$P = \int_0^{L/8} |\psi_n(x)|^2 dx = \frac{2}{L} \int_0^{L/8} \sin^2\left(\frac{n\pi x}{L}\right) dx$$
Using $\sin^2\theta = \frac{1 - \cos(2\theta)}{2}$:
$$P = \frac{2}{L} \left[ \frac{x}{2} - \frac{\sin(2n\pi x / L)}{4n\pi / L} \right]_0^{L/8} = \frac{2}{L} \left( \frac{L}{16} - \frac{\sin(n\pi / 4)}{4n\pi / L} \right) = \frac{1}{8} - \frac{\sin(n\pi/4)}{2n\pi}$$
For this probability to equal $1/8$, we must have:
$$\frac{\sin(n\pi/4)}{2n\pi} = 0 \implies \sin\left(\frac{n\pi}{4}\right) = 0$$
This requires $\frac{n\pi}{4} = k\pi$ for some integer $k \ge 1$, which gives $n = 4k$.
The minimum positive integer $n$ is for $k = 1$, giving $n = 4$.
Q3mcq
The energies of a two-state quantum system are $E_0$ and $E_0 + \alpha\hbar$ (where $\alpha > 0$ is a constant) and the corresponding normalized state vectors are $|0\rangle$ and $|1\rangle$, respectively. At time $t = 0$, when the system is in the state $|0\rangle$, the potential is altered by a time independent term $V$ such that $\langle 1|V|0\rangle = (\hbar\alpha / 10)$. The transition probability to the state $|1\rangle$ at times $t \ll (1/\alpha)$, is
a.
$\frac{\alpha^2 t^2}{25}$
b.
$\frac{\alpha^2 t^2}{50}$
c.
$\frac{\alpha^2 t^2}{100}$
Correct Answer
d.
$\frac{\alpha^2 t^2}{200}$
Step-by-Step AI Explanation
Verified Method
From time-dependent perturbation theory, the transition probability from $|0\rangle$ to $|1\rangle$ under a perturbation $V$ is given by:
$$P_{0\to 1}(t) = \frac{1}{\hbar^2} \left| \int_0^t \langle 1|V|0\rangle e^{i\omega_{10} t'} dt' \right|^2$$
where $\omega_{10} = \frac{E_1 - E_0}{\hbar} = \frac{\alpha\hbar}{\hbar} = \alpha$.
Given that $\langle 1|V|0\rangle = \frac{\hbar\alpha}{10}$, we have:
$$P_{0\to 1}(t) = \frac{1}{\hbar^2} \left| \frac{\hbar\alpha}{10} \int_0^t e^{i\alpha t'} dt' \right|^2 = \frac{\alpha^2}{100} \left| \frac{e^{i\alpha t} - 1}{i\alpha} \right|^2 = \frac{\alpha^2}{100} \frac{4\sin^2(\alpha t / 2)}{\alpha^2} = \frac{1}{25}\sin^2\left(\frac{\alpha t}{2}\right)$$
For $t \ll 1/\alpha$, we have $\alpha t \ll 1$, so we can approximate $\sin\left(\frac{\alpha t}{2}\right) \approx \frac{\alpha t}{2}$:
$$P_{0\to 1}(t) \approx \frac{1}{25} \left(\frac{\alpha t}{2}\right)^2 = \frac{\alpha^2 t^2}{100}.$$
Therefore, the correct option is C.
Q4mcq
A particle in one dimension executes oscillatory motion in a potential $V(x) = A|x|$, where $A > 0$ is a constant of appropriate dimension. If the time period $T$ of its oscillation depends on the total energy $E$ as $E^\alpha$, then the value of $\alpha$ is
a.
$1/3$
b.
$1/2$
Correct Answer
c.
$2/3$
d.
$3/4$
Step-by-Step AI Explanation
Verified Method
For a potential of the form $V(x) = A|x|^k$, the time period of oscillation scales with energy as $T \propto E^{\frac{1}{k} - \frac{1}{2}}$.
Here, the potential is $V(x) = A|x|^1$, so $k = 1$.
