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CSIR NET Physical Sciences Electromagnetic Theory Flashcards
50 question-and-answer cards covering Electromagnetic Theory as it is examined in CSIR NET Physical Sciences. 24 of them are printed below, taken from across the deck — no signup, no paywall on the preview.
24 sample cards from the Electromagnetic Theory deck
Sampled from the end of the deck, so these are different cards from the ones shown on the syllabus page.
Why is the dominant mode on an ideal two-conductor transmission line a TEM mode?
Because two conductors can support a transverse-electromagnetic mode in which both $\vec{E}$ and $\vec{B}$ are entirely transverse ($E_{z}=B_{z}=0$). TEM modes have no cutoff frequency and propagate at the medium speed $v = 1/\sqrt{LC} = c/\sqrt{\varepsilon_{r}}$.
Why can a hollow (single-conductor) waveguide NOT support a TEM mode?
A TEM mode requires a transverse static-like field with two conductors to terminate field lines; a hollow waveguide has only one conductor. Inside, Laplace's equation with a single equipotential boundary forces $\vec{E}_{\perp}=0$, so only TE and TM modes (with nonzero $E_{z}$ or $H_{z}$) exist.
Distinguish TE, TM, and TEM modes in a waveguide.
TEM: $E_{z}=H_{z}=0$ (both fields transverse). TE (transverse electric): $E_{z}=0$, $H_{z}\neq 0$. TM (transverse magnetic): $H_{z}=0$, $E_{z}\neq 0$. Hollow waveguides support only TE and TM modes.
Give the cutoff frequency formula for the $\text{TE}_{mn}$/$\text{TM}_{mn}$ mode of a rectangular waveguide of dimensions $a\times b$.
$$f_{c,mn} = \frac{c}{2}\sqrt{\left(\frac{m}{a}\right)^{2} + \left(\frac{n}{b}\right)^{2}}.$$ Only frequencies above $f_{c}$ propagate; below cutoff the mode is evanescent.
What is the dominant mode of a rectangular waveguide with $a > b$, and its cutoff frequency?
The dominant (lowest cutoff) mode is $\text{TE}_{10}$, with $$f_{c,10} = \frac{c}{2a}, \qquad \lambda_{c} = 2a.$$ TM modes require $m,n\geq 1$, so the lowest TM mode is $\text{TM}_{11}$, which has a higher cutoff.
Write the guide wavelength and phase velocity inside a waveguide for a mode with cutoff frequency $f_{c}$.
$$\lambda_{g} = \frac{\lambda}{\sqrt{1 - (f_{c}/f)^{2}}}, \qquad v_{p} = \frac{c}{\sqrt{1 - (f_{c}/f)^{2}}} > c.$$ The group velocity is $v_{g} = c\sqrt{1 - (f_{c}/f)^{2}} < c$, and $v_{p}v_{g} = c^{2}$.
What is the dispersion relation for a mode in a hollow waveguide?
$$\left(\frac{\omega}{c}\right)^{2} = k_{z}^{2} + k_{c}^{2}, \quad k_{c} = \frac{\omega_{c}}{c}.$$ Propagation ($k_{z}$ real) requires $\omega > \omega_{c}$; this is formally identical to the plasma/relativistic massive-particle dispersion relation.
Why is the $\text{TE}_{10}$ mode preferred for practical rectangular waveguides?
It has the lowest cutoff frequency (largest usable single-mode bandwidth), a simple field pattern, lowest attenuation in the dominant band, and allows a wide frequency range over which only one mode propagates, avoiding modal dispersion.
What are the fields radiated by a uniformly moving charge (constant velocity)?
A charge in uniform motion produces a 'pancake' field: the radial electric field is compressed toward the transverse plane. $$\vec{E} = \frac{q}{4\pi\varepsilon_{0}}\frac{(1-\beta^{2})}{(1-\beta^{2}\sin^{2}\theta)^{3/2}}\frac{\hat{R}}{R^{2}}.$$ It carries no radiation (no energy loss).
