BE Computer Engineering (Pokhara University) Applied Physics (PU, PHY 110) Question Paper 2079 Nepal
This is the official BE Computer Engineering (Pokhara University) Applied Physics (PU, PHY 110) question paper for 2079, as set in the regular annual examination. It carries 100 full marks and a time allowance of 180 minutes, across 13 questions. On Kekkei you can attempt this Applied Physics (PU, PHY 110) past paper online with a timer, get instant AI feedback and step-by-step solutions, and track the topics where you lose marks — completely free. Whether you are revising for your BE Computer Engineering (Pokhara University) Applied Physics (PU, PHY 110) exam or solving previous years' question papers, this 2079 paper is a great way to practise under real exam conditions.
Section A: Long Answer Questions
Attempt all / any as specified.
(a) Set up the differential equation of a damped harmonic oscillator and obtain its solution for the under-damped (weakly damped) case. Hence explain the terms under-damping, critical damping and over-damping with appropriate displacement–time sketches. (9)
(b) A body of mass 0.2 kg executes damped oscillations with a force constant of 80 N/m and a damping constant of 0.16 kg/s. Calculate the angular frequency of the damped oscillation and the time in which the amplitude falls to half of its initial value. (5)
(a) Damped harmonic oscillator (9 marks)
A particle of mass experiences a restoring force and a velocity-dependent damping force . By Newton's second law:
Trying gives the auxiliary equation , so
Under-damped case (): the root is complex, with . The solution is an exponentially decaying oscillation:
The amplitude decays slowly while the system oscillates at the reduced frequency .
Three cases
- Under-damping (): oscillatory motion with amplitude falling exponentially; the displacement crosses zero many times. Sketch: a cosine curve bounded by a decaying envelope.
- Critical damping (): equal roots; . The system returns to equilibrium in the shortest time without oscillating. Sketch: a single smooth curve rising/falling to zero with no overshoot.
- Over-damping (): two real negative roots; motion is a slow non-oscillatory return to equilibrium, slower than critical. Sketch: a sluggish exponential decay to zero, lying above the critical curve.
(b) Numerical (5 marks)
Given , , .
Damped angular frequency:
Time for amplitude to halve: amplitude , so :
(a) State Maxwell's equations of electromagnetism in differential form and explain the physical significance of each. Show how Maxwell modified Ampere's law by introducing the concept of displacement current. (8)
(b) Starting from Maxwell's equations in free space, derive the wave equation for the electric field and hence obtain an expression for the speed of electromagnetic waves in vacuum. (6)
(a) Maxwell's equations and displacement current (8 marks)
In differential form, in a medium of permittivity and permeability :
| Equation | Form | Physical significance |
|---|---|---|
| Gauss's law (electric) | Electric charges are the sources of the electric field. | |
| Gauss's law (magnetic) | No magnetic monopoles; magnetic field lines are closed. | |
| Faraday's law | A changing magnetic field induces an electric field. | |
| Ampère–Maxwell law | Conduction current and changing electric field both produce a magnetic field. |
Displacement current. The original Ampère's law gives , but the continuity equation requires , which is non-zero when charge accumulates (e.g. between capacitor plates while charging). Maxwell removed the inconsistency by adding a term. Using ,
The extra term is the displacement current density, giving the corrected law .
(b) Wave equation and speed of EM waves (6 marks)
In free space . Take the curl of Faraday's law:
Using the identity with :
Comparing with the standard wave equation gives the speed of EM waves in vacuum:
which matches the measured speed of light, establishing that light is an electromagnetic wave.
(a) Derive the time-independent Schrödinger wave equation for a particle of mass m moving in a region of potential energy V. (6)
(b) Apply the Schrödinger equation to a particle confined in a one-dimensional infinite potential well (rigid box) of width L. Obtain the normalized wave functions and show that the energy of the particle is quantized. Sketch the first three energy eigenstates. (6)
(a) Time-independent Schrödinger equation (6 marks)
A particle of mass is described by a wave . Starting from the classical plane wave and using the de Broglie relations and :
Total energy , hence . Substituting:
This is the time-independent Schrödinger equation (3-D form: ).
