PHY118 · TU past paper
Physics 2077 question paper
The complete TU 2077 exam paper for Physics (PHY118), all 12 questions with solved model answers written to the mark scheme.
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- 110 marksRTL and TTL gatesHideAnswer
Explain RTL and TTL gates. How memory and clock circuits can be made by using these gates? Explain how they work?[10]
--- RTL is one of the earliest logic gate families where resistors and transistors are used to implement logic functions. - When any input is HIGH, the corresponding transistor saturates (ON), pulling output LOW. - When all inputs are LO...
- 210 marksOscillation of springHideAnswer
Set up differential equation for an oscillation of a spring using Hooke's and Newton's second law. Find the general solution of this equation and hence the expressions for period, velocity and acceleration of oscillation.[10]
Differential Equation for Spring Oscillation, General Solution, Period, Velocity and Acceleration
1. Setting Up the Differential Equation
Physical Setup
Consider a spring of negligible mass with one end fixed. A particle of mass m is attached to the free end. When the mass is displaced by a distance x (or l) from its equilibrium position, the spring exerts a restoring force.
Applying Hooke's Law
From Hooke's Law, the restoring force developed in the spring is proportional to the displacement:
$$F = -kx$$
where:
- $k$ = spring constant (force per unit extension, in N/m)
- $x$ = displacement from equilibrium
- The negative sign indicates the restoring force acts opposite to the direction of displacement
Applying Newton's Second Law
From Newton's Second Law of Motion:
$$F = ma = m\frac{d^2x}{dt^2}$$
Combining Both Laws
Equating the two expressions:
$$m\frac{d^2x}{dt^2} = -kx$$
$$\boxed{\frac{d^2x}{dt^2} + \frac{k}{m}x = 0}$$
This is the differential equation of Simple Harmonic Motion (SHM).
Let $\omega^2 = \dfrac{k}{m}$, then:
$$\frac{d^2x}{dt^2} + \omega^2 x = 0$$
where $\omega$ is the angular frequency of oscillation.
2. General Solution of the Differential Equation
The differential equation:
$$\frac{d^2x}{dt^2} + \omega^2 x = 0$$
is a second-order linear homogeneous ODE. Its general solution is:
$$\boxed{x(t) = A\sin(\omega t + \phi)}$$
where:
- $A$ = amplitude of oscillation (maximum displacement)
- $\omega$ = angular frequency $= \sqrt{k/m}$
- $\phi$ = initial phase angle (determined by initial conditions)
Verification: Differentiating twice: $\dfrac{d^2x}{dt^2} = -A\omega^2\sin(\omega t + \phi) = -\omega^2 x$ which satisfies the equation.
3. Expression for Period
The angular frequency is:
$$\omega = \sqrt{\frac{k}{m}}$$
Since $\omega = \dfrac{2\pi}{T}$, the time period is:
$$T = \frac{2\pi}{\omega} = 2\pi\sqrt{\frac{m}{k}}$$
$$\boxed{T = 2\pi\sqrt{\frac{m}{k}}}$$
The frequency of oscillation is:
$$f = \frac{1}{T} = \frac{1}{2\pi}\sqrt{\frac{k}{m}}$$
4. Expression for Velocity
Starting from the displacement equation:
$$x = A\sin(\omega t + \phi)$$
Differentiating with respect to time:
$$v = \frac{dx}{dt} = A\omega\cos(\omega t + \phi)$$
This can be rewritten in terms of displacement $x$:
$$v = A\omega\cos(\omega t + \phi) = \omega\sqrt{A^2 - A^2\sin^2(\omega t + \phi)}$$
$$\boxed{v = \omega\sqrt{A^2 - x^2}}$$
Key observations:
Position Velocity At mean position ($x = 0$) $v_{max} = \omega A$ (maximum) At extreme position ($x = \pm A$) $v = 0$ (minimum)
5. Expression for Acceleration
Differentiating velocity with respect to time:
$$a = \frac{dv}{dt} = \frac{d^2x}{dt^2} = -A\omega^2\sin(\omega t + \phi)$$
Since $x = A\sin(\omega t + \phi)$:
$$\boxed{a = -\omega^2 x}$$
Key observations:
Position Acceleration At mean position ($x = 0$) $a = 0$ (minimum) At extreme position ($x = \pm A$) $a_{max} = \mp\omega^2 A$ (maximum) The negative sign confirms that acceleration is always directed towards the equilibrium position, which is the defining characteristic of SHM.
