Engineering Physics

A Comprehensive Course for First-Year B.Tech Students — Aligned with AICTE / GTU / AKTU / VTU / JNTU Model Curriculum

1. Units, Dimensions, and Errors

Physical Quantities and SI Units

Definition A physical quantity is any property of a physical system that can be quantified by measurement. Quantities are classified as fundamental (independent: length, mass, time, current, temperature, amount of substance, luminous intensity) or derived (combinations of fundamentals, e.g., velocity, force, energy).
Key Ideas The International System of Units (SI) defines seven base units. Since 2019 all seven are anchored to fixed numerical values of seven fundamental constants (\(c,\,h,\,e,\,k_B,\,N_A,\,\Delta\nu_{\text{Cs}},\,K_{\text{cd}}\)).
QuantityUnitSymbol
Lengthmetrem
Masskilogramkg
Timeseconds
Electric currentampereA
Thermodynamic temperaturekelvinK
Amount of substancemolemol
Luminous intensitycandelacd

Dimensional Analysis

Definition The dimension of a physical quantity is the power to which the base quantities must be raised to represent it, using the notation \([M],[L],[T],[I],[\Theta],[N],[J]\).

Examples: \([\text{Velocity}]=[LT^{-1}]\), \([\text{Force}]=[MLT^{-2}]\), \([\text{Energy}]=[ML^2T^{-2}]\), \([\text{Pressure}]=[ML^{-1}T^{-2}]\), \([\text{Charge}]=[IT]\).

Dimensional analysis is used to check equation homogeneity, derive relations between quantities, and convert units. The principle of homogeneity requires every term in a valid equation to share the same dimensions.

Limitations: it cannot determine dimensionless constants (e.g., the \(\tfrac{1}{2}\) in \(\tfrac{1}{2}mv^2\)), fails for transcendental functions, and cannot distinguish quantities with identical dimensions such as work and torque.

Errors in Measurement

Definition The difference between a measured value and the true value is the error. Errors are classified as systematic (consistent bias, e.g., calibration offset), random (unpredictable fluctuations, reduced by averaging), and gross (human mistakes).

For \(n\) repeated measurements \(a_1, a_2, \ldots, a_n\):

\[\bar{a} = \frac{1}{n}\sum_{i=1}^n a_i, \qquad \overline{\Delta a} = \frac{1}{n}\sum_i |a_i - \bar{a}|, \qquad \delta_r = \frac{\overline{\Delta a}}{\bar{a}}.\]

Propagation of Errors

For a function \(Z = f(A, B, \ldots)\): \[\text{Sum/difference:}\quad \Delta Z = \Delta A + \Delta B\] \[\text{Product/quotient:}\quad \frac{\Delta Z}{Z} = \frac{\Delta A}{A} + \frac{\Delta B}{B}\] \[\text{Power }Z = A^p B^q C^r:\quad \frac{\Delta Z}{Z} = |p|\frac{\Delta A}{A} + |q|\frac{\Delta B}{B} + |r|\frac{\Delta C}{C}\]
Worked Example Problem. The period of a simple pendulum is \(T = 2\pi\sqrt{L/g}\) with \(L = 1.00 \pm 0.01\) m and \(T = 2.00 \pm 0.02\) s. Find \(g\) and its percentage error. Solution. Since \(g = 4\pi^2 L/T^2\): \[\frac{\Delta g}{g} = \frac{\Delta L}{L} + 2\frac{\Delta T}{T} = 0.01 + 2(0.01) = 0.03\] \[g = \frac{4\pi^2 \times 1.00}{(2.00)^2} \approx 9.87\ \text{m s}^{-2}, \qquad \Delta g \approx 0.30\ \text{m s}^{-2}.\] Result: \(g = 9.87 \pm 0.30\ \text{m s}^{-2}\) (~3% error).
Likely University Questions
  1. State and explain the principle of homogeneity of dimensions. Verify \(s = ut + \tfrac{1}{2}at^2\).
  2. Differentiate between systematic and random errors with examples.
  3. Derive the percentage error in \(g\) measured by a simple pendulum.
  4. Discuss the limitations of dimensional analysis.
  5. Convert 1 newton into the CGS system using dimensional analysis.

2. Waves and Oscillations

Simple Harmonic Motion (SHM)

Definition Simple harmonic motion is periodic motion in which the restoring force is directly proportional to the displacement and directed toward the mean position: \(F = -kx.\)

Newton's second law gives \(m\ddot{x} = -kx\), i.e., \(\ddot{x} + \omega_0^2 x = 0\) with \(\omega_0 = \sqrt{k/m}\). The general solution is

\[x(t) = A\cos(\omega_0 t + \phi),\] where \(A\) is the amplitude, \(\omega_0\) is the angular frequency, period \(T = 2\pi/\omega_0\), frequency \(f = 1/T\), and \(\phi\) is the initial phase.

Energy in SHM

\[\text{KE} = \tfrac{1}{2}mv^2 = \tfrac{1}{2}m\omega_0^2(A^2 - x^2), \qquad \text{PE} = \tfrac{1}{2}kx^2\] \[E = \text{KE} + \text{PE} = \tfrac{1}{2}m\omega_0^2 A^2 = \tfrac{1}{2}kA^2 = \text{const.}\]
Key Ideas Total energy of an SHM oscillator is constant and proportional to \(A^2\). Displacement leads velocity by \(\pi/2\).

Damped Harmonic Oscillator

With a velocity-dependent damping force \(-b\dot{x}\):

\[m\ddot{x} + b\dot{x} + kx = 0 \quad\Longrightarrow\quad \ddot{x} + 2\gamma\dot{x} + \omega_0^2 x = 0, \qquad \gamma = \frac{b}{2m}.\]

Three regimes determined by the trial solution \(x \propto e^{\alpha t}\):

  • Under-damped (\(\gamma < \omega_0\)): oscillatory decay, \(x(t) = A_0 e^{-\gamma t}\cos(\omega' t + \phi)\), \(\omega' = \sqrt{\omega_0^2 - \gamma^2}\).
  • Critically damped (\(\gamma = \omega_0\)): fastest non-oscillatory return to equilibrium.
  • Over-damped (\(\gamma > \omega_0\)): slow exponential return.
Under-damped oscillation showing exponentially decaying sinusoidal motion with the amplitude envelope e raised to the power negative gamma t
Under-damped harmonic oscillator showing the oscillatory displacement and its exponentially decaying amplitude envelope \(e^{-\gamma t}\).

Quality Factor and Logarithmic Decrement

\[Q = \frac{\omega_0}{2\gamma}, \qquad \delta = \ln\frac{x_n}{x_{n+1}} = \gamma T'.\]

High \(Q\) implies low damping and a sharp resonance peak; \(\delta\) measures the decay per cycle.

Forced Oscillations and Resonance

With a driving force \(F_0\cos\omega t\), the steady-state amplitude is

\[A(\omega) = \frac{F_0/m}{\sqrt{(\omega_0^2 - \omega^2)^2 + 4\gamma^2\omega^2}}.\]

Resonance occurs at \(\omega_r = \sqrt{\omega_0^2 - 2\gamma^2} \approx \omega_0\) for small damping.

Key Ideas Bridges, buildings, and rotating machinery must avoid operating near their resonance frequency \(\omega_r\) to prevent catastrophic failure.

Travelling Waves

A harmonic transverse wave on a string: \(y = A\sin(kx - \omega t)\), satisfying

\[\frac{\partial^2 y}{\partial t^2} = v^2 \frac{\partial^2 y}{\partial x^2}, \qquad v = \sqrt{T/\mu},\] where \(T\) is the tension and \(\mu\) is the linear mass density. The dispersion relation is \(\omega = vk\), wavelength \(\lambda = 2\pi/k\). A travelling wave carries energy proportional to \(A^2\omega^2\) per unit length.

Standing Waves

Superposition of two counter-propagating waves gives

\[y = 2A\sin(kx)\cos(\omega t).\]

Nodes at \(kx = n\pi\); antinodes at \(kx = (n + \tfrac{1}{2})\pi\). Normal modes of a string of length \(L\) fixed at both ends:

\[\lambda_n = \frac{2L}{n}, \qquad f_n = \frac{nv}{2L}, \qquad n = 1, 2, 3, \ldots\]

Sound Waves and Doppler Effect

Sound in air consists of longitudinal pressure waves with speed \(v = \sqrt{B/\rho}\) (\(B\) = bulk modulus). Intensity \(I = \tfrac{1}{2}\rho v\omega^2 A^2\). Sound level in decibels:

\[\beta = 10\log_{10}\!\left(\frac{I}{I_0}\right)\ \text{dB}, \qquad I_0 = 10^{-12}\ \text{W m}^{-2}.\]

For a source moving at velocity \(v_s\) and observer at \(v_o\) along the same line:

\[f' = f_0\,\frac{v \pm v_o}{v \mp v_s}.\]

Applications include radar speed guns, Doppler ultrasound, and astronomical redshift.

Phase Velocity and Group Velocity

A monochromatic wave travels at the phase velocity \(v_p = \omega/k\). A wave packet (real signal) has its envelope moving at the group velocity

\[v_g = \frac{d\omega}{dk}.\]
Key Ideas Information and energy travel at \(v_g\), not \(v_p\). In a non-dispersive medium \(\omega = vk\) so \(v_g = v_p\). In a dispersive medium (optical fiber, plasma) \(v_g \ne v_p\). For matter waves, \(E = \hbar\omega\) and \(p = \hbar k\), giving \(v_g = v_{\text{particle}}\), confirming the de Broglie packet moves with the particle.
Likely University Questions
  1. Derive the differential equation of a damped harmonic oscillator and discuss the three regimes.
  2. Define quality factor and logarithmic decrement; relate them.
  3. Derive the resonance amplitude formula for a driven oscillator.
  4. Obtain the speed of a transverse wave on a stretched string.
  5. State and prove the relations for nodes and antinodes in a standing wave on a fixed string.
  6. Derive the Doppler formula when source and observer both move.

3. Interference of Light

Wave Theory and Coherence

Light is a transverse electromagnetic wave with visible wavelengths from 400 to 700 nm. Two beams from coherent sources combine by linear superposition, producing intensity variations called interference.