Therefore, the energy dependence is:
$$T \propto E^{\frac{1}{1} - \frac{1}{2}} = E^{1/2}$$
Hence, $\alpha = 1/2$, which corresponds to Option B.
Alternatively, calculating directly:
$$T = 4\int_0^{x_{\max}} \frac{dx}{\sqrt{\frac{2}{m}(E - Ax)}} = 4\sqrt{\frac{m}{2}} \left[ -\frac{2}{A} \sqrt{E - Ax} \right]_0^{E/A} = \frac{8\sqrt{m}}{A\sqrt{2}} E^{1/2} \propto E^{1/2}.$$
Thus, $\alpha = 1/2$.
Q4mcq
The Newton-Raphson method is to be used to determine the reciprocal of the number $x = 4$. If we start with the initial guess $0.20$ then after the first iteration the reciprocal is
a.
0.23
b.
0.24
Correct Answer
c.
0.25
d.
0.26
Step-by-Step AI Explanation
Verified Method
To find the reciprocal of $N = 4$ using the Newton-Raphson method, we define the function whose zero is $1/N$:
$$f(y) = \frac{1}{y} - N = 0$$
The derivative is $f'(y) = -\frac{1}{y^2}$.
The Newton-Raphson iteration formula is:
$$y_{n+1} = y_n - \frac{f(y_n)}{f'(y_n)} = y_n - \frac{\frac{1}{y_n} - N}{-\frac{1}{y_n^2}} = y_n + y_n^2\left(\frac{1}{y_n} - N\right) = y_n(2 - Ny_n)$$
Given the initial guess $y_0 = 0.20$ and $N = 4$:
$$y_1 = 0.20 \times (2 - 4 \times 0.20) = 0.20 \times (2 - 0.80) = 0.20 \times 1.20 = 0.24$$
Thus, after the first iteration, the value is $0.24$.
Q5mcq
Which of the following two physical quantities cannot be measured simultaneously with arbitrary accuracy for the motion of a quantum particle in three dimensions ?
a.
Square of the radial position and $z$-component of angular momentum ($r^2$ and $L_z$)
b.
$x$-components of linear and angular momenta ($p_x$ and $L_x$)
c.
$y$-components of position and $z$-component of angular momentum ($y$ and $L_z$)
Correct Answer
d.
Square of the magnitudes of the linear and angular momenta ($\mathbf{p}^2$ and $\mathbf{L}^2$)
Step-by-Step AI Explanation
Verified Method
Two observables cannot be measured simultaneously with arbitrary accuracy if their corresponding quantum operators do not commute, i.e., $[A, B] \neq 0$.
Let us evaluate the commutators for each pair:
- **Option A:** $[r^2, L_z] = [x^2+y^2+z^2, x p_y - y p_x] = [x^2+y^2, x p_y - y p_x] = 0$. Since $r^2$ is a scalar (rotationally invariant), it commutes with all components of angular momentum.
- **Option B:** $[p_x, L_x] = [p_x, y p_z - z p_y] = 0$, because $p_x$ commutes with $y, z, p_y, p_z$.
- **Option C:** Using $L_z = x p_y - y p_x$, we find:
$$[y, L_z] = [y, x p_y - y p_x] = x [y, p_y] = i\hbar x \neq 0$$
Since the commutator is non-zero, $y$ and $L_z$ are incompatible observables and cannot be measured simultaneously with arbitrary precision.
- **Option D:** $\mathbf{p}^2$ is proportional to the kinetic energy operator for a free particle, which is a scalar under rotations, so $[\mathbf{p}^2, L_i] = 0$ for all components $i=x,y,z$. Consequently, $[\mathbf{p}^2, \mathbf{L}^2] = 0$.
Therefore, the correct pair is given in Option C.
Q5mcq
A satellite of mass $m$ orbits around earth in an elliptic trajectory of semi-major axis $a$. At a radial distance $r = r_0$, measured from the centre of the earth, the kinetic energy is equal to half the magnitude of the total energy. If $M$ denotes the mass of the earth and the total energy is $-\frac{GMm}{2a}$, the value of $r_0/a$ is nearest to
a.
1.33
Correct Answer
b.
