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Section 1.1 Paper I

Hint

Must account for error properly.

Answer

(C).

Solution

The figure on the left gives the zero reading.

\begin{equation*} x_0 = -0.1 \text{ (Main) } + 0.06 \text{ (Vernier) } = -0.04 \text{ cm}. \end{equation*}

Reading for the diameter from the figure on the right

\begin{equation*} x = 3.1 \text{ (Main) } + 0.01 \text{ (Vernier) } = 3.11 \text{ cm}. \end{equation*}

Now, we subtract the zero reading to get the actual diamter.

\begin{equation*} D = x - x _0 = 3.15\text{ cm}. \end{equation*}

Hence (C).

Hint

Use \(U=\frac{3}{2}nRT = \frac{3}{2}pV\) for internal energy and first law \(U_2 - U_1 = Q_\text{in} - \int_1^2 pdV\) to find sign of \(Q_\text{in}\) for each step.

Answer

(C).

Solution

From first law of thermodynamics for a gas process from state 1 to state 2, we have

\begin{equation*} U_2 - U_1 = Q_\text{in} - \int_1^2 pdV, \end{equation*}

where minus sign in the work integral takes care of energy loss by the gas in expansion. For internal energy of an (monatomic - not given in the problem) ideal gas we have the following for internal energy in a state \((n, p, V, T)\text{:}\)

\begin{equation*} U = \frac{3}{2}n R T = \frac{3}{2}pV. \end{equation*}

Now, we look at each process with notation for states as shown in Figure 1.1.3. States correspond to \((n,p,V,T)\) at the corners of the diagram are labeled with subscripts 1, 2, 3, 4.

Figure 1.1.3.

Process (1):

\begin{align*} \amp \int_1^2 pdV = p_1(V_2 - V_1). \\ \amp U_2 - U_1 = \frac{3}{2}p_2V_2 - \frac{3}{2}p_1V_1 = \frac{3}{2}p_1(V_2 - V_1) \end{align*}

Therefore,

\begin{equation*} Q_\text{in} = \frac{5}{2}p_1(V_2 - V_1)\ \gt 0. \end{equation*}

So, (1) has heat going into the system.

Process (2):

\begin{align*} \amp \int_1^2 pdV = 0. \\ \amp U_3 - U_2 = \frac{3}{2}\left( p_3 - p_2\right) V_2. \end{align*}

Therefore,

\begin{equation*} Q_\text{in} = \frac{3}{2}\left( p_3 - p_2\right) V_2\ \lt 0. \end{equation*}

So, (2) has heat going out of the system.

Process (3):

\begin{align*} \amp \int_1^2 pdV = p_3(V_4 - V_3) = - p_3(V_3 - V_4). \\ \amp U_2 - U_1 = \frac{3}{2}p_3(V_4 - V_3) = -\frac{3}{2}p_3(V_3 - V_4) \end{align*}

Therefore,

\begin{equation*} Q_\text{in} = -\frac{5}{2}p_3(V_3 - V_4)\ \lt 0. \end{equation*}

So, (3) has heat going out of the system.

Process (4):

\begin{align*} \amp \int_1^2 pdV = 0. \\ \amp U_1 - U_4 = \frac{3}{2}\left(p_1 - p_4\right) V_4. \end{align*}

Therefore,

\begin{equation*} Q_\text{in} = \frac{3}{2}\left(p_1 - p_4\right) V_4\ \gt 0. \end{equation*}

So, (4) has heat going into the system.

Hence, answer is (1) and (4). That would be (C).

Hint

You need to recall lens maker's formula to get focal lengths of the lenses. For power of a lens it is

\begin{equation*} P = \frac{1}{f} = \left( \frac{n_\text{lens} - n_0}{n_0} \right)\left( \frac{1}{R_1} + \frac{1}{R_2} \right). \end{equation*}

Work one lens at a time, using the image from first lens as object for the second lens.

Answer

(B).