Principle Two sources are coherent if they emit waves of the same frequency with a constant phase difference. For sustained interference the sources must also be narrow and close, with nearly equal amplitudes and matching polarization states.

Intensity Distribution

For fields \(E_1 = E_0\cos\omega t\) and \(E_2 = E_0\cos(\omega t + \delta)\), the resultant time-averaged intensity is

\[I = 4I_0\cos^2(\delta/2).\]

Maxima when \(\delta = 2n\pi\); minima when \(\delta = (2n+1)\pi\).

Young's Double-Slit Experiment (YDSE)

For slit separation \(d\) and screen distance \(D\), the path difference for a point at height \(y\) is \(\Delta = yd/D\). Bright fringes at \(\Delta = n\lambda\), dark at \(\Delta = (n + \tfrac{1}{2})\lambda\). The fringe width (spacing between successive bright or dark fringes) is

\[\beta = \frac{\lambda D}{d}.\]
Young's double-slit experiment diagram showing two slits S1 and S2, the screen at distance D, and the interference fringe pattern with alternating bright and dark bands
Young's double-slit experiment: slits \(S_1\) and \(S_2\) separated by \(d\) produce alternating bright and dark fringes on a screen at distance \(D\). Fringe width \(\beta = \lambda D/d\).
Worked Example In a YDSE, \(d = 0.5\) mm, \(D = 1.0\) m, \(\lambda = 589\) nm. Find the fringe width. \[\beta = \frac{(589 \times 10^{-9})(1.0)}{0.5 \times 10^{-3}} = 1.18\ \text{mm}.\] Consecutive bright fringes are separated by approximately 1.18 mm.

Thin-Film Interference

For a film of refractive index \(\mu\) and thickness \(t\), with light incident at angle \(i\) refracting at \(r\):

\[\Delta = 2\mu t\cos r \pm \frac{\lambda}{2}.\]

The \(\lambda/2\) term arises from the phase reversal on reflection at the denser medium. For reflected light: maxima when \(2\mu t\cos r = (n + \tfrac{1}{2})\lambda\); minima when \(2\mu t\cos r = n\lambda\).

Newton's Rings

A plano-convex lens of radius \(R\) resting on a flat glass plate creates an air wedge. In reflected monochromatic light the radii of dark and bright rings are

\[r_n^{\text{dark}} = \sqrt{n\lambda R}, \qquad r_n^{\text{bright}} = \sqrt{(n + \tfrac{1}{2})\lambda R}.\]
Newton's rings setup showing a plano-convex lens of radius R resting on a flat glass plate, creating concentric circular interference rings in reflected light
Newton's rings formed by a plano-convex lens on a flat plate. The dark central spot confirms the half-wavelength phase shift at the glass–air interface at normal incidence.

Wavelength determination using two ring orders \(n\) and \(n+p\):

\[\lambda = \frac{D_{n+p}^2 - D_n^2}{4pR}, \qquad D = 2r.\]
Likely University Questions
  1. Define coherence. State the conditions for sustained interference.
  2. Derive the expression for fringe width in YDSE.
  3. Explain colours observed in thin films and derive the path-difference condition.
  4. Describe Newton's rings experiment and derive the formula for \(\lambda\).

4. Diffraction

Definition and Types

Definition Diffraction is the bending of light into the geometrical shadow of an obstacle, accompanied by intensity redistribution. Fresnel diffraction occurs when source or screen is at a finite distance (curved wavefronts); Fraunhofer diffraction requires source and screen effectively at infinity (plane wavefronts), achieved practically with lenses.

Single-Slit Fraunhofer Diffraction

For slit width \(a\) and wavelength \(\lambda\), the intensity at angle \(\theta\) is

\[I(\theta) = I_0\left(\frac{\sin\beta}{\beta}\right)^2, \qquad \beta = \frac{\pi a\sin\theta}{\lambda}.\]

Minima (nodes) occur when \(a\sin\theta = m\lambda\), \(m = \pm 1, \pm 2, \ldots\) The width of the central maximum on a screen at focal length \(f\) is \(w_0 = 2\lambda f/a\).

Single-slit Fraunhofer diffraction intensity pattern showing a dominant central maximum with progressively weaker secondary maxima on either side, plotted against the variable beta
Fraunhofer single-slit diffraction pattern. The central maximum carries approximately 84% of the total energy, with secondary maxima decreasing rapidly in intensity.
Worked Example A single slit of width 0.1 mm is illuminated by light of wavelength 600 nm. Find the angular width of the central maximum. \[\sin\theta_1 = \frac{\lambda}{a} = \frac{600 \times 10^{-9}}{0.1 \times 10^{-3}} = 6 \times 10^{-3}.\] Angular full-width \(\approx 0.687°\) or 12 mrad.

Double-Slit Diffraction

The pattern combines the single-slit envelope with two-source interference:

\[I(\theta) = I_0\left(\frac{\sin\beta}{\beta}\right)^2\cos^2\gamma, \qquad \beta = \frac{\pi a\sin\theta}{\lambda},\quad \gamma = \frac{\pi d\sin\theta}{\lambda}.\]

Missing orders occur when \(d/a\) is an integer, causing an interference maximum to coincide with a diffraction minimum.

Diffraction Grating

For \(N\) slits with grating element \(d = a + b\), the principal maxima satisfy the grating equation \(d\sin\theta = n\lambda\). The resolving and dispersive powers are

\[R = \frac{\lambda}{\Delta\lambda} = nN, \qquad \frac{d\theta}{d\lambda} = \frac{n}{d\cos\theta}.\]

Applications include spectrometers, wavelength-division multiplexing (WDM) in optical fiber systems, and astronomical spectroscopy.

Resolving Power of Optical Instruments

For a telescope with circular aperture \(D\): \(\theta_{\min} = 1.22\lambda/D\). For a microscope with numerical aperture \(NA\): \(d_{\min} = 0.61\lambda/NA\).

Key Ideas The diffraction limit is a fundamental cap on resolution. Super-resolution techniques (STED, PALM, STORM) use quantum optical effects to circumvent it.
Likely University Questions
  1. Distinguish between Fresnel and Fraunhofer diffraction.
  2. Derive the intensity formula for single-slit Fraunhofer diffraction.
  3. Discuss missing orders in the double-slit pattern.
  4. Define dispersive power and resolving power of a grating.
  5. State and derive the Rayleigh criterion.

5. Polarization

Definition Polarization is the orientation of the electric-field vector of a transverse wave. Light is polarized when its \(\vec{E}\) vibrates along a specific direction. Types include linear (plane), circular, and elliptical polarization; natural (unpolarized) light has random \(\vec{E}\) orientations.

Methods of producing polarized light: reflection (Brewster's law), refraction in birefringent crystals, selective absorption (Polaroid films), and Rayleigh scattering.

Brewster's Law

At the polarizing angle \(\theta_p\), the reflected beam is completely plane-polarized:

\[\tan\theta_p = \mu.\]

For glass (\(\mu = 1.5\)), \(\theta_p \approx 56.3°\). The reflected and refracted rays are perpendicular. Applications: polarizing sunglasses, laser Brewster windows.

Malus's Law

Linearly polarized light of intensity \(I_0\) transmitted through an analyzer at angle \(\theta\):

\[I = I_0\cos^2\theta.\]

Double Refraction and Wave Plates

Calcite and quartz are birefringent: the incident ray splits into an ordinary ray (obeys Snell's law) and an extraordinary ray (direction-dependent index \(n_e\)). The optic axis is the direction along which \(n_o = n_e\). A quarter-wave plate has thickness such that \((n_o - n_e)t = \lambda/4\), converting linear to circular polarization; a half-wave plate satisfies \((n_o - n_e)t = \lambda/2\) and rotates the plane of polarization by 90°.

Engineering Applications LCD displays (each pixel is a polarization gate), 3-D cinema, photoelastic stress analysis, saccharimetry, and polarization-maintaining optical fibers.
Likely University Questions
  1. State and prove Brewster's law.
  2. Derive Malus's law from electric-field projection.
  3. Explain double refraction and define optic axis.
  4. Differentiate quarter-wave and half-wave plates.

6. Lasers

Principle of Laser Action

LASER stands for Light Amplification by Stimulated Emission of Radiation. Three processes operate between atomic levels \(E_1\) and \(E_2\) (\(E_2 > E_1\)): stimulated absorption (\(E_1 \to E_2\)), spontaneous emission (\(E_2 \to E_1\), random phase), and stimulated emission (incident photon induces an identical coherent photon).

Einstein Coefficients

In thermal equilibrium with radiation density \(\rho(\nu)\):

\[\frac{A_{21}}{B_{21}} = \frac{8\pi h\nu^3}{c^3}, \qquad B_{12}g_1 = B_{21}g_2.\]

Population Inversion and Pumping

Principle Laser action requires the upper level population to exceed the lower level population, \(N_2 > N_1\) — a non-thermal condition called population inversion. A two-level system cannot achieve inversion; three- or four-level schemes with a metastable upper state are required.

Three- and Four-Level Laser Schemes

Energy level diagram comparing three-level laser scheme (Ruby) and four-level laser scheme (Nd:YAG, He-Ne) showing pump transitions, fast relaxation, and laser transitions
Comparison of three-level (Ruby) and four-level (Nd:YAG, He–Ne) laser energy schemes. Four-level lasers are more efficient because the lower laser level rapidly empties.

An optical resonator (high-reflectance mirror + output coupler) provides feedback to sustain and amplify the stimulated emission.

Properties of Laser Light

  • Monochromaticity: extreme spectral purity, \(\Delta\lambda/\lambda \sim 10^{-8}\).
  • Coherence: high spatial and temporal coherence.
  • Directionality: divergence \(\theta \sim \lambda/D\).
  • High intensity/brightness.

Specific Laser Types

Ruby Laser

Active medium: Cr³⁺-doped Al₂O₃. Pump: xenon flash lamp. Wavelength: 694.3 nm (red). Pulsed 3-level operation. Efficiency ~1%. Applications: holography, ranging, tattoo removal.

He–Ne Laser

Active medium: He–Ne gas (10:1) at low pressure. Pump: DC discharge. Principal wavelength: 632.8 nm (red). Continuous wave, 4-level operation. Applications: interferometry, alignment, barcode readers.