1.48
c.
1.25
d.
1.67
Step-by-Step AI Explanation
Verified Method
The total energy in an elliptical orbit is given by $E = -\frac{GMm}{2a}$.
The kinetic energy is $T$ and the potential energy is $V(r) = -\frac{GMm}{r}$.
We are given that at $r = r_0$, the kinetic energy is half the magnitude of the total energy:
$$T = \frac{1}{2} |E| = \frac{1}{2} \left(\frac{GMm}{2a}\right) = \frac{GMm}{4a}$$
Since $E = T + V(r_0)$, we have:
$$-\frac{GMm}{2a} = \frac{GMm}{4a} - \frac{GMm}{r_0}$$
Dividing by $GMm$:
$$-\frac{1}{2a} = \frac{1}{4a} - \frac{1}{r_0} \implies \frac{1}{r_0} = \frac{1}{4a} + \frac{1}{2a} = \frac{3}{4a}$$
Thus,
$$\frac{r_0}{a} = \frac{4}{3} \approx 1.33$$
Hence, the correct choice is A.
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A two-state system evolves under the action of the Hamiltonian $H = E_0 |A\rangle\langle A| + (E_0 + \Delta)|B\rangle\langle B|$, where $|A\rangle$ and $|B\rangle$ are its two orthonormal states. These states transform to one another under parity i.e., $P|A\rangle = |B\rangle$ and $P|B\rangle = |A\rangle$. If at time $t = 0$ the system is in a state of definite parity $P = 1$, the earliest time $t$ at which the probability of finding the system in a state of parity $P = -1$ is one, is
a.
$\frac{\pi\hbar}{2\Delta}$
b.
$\frac{\pi\hbar}{\Delta}$
c.
$\frac{3\pi\hbar}{2\Delta}$
d.
$\frac{2\pi\hbar}{\Delta}$
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A laser beam propagates from fiber 1 to fiber 2 in a cavity made up of two optical fibers (as shown in the figure). The loss factor of fiber 2 is $10\text{ dB/km}$. If $E_2(d)$ denotes the magnitude of the electric field in fiber 2 at a distance $d$ from the interface, the ratio $\frac{E_2(0)}{E_2(d)}$ for $d = 10\text{ km}$, is
a.
$10^2$
b.
$10^3$
c.
$10^5$
d.
$10^7$
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A generic $3 \times 3$ real matrix $A$ has eigenvalues $0$, $1$ and $6$, and $I$ is the $3 \times 3$ identity matrix. The quantity/quantities that cannot be determined from this information is/are the
a.
eigenvalues of $(I + A)^{-1}$
b.
eigenvalues of $(I + A^TA)$
c.
determinant of $A^TA$
d.
rank of $A$
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The $|3, 0, 0\rangle$ state (in the standard notation $|n, l, m\rangle$ of the H-atom in the non-relativistic theory decays to the state $|1, 0, 0\rangle$ via two dipole transitions. The transition route and the corresponding probability are
In the LCR circuit shown below, the resistance $R = 0.05\,\Omega$, the inductance $L = 1\text{ H}$ and the capacitance $C = 0.04\text{ F}$.
If the input $v_{\text{in}}$ is a square wave of angular frequency $1\text{ rad/sec}$, the output $v_{\text{out}}$ is best approximated by a
a.
square wave of angular frequency $1\text{ rad/sec}$.
b.
sine wave of angular frequency $1\text{ rad/sec}$.
c.
square wave of angular frequency $5\text{ rad/sec}$.
d.
sine wave of angular frequency $5\text{ rad/sec}$.
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The dispersion relation of a gas of non-interacting bosons in $d$ dimensions is $E(k) = ak^s$, where $a$ and $s$ are positive constants. Bose-Einstein condensation will occur for all values of
a.
$d > s$
b.
$d + 2 > s > d - 2$
c.
$s > 2$ independent of $d$
d.