Summary Table
Quantity Expression Differential Equation $\dfrac{d^2x}{dt^2} + \omega^2 x = 0$ General Solution $x = A\sin(\omega t + \phi)$ Angular Frequency $\omega = \sqrt{k/m}$ Period $T = 2\pi\sqrt{m/k}$ Velocity $v = \omega\sqrt{A^2 - x^2}$ Acceleration $a = -\omega^2 x$ - 310 marksFranck-Hertz experimentHideAnswer
Describe Frank-Hertz experiment. Interpret how the results of this experiment advocate atomic model proposed by Bohr?[10]
The Frank-Hertz experiment, performed by James Franck and Gustav Hertz in 1914, provided direct experimental evidence for the existence of discrete (quantized) energy levels in atoms. This experiment strongly supported the atomic model p...
- 45 marksmagnetic dipole momentHideAnswer
Discuss magnetic dipole moment. What is its effect on atom and on molecules? Explain. [5]
Magnetic Dipole Moment: Effect on Atoms and Molecules
1. Magnetic Dipole Moment
A magnetic dipole moment is a measure of the strength of a magnetic dipole (a tiny current loop or a spinning charged particle). It is defined as the product of the current flowing in a loop and the area enclosed by that loop.
$$\vec{\mu} = I \cdot \vec{A}$$
where:
- $I$ = current in the loop
- $A$ = area of the loop
- Direction: perpendicular to the plane of the loop (right-hand rule)
SI Unit: A·m² (Ampere-square metre)
2. Magnetic Dipole Moment of an Electron in an Atom
Consider an electron moving in a circular orbit of radius $r$ with linear velocity $v$ and angular velocity $\omega$ around the nucleus.
- Charge of electron = $e$
- Mass of electron = $m$
The electron completes one revolution in time period: $$T = \frac{2\pi r}{v} = \frac{2\pi}{\omega}$$
This constitutes a current (since a moving charge is equivalent to a current): $$I = \frac{e}{T} = \frac{e\omega}{2\pi}$$
The area of the circular orbit: $$A = \pi r^2$$
Therefore, the orbital magnetic dipole moment: $$\boxed{\mu = IA = \frac{e\omega}{2\pi} \cdot \pi r^2 = \frac{e\omega r^2}{2}}$$
Since angular momentum $L = m\omega r^2$, we can write: $$\mu = \frac{e}{2m} L$$
This is the gyromagnetic ratio relation.
3. Effect of Magnetic Dipole Moment on the Atom
When an atom (with magnetic dipole moment $\vec{\mu}$) is placed in an external magnetic field $\vec{B}$:
(a) Torque on the Atom
The atom experiences a torque that tends to align its magnetic moment with the field: $$\vec{\tau} = \vec{\mu} \times \vec{B} \quad \Rightarrow \quad \tau = \mu B \sin\theta$$
where $\theta$ is the angle between $\vec{\mu}$ and $\vec{B}$.
(b) Potential Energy
The atom has a potential energy in the field: $$U = -\vec{\mu} \cdot \vec{B} = -\mu B \cos\theta$$
- Minimum energy (stable): when $\theta = 0°$ (parallel alignment)
- Maximum energy (unstable): when $\theta = 180°$ (anti-parallel)
(c) Translatory Force (Non-uniform Field)
In a non-uniform magnetic field (gradient $dB/dz$), the atom experiences a translatory force: $$F = \mu \frac{dB}{dz}$$
This is the basis of the Stern-Gerlach experiment, where atoms with different orientations of $\vec{\mu}$ are deflected by different amounts, demonstrating space quantization.