Semiconductor (Diode) Laser

Stimulated emission across the band gap in a heavily doped p–n junction. Wavelength: \(\lambda = hc/E_g\) (e.g., GaAs at ~840 nm, InGaAsP at 1.55 μm). Electrically pumped, compact, efficiency >50%. Applications: optical communication, DVD/Blu-ray, LiDAR.

Worked Example A 1-mW He–Ne laser emits at 632.8 nm. Photons per second? \[E_{\text{ph}} = \frac{hc}{\lambda} = \frac{6.626 \times 10^{-34} \times 3 \times 10^8}{632.8 \times 10^{-9}} \approx 3.14 \times 10^{-19}\ \text{J}\] \[N = \frac{P}{E_{\text{ph}}} = \frac{10^{-3}}{3.14 \times 10^{-19}} \approx 3.18 \times 10^{15}\ \text{s}^{-1}.\]

Holography

Definition A hologram records both amplitude and phase of scattered light by interfering the object beam with a coherent reference beam. Illuminating the recording with the reference reconstructs the original three-dimensional wavefront.

Recording intensity: \(I(\vec{r}) = |E_R + E_O|^2 = |E_R|^2 + |E_O|^2 + 2\,\text{Re}(E_R^* E_O)\). The cross term carries the object phase. Reconstruction with \(E_R\) produces the term \(\propto E_O\). Applications: security holograms, holographic data storage, head-up displays, vibration analysis.

Engineering Applications Material processing (cutting, welding), optical communication, medicine (LASIK, surgery), defense (LiDAR, range-finding), holography, precision metrology, and fusion research (NIF).
Likely University Questions
  1. Derive the relations among Einstein's \(A\) and \(B\) coefficients.
  2. Explain population inversion and pumping mechanisms.
  3. Describe the construction and working of the Ruby, He–Ne, or semiconductor laser.
  4. List four properties of laser light with engineering examples.

7. Fiber Optics

Basic Principle

An optical fiber is a glass or plastic cylinder guiding light by repeated total internal reflection (TIR) at the core–cladding interface. The core has refractive index \(n_1\), the cladding \(n_2 < n_1\).

Acceptance Angle and Numerical Aperture

TIR condition at the core–cladding interface: \(\sin\theta_c = n_2/n_1\). The acceptance (half-)cone angle in air:

\[\text{NA} = \sin\theta_a = \sqrt{n_1^2 - n_2^2} \approx n_1\sqrt{2\Delta}, \qquad \Delta = \frac{n_1 - n_2}{n_1}.\]
Cross-section of an optical fiber showing a ray undergoing repeated total internal reflection between the high-index core and lower-index cladding, with the acceptance cone at the input end
Ray path in a step-index optical fiber demonstrating total internal reflection. Light entering within the acceptance cone (half-angle \(\theta_a\)) is guided along the core.

Classification of Optical Fibers

TypeRefractive index profileUse
Step-index single-mode (SMF)Step, \(V < 2.405\)Long-haul telecom
Step-index multi-mode (MMF)Step, \(V > 2.405\)Short links, sensors
Graded-index multi-modeParabolic profileMedium distance, low dispersion

The V-number \(V = (2\pi a/\lambda)\,\text{NA}\) determines how many modes propagate. Single-mode operation requires \(V < 2.405\).

Attenuation and Dispersion

Attenuation: \(\alpha = \frac{10}{L}\log_{10}(P_{\text{in}}/P_{\text{out}})\) [dB/km]. Typical silica fiber: ~0.2 dB/km at 1.55 μm. Sources of loss: absorption (OH ions, IR lattice), Rayleigh scattering (\(\propto 1/\lambda^4\)), and bending losses. Dispersion (modal, material, waveguide) broadens pulses and limits data rate.

Worked Example A step-index fiber has \(n_1 = 1.500\), \(n_2 = 1.480\). \[\text{NA} = \sqrt{1.500^2 - 1.480^2} = \sqrt{0.0596} \approx 0.244\] \[\theta_a = \sin^{-1}(0.244) \approx 14.1°.\] Light entering within a ±14° cone is guided.
Likely University Questions
  1. Derive expressions for acceptance angle and numerical aperture.
  2. Classify optical fibers based on RI profile and mode count.
  3. Discuss losses and dispersion in optical fibers.
  4. Explain the block diagram of an optical-fiber communication system.

8. Origins of Quantum Mechanics

Failure of Classical Physics

By 1900, several experimental results could not be explained by classical theory: the blackbody radiation spectrum (UV catastrophe), photoelectric effect, Compton scattering, atomic emission line spectra, and the specific heats of solids at low temperature. These resolutions gave birth to quantum mechanics.

Planck's Radiation Law (1900)

Energy of a harmonic oscillator is quantized: \(E_n = nh\nu\). Planck's radiation law:

\[u(\nu, T)\,d\nu = \frac{8\pi h\nu^3}{c^3}\frac{1}{e^{h\nu/k_BT} - 1}\,d\nu.\]

Low-frequency limit recovers the Rayleigh–Jeans law; high-frequency limit gives Wien's law. The Stefan–Boltzmann result \(E = \sigma T^4\) with \(\sigma = 5.67 \times 10^{-8}\ \text{W m}^{-2} \text{K}^{-4}\) follows by integration.

Photoelectric Effect (Einstein, 1905)

Einstein's equation:

\[h\nu = \phi + \tfrac{1}{2}mv_{\max}^2,\] where \(\phi\) is the work function, threshold frequency \(\nu_0 = \phi/h\), and stopping potential \(eV_s = h\nu - \phi\). Photocurrent is proportional to intensity (one electron per photon).

Compton Scattering (1923)

An X-ray photon of wavelength \(\lambda\) scattered through angle \(\theta\) by a free electron shifts to

\[\Delta\lambda = \lambda' - \lambda = \frac{h}{m_e c}(1 - \cos\theta), \qquad \frac{h}{m_e c} = 2.43 \times 10^{-12}\ \text{m.}\]

This establishes the photon as a relativistic particle with energy \(h\nu\) and momentum \(h\nu/c\).

de Broglie Hypothesis (1924)

Every particle has an associated matter wave:

\[\lambda = \frac{h}{p} = \frac{h}{mv}.\]

For an electron accelerated through potential \(V\): \(\lambda = 12.27/\sqrt{V}\ \text{Å}\). The Davisson–Germer experiment (1927) confirmed this via electron diffraction from a nickel crystal (\(\lambda_{\text{de Broglie}} \approx 1.67\ \text{Å}\), \(\lambda_{\text{exp}} \approx 1.65\ \text{Å}\) from Bragg's law on Ni (110) planes).

Heisenberg Uncertainty Principle

For conjugate variables:

\[\Delta x\,\Delta p \ge \frac{\hbar}{2}, \qquad \Delta E\,\Delta t \ge \frac{\hbar}{2}.\]
Key Ideas A particle's position and momentum cannot both be known exactly. Confinement forces a minimum (zero-point) kinetic energy — the basis of atomic stability and zero-point motion in solids.
Worked Example An electron is confined within \(\Delta x = 10^{-10}\) m: \[\Delta p \ge \frac{\hbar}{2\Delta x} = \frac{1.054 \times 10^{-34}}{2 \times 10^{-10}} \approx 5.27 \times 10^{-25}\ \text{kg m s}^{-1}\] \[E_{\min} \approx \frac{(\Delta p)^2}{2m_e} \approx 1.52 \times 10^{-19}\ \text{J} \approx 0.95\ \text{eV}.\]

Wave Function — Born Interpretation

A particle is described by a complex wave function \(\psi(\vec{r}, t)\) such that \(|\psi(\vec{r}, t)|^2\,dV\) is the probability of finding the particle in volume \(dV\). Normalization: \(\int|\psi|^2\,dV = 1\). The wave function must be single-valued, finite, continuous, with continuous first derivative wherever the potential is finite.

Likely University Questions
  1. Derive Planck's radiation law and discuss its classical limits.
  2. Explain Einstein's interpretation of the photoelectric effect.
  3. Derive the de Broglie wavelength of an electron accelerated through potential \(V\).
  4. Derive the time-independent Schrödinger equation by separation of variables.

9. Schrödinger Equation

Time-Dependent Schrödinger Equation

For a non-relativistic particle of mass \(m\) in potential \(V(\vec{r}, t)\):

\[i\hbar\frac{\partial\psi}{\partial t} = -\frac{\hbar^2}{2m}\nabla^2\psi + V(\vec{r}, t)\psi.\]

For a free particle (\(V = 0\)), the plane wave \(\psi = e^{i(\vec{k}\cdot\vec{r} - \omega t)}\) requires \(\hbar\omega = \hbar^2 k^2/2m\), recovering the de Broglie relation.

Time-Independent Schrödinger Equation (TISE)

If \(V = V(\vec{r})\), writing \(\psi = u(\vec{r})e^{-iEt/\hbar}\) leads to the eigenvalue equation:

\[-\frac{\hbar^2}{2m}\nabla^2 u + Vu = Eu.\]

For a stationary state, \(|\psi|^2\) is independent of time.

Probability Current

\(\vec{J} = \frac{\hbar}{2mi}\left[\psi^*\nabla\psi - \psi\nabla\psi^*\right]\) satisfies the continuity equation \(\partial|\psi|^2/\partial t + \nabla\cdot\vec{J} = 0\). Probability is conserved. This describes tunneling currents in scanning tunneling microscopes.

Postulates of Quantum Mechanics

  1. Physical state described by \(\psi\), a vector in Hilbert space.
  2. Every observable is represented by a Hermitian operator.
  3. The only possible measurement results are eigenvalues of that operator.
  4. Probability of obtaining eigenvalue \(a_i\) is \(|\langle\phi_i|\psi\rangle|^2\).
  5. After measurement of \(a_i\), \(\psi\) collapses to \(\phi_i\).
  6. Time evolution between measurements governed by the Schrödinger equation.
Likely University Questions
  1. Derive Planck's radiation law and its classical limits.
  2. Explain the photoelectric effect — Einstein's interpretation.
  3. Derive the de Broglie wavelength; describe the Davisson–Germer experiment.
  4. Derive the TISE by separation of variables from the TDSE.