State the Liénard–Wiechert potentials for a point charge.
$$\phi(\vec{r},t) = \frac{1}{4\pi\varepsilon_{0}}\frac{qc}{(Rc - \vec{R}\cdot\vec{v})}, \qquad \vec{A}(\vec{r},t) = \frac{\mu_{0}}{4\pi}\frac{qc\,\vec{v}}{(Rc - \vec{R}\cdot\vec{v})}$$ evaluated at the retarded time; $\vec{R}$ points from the charge to the field point.
State the Larmor formula for the power radiated by a nonrelativistic accelerating charge.
$$P = \frac{\mu_{0}q^{2}a^{2}}{6\pi c} = \frac{q^{2}a^{2}}{6\pi\varepsilon_{0}c^{3}}.$$ Radiated power is proportional to the square of the acceleration $a$ and the square of the charge.
Write the relativistic (Liénard) generalization of the Larmor formula.
$$P = \frac{\mu_{0}q^{2}\gamma^{6}}{6\pi c}\left[a^{2} - \left(\frac{\vec{v}\times\vec{a}}{c}\right)^{2}\right]$$ where $\gamma = (1-\beta^{2})^{-1/2}$. It reduces to the Larmor formula when $v \ll c$.
What is the angular distribution of radiation from a nonrelativistic accelerated charge, and where is it maximum?
$$\frac{dP}{d\Omega} = \frac{\mu_{0}q^{2}a^{2}}{16\pi^{2}c}\sin^{2}\theta,$$ where $\theta$ is measured from the acceleration direction. It is zero along the acceleration axis and maximum perpendicular to it ($\theta = 90^{\circ}$).
Define cyclotron versus synchrotron radiation.
Both arise from charges accelerated in magnetic fields. Cyclotron radiation is emitted by nonrelativistic charges (narrow band at the gyrofrequency, broad dipole pattern). Synchrotron radiation is emitted by relativistic charges, beamed into a narrow forward cone of half-angle $\sim 1/\gamma$ with a broad spectrum.
What is the electric potential of an ideal electric dipole?
$$V(\vec{r}) = \frac{1}{4\pi\varepsilon_{0}}\frac{\vec{p}\cdot\hat{r}}{r^{2}} = \frac{1}{4\pi\varepsilon_{0}}\frac{p\cos\theta}{r^{2}}$$ where $\vec{p} = q\vec{d}$ is the dipole moment. It falls off as $1/r^{2}$, faster than a monopole's $1/r$.
Write the electric field of an ideal electric dipole in spherical coordinates.
$$\vec{E} = \frac{p}{4\pi\varepsilon_{0}r^{3}}\left(2\cos\theta\,\hat{r} + \sin\theta\,\hat{\theta}\right).$$ The field strength falls off as $1/r^{3}$.
Give the torque and potential energy of a dipole $\vec{p}$ in a uniform field $\vec{E}$.
Torque: $\vec{\tau} = \vec{p}\times\vec{E}$. Potential energy: $U = -\vec{p}\cdot\vec{E} = -pE\cos\theta$. The energy is minimized when $\vec{p}$ aligns with $\vec{E}$ ($\theta = 0$). Net force is zero in a uniform field.
What is the total power radiated by an oscillating electric dipole, and its frequency dependence?
$$P = \frac{\mu_{0}p_{0}^{2}\omega^{4}}{12\pi c} = \frac{p_{0}^{2}\omega^{4}}{12\pi\varepsilon_{0}c^{3}}.$$ It scales as $\omega^{4}$ (the $\omega^{4}$ law underlying Rayleigh scattering and the blue sky).
Give the radiation (far-field) electric field and the angular power distribution of an oscillating electric dipole.
