Question.1[(a) (i)].2019-May-Physics_paper_2__TZ2_HL
Topic: Forces
Given: A student strikes a tennis ball that is initially at rest so that it leaves the racquet at a speed of $64 \mathrm{~m} \mathrm{~s}^{-1}$. The ball has a mass of $0.058 \mathrm{~kg}$ and the contact between the ball and the racquet lasts for $25 \mathrm{~ms}$.
Calculate: the average force exerted by the racquet on the ball.
▶️Answer/Explanation
Solution:
To calculate the average force exerted by the racquet on the ball, we can use the impulse-momentum theorem, which relates the impulse applied to an object to the change in its momentum. The impulse is the product of the force and the time during which it acts:
$$
\text{Impulse} = \text{Force} \times \text{Time}
$$
The momentum of the ball before it is struck is zero, since it is at rest. After it is struck, its momentum is:
$$
p = mv = (0.058~\mathrm{kg})(64~\mathrm{m/s}) = 3.712~\mathrm{kg\cdot m/s}
$$
The change in momentum is therefore:
$$
\Delta p = p – 0 = 3.712~\mathrm{kg\cdot m/s}
$$
The time during which the force acts is given as $t=25~\mathrm{ms}=0.025~\mathrm{s}$.
Therefore, the average force exerted by the racquet on the ball is:
$$
\text{Force} = \frac{\text{Impulse}}{\text{Time}} = \frac{\Delta p}{t} = \frac{3.712~\mathrm{kg\cdot m/s}}{0.025~\mathrm{s}} = 148.48~\mathrm{N}
$$
So the average force exerted by the racquet on the ball is $148.48~\mathrm{N}$.
Question.1[(a) (ii)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Calculate: the average power delivered to the ball during the impact.
▶️Answer/Explanation
Solution:
Using the formula for kinetic energy and the definition of power. Plugging in the given values, we get:
$$
E_K = \frac{1}{2}mv^2 = \frac{1}{2}(0.058~\mathrm{kg})(64~\mathrm{m/s})^2 = 118.144~\mathrm{J}
$$
The time during which this energy is transferred is the same as the contact time, which is given as $t=25~\mathrm{ms}=0.025~\mathrm{s}$. Therefore, the average power delivered to the ball during the impact is:
$$
P = \frac{E_K}{t} = \frac{118.144~\mathrm{J}}{0.025~\mathrm{s}} = 4725.76~\mathrm{W} \approx 4.8~\mathrm{kW}
$$
So the average power delivered to the ball during the impact is approximately $4.8~\mathrm{kW}$. This result is consistent with the answer obtained using the impulse-momentum theorem in the previous part of the question.
Question.1[(b) (i)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: The student strikes the tennis ball at point $\mathrm{P}$. The tennis ball is initially directed at an angle of $7.00^{\circ}$ to the horizontal.
Calculate: the time it takes the tennis ball to reach the net.
▶️Answer/Explanation
Solution:
Constant speed motion to the right at $64 \cos 7^{\circ} \mathrm{m} / \mathrm{s} . \mathrm{d}=11.9 \mathrm{~m}$$$
\begin{aligned}
& v=\frac{d}{t}=>t=\frac{d}{v} \\
& t=\frac{11.9}{64 \cos 7^{\circ}} \\
& t=0.187 \mathrm{~s}
\end{aligned}
$$
Question.1[(b) (ii)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Show: that the tennis ball passes over the net.
▶️Answer/Explanation
Solution:
Actually, what is the height when ball passes the net.Lets choose the positive direction upwards: $x=2.80+S$
$\mathrm{T}=0.187 \mathrm{~s}, \mathrm{u}=-64 \sin 7^0=-7.80, \mathrm{a}=-9.81$
Constant acceleration downwards:
$2.1 \mathrm{~s}=u \mathrm{ut}+\frac{1}{2} \mathrm{at}^2$
$S=-7.80 \times 0.187+0.5 \times(-0.981)(0.187)^2$
$\mathrm{S}=-1.63 \mathrm{~m}$
$X=2.80+S$
$X=2.80-1.63$
$X=1.17 \mathrm{~m} \approx 1.2 \mathrm{~m}$ so the height so passes above net $(0.910 \mathrm{~m})$.
Question.1[(b) (iii)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Calculate: the speed of the tennis ball as it strikes the ground.
▶️Answer/Explanation
Solution:
Conservation of energy:
$$
\begin{aligned}
& \triangle K E=\triangle G P E \\
& 1 / 2 m v^2-1 / 2 m u^2=m g H \\
& 1 / 2 m v^2=m g H+1 / 2 \mathrm{mu}^2 \\
& 1 / 2 m v^2=m\left(9.81 \times 2.80+0.5 \times 64^2\right) \\
& 1 / 2 v^2=9.81 \times 2.80+0.5 \times 64^2 \\
& 1 / 2 v^2=2075 \\
& V=\sqrt{2 \times 2075}=64.4 \mathrm{~m} / \mathrm{s}
\end{aligned}
$$
Question.1(c) .2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: The student models the bounce of the tennis ball to predict the angle θ at which the ball leaves a surface of clay and a surface of grass.