10. Particle in a Box

One-Dimensional Infinite Well

Potential: \(V(x) = 0\) for \(0 < x < L\), \(V = \infty\) elsewhere. Inside the box TISE gives \(u'' + k^2 u = 0\) with \(k = \sqrt{2mE}/\hbar\). Boundary conditions \(u(0) = u(L) = 0\) quantize \(k\) to \(k_n = n\pi/L\):

\[u_n(x) = \sqrt{\frac{2}{L}}\sin\!\left(\frac{n\pi x}{L}\right), \qquad E_n = \frac{n^2\pi^2\hbar^2}{2mL^2}, \quad n = 1, 2, 3, \ldots\]

Key features: energies scale as \(n^2\); there is a non-zero zero-point energy \(E_1\); nodes increase with \(n\); spacing widens as \(L\) shrinks — the basis of quantum confinement.

Wavefunctions of the first four energy states (n equals 1 to 4) for a particle in a one-dimensional infinite square well, showing increasing number of nodes with quantum number
Normalized wavefunctions \(\psi_n(x)\) for states \(n = 1\) to \(4\) inside a 1-D infinite potential well of width \(L\). Each successive state has one additional node.
Worked Example An electron is confined in a 1-D box of width 1 nm. Find \(E_1\) and \(E_3\): \[E_1 = \frac{\pi^2(1.054 \times 10^{-34})^2}{2(9.11 \times 10^{-31})(10^{-9})^2} \approx 6.02 \times 10^{-20}\ \text{J} \approx 0.376\ \text{eV}.\] \[E_3 = 9E_1 \approx 3.38\ \text{eV}.\]

Three-Dimensional Infinite Box

Inside a cube of side \(L\):

\[E_{n_x n_y n_z} = \frac{\pi^2\hbar^2}{2mL^2}(n_x^2 + n_y^2 + n_z^2).\]

Different triples \((n_x, n_y, n_z)\) with the same sum of squares are degenerate.

Engineering Applications Quantum dots are real-world realizations of 3-D boxes; their photoluminescence wavelength is tunable by size. They are used in QLED displays, semiconductor lasers, photovoltaics, and single-photon sources.
Likely University Questions
  1. Solve the 1-D infinite well and obtain \(E_n\) and \(\psi_n\).
  2. Discuss zero-point energy and degeneracy in a 3-D box.
  3. Determine the most probable position of a particle in the \(n = 2\) state.

11. Free Electron Theory and Band Theory

Classical (Drude) Free Electron Theory

Valence electrons are treated as a classical ideal gas colliding with positive ions (relaxation time \(\tau\)). Electrical conductivity: \(\sigma = ne^2\tau/m\). Wiedemann–Franz law: \(\kappa/\sigma = LT\) with \(L \approx 2.45 \times 10^{-8}\ \text{W}\Omega\,\text{K}^{-2}\). The model fails to predict the correct electronic specific heat and has no explanation for insulators.

Sommerfeld Quantum Free-Electron Theory

Electrons are non-interacting fermions filling states up to the Fermi energy \(E_F\):

\[g(E) = \frac{1}{2\pi^2}\left(\frac{2m}{\hbar^2}\right)^{3/2}E^{1/2}, \qquad E_F = \frac{\hbar^2}{2m}(3\pi^2 n)^{2/3}.\]

At \(T > 0\), electrons obey the Fermi–Dirac distribution:

\[f(E) = \frac{1}{e^{(E-\mu)/k_BT} + 1}.\]

This gives the correct \(T\)-linear electronic specific heat \(C_v^{\text{el}} = \frac{\pi^2}{2}nk_B(T/T_F)\) and recovers the Wiedemann–Franz law.

Bloch's Theorem and Band Formation

A periodic potential \(V(\vec{r}) = V(\vec{r} + \vec{R})\) leads to Bloch eigenfunctions:

\[\psi_{\vec{k}}(\vec{r}) = e^{i\vec{k}\cdot\vec{r}}u_{\vec{k}}(\vec{r}), \qquad u_{\vec{k}}(\vec{r}) = u_{\vec{k}}(\vec{r} + \vec{R}).\]

Allowed energies form continuous bands separated by forbidden gaps.

Kronig–Penney Model

A 1-D periodic square-well potential (barrier strength \(P\)) gives the condition

\[\cos(ka) = \cos(\alpha a) + P\frac{\sin(\alpha a)}{\alpha a}, \qquad \alpha = \frac{\sqrt{2mE}}{\hbar}.\]

Forbidden gaps appear at Brillouin-zone boundaries \(k = n\pi/a\). As \(P \to 0\) the free-electron parabola is recovered; as \(P \to \infty\) discrete atomic levels emerge.

Effective Mass

The curvature of the dispersion relation \(E(k)\) defines the effective mass:

\[\frac{1}{m^*} = \frac{1}{\hbar^2}\frac{d^2E}{dk^2}.\]

Near band minima \(m^* > 0\) (electron-like); near band maxima \(m^* < 0\) leading to hole behavior. The effective mass controls carrier mobility and density of states.

Classification by Band Filling

Conductors have overlapping valence and conduction bands. Semiconductors have a small gap (~1 eV); insulators have a large gap (>5 eV).

Likely University Questions
  1. Compare classical, Sommerfeld, and band theories of metals.
  2. Derive the Fermi energy of a 3-D free-electron gas.
  3. State and discuss Bloch's theorem.
  4. Discuss the Kronig–Penney model qualitatively.
  5. Define effective mass and explain its physical significance.

12. Semiconductor Physics

Intrinsic Semiconductors

In a pure semiconductor, thermal generation across the band gap governs carrier concentration:

\[n_i = \sqrt{N_c N_v}\,e^{-E_g/2k_BT},\] where \(N_c\) and \(N_v\) are the effective densities of states in the conduction and valence bands. The Fermi level lies near the mid-gap:

\[E_F = \frac{E_c + E_v}{2} + \frac{k_BT}{2}\ln\frac{N_v}{N_c}.\]

Typical band gaps: Si (1.12 eV), Ge (0.67 eV), GaAs (1.43 eV).

Extrinsic Semiconductors — Doping

n-type: pentavalent donors (P, As, Sb) donate electrons; donor level \(E_d\) just below \(E_c\). For fully ionized donors: \(n \approx N_D\), \(p = n_i^2/N_D\). p-type: trivalent acceptors (B, Al) create holes; acceptor level \(E_a\) just above \(E_v\). Law of mass action: \(np = n_i^2\).

Carrier Transport: Drift and Diffusion

Drift: \(J_n^{\text{drift}} = en\mu_n E\), \(J_p^{\text{drift}} = ep\mu_p E\). Diffusion: \(J_n^{\text{diff}} = eD_n(dn/dx)\), \(J_p^{\text{diff}} = -eD_p(dp/dx)\). Einstein relation: \(D/\mu = k_BT/e\).

Hall Effect

A current-carrying conductor in a transverse magnetic field develops a transverse Hall voltage \(V_H = IB/(net)\). Hall coefficient \(R_H = 1/(nq)\); its sign identifies the carrier type and its magnitude gives carrier density.

Worked Example \(V_H = 6.25\) mV, \(I = 10\) mA, \(B = 0.5\) T, \(t = 1\) mm: \[R_H = \frac{V_H\,t}{IB} = \frac{(6.25 \times 10^{-3})(10^{-3})}{(10^{-2})(0.5)} = 1.25 \times 10^{-3}\ \text{m}^3\ \text{C}^{-1}\] \[n = \frac{1}{eR_H} \approx 5 \times 10^{21}\ \text{m}^{-3}.\]

p–n Junction

Diffusion of carriers creates a depletion region with a built-in potential:

\[V_{\text{bi}} = \frac{k_BT}{e}\ln\!\left(\frac{N_A N_D}{n_i^2}\right).\]

Shockley ideal diode equation: \(I = I_S(e^{eV/k_BT} - 1)\). Reverse breakdown: Zener (tunneling, narrow depletion layer, \(|V_z| \lesssim 5\) V, negative temperature coefficient) and avalanche (impact ionization, positive \(T\)-coefficient).

Likely University Questions
  1. Derive expressions for \(n_i\) and \(E_F\) in intrinsic semiconductors.
  2. Derive the law of mass action and the Einstein relation.
  3. Describe the Hall effect and its applications.
  4. Derive the diode equation; explain Zener and avalanche breakdown.

13. Diodes and Transistors

Diode Types

Rectifier diodes (power conversion), Zener diodes (voltage regulation), LEDs (electroluminescence), photodiodes (optical detection), solar cells (photovoltaics), Schottky diodes (fast switching), tunnel diodes (negative resistance), and varactors (voltage-controlled capacitance).

Rectifier Circuits

Half-wave rectifier: \(V_{\text{dc}} = V_m/\pi\), efficiency \(\eta = 40.6\%\), ripple \(\gamma = 1.21\). Full-wave bridge rectifier: \(V_{\text{dc}} = 2V_m/\pi\), \(\eta = 81.2\%\), \(\gamma = 0.48\). LC or capacitor filters reduce ripple.

Bipolar Junction Transistor (BJT)

Two back-to-back p–n junctions (NPN or PNP). In active mode (EB forward, CB reverse): \(I_E = I_B + I_C\), \(\alpha = I_C/I_E < 1\), \(\beta = I_C/I_B = \alpha/(1-\alpha) \gg 1\).

ParameterCBCECC
Input impedanceLowMediumHigh
Output impedanceHighMediumLow
Voltage gainHighHigh<1
Current gain\(\alpha < 1\)\(\beta\) highHigh
Phase shift180°
UseRF ampGeneral ampBuffer/follower

Field-Effect Transistors (FETs)

JFET: current controlled by reverse-biased gate; very high input impedance (>10⁹ Ω). MOSFET: oxide-isolated gate; enhancement or depletion mode. Saturation drain current (enhancement MOSFET):

\[I_D = \frac{1}{2}\mu_n C_{ox}\frac{W}{L}(V_{GS} - V_{TH})^2.\]

CMOS (complementary MOSFET) is the foundation of modern digital electronics.