$d > 2$ independent of $s$
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In an experiment, the velocity of a non-relativistic neutron is determined by measuring the time ($\sim 50\text{ ns}$) it takes to travel from the source to the detector kept at a distance $L$. Assume that the error in the measurement of $L$ is negligibly small. If we want to estimate the kinetic energy $T$ of the neutron to within $5\%$ accuracy, i.e., $|\delta T/T| \le 0.05$, the maximum permissible error $|\delta t|$ in measuring the time of flight is nearest to
a.
$1.75\text{ ns}$
b.
$0.75\text{ ns}$
c.
$2.25\text{ ns}$
d.
$1.25\text{ ns}$
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A linear diatomic molecule consists of two identical small electric dipoles with an equilibrium separation $R$, which is assumed to be a constant. Each dipole has charges $+q$ of mass $m$ separated by $r$ when the molecule is at equilibrium. Each dipole can execute simple harmonic motion of angular frequency $\omega$. Recall that the interaction potential between two dipoles of moments $\boldsymbol{p}_1$ and $\boldsymbol{p}_2$, separated by $\mathbf{R}_{12} = R_{12}\hat{\mathbf{n}}$ is $(\boldsymbol{p}_1 \cdot \boldsymbol{p}_2 - 3(\boldsymbol{p}_1 \cdot \hat{\mathbf{n}})(\boldsymbol{p}_2 \cdot \hat{\mathbf{n}}))/(4\pi \varepsilon_0 R_{12}^3)$.
Assume that $R \gg r$ and let $\Omega^2 = \frac{q^2}{4\pi \varepsilon_0 m R^3}$. The angular frequencies of small oscillations of the diatomic molecule are
a.
$\sqrt{\omega^2 + \Omega^2}$ and $\sqrt{\omega^2 - \Omega^2}$
b.
$\sqrt{\omega^2 + 3\Omega^2}$ and $\sqrt{\omega^2 - 3\Omega^2}$
c.
$\sqrt{\omega^2 + 4\Omega^2}$ and $\sqrt{\omega^2 - 4\Omega^2}$
d.
$\sqrt{\omega^2 + 2\Omega^2}$ and $\sqrt{\omega^2 - 2\Omega^2}$
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The door of an X-ray machine room is fitted with a sensor D (0 is open and 1 is closed). It is also equipped with three fire sensors F1, F2 and F3 (each is 0 when disabled and 1 when enabled). The X-ray machine can operate only if the door is closed and at least 2 fire sensors are enabled. The logic circuit to ensure that the machine can be operated is
a.
Circuit (a)
b.
Circuit (b)
c.
Circuit (c)
d.
Circuit (d)
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In the reaction $p + n \to p + K^+ + X$, mediated by strong interaction, the baryon number $B$, strangeness $S$ and the third component of isospin $I_3$ of the particle $X$ are, respectively.
a.
$-1, -1$ and $-1$
b.
$+1, -1$ and $-1$
c.
$+1, -2$ and $-1/2$
d.
$-1, -1$ and $0$
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A monochromatic source emitting radiation with a certain frequency moves with a velocity $v$ away from a stationary observer $A$. It is moving towards another observer $B$ (also at rest) along a line joining the two. The frequencies of the radiation recorded by $A$ and $B$ are $\nu_A$ and $\nu_B$, respectively. If the ratio $\frac{\nu_B}{\nu_A} = 7$, then the value of $v/c$ is
a.
$\frac{1}{2}$
b.
$\frac{1}{4}$
c.
$\frac{3}{4}$
d.
$\frac{\sqrt{3}}{2}$
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The pressure of a gas in a vessel needs be maintained between $1.5\text{ bar}$ to $2.5\text{ bar}$ in an experiment. The vessel is fitted with a pressure transducer that generates $4\text{ mA}$ to $20\text{ mA}$ current for pressure in the range $1\text{ bar}$ to $5\text{ bar}$. The current output of the transductor has a linear dependence on the pressure.
The reference voltage $\text{V}_1$ and $\text{V}_2$ in the comparators in the circuit (shown in figure above) suitable for the desired operating conditions are, respectively
a.
$2\text{ V}$ and $10\text{ V}$
b.
$2\text{ V}$ and $5\text{ V}$
c.
$3\text{ V}$ and $10\text{ V}$
d.