Solution

For biconvex lens \(R_1\gt 0\) and \(R_2\lt 0\text{.}\) Therefore,

\begin{equation*} \frac{1}{f_1} = \left( \frac{1.5 - 1.0}{1.0} \right)\left( \frac{1}{20} + \frac{1}{20} \right) = \frac{1}{20}\ \ \ f_1 = 20\text{ cm}. \end{equation*}

For biconcave lens \(R_1\lt 0\) and \(R_2\gt 0\text{.}\) Therefore,

\begin{equation*} \frac{1}{f_2} = \left( \frac{1.5 - 1.0}{1.0} \right)\left( -\frac{1}{20} + \frac{1}{20} \right) = -\frac{1}{20}\ \ \ f_2 = 20\text{ cm}. \end{equation*}

To find the final image, we work one lens at a time. Working with first lens, we find the image \(I_1\) from this lens will be at \(q_1\) give by

\begin{equation*} \frac{1}{q_1} = \frac{1}{f_1} - \frac{1}{p} = \frac{1}{20} - \frac{1}{10} = -\frac{1}{20}. \end{equation*}

That is \(q_1 = -20\text{ cm}\text{.}\) Since it is negative, image is to the left of this lens. The magnification by this lens will be

\begin{equation*} m_1 = -\frac{q_1}{p_1} = -\frac{-20}{10} = 2. \end{equation*}

Now, to work with the second lens, image \(I_1\) serves as object to the second lens. Hence, object distance will be

\begin{equation*} p_2 = \text{separation} - q_1= 10 + 20 = 30\text{ cm}. \end{equation*}

Therefore, final image \(I_2\) will form at \(q_2\) givem by

\begin{equation*} \frac{1}{q_1} = \frac{1}{f_2} - \frac{1}{p_2} = -\frac{1}{20} - \frac{1}{30} = -\frac{3+2}{60} = -\frac{1}{12}. \end{equation*}

Therefore, \(q_2 = -12\text{ cm}\text{,}\) i.e., \(12\text{ cm}\) to the left (since negative) of second lems. Magnification by second lens will be

\begin{equation*} m_2 = - \frac{q_2}{p_2} = - \frac{-12}{30} = +0.4. \end{equation*}

Hence, net magnification is

\begin{equation*} m_1m_2 = 2\times 0.4 = 0.8. \end{equation*}

This is (B). The image has same oriantation as the original object and is \(80\%\) as tall.

Hint

Use nuclear decay law, number \(N\) remaining after time \(t\) is \(N = N_0\,e^{-\lambda t}\text{.}\)

Answer

(D).

Solution

Let \(N(t)\) is the number of undecayed nuclei that ramain in the sample after time \(t\text{.}\) From the nuclear decay law

\begin{equation*} \dfrac{dN}{dt} = - \lambda\, N, \end{equation*}

we immediately get

\begin{equation*} N_\text{remains} = N_0\, e^{-\lambda\, t}. \end{equation*}

We can write \(\lambda\) in terms of half life \(t_\text{1/2}\) by noting the condition for \(t= t_\text{1/2}\text{.}\)

\begin{equation*} \frac{N}{N_0} = \frac{1}{2} = e^{-\lambda\, t_\text{1/2}} \end{equation*}

Hence,

\begin{equation*} \lambda = \frac{\ln2}{ t_\text{1/2} }. \end{equation*}

Thus, we can write the decay law also as (you could start from this formula if you remember it.)

\begin{equation*} N_\text{remains} = N_0\, e^{-(\ln2) t/ t_\text{1/2} }. \end{equation*}

Thus, starting with \(1000\) active nuclei, after one hour we will have remaining (no calculator required!):

\begin{align*} N_\text{remains} \amp = 1000\times e^{ -(\ln2) \times 60\text{ min}/ 20\text{ min} } \\ \amp 1000\, e^{-\ln\, 8} = 1000 \times \frac{1}{8} = 125. \end{align*}

Thus, number of decays are

\begin{equation*} N_\text{decays} = 1000 - 125 = 875. \end{equation*}

Now, \(60\%\) of them are \(\alpha\)-decays. Hence,

\begin{equation*} N_\alpha = 875\times 0.6 = 525. \end{equation*}

This is (D).

Hint

You need to analyze four processes. At the splitting point, implement momentum conservation.

Answer

Q5: \(0.5\text{ sec}\text{,}\) Q6: \(7.5\text{ m}\text{.}\)

Solution

Strategy. Figure 1.1.7 shows the full extent of this problem. We have four processes (1) projectile motion O-to-A, (2) momentum conservation at A, (3) one-dimensional motion A-to-B, and (4) projectile motion A-to-C.

Figure 1.1.7.