Likely University Questions
  1. Derive the efficiency and ripple factor of half- and full-wave rectifiers.
  2. Compare CE, CB, CC configurations of a BJT.
  3. Derive the drain-current expression for a saturated MOSFET.
  4. Explain LED operation and its difference from a normal diode.

14. Superconductivity

Definition A superconductor is a material that exhibits zero electrical resistance below a critical temperature \(T_c\) and completely expels magnetic flux from its interior (Meissner effect). Discovered by Kamerlingh Onnes (1911) in mercury at 4.2 K.

Critical Parameters

The superconducting state is bounded by three quantities: critical temperature \(T_c\), critical field \(H_c(T) = H_0[1-(T/T_c)^2]\), and critical current density \(J_c\). The Meissner effect (\(\vec{B} = 0\) inside the bulk below \(T_c\)) distinguishes a superconductor from a perfect conductor.

Type-I vs Type-II Superconductors

Type-IType-II
Critical field(s)Single \(H_c\)\(H_{c1}\) and \(H_{c2}\)
Mixed stateNoneFlux vortices between \(H_{c1}\) and \(H_{c2}\)
ExamplesHg, Pb, SnNb-Ti, Nb₃Sn, YBCO (HTS, \(T_c \sim 92\) K)
UseLab curiositiesMRI, accelerators, motors

BCS Theory

Bardeen–Cooper–Schrieffer (1957): phonon-mediated attraction causes pairs of electrons with opposite momenta and spins (Cooper pairs) to condense into a coherent macroscopic quantum state below \(T_c\). An energy gap \(2\Delta\) forms; excitation requires breaking pairs, hence zero resistance. BCS prediction: \(2\Delta(0) \approx 3.52\,k_BT_c\).

London Equations and Penetration Depth

\[\nabla^2\vec{B} = \frac{\vec{B}}{\lambda_L^2}, \qquad \lambda_L = \sqrt{\frac{m}{\mu_0 n_s e^2}}.\]

\(\lambda_L\) is the London penetration depth, the skin depth for magnetic flux.

Josephson Effects

DC Josephson: Cooper-pair tunneling through a thin insulating barrier gives \(I = I_c\sin\phi\) at zero voltage. AC Josephson: a constant voltage \(V\) produces oscillating current at \(\omega = 2eV/\hbar\). Applications: SQUIDs (world's most sensitive magnetometers), voltage standards, superconducting qubits.

Engineering Applications MRI scanners, LHC dipole magnets, maglev trains, fault-current limiters, superconducting power cables, SQUID magnetometers, and quantum computing (transmon qubits).
Likely University Questions
  1. State the properties of superconductors. Distinguish Type-I and Type-II.
  2. Explain the Meissner effect and its significance.
  3. Briefly describe BCS theory and the energy gap.
  4. Describe DC and AC Josephson effects and give one application.

15. Nanotechnology

Definition Nanotechnology is the design, characterization, production, and application of structures, devices, and systems with dimensions in the range 1–100 nm.

At the nanoscale: quantum confinement modifies electronic properties, the surface-to-volume ratio is enormously enhanced, mean-free-path effects govern transport, and optical resonances (plasmons) appear at characteristic sizes.

Dimensional Classification of Nanostructures

DimensionalityConfined directionsExamples
3-D bulk0Bulk metal, semiconductor
2-D thin films / quantum wells1GaAs/AlGaAs heterostructure
1-D nanowires / quantum wires2Si nanowire, CNT, ZnO
0-D quantum dots3CdSe, PbS QD, colloidal QD

Synthesis Methods

Top-down (start large, carve to nanoscale): lithography (photo, e-beam, EUV), etching (RIE, wet), ball milling. Bottom-up (atom-by-atom assembly): CVD/PVD, MBE, ALD, sol-gel, self-assembly, colloidal chemistry.

Characterization Techniques

ToolInformation
SEM, TEMMorphology, crystallography
AFM, STMSurface topography, atomic imaging
XRDCrystal structure, phase
Raman, FTIRVibrational fingerprint, bonds
UV-vis, PLOptical band gap, excitons
XPS, EDXElemental and chemical state
BETSpecific surface area

Special Nanomaterials

Carbon nanotubes (CNTs): rolled graphene, ballistic transport, Young's modulus ~TPa. Graphene: monolayer carbon, massless Dirac fermions, extremely high conductivity. Quantum dots: size-tunable photoluminescence. Nano-Ag, Nano-Au: plasmonic absorption, sensing, antibacterial. TiO₂, ZnO nanoparticles: photocatalysis, UV protection.

Likely University Questions
  1. Define nanomaterials and classify them by dimensionality.
  2. Compare top-down and bottom-up approaches with examples.
  3. Discuss synthesis and applications of carbon nanotubes.
  4. Mention three applications of nanotechnology in energy.

16. Electromagnetism

Vector Calculus Toolkit

Gradient \(\nabla\phi\) (steepest rise), divergence \(\nabla\cdot\vec{F}\) (source density), curl \(\nabla\times\vec{F}\) (rotation), Laplacian \(\nabla^2\phi = \nabla\cdot(\nabla\phi)\). Gauss's theorem: \(\oint_S \vec{F}\cdot d\vec{A} = \int_V (\nabla\cdot\vec{F})\,dV\). Stokes' theorem: \(\oint_C \vec{F}\cdot d\vec{\ell} = \int_S (\nabla\times\vec{F})\cdot d\vec{A}\).

Electrostatics

Coulomb force: \(\vec{F}_{12} = \frac{1}{4\pi\varepsilon_0}\frac{q_1 q_2}{r_{12}^2}\hat{r}_{12}\). Gauss's law: \(\oint\vec{E}\cdot d\vec{A} = Q_{\text{enc}}/\varepsilon_0\), equivalently \(\nabla\cdot\vec{E} = \rho/\varepsilon_0\). Potential: \(\vec{E} = -\nabla V\). Energy stored in a field: \(U = \frac{\varepsilon_0}{2}\int E^2\,dV\). Parallel-plate capacitance: \(C = \varepsilon_0\varepsilon_r A/d\).

Magnetostatics

Biot–Savart law: \(d\vec{B} = \frac{\mu_0}{4\pi}\frac{I\,d\vec{\ell}\times\hat{r}}{r^2}\). Ampère's law: \(\oint\vec{B}\cdot d\vec{\ell} = \mu_0 I_{\text{enc}}\), \(\nabla\times\vec{B} = \mu_0\vec{J}\). Lorentz force: \(\vec{F} = q(\vec{E} + \vec{v}\times\vec{B})\).

Electromagnetic Induction

Faraday's law: \(\varepsilon = -d\Phi_B/dt\), \(\nabla\times\vec{E} = -\partial\vec{B}/\partial t\). Lenz's law: induced current opposes change. Self-inductance: \(\varepsilon = -L\,dI/dt\), energy \(U = \tfrac{1}{2}LI^2\). Mutual inductance: \(M = \Phi_{21}/I_1\) — basis of transformers.

Series LCR Circuit and Resonance

For a series LCR driven at angular frequency \(\omega\):

\[Z = \sqrt{R^2 + (X_L - X_C)^2}, \qquad \tan\phi = \frac{X_L - X_C}{R}.\]
Principle At resonance \(\omega_0 = 1/\sqrt{LC}\), \(X_L = X_C\) and impedance is purely resistive (\(Z = R\)); current is maximum and in phase with the source.

Quality factor and bandwidth: \(Q = \omega_0 L/R = (1/R)\sqrt{L/C}\), \(\Delta\omega = \omega_0/Q\). Engineering uses: radio/TV tuning, band-pass filters, power-factor correction, MRI coils, wireless charging.

Likely University Questions
  1. State and prove Gauss's law in electrostatics.
  2. Derive the magnetic field of a long straight current using Ampère's law.
  3. Define self- and mutual-inductance with examples.
  4. Express electric and magnetic energy density in terms of the fields.

17. Maxwell's Equations and EM Waves

Displacement Current

Ampère's law fails for a charging capacitor. Maxwell introduced the displacement current density \(\vec{J}_d = \varepsilon_0\,\partial\vec{E}/\partial t\), modifying Ampère's law to

\[\nabla\times\vec{B} = \mu_0\!\left(\vec{J} + \varepsilon_0\frac{\partial\vec{E}}{\partial t}\right).\]

Maxwell's Equations in Vacuum

\[\nabla\cdot\vec{E} = \rho/\varepsilon_0, \qquad \nabla\cdot\vec{B} = 0,\] \[\nabla\times\vec{E} = -\frac{\partial\vec{B}}{\partial t}, \qquad \nabla\times\vec{B} = \mu_0\vec{J} + \mu_0\varepsilon_0\frac{\partial\vec{E}}{\partial t}.\]

EM Wave Equation

In free space (\(\rho = 0\), \(\vec{J} = 0\)), taking the curl of Faraday's law:

\[\nabla^2\vec{E} = \mu_0\varepsilon_0\frac{\partial^2\vec{E}}{\partial t^2}, \qquad c = \frac{1}{\sqrt{\mu_0\varepsilon_0}} \approx 3 \times 10^8\ \text{m s}^{-1}.\]

The same equation holds for \(\vec{B}\). EM waves are transverse (\(\vec{E} \perp \vec{B} \perp \hat{k}\)), in phase, with \(E = cB\).

Energy and Poynting Vector

Energy density: \(u = \varepsilon_0 E^2\). Poynting vector: \(\vec{S} = (1/\mu_0)\vec{E}\times\vec{B}\). Time-averaged intensity: \(\langle S\rangle = \frac{1}{2}c\varepsilon_0 E_0^2\).

Electromagnetic Spectrum

BandWavelengthEngineering Use
Radio>1 mBroadcasting, mobile communication
Microwave1 mm – 1 mRadar, microwave heating
Infrared700 nm – 1 mmRemote sensing, thermal imaging
Visible400 – 700 nmVision, photonics
Ultraviolet10 – 400 nmSterilization, lithography
X-ray0.01 – 10 nmMedical imaging, crystallography
Gamma<0.01 nmNuclear medicine
Likely University Questions
  1. State Maxwell's equations and explain the physical meaning of each.
  2. Derive the EM wave equation in vacuum from Maxwell's equations.
  3. Define the Poynting vector and derive average intensity of a plane wave.
  4. Discuss the EM spectrum and engineering applications of any three bands.