The model assumes
- during contact with the surface the ball slides.
- the sliding time is the same for both surfaces.
- the sliding frictional force is greater for clay than grass.
- the normal reaction force is the same for both surfaces.
Discuss: for the student’s model, without calculation, whether θ is greater for a clay surface or for a grass surface.
▶️Answer/Explanation
Solution:
normal force is the same so vertical component of velocity is the same
During contact frictional force will decrease horizontal component but not vertical component.
Horizontal component will be decreased more for grass hence angle $\theta$ greater.
Question.2(a) .2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: A container of volume $3.2 \times 10^{-6} \mathrm{~m}^3$ is filled with helium gas at a pressure of $5.1 \times 10^5 \mathrm{~Pa}$ and temperature $320 \mathrm{~K}$. Assume that this sample of helium gas behaves as an ideal gas. The mass of a helium atom is $6.6 \times 10^{-27} \mathrm{~kg}$.
Calculate: the average speed of the helium atoms in the container.
▶️Answer/Explanation
Solution:
The average speed of the helium atoms in the container can be calculated using the root-mean-square (rms) speed formula for ideal gases:
$$
v_{\text{rms}} = \sqrt{\frac{3kT}{m}}
$$
where $k$ is the Boltzmann constant, $T$ is the temperature in kelvins, $m$ is the mass of one helium atom, and $v_{\text{rms}}$ is the root-mean-square speed of the gas particles.
First, we need to find the number of helium atoms in the container. We can use the ideal gas law:
$$
PV = nRT
$$
where $P$ is the pressure, $V$ is the volume, $n$ is the number of moles of gas, $R$ is the universal gas constant, and $T$ is the temperature in kelvins.
Solving for $n$ gives:
$$
n = \frac{PV}{RT}
$$
Substituting the given values, we get:
$$
n = \frac{(5.1 \times 10^5~\mathrm{Pa})(3.2 \times 10^{-6}~\mathrm{m}^3)}{(8.31~\mathrm{J/(mol~K)})(320~\mathrm{K})} \approx 6.63 \times 10^{-8}~\mathrm{mol}
$$
Next, we can find the number of helium atoms in the container using Avogadro’s number:
$$
N = nN_{\text{A}}
$$
where $N_{\text{A}}$ is Avogadro’s number ($6.02 \times 10^{23}~\mathrm{mol}^{-1}$). Substituting the values, we get:
$$
N = (6.63 \times 10^{-8}~\mathrm{mol})(6.02 \times 10^{23}~\mathrm{mol}^{-1}) \approx 3.99 \times 10^{16}
$$
Finally, we can calculate the rms speed of the helium atoms:
$$
v_{\text{rms}} = \sqrt{\frac{3kT}{m}} = \sqrt{\frac{3(1.38 \times 10^{-23}~\mathrm{J/K})(320~\mathrm{K})}{6.6 \times 10^{-27}~\mathrm{kg}}} \approx 1400~\mathrm{m/s}
$$
Therefore, the average speed of the helium atoms in the container is approximately $1400~\mathrm{m/s}$.
Question.2 (b).2019-May-Physics_paper_2__TZ2_HL
Topic:
Show: that the number of helium atoms in the container is $4 \times 10^{20}$.
▶️Answer/Explanation
Solution:
To calculate the number of helium atoms in the container, we can use the ideal gas law in terms of the number of particles instead of moles:
$$
PV = NkT
$$
where $N$ is the number of particles (in this case, helium atoms) and all other variables have their usual meanings. Rearranging the equation gives:
$$
N = \frac{PV}{kT}
$$
Substituting the given values, we get:
$$
N = \frac{(5.1 \times 10^5~\mathrm{Pa})(3.2 \times 10^{-6}~\mathrm{m}^3)}{(1.38 \times 10^{-23}~\mathrm{J/K})(320~\mathrm{K})} \approx 3.98 \times 10^{20}
$$
Therefore, the number of helium atoms in the container is approximately $4 \times 10^{20}$.
Question.2[(c) (i)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: A helium atom has a volume of $4.9 \times 10^{-31} \mathrm{~m}^3$.
Calculate: the ratio $\frac{\text { volume of helium atoms }}{\text { volume of helium gas }}$.