$3\text{ V}$ and $5\text{ V}$
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A ${}^{60}\text{Co}$ nucleus $\beta$-decays from its ground state with $J^P = 5^+$ to a state of ${}^{60}\text{Ni}$ with $J^P = 4^+$. From the angular momentum selection rules, the allowed values of the orbital angular momentum $L$ and the total spin $S$ of the electron-antineutrino pair are
a.
$L = 0$ and $S = 1$
b.
$L = 1$ and $S = 0$
c.
$L = 0$ and $S = 0$
d.
$L = 1$ and $S = 1$
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A discrete random variable $X$ takes a value from the set $\{-1, 0, 1, 2\}$ with the corresponding probabilities $p(X) = \frac{3}{10}, \frac{2}{10}, \frac{2}{10}\text{ and } \frac{3}{10}$, respectively. The probability distribution $q(Y) = (q(0), q(1), q(4))$ of the random variable $Y = X^2$ is
Diffuse hydrogen gas within a galaxy may be assumed to follow a Maxwell distribution at temperature $10^6\text{ K}$, while the temperature appropriate for the H gas in the inter-galactic space, following the same distribution, may be taken to be $10^4\text{ K}$. The ratio of thermal broadening $\Delta v_G/\Delta v_{IG}$ of the Lyman-$\alpha$ line from the H-atoms within the galaxy to that from the inter-galactic space is closest to
a.
$100$
b.
$1/100$
c.
$10$
d.
$1/10$
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A polymer made up of $N$ monomers, is in thermal equilibrium at temperature $T$. Each monomer could be of length $a$ or $2a$. The first contributes zero energy, while the second one contributes $\varepsilon$. The average length (in units of $Na$) of the polymer at temperature $T = (\varepsilon/k_B)$ is
a.
$\frac{5+e}{4+e}$
b.
$\frac{4+e}{3+e}$
c.
$\frac{3+e}{2+e}$
d.
$\frac{2+e}{1+e}$
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The total number of phonon modes in a solid of volume $V$ is $\int_0^{\omega_D} g(\omega) d\omega = 3N$, where $N$ is the number of primitive cells, $\omega_D$ is the Debye frequency and density of photon modes is $g(\omega) = AV\omega^2$ (with $A > 0$ a constant). If the density of the solid doubles in a phase transition, the Debye temperature $\theta_D$ will
a.
increase by a factor of $2^{2/3}$
b.
increase by a factor of $2^{1/3}$
c.
decrease by a factor of $2^{2/3}$
d.
decrease by a factor of $2^{1/3}$
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The volume of the region common to the interiors of two infinitely long cylinders defined by $x^2 + y^2 = 25$ and $x^2 + 4z^2 = 25$ is best approximated by
a.
$225$
b.
$333$
c.
$423$
d.
$625$
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A perfectly conducting fluid, of permittivity $\varepsilon$ and permeability $\mu$, flows with a uniform velocity $v$ in the presence of time dependent electric and magnetic fields $\boldsymbol{E}$ and $\boldsymbol{B}$, respectively. If there is a finite current density in the fluid, then
In an experiment to measure the charge to mass ratio $e/m$ of the electron by Thomson's method, the value of the deflecting electric field and the accelerating potential are $6 \times 10^6\text{ N/C}$ (Newton per coulomb) and $150\text{ V}$, respectively. The magnitude of the magnetic field that leads to zero deflection of the electron beam is closest to
a.
$0.6\text{ T}$
b.
$1.2\text{ T}$
c.
$0.4\text{ T}$
d.
$0.8\text{ T}$
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The energy levels of a non-degenerate quantum system are $\varepsilon_n = nE_0$, where $E_0$ is a constant and $n = 1, 2, 3,...$ At a temperature $T$, the free energy $F$ can be expressed in terms of the average energy $E$ by
a.
$E_0 + k_B T \ln \frac{E}{E_0}$
b.
$E_0 + 2k_B T \ln \frac{E}{E_0}$
c.
$E_0 - k_B T \ln \frac{E}{E_0}$
d.