(1) Projectile motion O-to-A:

Let us denote the time taken by \(\Delta t = t_0\text{.}\) Since \(\theta=45^\circ\text{,}\) we have

\begin{align*} \amp v_{0x} = 5\sqrt{2}\cos\,45^\circ = 5,\ \ v_{0x} = 5\sqrt{2}\sin\,45^\circ = 5 \\ \amp d_1 = v_{0x} t_0 = 5 t_0 \\ \amp 0 = v_{0y} - g t_0\ \ \longrightarrow\ \ 0 = 5 - 10 t_0 \\ \amp h = v_{0y} t_0 - \frac{1}{2}g t_0^2 = 5 t_0 - 5 t_0^2 \end{align*}

From these, we get

\begin{equation*} t_0 = \frac{1}{2},\ \ h = 5 \left( \frac{1}{2} - \frac{1}{4} \right) = \frac{5}{4}, \end{equation*}

and

\begin{equation} d_1 = \frac{5}{2}\text{ m}.\label{eq-pap1-q5-and-q6-d1}\tag{1.1.1} \end{equation}

(2) Momentum conservation at A:

We implement momentum conservation at A for horizontal and vertical components as shown in Figure 1.1.8.

Figure 1.1.8.
\begin{align*} \amp 2m\times v_{0x} = m v_{2x} \\ \amp 2m\times 0 = m v_{2y} - m v_1 \end{align*}

Upon using numerical values, we get

\begin{equation} v_{2x} = 10,\ \ v_{2y} = v_1\label{eq-pap1-q5-and-q6-v2x-v2y}\tag{1.1.2} \end{equation}

We will get value of \(v_1\) from analysis of A-to-B motion, which we do next.

(3) One-dimensional motion A-to-B:

Here, initial velocity has magnitude \(v_1\) and direction down and acceleration is \(g\) pointed down. It covers a distance \(h=\frac{5}{4}\text{ m}\) found from O-to-A motion in time \(t_1=\frac{1}{2}\text{ sec}\text{.}\) Therefore,

\begin{equation*} h = v_1 t_1 + \frac{1}{2}g t_1^2. \end{equation*}

Therefore,

\begin{equation*} \frac{5}{4} = \frac{v_1}{2} + \frac{1}{2}\times 10 \times \frac{1}{4}. \end{equation*}

Hence, \(v_1=0\text{.}\) Using this in second equation in (1.1.2) give

\begin{equation*} v_{2y}=0. \end{equation*}

(4) Projectile motion A-to-C:

Here, we have \(v_{2x}=10\text{,}\) \(v_{2y}=0\text{,}\) \(h=5/4\text{.}\) The time of flight is given by symbol \(t\) in the problem. Therefore,

\begin{align*} \amp d_2 = v_{2x} t = 10 t \\ \amp -h = v_{2y} t - \frac{1}{2}gt^2\ \ \longrightarrow\ \ -\frac{5}{4} = -5 t^2 \end{align*}

Therefore, answer to Q5 is

\begin{equation} t = 0.5\text{ sec}.\tag{1.1.3} \end{equation}

The horizontal distance from the point of split will be

\begin{equation} d_2 = 10\times 0.5 = 5.\label{eq-pap1-q5-and-q6-d2}\tag{1.1.4} \end{equation}

Finally, from \(d_1\) and \(d_2\) computed above, we have distance from O to be

\begin{equation*} d_1 + d_2 = \frac{5}{2} + 5 = 7.5\text{ m}. \end{equation*}
Hint

Answer

Q8: \(\frac{4}{3}\,\mu\text{C}\text{,}\) Q9: \(\frac{2}{3}\,\mu\text{C}\text{.}\)

Solution 1 Q8

Since capacitor would be fully charged, there will be no current in the branch that has capacitor. Therefore, same current \(I\) will flow in the a-d-b-c-a circuit.

Starting at point b, where we will choose the ground, hence \(V_b=0\text{,}\) and going counterclockwise, Kirchhoff's loop rule gives

\begin{equation*} 2 - 2 I - I - 1 = 0. \end{equation*}
Figure 1.1.10.

Therefore \(I = \frac{1}{3}\text{.}\) By using \(I\text{,}\) we can get voltage at point a.

\begin{equation*} V_c - V_a = 2\times I = \frac{2}{3}. \end{equation*}

Since \(V_c = 2\text{ V}\text{,}\) we get \(V_a = 4/3\text{ V}\text{.}\) Since \(V_b=0\text{,}\) the voltage across capacitor is

\begin{equation*} \Delta V = V_a - V_b = 4/3\text{ V}. \end{equation*}

Now, using the capacitor formula, \(q = C\Delta V\text{,}\) we get

\begin{equation*} q_1 = 1\,\mu\text{F}\times \frac{4}{3}\text{ V} = \frac{4}{3}\,\mu\text{C} = 1.33\,\mu\text{C}. \end{equation*}
Solution 2 Q9

Again capacitor is fully charged, therefore, there will be no current in the branch that has capacitor. But now, the battery on the left is outside the circuit in which current flows as shown in Figure 1.1.11

Now, from the circuit b-c-a-Q-b, we get

\begin{equation*} 2 - 2I-I = 0. \end{equation*}

Hence \(I = 2/3\text{ A}\text{.}\)

Figure 1.1.11.