18. Special Theory of Relativity

Postulates

  1. The laws of physics are identical in every inertial frame.
  2. The speed of light in vacuum, \(c\), is the same in all inertial frames, independent of source motion.

Lorentz Transformations

For frame \(S'\) moving at velocity \(v\) along \(x\):

\[x' = \gamma(x - vt), \qquad t' = \gamma\!\left(t - \frac{vx}{c^2}\right), \qquad \gamma = \frac{1}{\sqrt{1 - v^2/c^2}}.\]

Maxwell's equations are invariant under Lorentz transformations (unlike Galilean ones).

Time Dilation and Length Contraction

Moving clocks run slow: \(\Delta t = \gamma\,\Delta t_0\). Moving lengths contract: \(L = L_0/\gamma\). Example: muons at \(0.99c\) (\(\gamma \approx 7.09\)) survive to reach detectors on Earth — confirming time dilation.

Relativistic Velocity Addition

\[u = \frac{u' + v}{1 + u'v/c^2}.\]

Two photons approaching each other still give a relative speed \(c\), never \(2c\).

Relativistic Energy and Momentum

\[m = \gamma m_0, \qquad E = \gamma m_0 c^2 = m_0 c^2 + K, \qquad E^2 = (pc)^2 + (m_0 c^2)^2.\]

Rest energy \(E_0 = m_0 c^2\). Kinetic energy \(K = (\gamma - 1)m_0 c^2\).

Worked Example Kinetic energy of a proton at \(0.8c\) (\(m_0c^2 = 938\) MeV): \[\gamma = 1/\sqrt{1 - 0.64} = 1.667, \qquad K = (\gamma - 1)m_0c^2 = 0.667 \times 938 \approx 626\ \text{MeV}.\] Total energy \(\approx 1564\) MeV.
Engineering Applications Particle accelerators (synchrotrons), GPS satellite clock corrections, nuclear power and weapons (binding energy), mass spectrometry, and high-energy astrophysics detectors.
Likely University Questions
  1. State the postulates of SR and derive the Lorentz transformations.
  2. Derive expressions for time dilation and length contraction.
  3. Derive \(E = mc^2\) and discuss its physical meaning.
  4. Discuss three experimental verifications of SR.

19. Crystal Structure and X-Ray Diffraction

Crystalline vs Amorphous Solids

Crystalline solids have long-range periodic order, a sharp melting point, and are anisotropic (e.g., NaCl, metals). Amorphous solids have short-range order only, soften gradually, and are isotropic (e.g., glass, polymers). Most metals and ceramics are polycrystalline.

Definition A lattice is an infinite set of points generated by integer linear combinations of three primitive translation vectors. A basis is an atom or molecule placed at each lattice site. Crystal = Lattice + Basis. A unit cell is the smallest repeating portion.

Fourteen Bravais Lattices and Seven Crystal Systems

SystemRelationsBravais lattices
Cubic\(a=b=c\), \(\alpha=\beta=\gamma=90°\)P, I, F
Tetragonal\(a=b\ne c\)P, I
Orthorhombic\(a\ne b\ne c\)P, I, F, C
Hexagonal\(a=b\ne c\), \(\gamma=120°\)P
Rhombohedral\(a=b=c\), \(\alpha=\beta=\gamma\)P
Monoclinic\(a\ne b\ne c\), \(\beta\ne 90°\)P, C
TriclinicAll distinctP

Common Cubic Structures

PropertySCBCCFCCDiamond
Atoms/cell1248
Coordination number68124
Packing fraction0.520.680.740.34
ExamplesPoFe, CrCu, Al, NiC, Si, Ge

Miller Indices

To find the \((hkl)\) indices: (1) find intercepts on axes in units of lattice constants, (2) take reciprocals, (3) reduce to smallest integers. Interplanar spacing in cubic: \(d_{hkl} = a/\sqrt{h^2 + k^2 + l^2}\).

Bragg's Law of X-Ray Diffraction

Law \[2d_{hkl}\sin\theta = n\lambda.\] X-ray wavelengths (~1 Å) are comparable to interatomic spacings, so crystals act as three-dimensional diffraction gratings.
Worked Example Cu Kα X-rays (\(\lambda = 1.54\) Å) diffract from (100) planes of NaCl (\(a = 5.64\) Å): \[d_{100} = 5.64\ \text{Å}, \qquad \sin\theta = \frac{1.54}{2 \times 5.64} = 0.1365, \qquad \theta \approx 7.85°.\]

XRD Methods

Laue method (white X-rays, single crystal, spot pattern — orientation determination). Powder (Debye-Scherrer) method (monochromatic X-rays, powder sample, rings — phase identification, lattice constant). Rotating-crystal method (3-D structure information).

Crystal Defects

Point defects (vacancies, interstitials — Schottky, Frenkel), line defects (edge and screw dislocations → plastic deformation), planar defects (grain boundaries, stacking faults), and volume defects (voids, precipitates). Defects often govern mechanical, electrical, and optical properties of real materials.

Likely University Questions
  1. Define lattice, basis, and unit cell. State the seven crystal systems.
  2. Derive the packing fraction of BCC and FCC structures.
  3. Define Miller indices and derive \(d_{hkl}\) for cubic crystals.
  4. State and derive Bragg's law; describe the Debye-Scherrer method.
  5. Classify and describe common defects in solids.

20. Acoustics and Ultrasonics

Sound and Frequency Ranges

Audible: 20 Hz – 20 kHz. Infrasonic: <20 Hz (earthquakes, large animals). Ultrasonic: >20 kHz (medical, NDT). Speed of sound: \(v = \sqrt{B/\rho}\) (fluids), \(v = \sqrt{E/\rho}\) (solids, longitudinal).

Architectural Acoustics

Reverberation time \(T_{60}\) is the time for the sound level to drop 60 dB. Sabine's formula:

\[T_{60} = \frac{0.161\,V}{A}, \qquad A = \sum_i S_i\alpha_i,\] where \(V\) is the room volume (m³) and \(\alpha_i\) is the absorption coefficient of the \(i\)-th surface. Optimum values: concert hall ~1.8 s; lecture hall ~0.6 s.

Common acoustic defects and remedies: echo (use absorbers), excessive reverberation (acoustic panels), focusing from concave surfaces (use diffusers), dead spots (diffusers), outside noise (soundproofing).

Production of Ultrasonic Waves

Magnetostriction oscillator: ferromagnetic rod (Ni) elongates and contracts under alternating magnetic field; works up to ~100 kHz. Piezoelectric oscillator: quartz or PZT crystal in a tank circuit; high frequencies up to MHz, high power.

Engineering Applications Non-destructive testing of welds and castings (pulse-echo), medical imaging (2–20 MHz B-mode and Doppler), SONAR, ultrasonic cleaning and machining (cavitation), therapeutic uses (HIFU, lithotripsy).
Likely University Questions
  1. Define reverberation time. Derive Sabine's formula.
  2. Discuss acoustic defects in halls and their remedies.
  3. Describe piezoelectric and magnetostriction ultrasonic generators.
  4. Discuss four engineering applications of ultrasonics.

21. Dielectrics and Magnetic Materials

Dielectric Materials

Definition A dielectric is an insulator that polarizes in an applied electric field. Key relations: \(\vec{D} = \varepsilon_0\vec{E} + \vec{P} = \varepsilon_0\varepsilon_r\vec{E}\); electric susceptibility \(\chi_e = \varepsilon_r - 1\).

Polarization Mechanisms

  • Electronic: distortion of electron cloud relative to nucleus.
  • Ionic: relative displacement of positive and negative ions.
  • Orientational (dipolar): alignment of permanent dipoles.
  • Space-charge: at interfaces between media of different conductivity (Maxwell–Wagner).

Total: \(\alpha_{\text{tot}} = \alpha_e + \alpha_i + \alpha_o + \alpha_s\). As frequency increases, polarization mechanisms drop out successively.

Clausius–Mossotti relation:

\[\frac{\varepsilon_r - 1}{\varepsilon_r + 2} = \frac{N\alpha}{3\varepsilon_0}.\]

Dielectric loss is quantified by the loss tangent \(\tan\delta = \varepsilon''/\varepsilon'\). Dielectric strength is the maximum field before breakdown.

Magnetic Materials

Type\(\chi_m\)Examples
DiamagneticSmall, <0Cu, Ag, Bi, water
ParamagneticSmall, >0Al, Mn, Pt, O₂
FerromagneticLarge, >0, nonlinearFe, Co, Ni
AntiferromagneticSmall, >0MnO, NiO
FerrimagneticLarge, >0Fe₃O₄, ferrites

\(\vec{B} = \mu_0(\vec{H} + \vec{M})\), \(\vec{M} = \chi_m\vec{H}\), \(\mu_r = 1 + \chi_m\).

Ferromagnetism and Weiss Domains

Below the Curie temperature \(T_C\), exchange interaction aligns spins into magnetic domains. Above \(T_C\), the Curie–Weiss law governs: \(\chi_m = C/(T - T_C)\). The hysteresis loop is characterized by retentivity \(B_r\) (residual flux density) and coercivity \(H_c\) (field needed to demagnetize); its area equals energy lost per cycle per unit volume.

Soft vs Hard Magnetic Materials

SoftHard
Coercivity \(H_c\)LowHigh
Hysteresis areaSmallLarge
ExamplesSi–Fe, ferritesAlnico, NdFeB
UseTransformer cores, inductorsPermanent magnets, motors
Likely University Questions
  1. Discuss types of polarization and their frequency dependence.
  2. Derive the Clausius–Mossotti equation.
  3. Classify magnetic materials with examples.
  4. Explain hysteresis and define \(B_r\) and \(H_c\).
  5. Compare soft and hard magnetic materials; mention applications.

22. Modern Physics — Atom and Hydrogen Spectra

Hydrogen Atomic Spectrum

Empirical Rydberg formula: \(1/\lambda = R(1/n_1^2 - 1/n_2^2)\), \(R = 1.097 \times 10^7\ \text{m}^{-1}\). Spectral series: Lyman (\(n_1 = 1\), UV), Balmer (\(n_1 = 2\), visible), Paschen/Brackett/Pfund (IR).