▶️Answer/Explanation
Solution:
The number of helium atoms in the container was calculated to be $4 \times 10^{20}$ in part (b), so the volume occupied by the helium atoms can be calculated as follows:
$$
V_\text{atoms} = N \times v = (4 \times 10^{20}) \times (4.9 \times 10^{-31}) \approx 2 \times 10^{-10}~\mathrm{m}^3
$$
Therefore, the ratio of the volume of helium atoms to the volume of helium gas is:
$$
\frac{\text{volume of helium atoms}}{\text{volume of helium gas}} = \frac{V_\text{atoms}}{V} \approx \frac{2 \times 10^{-10}}{3.2 \times 10^{-6}} \approx 6.25 \times 10^{-5}
$$
So the correct ratio is approximately $6.25 \times 10^{-5}$.
Question.2[(c) (ii)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Discuss: by reference to the kinetic model of an ideal gas and the answer to (c)(i), whether the assumption that helium behaves as an ideal gas is justified.
▶️Answer/Explanation
Solution:
The kinetic model of an ideal gas assumes that the gas is made up of a large number of particles (atoms or molecules) that are in constant random motion and obey Newton’s laws of motion. The model also assumes that the particles are point masses with no intermolecular forces between them, except for instantaneous elastic collisions. This means that the volume occupied by the particles themselves is negligible compared to the total volume of the gas.
In part (c)(i), we calculated the ratio of the volume of helium atoms to the volume of helium gas to be approximately $6.25 \times 10^{-5}$. This means that the volume occupied by the helium atoms themselves is small compared to the total volume of the gas. Therefore, the assumption that helium behaves as an ideal gas is justified.
However, it is important to note that the ideal gas law is only an approximation and is not strictly valid for real gases at all pressures and temperatures. At high pressures and low temperatures, real gases can deviate significantly from the ideal gas behavior due to intermolecular forces and the finite size of the gas particles. In these cases, more complex equations of state, such as the van der Waals equation, are needed to describe the behavior of the gas accurately.
Question.3(a) .2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: The diagram shows the direction of a sound wave travelling in a metal sheet.
Particle $P$ in the metal sheet performs simple harmonic oscillations. When the displacement of $P$ is $3.2 \mu \mathrm{m}$ the magnitude of its acceleration is $7.9 \mathrm{~m} \mathrm{~s}^{-2}$.
Calculate: the magnitude of the acceleration of $\mathrm{P}$ when its displacement is $2.3 \mu \mathrm{m}$.
▶️Answer/Explanation
Solution:
$a=-\omega^2 x \Rightarrow a \sim x$ and ratio $\left|\frac{\mathrm{a}}{\mathrm{x}}\right|$ is constant $\left(=\omega^2\right)$
$\mathrm{x}_1=3.2 \mu \mathrm{m}, \mathrm{a}_1=7.9 \mathrm{~ms}^{-2}, \mathrm{x}_2=2.3 \mu \mathrm{m}, \mathrm{a}_2-?$
$\frac{\mathrm{a}_ 2}{\mathrm{x}_ 2}=\frac{\mathrm{a} _1}{\mathrm{x}_ 1} \Rightarrow \mathrm{a}_ 2=\mathrm{x}_ 2 \times \frac{\mathrm{a}_ 1}{\mathrm{x} _1} \Rightarrow \mathrm{a}_2=2.3 \times \frac{7.9}{3.2} \Rightarrow\mathrm{a}_ 2=5.7 \mathrm{~ms}^{-2}$
Question.3(b) .2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: The wave is incident at point $\mathrm{Q}$ on the metal-air boundary. The wave makes an angle of $54^{\circ}$ with the normal at Q. The speed of sound in the metal is $6010 \mathrm{~m} \mathrm{~s}^{-1}$ and the speed of sound in air is $340 \mathrm{~ms}^{-1}$.
Calculate: the angle between the normal at $\mathrm{Q}$ and the direction of the wave in air.
▶️Answer/Explanation
Solution:
$\begin{aligned} & \frac{\sin \theta_2}{\sin \theta_1}=\frac{v_2}{v_1} \\ & \sin \theta_2=\sin \theta_1 \times \frac{v_2}{v_1} \\ & \sin \theta_2=\sin 54^{\circ} \times \frac{340}{6010} \\ & \theta_2=\sin ^{-1}\left(\sin 54^{\circ} \times \frac{340}{6010}\right)=2.6^{\circ}\end{aligned}$
Question.3 (c) .2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: The frequency of the sound wave in the metal is 250 Hz.
Calculate: the wavelength of the wave in air.
▶️Answer/Explanation
Solution:
Frequency doesn’t change $\Rightarrow$ air $f=250 \mathrm{~Hz}$
wave equation: $c=f \cdot \lambda, c=340 \mathrm{~ms}^{-1}$
$$
\lambda=\frac{c}{f}=\frac{340}{250}=1.4 \mathrm{~m}
$$
Question.3[(d) (i)].2019-May-Physics_paper_2__TZ2_HL
Topic:
The sound wave in air in (c) enters a pipe that is open at both ends. The diagram shows the displacement, at a particular time $T$, of the standing wave that is set up in the pipe.