Therefore,

\begin{equation*} V_c-V_a = \frac{4}{3}\ \ \longrightarrow\ \ V_a = \frac{2}{3}\text{ V}. \end{equation*}

Since \(V_b=0\text{,}\) the voltage across capacitor is

\begin{equation*} \Delta V = V_a - V_b = 2/3\text{ V}. \end{equation*}

Now, using the capacitor formula, \(q = C\Delta V\text{,}\) we get

\begin{equation*} q_2 = 1\,\mu\text{F}\times \frac{2}{3}\text{ V} = \frac{2}{3}\,\mu\text{C} = 0.67\,\mu\text{C}. \end{equation*}
Hint

Demand potential at points corresponding to the circle be zero.

Answer

Q9: \(R=\sqrt{3}\text{,}\) Q10: \(b=3\text{.}\)

Solution

Strategy: I will write potential for general point in \(xy\)-plane and then demand that it be zero at all points of a sphere of radius \(R\) centered about \((b,0)\text{.}\) This should give necessary conditions. For this, we use Figure 1.1.13.

Figure 1.1.13.

Potential at an arbitray point \(P(x,y)\) by two charges \(-Q\) and Q/\sqrt{3} will be

\begin{equation*} V(x,y) = \frac{1}{4\pi\epsilon_0} \frac{-Q}{\sqrt{x^2 + y^2}} + \frac{1}{4\pi\epsilon_0} \frac{Q/\sqrt{3}}{\sqrt{(x-2)^2 + y^2}}. \end{equation*}

When \((x,y)\) is on sphere \((x-b)^2 + y^2 = R^2\text{,}\) potential would be zero. That is,

\begin{equation*} V(x,y) = 0\ \ \text{if}\ \ (x-b)^2 + y^2 = R^2,\ \text{i.e.,}\ \ x^2 + y^2 = R^2 - b^2 + 2 bx. \end{equation*}

Hence, we have

\begin{equation*} \frac{1}{\sqrt{ R^2 - b^2 + 2 bx}} = \frac{1/\sqrt{3}}{\sqrt{ R^2 + 4 - b^2 + 2bx - 4x }}. \end{equation*}

Squaring and then cross-multiplying gives us the following condition.

\begin{equation*} (2R^2 + 12 - 2 b^2) + (4 b - 12) x = 0. \end{equation*}

Since this must be true for every \(x\) on the sphere. That means, we must have

\begin{align*} \amp 2R^2 + 12 - 2 b^2 = 0\\ \amp 4 b - 12 = 0 \end{align*}

These can be solved to yield \(b=3\text{,}\) and \(R=\sqrt{3}\text{.}\)

Hint

Answer

(B), (D).

Solution 1 (A)

To check answer (A), we note forces on the rolling cylinder. The rotational equation of motion about point O, which is momentarily at rest is

\begin{equation*} F R = I_\text{abt O}\, \alpha, \end{equation*}

where \(\alpha\) is angular acceleration.

Figure 1.1.15.

Since rolling cylinder is not slippling, the center of mass motion is related to rotation such that acceleration of the CM will be

\begin{equation*} a = R\alpha. \end{equation*}

Hence,

\begin{equation} a = \frac{FR^2}{I_\text{abt O}}.\label{eq-pap1-q11-accl-part-a}\tag{1.1.5} \end{equation}

Since \(I_\text{abt O}\) depends on whether the cylinder is hollow or solid, \(a\) will depend on this aspect of cylinder. Hence, (A) is false.

Solution 2 (B)

Using Figure 1.1.15, we can write equation of motion about the center as

\begin{equation*} F_r R = I_0\alpha, \end{equation*}

where \(I_0 = \frac{1}{2}mR^2\) is moment of inertia about the CM. Assuming maximum rolling friction, we will have \(F_r = \mu N\text{.}\) Since no acceleration of the CM in the vertical direction, we also have \(N-mg=0\text{.}\) Hence, acceleration of CM will be

\begin{equation*} a = R\alpha = \frac{\mu mg R^2 }{ \frac{1}{2}mR^2 }= 2\mu g. \end{equation*}

This says (B) is correct.