Bohr Model

Postulates: (1) angular momentum is quantized \(L = n\hbar\); (2) radiation emitted or absorbed when transitioning between orbits \(h\nu = E_i - E_f\). For hydrogen-like atoms:

\[r_n = \frac{n^2 a_0}{Z}, \qquad E_n = -\frac{Z^2}{n^2} \times 13.6\ \text{eV}, \qquad a_0 = 0.529\ \text{Å}.\]
Worked Example Balmer-α line (\(n = 3 \to n = 2\)): \[\frac{1}{\lambda} = R\!\left(\frac{1}{4} - \frac{1}{9}\right) = R\cdot\frac{5}{36}, \qquad \lambda = \frac{36}{5R} \approx 656.3\ \text{nm.}\] This is the red H-α line.

Quantum Numbers and Pauli Exclusion Principle

The quantum-mechanical hydrogen atom is described by \(\psi_{nlm} = R_{nl}(r)Y_l^m(\theta,\phi)\) with: principal \(n = 1, 2, \ldots\); orbital \(\ell = 0, \ldots, n-1\) (s, p, d, f); magnetic \(m = -\ell, \ldots, +\ell\); spin \(s = \pm\tfrac{1}{2}\). The Pauli exclusion principle (no two fermions can share all four quantum numbers) determines the structure of the periodic table. Selection rules: \(\Delta\ell = \pm 1\), \(\Delta m = 0, \pm 1\), \(\Delta s = 0\).

Likely University Questions
  1. Derive expressions for Bohr radius and energy levels.
  2. Calculate the wavelength of the H-α (Balmer-α) line.
  3. State Pauli's exclusion principle and discuss its implications.

23. Nuclear Physics

Nuclear Properties

Nucleus contains \(Z\) protons and \(N\) neutrons (\(A = Z + N\)). Nuclear radius: \(R = R_0 A^{1/3}\), \(R_0 \approx 1.2\ \text{fm}\). Nuclear density is nearly constant, ~\(2.3 \times 10^{17}\ \text{kg m}^{-3}\).

Binding Energy and the Semi-Empirical Mass Formula

Mass defect: \(\Delta m = Zm_p + Nm_n - M_{\text{nucleus}}\). Binding energy: \(B = (\Delta m)c^2\). Binding energy per nucleon \(B/A\) peaks near \(A \approx 56\) (iron). Weizsäcker's formula:

\[B = a_v A - a_s A^{2/3} - a_c\frac{Z(Z-1)}{A^{1/3}} - a_a\frac{(A-2Z)^2}{A} + \delta.\]

Terms: volume, surface, Coulomb, asymmetry, pairing.

Graph of binding energy per nucleon in MeV versus mass number A, showing a peak near iron-56 and decreasing values for both light and heavy nuclei, illustrating why both fission and fusion release energy
Binding energy per nucleon as a function of mass number \(A\). The peak near iron-56 is why fission of heavy nuclei and fusion of light nuclei both release energy.

Radioactive Decay

\[N(t) = N_0 e^{-\lambda t}, \qquad T_{1/2} = \frac{\ln 2}{\lambda}, \qquad \bar{\tau} = \frac{1}{\lambda}.\]

Activity \(A(t) = \lambda N(t)\), measured in becquerels (1 Bq = 1 decay/s). Decay modes: alpha (emission of \({}^4_2\text{He}\)), beta-minus (\(n \to p + e^- + \bar{\nu}_e\)), beta-plus, electron capture, and gamma (nuclear de-excitation).

Nuclear Fission and Fusion

Fission: \(n + {}^{235}\text{U} \to {}^{141}\text{Ba} + {}^{92}\text{Kr} + 3n + 200\ \text{MeV}\). Fusion: \({}^{2}\text{H} + {}^{3}\text{H} \to {}^{4}\text{He} + n + 17.6\ \text{MeV}\). Fusion powers stars and is pursued in ITER and NIF.

Engineering Applications Nuclear power generation (PWR, BWR, CANDU), medical imaging and therapy (PET, radiotherapy), industrial radiography (NDT), radiocarbon dating, tracer studies, and nuclear batteries (RTG for spacecraft).
Likely University Questions
  1. Derive \(R = R_0 A^{1/3}\) and estimate nuclear density.
  2. State the semi-empirical mass formula and explain each term.
  3. Derive the law of radioactive decay; define half-life and mean life.
  4. Distinguish nuclear fission and fusion with energy calculations.

24. Renewable Energy Physics

Solar Photovoltaics

A p–n junction absorbs photons with \(h\nu > E_g\), generating electron–hole pairs separated by the built-in field. The equivalent circuit gives the solar cell I-V equation:

\[I = I_L - I_0\!\left[\exp\!\left(\frac{e(V+IR_s)}{nk_BT}\right)-1\right] - \frac{V+IR_s}{R_{\text{sh}}}.\]

Key parameters: short-circuit current \(I_{sc}\), open-circuit voltage \(V_{oc}\), fill factor \(\text{FF} = V_{mp}I_{mp}/(V_{oc}I_{sc})\), efficiency \(\eta = V_{oc}I_{sc}\cdot\text{FF}/P_{\text{in}}\). The Shockley–Queisser limit for a single junction is ~33%.

TechnologyLab EfficiencyComment
Mono-crystalline Si~26%Most installed globally
Multi-crystalline Si~23%Lower cost
Thin-film (a-Si)13%Flexible substrates
CIGS, CdTe22–23%Cost-effective thin films
GaAs single-junction29.1%High efficiency
Perovskite/Si tandem>33%Emerging technology
Multi-junction III-V>47%Space and concentrators

Wind Energy

Power available in wind crossing area \(A\) at speed \(v\): \(P = \tfrac{1}{2}\rho Av^3\). The Betz limit: only \(C_{P,\max} = 16/27 \approx 59.3\%\) of wind power can be extracted by an ideal turbine. Practical wind turbines achieve \(C_P \sim 0.4\text{–}0.5\).

Hydro, Tidal, and Wave Energy

Hydropower: \(P = \rho g Q H \eta\) (world's largest renewable contribution). Tidal range potential: \(E = \tfrac{1}{2}\rho Agh^2\). Wave energy flux proportional to \(H^2 T\).

Geothermal, Biomass, and Hydrogen

Geothermal uses Earth's internal heat (capacity factor often >90%). Biomass is carbon-neutral if sustainably sourced. Green hydrogen, produced by electrolysis from surplus renewables, is a promising energy carrier for fuel cells.

Energy Storage Technologies

Batteries (Li-ion, flow, Na-ion), pumped hydro (95% of global grid storage), compressed air (CAES), flywheels, supercapacitors, thermal storage (molten salts in CSP), and hydrogen as a chemical carrier. Key engineering challenges: round-trip efficiency, lifecycle, and cost.

Likely University Questions
  1. Derive the V–I equation of a solar cell.
  2. Define and explain fill factor and efficiency of a solar cell.
  3. Derive the Betz limit for a wind turbine.
  4. Discuss any two energy-storage technologies and their physics.

25. Engineering Applications of Physics

Engineering physics bridges fundamental principles and practical hardware across every engineering domain.

MEMS and NEMS

Micro/Nano-Electro-Mechanical Systems are miniaturized machines fabricated by IC-compatible processes, exploiting SHM, beam mechanics, and capacitive/piezoelectric transduction. Applications: accelerometers (airbag deployment, gaming), gyroscopes (drones), pressure sensors, microphones, lab-on-a-chip biosensors, RF MEMS filters and switches.

Display Technologies

  • LCD: birefringence and polarizers, requires backlight.
  • LED/mini-LED: direct emission from semiconductor junctions.
  • OLED: organic semiconductors, self-emissive, flexible.
  • Micro-LED: inorganic LED arrays <50 μm.
  • Quantum-dot LED (QLED): size-tunable color via quantum confinement.

Medical Imaging and Sensing

X-ray CT (absorption tomography), MRI (nuclear spin precession in \(\vec{B}\)), ultrasound (piezoelectric transduction), OCT (low-coherence interferometry), PET (positron annihilation), and hyperspectral imaging.

Communications and Computing

Optical fiber networks (EDFAs, DWDM), 5G mm-wave and MIMO antennas, quantum communication and QKD (BB84), photonic integrated circuits, spintronics (GMR/TMR in hard-disk read heads), and quantum computing (superconducting and trapped-ion qubits).

Likely University Questions
  1. Discuss MEMS technology and applications.
  2. Compare LCD, LED, and OLED display technologies.
  3. Briefly describe the physical principles of MRI.
  4. Explain spintronics and one of its applications.

Appendix A: Fundamental Physical Constants (CODATA)

QuantitySymbolValue (SI)
Speed of light in vacuum\(c\)\(2.998 \times 10^8\ \text{m s}^{-1}\)
Planck constant\(h\)\(6.626 \times 10^{-34}\ \text{J s}\)
Reduced Planck constant\(\hbar\)\(1.055 \times 10^{-34}\ \text{J s}\)
Elementary charge\(e\)\(1.602 \times 10^{-19}\ \text{C}\)
Electron rest mass\(m_e\)\(9.109 \times 10^{-31}\ \text{kg}\)
Proton rest mass\(m_p\)\(1.673 \times 10^{-27}\ \text{kg}\)
Neutron rest mass\(m_n\)\(1.675 \times 10^{-27}\ \text{kg}\)
Boltzmann constant\(k_B\)\(1.381 \times 10^{-23}\ \text{J K}^{-1}\)
Avogadro number\(N_A\)\(6.022 \times 10^{23}\ \text{mol}^{-1}\)
Gas constant\(R\)\(8.314\ \text{J mol}^{-1}\ \text{K}^{-1}\)
Permittivity of free space\(\varepsilon_0\)\(8.854 \times 10^{-12}\ \text{F m}^{-1}\)
Permeability of free space\(\mu_0\)\(1.257 \times 10^{-6}\ \text{H m}^{-1}\)
Gravitational constant\(G\)\(6.674 \times 10^{-11}\ \text{m}^3\ \text{kg}^{-1}\ \text{s}^{-2}\)
Stefan–Boltzmann constant\(\sigma\)\(5.670 \times 10^{-8}\ \text{W m}^{-2}\ \text{K}^{-4}\)
Rydberg constant\(R_\infty\)\(1.097 \times 10^7\ \text{m}^{-1}\)
Bohr radius\(a_0\)\(5.292 \times 10^{-11}\ \text{m}\)
Bohr magneton\(\mu_B\)\(9.274 \times 10^{-24}\ \text{J T}^{-1}\)
Fine-structure constant\(\alpha\)\(1/137.036\)
Atomic mass unit\(u\)\(1.661 \times 10^{-27}\ \text{kg}\)
Compton wavelength\(h/m_e c\)\(2.426 \times 10^{-12}\ \text{m}\)

