Question:

A conducting square loop initially lies in the $ XZ $ plane with its lower edge hinged along the $ X $-axis. Only in the region $ y \geq 0 $, there is a time dependent magnetic field pointing along the $ Z $-direction, $ \vec{B}(t) = B_0 (\cos \omega t) \hat{k} $, where $ B_0 $ is a constant. The magnetic field is zero everywhere else. At time $ t = 0 $, the loop starts rotating with constant angular speed $ \omega $ about the $ X $ axis in the clockwise direction as viewed from the $ +X $ axis (as shown in the figure). Ignoring self-inductance of the loop and gravity, which of the following plots correctly represents the induced e.m.f. ($ V $) in the loop as a function of time:

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For rotating loops in spatially varying magnetic fields, induced emf shows sinusoidal variation interrupted when the loop moves out of the field region.
Updated On: May 19, 2025
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The Correct Option is A

Solution and Explanation

To solve this problem, we need to determine the induced electromotive force (e.m.f., \(V\)) in a square loop rotating in a time-varying magnetic field. Let’s break it down step by step. 
Step 1: Understand the Setup

  • The square loop lies in the \(XZ\)-plane at \(t = 0\), with its lower edge hinged along the \(X\)-axis.
  • The loop rotates with a constant angular speed \(\omega\) about the \(X\)-axis in the clockwise direction (as viewed from the positive \(X\)-axis). Clockwise rotation from this perspective means the loop rotates from the \(Z\)-axis toward the negative \(Y\)-axis.
  • The magnetic field exists only in the region \(y \geq 0\) and is given by \(\vec{B}(t) = B_0 (\cos \omega t) \hat{k}\), where \(B_0\) is a constant, and \(\hat{k}\) is the unit vector along the \(Z\)-axis. The field is zero for \(y<0\).
  • We need to find the induced e.m.f. \(V\) as a function of time and match it with the given plots.

Step 2: Define the Loop’s Position and Area Vector Assume the square loop has a side length \(a\), so its area is \(A = a^2\). At \(t = 0\), the loop lies in the \(XZ\)-plane, meaning its area vector (normal to the plane) points along the \(Y\)-axis (positive \(Y\)-direction, \(\hat{j}\)). The loop rotates about the \(X\)-axis with angular speed \(\omega\). The angle of rotation \(\theta\) at time \(t\) is: \[ \theta = \omega t \] Since the rotation is clockwise as viewed from the positive \(X\)-axis, the loop’s plane tilts from the \(XZ\)-plane (where the normal is along \(+\hat{j}\)) toward the negative \(Y\)-axis. Let’s define the position:

  • At \(t = 0\), the loop is in the \(XZ\)-plane, and the area vector \(\vec{A} = a^2 \hat{j}\).
  • After time \(t\), the loop has rotated by an angle \(\omega t\). The normal vector (area vector direction) rotates in the \(YZ\)-plane.

The normal vector’s direction after rotation: Initially (at \(\theta = 0\)), the normal is along \(+\hat{j}\). After rotating by \(\theta = \omega t\) clockwise (from \(Z\) to \(-Y\)), we can determine the new normal using the rotation matrix about the \(X\)-axis. For a clockwise rotation by \(\theta\) about the \(X\)-axis:  The initial normal is \((0, 1, 0)\). 

After rotation: 
\[ \begin{pmatrix} 0 \\ \cos (\omega t) \\-\sin (\omega t) \end{pmatrix} \] So, the area vector becomes: \[ \vec{A}(t) = a^2 \left( \cos (\omega t) \hat{j} - \sin (\omega t)\hat{k} \right) \]

Step 3: Calculate the Magnetic Flux The magnetic flux \(\Phi\) through the loop is: \[ \Phi = \vec{B} \cdot \vec{A} \] The magnetic field is \(\vec{B}(t) = B_0 (\cos \omega t) \hat{k}\), and it exists only in the region \(y \geq 0\). This complicates things because part of the loop may be in \(y<0\), where \(\vec{B} = 0\). Let’s first compute the flux assuming the field were uniform across the loop, then adjust for the \(y \geq 0\) condition: \[ \vec{B}(t) \cdot \vec{A}(t) = \left( B_0 \cos \omega t \hat{k} \right) \cdot \left( a^2 \cos (\omega t) \hat{j} - a^2 \sin (\omega t) \hat{k} \right) \] \[ = (B_0 \cos \omega t) \cdot (- a^2 \sin (\omega t)) = - B_0 a^2 \cos (\omega t) \sin (\omega t) \] So, if the field were uniform: \[ \Phi_{\text{uniform}} = - B_0 a^2 \cos (\omega t) \sin (\omega t) \] However, the field is only present for \(y \geq 0\). As the loop rotates, its position in the \(Y\)-coordinate changes:

  • At \(t = 0\), the loop is in the \(XZ\)-plane (\(y = 0\)), so the entire loop is at the boundary of the field region.
  • As \(t\) increases, the loop tilts, and the \(Y\)-coordinate of points on the loop ranges from 0 (at the hinged edge along the \(X\)-axis) to \(y = -a \sin (\omega t)\) at the opposite edge (since it moves toward the negative \(Y\)-axis).