Solution 3 (C)

(C) is not correct since only maximum rolling friction will be \(\mu N=\mu m g\text{.}\)

Solution 4 (D)

The moment of inertia of a thin-walled cylinder about its symmetry axis through the CM is

\begin{equation*} I_0 = mR^2. \end{equation*}

Using parallel axis theorem, we get moment of inertia about O, the point touching the ground to be

\begin{equation*} I_\text{abt O} = I_0 + mR^2 = 2 mR^2. \end{equation*}

Therefore, using Eq. (1.1.5), we get acceleration of the CM to be

\begin{equation*} a = \frac{FR^2}{I_\text{abt O}} = \frac{F}{2m}. \end{equation*}

Hence, (D) is correct.

Hint

Make use of \(\sin\theta \gt 1/n_1\) and if \(x\) is real then \(\sin\, x\lt 1\text{.}\)

Answer

(B), (C), (D).

Solution

Main idea: \(x\) is not a real number if \(|\sin(x)| \gt 1\text{.}\) The incident ray in medium \(n_1\) has angle \(\theta\) such that \(\sin\theta \gt 1/n_1\text{,}\) i.e., \(n_1 \sin\theta \gt 1\text{.}\)

Choice (A) has case \(n_1=n_2\text{.}\) That would mean \(\theta_2=\theta\text{.}\) Therefore, we will have

\begin{equation*} n_0\sin\phi = n_1\sin\theta. \end{equation*}

With \(n_0=1\) and \(n_1\sin\theta \gt 1\text{,}\) this will mean \(\sin\phi \gt 1\text{,}\) which is not possible for real \(\phi\text{.}\) Therefore (A) is incorrect.

Figure 1.1.17. \(n_1=n_2\) .

Choice (B) has case \(n_2 \lt n_1\text{.}\) Figure 1.1.18 shows two ways, ray from \(n_1\) can turn back into \(n_1\) wwithout any transmission into air. Another way to answer this question is to just look at the second of these:

\begin{equation*} \sin\theta_2 = \frac{n_1}{n_2}\sin\theta. \end{equation*}

Figure 1.1.18. \(n_2\lt n_1\text{.}\)

Since \(n_2 \lt n_1\text{,}\) there would be some \(\theta\) at which this condition will have \(\sin\theta_2\gt 1\text{,}\) i.e., we wil lget total internal reflection back into \(n_1\text{.}\) Thus, (B) is correct.

Choice (C) has case \(n_1 \lt n_2\text{.}\) Figure 1.1.19 shows a ray diagram for this situation.

\begin{equation*} \sin\theta_2 = \frac{n_1}{n_2}\sin\theta \lt 1. \end{equation*}

This \(\theta_2\) is always possible. Let's look at the \(n_2/n_0\) interface.

Figure 1.1.19. \(n_1\lt n_2\text{.}\)

At \(n_2/n_0\) interface we have

\begin{equation*} \sin\phi = n_2\sin\theta_2 = n_1\sin\theta_1 \gt 1. \end{equation*}

Hence, this \(\phi\) is not possible. Hence, the ray will return back to \(n_1\text{.}\) That is, (C) is correct.

For (D), We have \(\theta_2=\phi\text{,}\) and we get

\begin{equation*} \sin\phi = n_1\sin\theta \gt 1. \end{equation*}

Hence, ray will be reflected back in \(n_1\text{.}\) That is, (D) is correct.

Hint

Use vector forms of mechanical quantities.

Answer

(A), (B), (C).

Solution

In (A), we are looking at a one-dimensional constant acceleration motion from A to B towards positive \(x\)-axis direction. Hence,

\begin{equation*} 2l = \frac{1}{2}at^2. \end{equation*}

Figure 1.1.21. \(\text{.}\)

This gives \(t = \sqrt{4l/a} = 2\text{ sec}\text{.}\) (A) is correct.

For (B), we implement definition of torque as \(\vec r \times \vec F\text{.}\)

\begin{equation*} \vec {\mathcal{T}} = \vec r \times \vec F = (10\hat i - \hat j)\times (0.2\times 10\hat i) = 2\,\hat k. \end{equation*}

Therefore, (B) is correct.

(C) First we find velocity at B.

\begin{equation*} v_x = a_x t = 10\times 2 = 20\text{ m/s}. \end{equation*}

Therefore, angular momentum about O will be

\begin{equation*} \vec L = \vec r \times \vec p = (10\hat i - \hat j) \times (0.2\times 20 \hat i ) = 4\hat k. \end{equation*}

Therefore, (C) is correct.