(b) Particle in a 1-D infinite well of width (6 marks)
Inside the box (); outside so . The equation becomes
General solution . Boundary condition . Condition
Quantized energy:
Energy is discrete (quantized) and the lowest state () has non-zero zero-point energy.
Normalization: , so
Sketch of first three eigenstates: is a single half-sine (one antinode, no node inside); is a full sine (one node at ); has two interior nodes. All vanish at and .
(a) Explain the principle of light propagation through an optical fibre based on total internal reflection. Define acceptance angle and numerical aperture, and derive an expression for the numerical aperture in terms of the refractive indices of the core and cladding. (8)
(b) An optical fibre has a core refractive index of 1.50 and a cladding refractive index of 1.46. Calculate its numerical aperture and the acceptance angle when the fibre is placed in air. (4)
(a) Light propagation, acceptance angle and numerical aperture (8 marks)
An optical fibre has a high-index core () surrounded by a lower-index cladding (). A ray entering the core strikes the core–cladding boundary; if the angle of incidence there exceeds the critical angle (where ), the ray undergoes total internal reflection and is guided down the fibre with negligible loss, repeatedly reflecting along its length.
Acceptance angle (): the maximum half-angle of the entrance cone for which an incident ray is still totally internally reflected inside the core. Rays within this cone are guided; rays outside it escape into the cladding.
Numerical aperture (NA): the light-gathering ability of the fibre, (with the index of the medium outside).
Derivation. Let a ray enter from a medium of index at angle , refracting to angle inside the core: . To be guided it must hit the wall at exactly the critical angle, so the angle with the wall normal is and
Therefore
(b) Numerical (4 marks)
Given , fibre in air ().
Numerical aperture ; acceptance angle .
Section B: Short Answer Questions
Attempt all / any as specified.
Explain the formation of Newton's rings in reflected light. Derive an expression for the diameter of the n-th dark ring and show how the wavelength of monochromatic light can be determined using this arrangement.
Newton's rings in reflected light
When a plano-convex lens of large radius rests on a flat glass plate, a thin air film of gradually increasing thickness forms between them. Monochromatic light incident from above is partly reflected at the top and bottom of the air film; these two beams interfere. Because of the circular symmetry of the film, loci of constant thickness are circles, so a pattern of alternately bright and dark concentric rings with a dark central spot is seen in reflected light.
For near-normal incidence the path difference between the two reflected rays is , plus an extra from the phase change on reflection at the glass surface (rarer-to-denser). For an air film :
- Dark ring:
- Bright ring:
Diameter of the -th dark ring
From the geometry of the lens, the film thickness at radius is . For the -th dark ring :
With diameter :
The diameter is proportional to , so rings get closer together outward.
Determination of wavelength
Measure the diameters of the -th and -th dark rings. Then
This subtraction eliminates errors from imperfect contact at the centre. Knowing (from a spherometer) and the measured diameters, is found.
What is a plane diffraction grating? Obtain the grating equation for the position of principal maxima. A grating having 5000 lines per cm is illuminated normally by light of wavelength 589 nm; find the angle of diffraction for the second-order maximum.
Plane diffraction grating
A plane diffraction grating is an optical component consisting of a large number of equally spaced, identical, parallel slits (rulings) on a flat transparent surface. If the slit width is and the opaque space between slits is , the grating element is , equal to the reciprocal of the number of lines per unit length.
Grating equation (principal maxima)
When light of wavelength falls normally on the grating, the secondary wavelets from corresponding points of adjacent slits travel an extra path in a direction making angle with the normal. Constructive interference (a principal maximum) occurs when this path difference is a whole number of wavelengths:
where is the order of the spectrum.
Numerical
Grating has lines/cm, so
For , :
Angle of diffraction for the second-order maximum .