When \(\omega t = 0\), the loop is entirely at \(y = 0\), so it’s in the field region. When \(\omega t = \pi/2\), the loop is in the \(XY\)-plane, with \(y\) ranging from 0 to \(-a\), so half the loop (on average) is in \(y<0\), where \(\vec{B} = 0\).
 
Step 4: Adjust for the Field Region The flux depends on the area of the loop in the region \(y \geq 0\). Let’s parameterize the loop:

  • The loop’s hinged edge is along the \(X\)-axis (from \(x = 0\) to \(x = a\), \(y = 0\), \(z = 0\)).
  • The opposite edge, initially at \(z = a\), rotates. Its \(y\)-coordinate becomes \(y = -a \sin (\omega t)\), and \(z = a \cos (\omega t)\).

As the loop rotates, the \(Y\)-coordinate of a point at height \(z\) (before rotation) becomes: \[ y = -z \sin (\omega t), \quad z = z \cos (\omega t) \] The original \(z\)-coordinate ranges from 0 to \(a\). So, \(y\) ranges from 0 to \(-a \sin (\omega t)\). The condition \(y \geq 0\) means: \[ -z \sin (\omega t) \geq 0 \implies z \leq 0 \quad \text{(if \(\sin (\omega t)>0\))} \] Since \(z \geq 0\), when \(\sin (\omega t)>0\), no part of the loop satisfies \(y \geq 0\) except at the hinge (\(z = 0\)). This suggests we need to compute the effective area in \(y \geq 0\). Instead, let’s reconsider the flux by integrating over the loop’s surface. The fraction of the loop in \(y \geq 0\) decreases as \(\sin (\omega t)\) increases. At \(\omega t = \pi/2\), \(y\) ranges from 0 to \(-a\), so half the loop is in \(y<0\). The effective area in the field region depends on the angle.  
Step 5: Induced e.m.f. The induced e.m.f. is given by Faraday’s Law: \[ V = -\frac{d\Phi}{dt} \] Let’s approximate the flux by considering the effective area. Notice the field and rotation have the same frequency \(\omega\), suggesting resonance effects. Let’s compute \(V\) using the uniform flux and adjust: \[ \Phi_{\text{uniform}} = - B_0 a^2 \cos (\omega t) \sin (\omega t) \] \[ \frac{d\Phi}{dt} = - B_0 a^2 \left[ (-\sin (\omega t)) \sin (\omega t) \omega + \cos (\omega t) (\cos (\omega t)) \omega \right] \] \[ = - B_0 a^2 \omega \left[ -\sin^2 (\omega t) + \cos^2 (\omega t) \right] = - B_0 a^2 \omega (\cos^2 (\omega t) - \sin^2 (\omega t)) \] \[ = - B_0 a^2 \omega \cos (2 \omega t) \] \[ V = -\frac{d\Phi}{dt} = B_0 a^2 \omega \cos (2 \omega t) \] This e.m.f. oscillates with frequency \(2\omega\), which matches the period in the plots (\(\pi/\omega\)). 
Step 6: Account for \(y \geq 0\) Condition When \(\omega t = \pi/2\), the loop is half in \(y<0\), so the flux is halved, but the derivative (e.m.f.) depends on the rate of change. The \(\cos (2 \omega t)\) form arises from the product of \(\cos (\omega t)\) (from the field) and \(\sin (\omega t)\) (from the area vector’s \(Z\)-component), and the \(y \geq 0\) condition modulates the amplitude, not the frequency. 
Step 7: Match with Plots

  • The e.m.f. \(V \propto \cos (2 \omega t)\) has a period of \(\pi/\omega\).
  • Option (A) shows a period of \(\pi/\omega\), matching \(\cos (2 \omega t)\).
  • Option (B) shows a period of \(2\pi/\omega\), incorrect.
  • Option (C) shows a period of \(2\pi/\omega\), incorrect.
  • Option (D) shows a period of \(\pi/\omega\), but the phase differs.

Since \(\cos (2 \omega t)\) starts at a maximum, option (A) matches best. 
Final Answer \[ \boxed{\text{A}} \]

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