Torque here is same as we found in (B). That is \(\vec \tau = \vec r \times \vec F = 2\hat k\text{,}\) which means (D) is incorrect.

Hint

Use Rydberg formula.

Answer

(A), (D)

Solution

This question is about Rydberg formula.

\begin{equation*} \frac{1}{\lambda} = Z^2 R_y \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right). \end{equation*}

Here \(n_1=1\) for Lyman series, \(n_1=2\) for Balmer series, and \(n_1=3\) for Paschen series. Shortest wavelength occurs when \(n_2=\infty\text{.}\)

To check (A), we note that longest wavelength for Balmer will occur when \(n_2=3\text{.}\) Therefore, the raito we seek is

\begin{equation*} \frac{\lambda_\text{max}}{ \lambda_\text{min} } = \left( \frac{1}{2^2} \right) \times \left( \frac{1}{2^2} - \frac{1}{3^2} \right)^{-1} = \frac{9}{5}. \end{equation*}

That is, (A) is true.

Paschen series is in general higher wavelengths than Balmer. Therefore, for (B), we need to just check whether min wavelength of Paschen series is smaller than max wavelength of Balmer.

\begin{align*} \amp \frac{1}{\lambda_\text{min,P}} = Z^2 R_y \left( \frac{1}{3^2} - \frac{1}{4^2} \right) = \frac{7}{128}\,Z^2 R_y. \\ \amp \frac{1}{\lambda_\text{max,B}} = Z^2 R_y \frac{1}{2^2} = \frac{1}{4} Z^2 R_y. \end{align*}

Since \(\lambda_\text{min,P} \gt \lambda_\text{max,B}\text{,}\) there is no overlap between the two series. Therefore, (B) is false.

For (C), let's see if we can rewrite formula for Lyman series in the form in the question.

\begin{align*} \lambda_\text{Ly} \amp = \frac{1}{Z^2 R_y} \left( 1 - \frac{1}{n_2^2} \right)^{-1} \\ \amp = \frac{1}{Z^2 R_y} \left( 1 + \frac{1}{n_2^2} - \frac{1}{n_2^4} + \cdots \right) \end{align*}

Therefore, (C) is false.

For (D), we need to just check whether min wavelength of Balmer series is smaller than max wavelength of Lyman.

\begin{align*} \amp \frac{1}{\lambda_\text{min,B}} = Z^2 R_y \left( \frac{1}{2^2} - \frac{1}{3^2} \right) = \frac{5}{9}\,Z^2 R_y. \\ \amp \frac{1}{\lambda_\text{max,L}} = Z^2 R_y \frac{1}{1^2} = Z^2 R_y. \end{align*}

Since \(\lambda_\text{min,B} \gt \lambda_\text{max,L}\text{,}\) there is no overlap between the two series. Therefore, (D) is true.

Hint

Magnetic flux changed in only rectangular part of the loop.

Answer

(A) and (C)

Solution

From Figure 1.1.24 we see that the magnetic field of the steady current \(I\) in the straight wire will pass through the area enclosed by the expanding circuit on the right. Hence, magnetic flux \(\Phi_B\) will change in the loop, which will cause induced current \(I_\text{ind}\text{.}\)

Figure 1.1.24.

Magnetic field at a distance \(r\) from the straight wire carrying steady current \(I\) is

\begin{equation*} B = \frac{\mu_0 I}{2\pi}\,\frac{1}{r}, \end{equation*}

in the direction shown in Figure 1.1.24. Since magnetic flus through the arc part is not changing, we will not compute that.

To calculate magnetic flux through the changing area, we write magnetic flux through a strip at a distance \(r\) as shown in Figure 1.1.25. This will be

\begin{equation*} d\Phi_B = B(r)\, vt dr. \end{equation*}

Figure 1.1.25.

Integrating from \(r=a\) to \(r=b\) we get

\begin{equation*} \Phi_B = \frac{\mu_0 I v t}{2\pi}\,\ln\left( \frac{b}{a} \right). \end{equation*}

Therefore, rate of change of flux will be

\begin{align*} \frac{d\Phi_B}{dt} \amp = \frac{\mu_0 I v}{2\pi}\,\ln\left( \frac{b}{a} \right)\\ \amp = \frac{4\pi \times 10^{-7} \text{ SI-units}}{2\pi} \times 2\text{ A} \times 3\text{ m/s} \times \ln(4)\\ \amp = 1.67\times 10^{-6} \text{ V}. \end{align*}