Far field: $\vec{E} \propto \dfrac{\sin\theta}{r}\,\omega^{2}p_{0}$. Angular power: $$\frac{dP}{d\Omega} = \frac{\mu_{0}p_{0}^{2}\omega^{4}}{32\pi^{2}c}\sin^{2}\theta,$$ maximum at $\theta = 90^{\circ}$, zero along the dipole axis.
Compare the radiated power and field falloff of electric dipole, magnetic dipole, and electric quadrupole radiation.
Electric dipole radiation dominates (power $\propto \omega^{4}$). Magnetic dipole and electric quadrupole radiation are weaker by a factor $\sim (a/\lambda)^{2}$ or $(v/c)^{2}$; quadrupole power scales as $\omega^{6}$. All radiation far-fields fall off as $1/r$ so that $\langle S\rangle \propto 1/r^{2}$.
What is the retarded time, and why is it required in time-dependent potentials?
$$t_{r} = t - \frac{|\vec{r} - \vec{r}'|}{c}.$$ It is the earlier time at which the source must be evaluated so that its influence, traveling at speed $c$, reaches the field point $\vec{r}$ at time $t$. It enforces causality.
Write the retarded potentials (solutions of the inhomogeneous wave equation in Lorenz gauge).
$$\phi(\vec{r},t) = \frac{1}{4\pi\varepsilon_{0}}\int\frac{\rho(\vec{r}',t_{r})}{|\vec{r}-\vec{r}'|}\,d^{3}r', \quad \vec{A}(\vec{r},t) = \frac{\mu_{0}}{4\pi}\int\frac{\vec{J}(\vec{r}',t_{r})}{|\vec{r}-\vec{r}'|}\,d^{3}r'$$ with $t_{r} = t - |\vec{r}-\vec{r}'|/c$.
What inhomogeneous wave equations do the potentials satisfy in the Lorenz gauge?
$$\Box^{2}\phi = \nabla^{2}\phi - \frac{1}{c^{2}}\frac{\partial^{2}\phi}{\partial t^{2}} = -\frac{\rho}{\varepsilon_{0}},$$ $$\Box^{2}\vec{A} = \nabla^{2}\vec{A} - \frac{1}{c^{2}}\frac{\partial^{2}\vec{A}}{\partial t^{2}} = -\mu_{0}\vec{J}.$$ The retarded potentials are their causal solutions.
Why are the advanced potentials usually discarded in favor of the retarded potentials?
The wave equation admits both retarded (evaluated at $t_{r} = t - R/c$) and advanced (at $t_{a} = t + R/c$) solutions. The advanced solution has the field depending on the future state of the source, violating causality, so it is discarded on physical grounds.
What this deck covers
The Electromagnetic Theory deck follows the CSIR NET Physical Sciences Electromagnetic Theory syllabus — 10 chapters and 8 topics — so questions land on material that is genuinely examinable rather than trivia around it. That works out to roughly 5.0 cards per chapter.
Answers are written to be recallable, not just readable — averaging about 238 characters, which is long enough to carry the reasoning and short enough to say out loud.
A deck like this earns its keep on the second and third pass. Read the syllabus first so you know the shape of the subject, then use the cards to find the specific facts that have not stuck.
Electromagnetic Theory flashcards FAQ
How many Electromagnetic Theory flashcards are in this CSIR NET Physical Sciences deck?
50 cards. This page previews 24 of them, sampled evenly across the deck so you can judge the difficulty before installing anything.
Are these CSIR NET Physical Sciences flashcards free?
Yes. The preview here is free to read with no signup, and the full 50-card deck is free inside the Examius app.
What do the Electromagnetic Theory cards cover?
They follow the CSIR NET Physical Sciences Electromagnetic Theory syllabus — 10 chapters and 8 topics — so the questions track what is actually examinable.
How should I use these flashcards?
Read the syllabus first so you know the shape of the subject, then drill the deck. Examius schedules each card with spaced repetition, so cards you keep missing come back sooner and ones you know drift further apart.