$E_0 - 2k_B T \ln \frac{E}{E_0}$
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The volume and temperature of a spherical cavity filled with black body radiation are $V$ and $300\text{ K}$, respectively. If it expands adiabatically to a volume $2V$, its temperature will be closest to
a.
$150\text{ K}$
b.
$300\text{ K}$
c.
$250\text{ K}$
d.
$240\text{ K}$
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The unnormalized wavefunction of a particle in one dimension in an infinite square well with walls at $x = 0$ and $x = a$, is $\psi(x) = x(a - x)$. If $\psi(x)$ is expanded as a linear combination of the energy eigenfunctions, $\int_0^a |\psi(x)|^2 dx$ is proportional to the infinite series
[You may use: $\int_0^a t \sin t \, dt = -a \cos a + \sin a$ and $\int_0^a t^2 \sin t \, dt = -2 - (a^2 - 2)\cos a + 2a \sin a$ ]
a.
$\sum_{n=1}^\infty (2n-1)^{-6}$
b.
$\sum_{n=1}^\infty (2n-1)^{-4}$
c.
$\sum_{n=1}^\infty (2n-1)^{-2}$
d.
$\sum_{n=1}^\infty (2n-1)^{-8}$
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A particle, thrown with a speed $v$ from the earth's surface, attains a maximum height $h$ (measured from the surface of the earth). If $v$ is half the escape velocity and $R$ denotes the radius of earth, then $h/R$ is
a.
$2/3$
b.
$1/3$
c.
$1/4$
d.
$1/2$
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The Legendre polynomials $P_n(x), n = 0, 1, 2,...$, satisfying the orthogonality condition $\int_{-1}^1 P_n(x) P_m(x) dx = \frac{2}{2n+1} \delta_{nm}$ on the interval $[-1, +1]$, may be defined by the Rodrigues formula
$$P_n(x) = \frac{1}{2^n n!} \frac{d^n}{dx^n} (x^2 - 1)^n$$
The value of the definite integral $\int_{-1}^1 (4 + 2x - 3x^2 + 4x^3) P_3(x) dx$ is
a.
$3/5$
b.
$11/15$
c.
$23/32$
d.
$16/35$
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The vector potential for an almost point like magnetic dipole located at the origin is $A = \frac{\mu \sin\theta}{4\pi r^2}\hat{\phi}$, where $(r, \theta, \phi)$ denote the spherical polar coordinates and $\hat{\phi}$ is the unit vector along $\phi$. A particle of mass $m$ and charge $q$, moving in the equatorial plane of the dipole, starts at time $t = 0$ with an initial speed $v_0$ and an impact parameter $b$. Its instantaneous speed at the point of closest approach is
a.
$v_0$
b.
$0/0$
c.
$v_0 + \frac{\mu q}{4\pi m b^2}$
d.
$\sqrt{v_0^2 + \left(\frac{\mu q}{4\pi m b^2}\right)^2}$
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The figure below shows an ideal capacitor consisting of two parallel circular plates of radius $R$. Points $P_1$ and $P_2$ are at a transverse distance $r_1 > R$ from the line joining the centres of the plates, while points $P_3$ and $P_4$ are at a transverse distance $r_2 < R$.
If $B(x)$ denotes the magnitude of the magnetic fields at these points, which of the following holds while the capacitor is charging ?
a.
$B(P_1) < B(P_2)$ and $B(P_3) < B(P_4)$
b.
$B(P_1) > B(P_2)$ and $B(P_3) > B(P_4)$
c.
$B(P_1) = B(P_2)$ and $B(P_3) < B(P_4)$
d.
$B(P_1) = B(P_2)$ and $B(P_3) > B(P_4)$
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A conducting wire in the shape of a circle lies on the $(x, y)$-plane, with its centre at the origin. A bar magnet moves with a constant velocity towards the wire along the $z$-axis (as shown in the figure below).
We take $t = 0$ to be the instant at which the midpoint of the magnet is at the centre of the wire loop and the induced current to be positive when it is counter-clockwise as viewed by the observer facing the loop and the incoming magnet. In these conventions, the best schematic representation of the induced current $I(t)$ as a function of $t$, is
a.
(a)
b.
(b)
c.
(c)
d.