That means induced EMF will be

\begin{equation*} \mathcal{E} = \left| \frac{d\Phi_B}{dt} \right| = 1.67\times 10^{-6} \text{ V}. \end{equation*}

Now, notice that the loop acts as a charging RC-circuit with resistance \(R\text{,}\) capacitance \(C_0\) and EMF \(\mathcal{E}\text{.}\) Therefore, maximum current in this circuit will occur when all EMF falls around the resistor.

\begin{equation*} I_\text{ind}^\text{max}= \frac{\mathcal{E}}{R} = \frac{1.67\times 10^{-6} \text{ V}}{14\,\Omega} = 1.2\,\mu\text{A}. \end{equation*}

When capacitor is fully charged, all voltage will be falling around the capacitor.

\begin{equation*} q_\text{max} = C_0\mathcal{E} = 5\times 10^{-6}\text{ F}\times 1.67\times 10^{-6} \text{ V} = 8.4\text{ pC}. \end{equation*}

Therefore, (A) and (C) are true and (B) and (D) are false.

Hint

Write \(F=ma\) for an element of fluid at the bottom.

Answer

(A) and (C).

Solution

We examine an elment of water at the base with area of corss-section \(A\) and length \(d\sqrt{2}\text{.}\) Figure 1.1.27 shows forces \(mg\text{,}\) \(N\text{,}\) \((p_2-p_1)A\text{,}\) and \(F\text{.}\) As a result, the element has acceleration \(a\text{.}\)

Figure 1.1.27.

Let \(x\)-axis be pointed down the incline. Then, \(F_{\text{net},x} = ma_a\text{,}\) will be

\begin{equation*} (p_2-p_1)A + mg\sin\,45^\circ = m a. \end{equation*}

Here \(m = \rho A d\sqrt{2}\text{.}\) For \(p_1-p_2\) we get

\begin{equation*} p_1 - p_2 = \rho d\sqrt{2} \frac{g}{\sqrt{2}} - \rho d\sqrt{2} a. \end{equation*}

Therefore, \(\beta\) defined in the problem has

\begin{equation} \beta = \frac{p_1 - p_2}{\rho g d} = 1 - \frac{a}{g}\sqrt{2}.\label{eq-pap1-q16-beta-for-a}\tag{1.1.6} \end{equation}

Now, we check answers given for various values of \(a\text{.}\)

(A) and (B): When we use \(a= g/\sqrt{2}\) in Eq. (1.1.6), then we do get \(\beta-0\text{.}\) Therefore, (A) is true and (B) is false.

(C) and (D): When we use \(a= g/2\) in Eq. (1.1.6), we get

\begin{equation*} \beta = 1 - \frac{1}{\sqrt{2}} = \frac{\sqrt{2} - 1}{\sqrt{2}}. \end{equation*}

That is (C) is true and (D) is false.

Hint

Use energy arguments to find expression for speed and use that in the equation for circular motion.

Answer

\(4\text{.}\)

Solution

For a particle of charge \(q\) and mass \(m\) moving with speed \(v\) in a circular orbit of radius \(R\) in a magentic field \(B\text{,}\) we will have

\begin{equation*} qvB = \frac{mv^2}{R}. \end{equation*}

Therefore,

\begin{equation*} R = \frac{m v}{qB}. \end{equation*}

Now, in out case, speed is attained by accelerating the particle by a potential \(V\text{.}\)

\begin{equation*} qV = \frac{1}{2}mv^2\ \ \longrightarrow\ \ v = \sqrt{ \frac{2qV}{m} }. \end{equation*}

Hence, for the radius of the orbit, we get

\begin{equation*} R = \frac{1}{B} \sqrt{ 2mV/q }. \end{equation*}

Therefore, the ratio of radii of orbits for two charges we will have

\begin{equation*} \frac{R_1}{R_2} = \sqrt{ \frac{q_2 m_1 }{ q_1 m_2 } }. \end{equation*}

Hence,

\begin{gather*} \frac{r_S}{r_\alpha} = \sqrt{ \frac{2 \times 32 }{ 1\times 4} } = 4. \end{gather*}
Hint

Add angular momenta of rod and disk. For disk, angular momentum will be from spin and from motion of CM.

Answer

\(49\text{.}\)

Solution

We just add angular momenta of rod and the disk. Let \(z\)-axis be pointed up in the figure.

For rod, angular momentum will be \(I_\text{abt O}\Omega\) pointed towards positive \(z\)-axis. Since axis is at the end of the rod, we have \(I=ML^2/3\) formula.

\begin{equation*} \vec L_\text{rod, abt O} = \frac{1}{3} M a^2 \Omega\, \hat k. \end{equation*}

Figure 1.1.30.