As stated in the notes: "The Ag atom which has dipole moment aligned at angle $\theta$ will experience torque and potential energy which tries to align in the parallel direction to the field. The atoms already aligned parallel to the field pass without deviation. But other atoms experience translatory motion in the magnetic gradient $dB/dz$."
4. Effect of Magnetic Dipole Moment on Molecules
Molecules can possess magnetic dipole moments due to:
Source Description Orbital motion of electrons Electrons orbiting nuclei create tiny current loops Electron spin Intrinsic spin of electrons contributes a spin magnetic moment Nuclear spin Much smaller contribution from nuclear magnetic moments Types of Molecular Magnetic Behavior:
(a) Diamagnetic Molecules:
- All electron spins are paired, so net $\mu = 0$
- When placed in a field, they are weakly repelled
- Example: $H_2$, $N_2$
(b) Paramagnetic Molecules:
- Have unpaired electrons, so net $\mu \neq 0$
- Dipoles tend to align with the field, causing weak attraction
- Example: $O_2$, $NO$
(c) Ferromagnetic Materials:
- Large regions (domains) of aligned dipole moments
- Very strong attraction to magnetic fields
- Example: Fe, Ni, Co
5. Numerical Example (from notes)
Example: Electron in hydrogen atom orbits at radius $r = 0.5 \times 10^{-10}$ m with frequency $f = 10^{14}$ Hz.
$$\omega = 2\pi f = 2\pi \times 10^{14} \text{ rad/s}$$
$$\mu = \frac{e\omega r^2}{2} = \frac{(1.6\times10^{-19})(2\pi \times 10^{14})(0.5\times10^{-10})^2}{2}$$
$$\mu = \frac{1.6\times10^{-19} \times 6.28\times10^{14} \times 0.25\times10^{-20}}{2}$$
$$\boxed{\mu \approx 1.256 \times 10^{-25} \text{ A·m}^2}$$
This is about one seventieth of the Bohr magneton ($\mu_B = 9.27 \times 10^{-24}$ A·m²), the fundamental unit of atomic magnetic moment. The Bohr magneton itself corresponds to the true hydrogen ground state orbital frequency of about $6.6 \times 10^{15}$ Hz rather than the $10^{14}$ Hz assumed here.
Summary
Aspect Effect Torque Aligns dipole with field Potential energy Determines stable/unstable orientation Non-uniform field Causes translatory deflection of atoms Molecular effect Determines diamagnetic, paramagnetic or ferromagnetic behaviour Note on the worked value: the arithmetic in the example gives $\mu = 1.256 \times 10^{-25}$ A$\cdot$m$^2$, so the exponent printed in the box above should read $-25$, and the value is then about one seventieth of the Bohr magneton rather than close to it. Substituting the true ground state orbital frequency of hydrogen, about $6.6 \times 10^{15}$ Hz, in the same formula does return $\mu \approx \mu_B = 9.27 \times 10^{-24}$ A$\cdot$m$^2$.
Conclusion
The magnetic dipole moment of an atom comes from the orbital motion of its electrons and from electron spin, and the relation $\mu = \dfrac{e}{2m}L$ ties it directly to angular momentum, which is why it is quantized in units of the Bohr magneton. In a uniform field the moment feels a torque that aligns it and acquires an orientation dependent energy $U = -\mu B\cos\theta$; in a non uniform field it feels a net force $\mu,dB/dz$ that deflects the whole atom, as the Stern-Gerlach experiment demonstrates. At the molecular level the vector sum of these moments decides the magnetic character of the substance: paired spins cancel and leave a diamagnetic molecule, unpaired spins leave a permanent moment and give paramagnetism, and cooperative alignment of such moments over whole domains produces ferromagnetism.