Useful Conversion Factors

QuantityValue
1 electronvolt\(1.602 \times 10^{-19}\ \text{J}\)
1 calorie (thermochemical)4.184 J
1 u (in energy, \(\times c^2\))931.494 MeV
1 Ångström\(10^{-10}\ \text{m}\)
1 femtometre (fermi)\(10^{-15}\ \text{m}\)
1 barn\(10^{-28}\ \text{m}^2\)
1 atmosphere\(1.013 \times 10^5\ \text{Pa}\)
1 horsepower745.7 W
\(k_BT\) at 300 K25.85 meV
\(\hbar c\)197.3 MeV fm

Appendix B: Formula Cheat Sheet

Mechanics and Oscillations

  • SHM: \(x(t) = A\cos(\omega t + \phi)\), \(\omega = \sqrt{k/m}\)
  • Energy: \(E = \tfrac{1}{2}kA^2 = \tfrac{1}{2}m\omega^2 A^2\)
  • Damped: \(\ddot{x} + 2\gamma\dot{x} + \omega_0^2 x = 0\); quality factor \(Q = \omega_0/2\gamma\)
  • Wave equation: \(\partial^2 y/\partial t^2 = v^2\,\partial^2 y/\partial x^2\)
  • Group / phase velocity: \(v_g = d\omega/dk\), \(v_p = \omega/k\)

Optics

  • YDSE fringe width: \(\beta = \lambda D/d\)
  • Thin film (constructive, reflected): \(2\mu t\cos r = (n + \tfrac{1}{2})\lambda\)
  • Newton's rings (dark, reflected): \(r_n^2 = n\lambda R\)
  • Single-slit minima: \(a\sin\theta = m\lambda\)
  • Grating principal maxima: \((a + b)\sin\theta = m\lambda\)
  • Rayleigh criterion: \(\sin\theta_{\min} = 1.22\lambda/D\)
  • Brewster: \(\tan\theta_p = n_2/n_1\); Malus: \(I = I_0\cos^2\theta\)
  • Fiber NA: \(\text{NA} = \sqrt{n_1^2 - n_2^2} = n_0\sin\theta_a\)
  • V-number: \(V = (2\pi a/\lambda)\,\text{NA}\); single mode if \(V < 2.405\)

Quantum and Atomic

  • de Broglie: \(\lambda = h/p\)
  • Uncertainty: \(\Delta x\,\Delta p \ge \hbar/2\)
  • TISE: \(-(\hbar^2/2m)\nabla^2\psi + V\psi = E\psi\)
  • Particle in 1-D box: \(E_n = n^2\pi^2\hbar^2/(2mL^2)\), \(\psi_n = \sqrt{2/L}\sin(n\pi x/L)\)
  • Hydrogen: \(E_n = -13.6/n^2\ \text{eV}\); \(1/\lambda = R_H(1/n_1^2 - 1/n_2^2)\)
  • Bohr radius: \(a_0 = 4\pi\varepsilon_0\hbar^2/(m_e e^2)\)
  • Compton shift: \(\Delta\lambda = (h/m_e c)(1 - \cos\theta)\)
  • Planck radiation: \(u(\nu, T) = \frac{8\pi h\nu^3}{c^3}\frac{1}{e^{h\nu/k_BT}-1}\)

Solid State, Semiconductors, Superconductivity

  • Bragg: \(2d\sin\theta = n\lambda\); interplanar: \(d = a/\sqrt{h^2+k^2+l^2}\) (cubic)
  • Fermi–Dirac: \(f(E) = 1/[1 + \exp((E - E_F)/k_BT)]\)
  • Intrinsic carriers: \(n_i = \sqrt{N_cN_v}\exp(-E_g/2k_BT)\)
  • Mass action: \(np = n_i^2\)
  • Hall coefficient: \(R_H = 1/(nq)\)
  • Shockley diode: \(I = I_0(e^{qV/k_BT} - 1)\)
  • BCS gap (\(T=0\)): \(2\Delta(0) \approx 3.52\,k_BT_c\)
  • London penetration: \(\lambda_L = \sqrt{m/(\mu_0 n_s e^2)}\)
  • Flux quantum: \(\Phi_0 = h/(2e) = 2.07 \times 10^{-15}\ \text{Wb}\)

Electromagnetism and Relativity

Maxwell's equations (vacuum, differential form):

\[\nabla\cdot\vec{E} = \rho/\varepsilon_0, \quad \nabla\cdot\vec{B} = 0, \quad \nabla\times\vec{E} = -\partial\vec{B}/\partial t, \quad \nabla\times\vec{B} = \mu_0\vec{J} + \mu_0\varepsilon_0\,\partial\vec{E}/\partial t.\]

EM waves: \(c = 1/\sqrt{\mu_0\varepsilon_0}\); intensity \(I = \tfrac{1}{2}\varepsilon_0 c E_0^2\).

Special relativity: \(\gamma = 1/\sqrt{1-v^2/c^2}\); time dilation \(\Delta t = \gamma\,\Delta t_0\); length contraction \(L = L_0/\gamma\); energy-momentum \(E^2 = (pc)^2 + (m_0c^2)^2\); velocity addition \(u = (u'+v)/(1+u'v/c^2)\).

Appendix C: Greek Letters and Mathematical Operators in Physics

SymbolNameTypical useSymbolNameTypical use
\(\alpha\)alphaFine-structure, absorption coeff.\(\nu\)nuFrequency
\(\beta\)beta\(v/c\), transistor current gain\(\xi, \Xi\)xiDamping ratio, position
\(\gamma, \Gamma\)gammaLorentz factor, photon\(\pi, \Pi\)pi3.14159…, products
\(\delta, \Delta\)deltaChange/increment, skin depth\(\rho\)rhoDensity, resistivity, charge density
\(\varepsilon\)epsilonPermittivity, strain\(\sigma, \Sigma\)sigmaConductivity, cross-section
\(\zeta\)zetaDamping ratio\(\tau\)tauTime constant, torque
\(\eta\)etaEfficiency, viscosity\(\phi, \varphi, \Phi\)phiPhase, magnetic flux, work function
\(\theta, \Theta\)thetaAngle, temperature\(\chi\)chiSusceptibility
\(\kappa\)kappaThermal conductivity, curvature\(\psi, \Psi\)psiWavefunction
\(\lambda, \Lambda\)lambdaWavelength, decay constant\(\omega, \Omega\)omegaAngular frequency, ohm
\(\mu\)muPermeability, mobility, \(10^{-6}\)

Common Mathematical Operators

  • Gradient: \(\nabla f = (\partial_x f, \partial_y f, \partial_z f)\)
  • Divergence: \(\nabla\cdot\vec{A} = \partial_x A_x + \partial_y A_y + \partial_z A_z\)
  • Curl: \(\nabla\times\vec{A}\)
  • Laplacian: \(\nabla^2 f = \nabla\cdot\nabla f\)
  • D'Alembertian: \(\Box = \nabla^2 - (1/c^2)\partial_t^2\)
  • Commutator: \([\hat{A}, \hat{B}] = \hat{A}\hat{B} - \hat{B}\hat{A}\)
  • Expectation value: \(\langle\hat{O}\rangle = \int\psi^*\hat{O}\psi\,d\tau\)
  • Inner product: \(\langle\phi|\psi\rangle = \int\phi^*\psi\,d\tau\)
  • Dirac delta: \(\int\delta(x-a)f(x)\,dx = f(a)\)

References and Bibliography

  1. D. Halliday, R. Resnick, J. Walker, Fundamentals of Physics, 10th ed., Wiley, 2014.
  2. A. Beiser, Concepts of Modern Physics, 6th ed., McGraw-Hill, 2003.
  3. D. J. Griffiths, Introduction to Electrodynamics, 4th ed., Pearson, 2013.
  4. D. J. Griffiths, Introduction to Quantum Mechanics, 3rd ed., Cambridge, 2018.
  5. A. Ghatak, Optics, 6th ed., McGraw-Hill, 2017.
  6. C. Kittel, Introduction to Solid State Physics, 8th ed., Wiley, 2005.
  7. N. W. Ashcroft, N. D. Mermin, Solid State Physics, Cengage, 1976.
  8. S. O. Pillai, Solid State Physics, 8th ed., New Age International, 2018.
  9. B. K. Pandey, S. Chaturvedi, Engineering Physics, Cengage, 2012.
  10. H. K. Malik, A. K. Singh, Engineering Physics, McGraw-Hill, 2010.
  11. P. A. Tipler, R. Llewellyn, Modern Physics, 6th ed., W. H. Freeman, 2012.
  12. S. M. Sze, K. K. Ng, Physics of Semiconductor Devices, 3rd ed., Wiley, 2007.
  13. B. G. Streetman, S. K. Banerjee, Solid State Electronic Devices, 7th ed., Pearson, 2016.
  14. K. S. Krane, Introductory Nuclear Physics, Wiley, 1987.
  15. M. Tinkham, Introduction to Superconductivity, 2nd ed., Dover, 2004.
  16. C. P. Poole et al., Introduction to Nanotechnology, Wiley, 2003.
  17. J. D. Jackson, Classical Electrodynamics, 3rd ed., Wiley, 1998.
  18. A. P. French, Vibrations and Waves, Nelson Thornes, 1971.
  19. B. D. Cullity, Elements of X-Ray Diffraction, 3rd ed., Prentice Hall, 2001.
  20. B. E. A. Saleh, M. C. Teich, Fundamentals of Photonics, 2nd ed., Wiley, 2007.