Now, disk is rotating about an axis through its CM and its CM is also moving. Therefore, we will have

\begin{equation*} \vec L_\text{disk, abt O} = \vec L_\text{abt cm} + M \vec V_\text{cm} \times R_\text{cm}. \end{equation*}

Figure 1.1.31.

From the counterclockwise spinning of the disk we get

\begin{equation*} \vec L_\text{abt cm} = \frac{1}{2}M \left(\frac{a}{4} \right)^2 \times 4\Omega\, \hat k, \end{equation*}

where I have used \(I=\frac{1}{2}MR^2\) formula for the disk with \(R=a/4\text{.}\)

Now, the CM is located at a distance \(3a/4\) from O about which CM is moving in a circle with angular speed \(\Omega\) as shown in Figure 1.1.31. Therefore,

\begin{equation*} V_\text{cm} = \Omega\, \frac{3a}{4}. \end{equation*}

Using right hand rule for cross product we get the direction to be also towards positive \(z\)-axis. Therefore,

\begin{equation*} M \vec V_\text{cm} \times R_\text{cm} = M \Omega\, \left(\frac{3a}{4}\right)^2\, \hat k. \end{equation*}

Adding all angular momenta, we have

\begin{align*} \vec L_\text{net, abt O} \amp = \vec L_\text{rod abt O} + \vec L_\text{disk abt O} \\ \amp = Ma^2\Omega\left( \frac{1}{3} + \frac{1}{8} + \frac{9}{16} \right) \\ \amp = \frac{Ma^2\Omega}{48}\left( 16 + 6 + 27 \right) = \frac{Ma^2\Omega}{48}\times 49. \end{align*}

Hence, answer is \(n=49\text{.}\)

Hint

Equate the rate at which temperature drops to the rate at which energy radiate out.

Answer

\(9\text{.}\)

Solution

We will need two formulas for this problem. (1) One is the formula for power radiated from the object which is taken to be a blackbody at temperature \(T\) to the outer container kept at zero degree Kelvin.

\begin{equation*} P = \sigma \epsilon A T^4, \end{equation*}

where \(A\) is the surface area of the body, \(\epsilon\) its emissivity, and \(\sigma\) is a universal constant - we do not need values of these quantities for this problem since they will cancel out in the end. If hollow container was not at zero degree kelvin, it will also emit radiation, some of which will be absorbed by the body; in that case we would have \(P = \sigma \epsilon A T^4\) \(- \sigma a A T_\text{container}^4\text{,}\) but we do not have this here.

(2) The other formula we need is for the rate of decrease of temperature of the body as a result of loss of energy \(U\) in the form f heat.

\begin{equation*} \frac{dU}{dt} = -mc\frac{dT}{dt}. \end{equation*}

Since, body lose energy only by radiation, we can equate the rate of decrease of energy of the body to the rate of radiation of energy from the body to get the necessary equation for solving this problem.

\begin{equation*} -mc\frac{dT}{dt} = \sigma \epsilon A T^4. \end{equation*}

Therefore,

\begin{equation*} \frac{dT}{dt} = - \alpha T^4,\ \ \alpha = \frac{\sigma \epsilon A }{m c}. \end{equation*}

Solving this differential equation, from \(T=T_0\) at \(t=0\) to \(T=T\) at \(t=t\text{,}\) we get

\begin{equation*} t = \frac{1}{3\alpha}\left( \frac{1}{T^3} - \frac{1}{T_0^3} \right). \end{equation*}

We apply this for \(t=t_1\) and \(t=t_2\) given in the problem statement to get

\begin{align*} \frac{t_2}{t_1} \amp = \frac{ \frac{1}{T_2^3} - \frac{1}{T_0^3} }{ \frac{1}{T_1^3} - \frac{1}{T_0^3} }\\ \amp = \frac{ T_0^3 - T_2^3 }{ T_0^3 - T_1^3 } \,\times\, \frac{ T_1^3 }{ T_2^3 } \end{align*}

Since ratios will kill common factors, I will divide out given values of temperatures by 100 before using them. This gives

\begin{align*} \frac{t_2}{t_1} \amp = \frac{ 2^3 - 0.5^3 }{ 2^3 - 1^3 } \, \frac{ 1^3 }{ 0.5^3 }\\ \amp = \frac{ 8 - (1/8) }{ 8 - 1 } \times 8= \frac{63}{7} = 9. \end{align*}