- 55 marksProcesses of IC productionHideAnswer
Describe the following process of IC production: (a) Oxidation, (b) Pattern definition, and (c) Doping [5]
--- Oxidation is the process of growing a layer of silicon dioxide (SiO₂) on the surface of the silicon wafer. This is achieved by exposing the silicon wafer to an oxidizing environment (oxygen or steam) at high temperatures (around 900°...
- 65 marksBipolar junction transistorHideAnswer
Explain the construction and bipolar junction transistor (BJT). [5]
A Bipolar Junction Transistor (BJT) is a three-terminal semiconductor device formed by combining two PN junctions in a specific manner. It is called "bipolar" because its operation involves both types of charge carriers -- holes and elec...
- 75 marksNumericalMoment of inertia and torqueHideAnswer
A roulette wheel with moment of inertia $I = 0.5\ \mathrm{kgm^2}$ rotating initially at 2 rev/sec coasts to a stop from the constant friction torque of bearing. If the torque is 0.4 Nm, how long does it take to stop? [5]
Quantity Value ------ Moment of inertia, $I$ $0.5\ \text{kg m}^2$ Initial rotation rate, $n0$ $2\ \text{rev/s}$ Final rotation rate, $n$ $0\ \text{rev/s}$ Friction torque, $T$ $0.4\ \text{N m}$ Newton's second law for rotation:
- 85 marksNumericalElectric and magnetic field and potentialHideAnswer
Two large parallel plates are separated by a distance of 5 cm. The plates have equal but opposite charges that create an electric field in the region between the plates. An α particle (q = $3.2 \times 10^{-27}$ kg) is released from the positively charged plate, and strikes the negatively charged plate $2 \times 10^{-6}$ sec. later. Assuming that the electric field between the plates is uniform and perpendicular to the plates, what is the strength of the electric field? [5]
Quantity Value ------ Plate separation $d = 5 \text{ cm} = 0.05 \text{ m}$ Mass of α-particle $m = 6.68 \times 10^{-27} \text{ kg}$ (standard value) Charge of α-particle $q = 3.2 \times 10^{-19} \text{ C}$ (standard value) Time to cross ...
- 95 marksconductors, insulators and semiconductorsHideAnswer
The energy gap in silicon is 1.1 eV, whereas in diamond it is 6 eV. What conclusion can you draw about the transparency of the two materials to visible light ($4000 \text{ A}^{\circ} \text{ to } 7000 \text{ A}^{\circ}$)? [5]
Material Band Gap Energy (Eg) -------------------------------- Silicon (Si) 1.1 eV Diamond 6.0 eV Visible light wavelength range: 4000 A° to 7000 A° --- The energy of a photon is given by: $$E = hf = \frac{hc}{\lambda}$$ $$E = \frac{hc}{...
- 105 marksNumericalUniversal gatesHideAnswer
Find the truth table for the circuit shown in the figure. What logic function will the circuit perform if the constant +5 V input to the first two gates is changed to ground potential? [5]
The problem refers to "the circuit shown in the figure," which is not provided. However, this is a standard, well-known textbook problem (Malvino/Tocci style). The identifiable data are: - Three gates, with the first two receiving a cons...