(a) State and explain Brewster's law and use it to define the polarizing angle. (4)
(b) Distinguish between a quarter-wave plate and a half-wave plate, stating one practical use of each. (3)
(a) Brewster's law and polarizing angle (4 marks)
Brewster's law: When unpolarized light is incident on a transparent dielectric, there is a particular angle of incidence, the polarizing (Brewster) angle , at which the reflected light is completely plane-polarized (vibrations perpendicular to the plane of incidence). At this angle the refractive index equals the tangent of the polarizing angle:
At the reflected and refracted rays are mutually perpendicular (). Proof: by Snell's law . The polarizing angle is thus the angle of incidence for which the reflected beam is fully polarized.
(b) Quarter-wave vs half-wave plate (3 marks)
| Quarter-wave plate | Half-wave plate | |
|---|---|---|
| Path difference introduced | ||
| Phase difference | ||
| Effect | Converts linearly polarized light into circularly/elliptically polarized light (and vice versa) | Rotates the plane of linearly polarized light by (keeps it linear) |
| Thickness | ||
| Practical use | Production/analysis of circularly polarized light (e.g. in optical isolators, anti-glare devices) | Rotating the polarization plane in polarimeters and laser optics |
Explain the terms spontaneous emission, stimulated emission and population inversion. Why is population inversion essential for laser action, and how is it achieved in a three-level laser system?
Emission processes and population inversion
Spontaneous emission: An atom in an excited state decays on its own to a lower state , emitting a photon of energy . The photons are emitted in random directions, with random phase — the light is incoherent (ordinary light).
Stimulated emission: An incident photon of energy induces an excited atom to drop to , emitting a second photon identical in frequency, phase, direction and polarization to the incident one. This produces coherent light amplification — the basis of laser action.
Population inversion: A non-equilibrium condition in which the number of atoms in the higher energy state exceeds that in the lower state (). In thermal equilibrium the Boltzmann distribution gives , so inversion must be created artificially.
Why population inversion is essential
Stimulated emission (gain) competes with absorption. The net rate of stimulated emission , so a photon beam is amplified only if ; otherwise absorption dominates and there is no light amplification. Hence population inversion is a necessary condition for laser action.
Three-level system
Atoms are pumped (optically) from the ground state to a high state . From they decay rapidly and non-radiatively to a metastable state which has a long lifetime, so atoms accumulate there. When the population of exceeds that of the ground state , inversion between and is achieved, and lasing occurs on the transition (e.g. the ruby laser). A drawback is that the lower laser level is the heavily populated ground state, so very strong pumping is required.
Describe the formation of a depletion region in an unbiased p–n junction diode. Explain qualitatively, with the help of energy-band diagrams, how the junction behaves under forward bias and reverse bias.
Formation of the depletion region
When p-type and n-type semiconductors are joined, the large concentration gradient causes majority electrons to diffuse from n to p and holes from p to n. Near the junction electrons fill holes; the n-side is left with fixed positive donor ions and the p-side with fixed negative acceptor ions. This region, depleted of mobile charge carriers, is the depletion region. The exposed immobile ions set up an internal electric field (and a built-in potential barrier , about 0.7 V for Si, 0.3 V for Ge) directed from n to p, which opposes further diffusion. At equilibrium the diffusion current is exactly balanced by the drift current and no net current flows.
In the band picture, the Fermi levels of the two sides align; the conduction and valence bands of the p-side bend upward relative to the n-side, the offset being the barrier height.
Forward bias
The p-side is connected to the positive terminal and the n-side to the negative terminal. The external field opposes the built-in field, reducing the barrier height to and narrowing the depletion region. The bands shift so the offset decreases. Majority carriers cross the junction easily, and a large current flows that rises steeply once exceeds the knee voltage.
Reverse bias
The p-side is made negative and the n-side positive. The external field aids the built-in field, increasing the barrier to and widening the depletion region. The bands bend further apart. Majority-carrier flow is blocked; only a tiny reverse saturation current due to thermally generated minority carriers flows, nearly independent of voltage until breakdown.
State the Hall effect and derive an expression for the Hall coefficient. Mention two important applications of the Hall effect in characterizing semiconductor materials.
Hall effect
When a current-carrying conductor (or semiconductor) is placed in a magnetic field perpendicular to the current, a transverse potential difference (the Hall voltage ) develops across the specimen, perpendicular to both the current and the field. This is the Hall effect, and it arises from the magnetic Lorentz force on the moving charge carriers.