(d)
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Balls of ten different colours labeled by $a = 1, 2, \dots, 10$ are to be distributed among different coloured boxes. A ball can only go in a box of the same colour, and each box can contain at most one ball. Let $n_a$ and $N_a$ denote, respectively, the numbers of balls and boxes of colour $a$. Assuming that $N_a \gg n_a \gg 1$, the total entropy (in units of the Boltzmann constant) can be best approximated by
To measure the height $h$ of a column of liquid helium in a container, a constant current $I$ is sent through an NbTi wire of length $l$, as shown in the figure. The normal state resistance of the NbTi wire is $R$.
If the superconducting transition temperature of NbTi is $\approx 10\text{ K}$, then the measured voltage $V(h)$ is best described by the expression.
a.
$IR\left(\frac{1}{2} - \frac{2h}{l}\right)$
b.
$IR\left(1 - \frac{h}{l}\right)$
c.
$IR\left(\frac{1}{2} - \frac{h}{l}\right)$
d.
$IR\left(1 - \frac{2h}{l}\right)$
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The components of the electric field, in a region of space devoid of any charge or current sources, are given to be $E_i = a_i + \sum_{j=1,2,3} b_{ij} x_j$, where $a_i$ and $b_{ij}$ are constants independent of the coordinates.
The number of independent components of the matrix $b_{ij}$ is
a.
5
b.
6
c.
3
d.
4
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The equation of motion of a one-dimensional forced harmonic oscillator in the presence of a dissipative force is described by $\frac{d^2x}{dt^2} + 10\frac{dx}{dt} + 16x = 6te^{-8t} + 4t^2 e^{-2t}$. The general form of the particular solution, in terms of constants $A, B$ etc., is
a.
$t(At^2 + Bt + C)e^{-2t} + (Dt + E)e^{-8t}$
b.
$(At^2 + Bt + C)e^{-2t} + (Dt + E)e^{-8t}$
c.
$t(At^2 + Bt + C)e^{-2t} + t(Dt + E)e^{-8t}$
d.
$(At^2 + Bt + C)e^{-2t} + t(Dt + E)e^{-8t}$
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A particle of mass $m$ in one dimensions is in the ground state of a simple harmonic oscillator described by a Hamiltonian $H = \frac{p^2}{2m} + \frac{1}{2}m\omega^2 x^2$ in the standard notation. An impulsive force at time $t = 0$ suddenly imparts a momentum $p_0 = \sqrt{\hbar m\omega}$ to it. The probability that the particle remains in the original ground state is
a.
$e^{-2}$
b.
$e^{-3/2}$
c.
$e^{-1}$
d.
$e^{-1/2}$
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The position of a particle in one dimension changes in discrete steps. With each step it moves to the right, however, the length of the step is drawn from a uniform distribution from the interval $\left[\lambda - \frac{1}{2}w, \lambda + \frac{1}{2}w\right]$, where $\lambda$ and $w$ are positive constants. If $X$ denotes the distance from the starting point after $N$ steps, the standard deviation $\sqrt{\langle X^2 \rangle - \langle X \rangle^2}$ for large values of $N$ is
a.
$\frac{\lambda}{2} \times \sqrt{N}$
b.
$\frac{\lambda}{2} \times \sqrt{\frac{N}{3}}$
c.
$\frac{w}{2} \times \sqrt{N}$
d.
$\frac{w}{2} \times \sqrt{\frac{N}{3}}$
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A particle in two dimensions is found to trace an orbit $r(\theta) = r_0 \,\theta^2$. If it is moving under the influence of a central potential $V(r) = c_1 r^{-a} + c_2 r^{-b}$, where $r_0$, $c_1$ and $c_2$ are constants of appropriate dimensions, the values of ‘$a$’ and ‘$b$’, respectively, are
a.
2 and 4
b.
2 and 3
c.
3 and 4
d.
1 and 3
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The figures below depict three different wavefunctions of a particle confined to a one-dimensional box $-1 \le x \le 1$.
The wavefunctions that correspond to the maximum expectation values $|\langle x \rangle|$ (absolute value of the mean position) and $\langle x^2 \rangle$, respectively, are
a.