- 115 marksNumericalde Broglie's hypothesis and its experimentHideAnswer
In neutron spectroscopy a beam of monoenergetic neutrons is obtained by reflecting reactor neutrons from a beryllium crystal. If the separation between the atomic planes of the beryllium crystal is $0.732 \text{ Å}$, what is the angle between the incident neutron beam and the atomic planes that will yield a monochromatic beam of neutrons of wavelength $0.1 \text{ Å}$? [5]
Neutron Spectroscopy: Bragg Diffraction Angle
Step 1 - Given Data
- Plane separation: $d = 0.732\ \text{Å} = 0.732 \times 10^{-10}\ \text{m}$
- Required wavelength: $\lambda = 0.1\ \text{Å} = 0.1 \times 10^{-10}\ \text{m}$
- Order of diffraction: $n = 1$ (first order, assumed)
Step 2 - Solve
Bragg's Law:
$$n\lambda = 2d\sin\theta$$
For first order ($n=1$):
$$\sin\theta = \frac{\lambda}{2d} = \frac{0.1 \times 10^{-10}}{2 \times 0.732 \times 10^{-10}}$$
$$\sin\theta = \frac{0.1}{1.464} = 0.068306$$
Therefore:
$$\theta = \sin^{-1}(0.068306) \approx 3.915^\circ$$
Result
The angle between the incident neutron beam and the atomic planes is approximately
$$\boxed{\theta \approx 3.92^\circ}$$
This is the glancing angle for first-order Bragg reflection.
- 125 marksNumericalSchrodinger theory of quantum mechanics anHideAnswer
What is the probability of finding a particle in a well of width $a$ at a position $\frac{a}{4}$ from the wall if $n=1$, if $n=2$, if $n=3$. Use the normalized wavefunction $$\psi(x,t) = \left(\frac{2}{a}\right)^{\frac{1}{2}} \sin\left(\frac{n\pi x}{a}\right) e^{-\frac{iEt}{\hbar}}$$ [5]
Probability of Finding a Particle in an Infinite Square Well at x = a/4
STEP 1 - Given Data
- Normalized wavefunction: $\psi(x,t) = \left(\dfrac{2}{a}\right)^{1/2} \sin\left(\dfrac{n\pi x}{a}\right) e^{-iEt/\hbar}$
- Well width: $a$
- Position of interest: $x = \dfrac{a}{4}$
- Quantum numbers: $n = 1, 2, 3$
Note on interpretation: The wavefunction gives a probability density $|\psi|^2$ (probability per unit length). A true probability requires integration over an interval. Since the question asks for "the probability of finding a particle... at a position $a/4$," the standard textbook interpretation is the probability density evaluated at that point, which is what we compute below.
STEP 2 - Solve
The probability density is:
$$P(x) = |\psi(x,t)|^2 = \frac{2}{a}\sin^2\left(\frac{n\pi x}{a}\right)$$
since $\left|e^{-iEt/\hbar}\right|^2 = 1$.
At $x = \dfrac{a}{4}$:
$$P\left(\frac{a}{4}\right) = \frac{2}{a}\sin^2\left(\frac{n\pi}{4}\right)$$
Case n = 1
$$P = \frac{2}{a}\sin^2\left(\frac{\pi}{4}\right) = \frac{2}{a}\left(\frac{1}{\sqrt{2}}\right)^2 = \frac{2}{a}\cdot\frac{1}{2} = \boxed{\frac{1}{a}}$$
Case n = 2
$$P = \frac{2}{a}\sin^2\left(\frac{2\pi}{4}\right) = \frac{2}{a}\sin^2\left(\frac{\pi}{2}\right) = \frac{2}{a}(1) = \boxed{\frac{2}{a}}$$
Case n = 3
$$P = \frac{2}{a}\sin^2\left(\frac{3\pi}{4}\right) = \frac{2}{a}\left(\frac{1}{\sqrt{2}}\right)^2 = \frac{2}{a}\cdot\frac{1}{2} = \boxed{\frac{1}{a}}$$
Summary
$n$ $\sin^2(n\pi/4)$ Probability density $P(a/4)$ 1 $1/2$ $1/a$ 2 $1$ $2/a$ 3 $1/2$ $1/a$ Observation: The density is largest for $n=2$, where $x=a/4$ coincides with an antinode of the wavefunction. For $n=1$ and $n=3$ the density is equal, each half the $n=2$ value.
(If a small interval $dx$ around $a/4$ is intended, multiply each density by $dx$: $P = \frac{2}{a}\sin^2(n\pi/4),dx$.)