Derivation of the Hall coefficient
Let current flow along in a slab of width and thickness , with magnetic field along . Carriers of charge drift with velocity . The Lorentz force pushes them sideways (along ) until the resulting transverse electric field balances it:
The current density is , where is the carrier concentration, so and
The Hall coefficient is defined as :
In terms of measurable quantities, and , giving and . The sign of is negative for n-type (electrons) and positive for p-type (holes).
Applications
- Determination of carrier type and concentration — the sign of gives the majority-carrier type and its magnitude gives .
- Measurement of carrier mobility — combining with the conductivity gives the Hall mobility . (Also used in Hall-effect magnetic-field sensors/probes.)
Explain the different types of polarization mechanisms in a dielectric material. Derive the Clausius–Mossotti relation connecting the dielectric constant of a material to its atomic polarizability.
Polarization mechanisms in dielectrics
When a dielectric is placed in an electric field, bound charges shift slightly, giving each unit volume a dipole moment (polarization ). The main mechanisms are:
- Electronic polarization: displacement of the electron cloud relative to the nucleus of each atom. Present in all dielectrics, very fast (up to optical frequencies).
- Ionic (atomic) polarization: in ionic solids, positive and negative ions displace in opposite directions, changing inter-ionic distances.
- Orientational (dipolar) polarization: in polar molecules (with permanent dipoles, e.g. water), the field tends to align the dipoles against thermal randomization; strongly temperature-dependent.
- Space-charge (interfacial) polarization: accumulation of mobile charges at grain boundaries/interfaces; significant only at low frequencies.
Clausius–Mossotti relation
For a non-polar dielectric, the local field acting on an atom (Lorentz field) is
The induced dipole moment per atom is , and with atoms per unit volume the polarization is
Solving for :
Using to eliminate and simplifying gives the Clausius–Mossotti relation:
This links the macroscopic dielectric constant to the microscopic atomic polarizability and the number density .
Distinguish between diamagnetic, paramagnetic and ferromagnetic materials on the basis of their magnetic susceptibility and behaviour in an external magnetic field, giving one example of each.
Classification of magnetic materials
| Property | Diamagnetic | Paramagnetic | Ferromagnetic |
|---|---|---|---|
| Susceptibility | Small, negative () | Small, positive () | Very large, positive (–) |
| Relative permeability | Slightly | Slightly | |
| Behaviour in a field | Weakly repelled; moves from strong to weak field | Weakly attracted; moves from weak to strong field | Strongly attracted; can be permanently magnetized |
| Atomic origin | No permanent dipoles; induced moments oppose field | Permanent dipoles randomly oriented, partly align with field | Permanent dipoles align in domains; strong exchange coupling |
| Temperature dependence | Independent of | (Curie law) | Ferromagnetic below Curie temperature; paramagnetic above it |
| Example | Bismuth, copper, water | Aluminium, platinum, manganese | Iron, cobalt, nickel |
Summary: Diamagnetics oppose the applied field weakly, paramagnetics enhance it weakly, and ferromagnetics enhance it enormously and retain magnetization.
State Heisenberg's uncertainty principle. Using it, estimate the minimum energy (zero-point energy) of an electron confined within a nucleus of dimension 10⁻¹⁴ m and comment on whether electrons can exist inside the nucleus.
Heisenberg's uncertainty principle
It is impossible to determine simultaneously, with unlimited precision, both the position and the momentum of a particle. The product of the uncertainties is at least of the order of :
Minimum energy of an electron confined in a nucleus
If the electron is confined within a nucleus, . Taking the minimum momentum :
Since is far larger than the electron rest energy , the electron must be treated relativistically, :
Comment
An electron bound inside the nucleus would need a minimum energy of about 20 MeV. However, electrons emitted in beta decay have energies of only a few MeV, and no nuclear binding mechanism can hold an electron with 20 MeV. Therefore electrons cannot exist inside the nucleus; the beta-decay electron is created at the instant of decay.
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