B and C
b.
B and A
c.
C and B
d.
A and B
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In the following circuit the input voltage $V_{\text{in}}$ is such that $|V_{\text{in}}| < |V_{\text{sat}}|$, where $V_{\text{sat}}$ is the saturation voltage of the op-amp. (Assume that the diode is an ideal one and $R_LC$ is much larger than the duration of the measurement) For the input voltage as shown in the figure above, the output voltage $\text{V}_{\text{out}}$ is best represented by
a.
(a)
b.
(b)
c.
(c)
d.
(d)
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The volume integral $I = \iiint_V \mathbf{A} \cdot (\nabla \times \mathbf{A})\, d^3x$ is over a region $V$ bounded by a surface $\Sigma$ (an infinitesimal area element being $\hat{\mathbf{n}} dS$, where $\hat{\mathbf{n}}$ is the outward unit normal). If it changes to $I + \Delta I$, when the vector $\mathbf{A}$ is changed to $\mathbf{A} + \nabla \Lambda$, then $\Delta I$ can be expressed as:
Lead is superconducting below $7\text{ K}$ and has a critical magnetic field $800 \times 10^{-4}\text{ Tesla}$ close to $0\text{ K}$. At $2\text{ K}$ the critical current that flows through a long lead wire of radius $5\text{ mm}$ is closest to
a.
$1760\text{ A}$
b.
$1670\text{ A}$
c.
$1950\text{ A}$
d.
$1840\text{ A}$
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If we use the Fourier transform $\phi(x, y) = \int e^{ikx} \phi_k(y) dk$ to solve the partial differential equation:
$$-\frac{\partial^2\phi(x, y)}{\partial y^2} - \frac{1}{y^2} \frac{\partial^2\phi(x, y)}{\partial x^2} + \frac{m^2}{y^2}\phi(x, y) = 0$$
in the half-plane $\{(x, y): -\infty < x < \infty, 0 < y < \infty\}$ the Fourier modes $\phi_k(y)$ depend on $y$ as $y^\alpha$ and $y^\beta$. The values of $\alpha$ and $\beta$ are
The fulcrum of a simple pendulum (consisting of a particle of mass $m$ attached to the support by a massless string of length $l$ ) oscillates vertically as $\sin z(t) = a\sin\omega t$, where $\omega$ is a constant. The pendulum moves in a vertical plane and $\theta(t)$ denotes its angular position with respect to the $z$-axis.
If $l\frac{d^2\theta}{dt^2} + \sin\theta(g - f(t)) = 0$, (where $g$ is the acceleration due to gravity) describes the equation of motion of the mass, then $f(t)$ is
a.
$a\omega^2\cos\omega t$
b.
$a\omega^2\sin\omega t$
c.
$-a\omega^2\cos\omega t$
d.
$-a\omega^2\sin\omega t$
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The $Q$-value of the $\alpha$-decay of $^{232}\text{Th}$ to the ground state of $^{228}\text{Ra}$ is $4082\text{ keV}$. The maximum possible kinetic energy of the $\alpha$-particle is closest to
a.
$4082\text{ keV}$
b.
$4050\text{ keV}$
c.
$4035\text{ keV}$
d.
$4012\text{ keV}$
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The nuclei of $^{137}\text{Cs}$ decay by the emission of $\beta$-particles with a half-life of $30.08\text{ years}$. The activity (in units of disintegrations per second or $\text{Bq}$) of a $1\text{ mg}$ source of $^{137}\text{Cs}$, prepared on January 1, 1980, as measured on January 1, 2021 is closest to
a.
$1.79 \times 10^{16}$
b.
$1.79 \times 10^9$
c.
$1.24 \times 10^{16}$
d.
$1.24 \times 10^9$
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In an elastic scattering process at an energy $E$, the phase shifts satisfy $\delta_0 \approx 30^\circ, \delta_1 \approx 10^\circ$, while the other phase shifts are zero. The polar angle at which the differential cross-section peaks is closest to
a.
$20^\circ$
b.
$10^\circ$
c.
$0^\circ$
d.
$30^\circ$
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