A particular air molecule has its equilibrium position at the point labelled M.
On the diagram, at time $T$
draw: an arrow to indicate the acceleration of this molecule.
▶️Answer/Explanation
Solution:
$X$ $-$ to the right $=>$ acceleration to th left: $a=-\omega^2 x$
Question.3[(d) (ii)].2019-May-Physics_paper_2__TZ2_HL
Topic:
label with the letter $\mathrm{C}$ a point in the pipe that is at the centre of a compression.
▶️Answer/Explanation
Solution:
Molecules around red line are approaching each other creating compression.
Question.3[(e) (i)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: Sound of frequency $f=2500 \mathrm{~Hz}$ is emitted from an aircraft that moves with speed $v=280 \mathrm{~m} \mathrm{~s}^{-1}$ away from a stationary observer. The speed of sound in still air is $c=340 \mathrm{~ms}^{-1}$.
Calculate: the frequency heard by the observer.
▶️Answer/Explanation
Solution:
Using the formula for a moving source, we have:
$$f^{\prime}=f\left(\frac{v}{v\pm u_s}\right)$$
where $f$ is the emitted frequency, $u_s$ is the speed of the source relative to the medium (in this case, air), $v$ is the speed of sound in the medium, and $f^{\prime}$ is the frequency heard by the observer. Since the source is moving away from the observer, we use the formula with a “+” sign in the denominator. Plugging in the given values, we have:
$$f^{\prime}=2500\left(\frac{340}{340+280}\right)=1400\text{ Hz}$$
So the frequency heard by the observer is 1400 Hz, rounded to 2 significant figures.
Question.3[(e) (ii)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Calculate: the wavelength measured by the observer.
▶️Answer/Explanation
Solution:
The wavelength $\lambda^\prime$ measured by the observer can be found using the equation:
$$\lambda^\prime = \frac{c}{f^\prime}$$
where $c$ is the speed of sound in still air and $f^\prime$ is the frequency heard by the observer. From part (i), we have $f^\prime = 1400$ Hz, so:
$$\lambda^\prime = \frac{340}{1400} \approx 0.243\text{ m}$$
Therefore, the wavelength of the sound wave measured by the observer is approximately 0.243 m.
Question.4(a) .2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: Three identical light bulbs, $X, Y$ and $Z$, each of resistance $4.0 \Omega$ are connected to a cell of emf $12 \mathrm{~V}$. The cell has negligible internal resistance.
The switch $S$ is initially open.
Calculate: the total power dissipated in the circuit.
▶️Answer/Explanation
Solution:
$\begin{aligned} & P=V I=I^2 \mathrm{R}=\frac{V^2}{R} \\ & \text { We choose } p=\frac{V^2}{R} ; V=12 \mathrm{~V}, \mathrm{R}=\mathrm{R}_{\text {total }}=(\text { in series }\Rightarrow \text { add })=4.0+4.0=8.0 \Omega \\ & \mathrm{P}=\frac{V^2}{R}=\frac{12^2}{8.0}=18 \mathrm{~W}\end{aligned}$
Question.4[(b) (i)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: The switch is now closed.
Discuss, without calculation, why the current in the cell will increase.
▶️Answer/Explanation
Solution:
When the switch is closed, the total resistance of the circuit decreases as the bulbs are connected in parallel. According to Ohm’s Law, when the resistance of a circuit decreases, the current in the circuit increases, as long as the emf of the cell is held constant. Therefore, the current in the cell will increase when the switch is closed.
Question.4 [(b)(ii)] .2019-May-Physics_paper_2__TZ2_HL
Topic:
Calculate: the ratio $\frac{\text { power dissipated in } Y \text { with } S \text { open }}{\text { power dissipated in } Y \text { with } S \text { closed }}$.
▶️Answer/Explanation
Solution:
$P=V I=I^2 R=\frac{V^2}{R}$ We choose $p=\frac{V^2}{R}$ For $Y$ no change in $V$ and $R \Rightarrow$ ratio $=1$
Question.4(c) .2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: The cell is used to charge a parallel-plate capacitor in a vacuum. The fully charged capacitor is then connected to an ideal voltmeter.
The capacitance of the capacitor is $6.0 \mu \mathrm{F}$ and the reading of the voltmeter is $12 \mathrm{~V}$.
Calculate: the energy stored in the capacitor.
▶️Answer/Explanation
Solution:
The energy stored in a capacitor is given by:
$$E=\frac{1}{2}CV^2$$
where $C$ is the capacitance of the capacitor and $V$ is the voltage across the capacitor.
Substituting the given values, we get:
$$E=\frac{1}{2}(6.0 \mu \mathrm{F})(12 \mathrm{~V})^2=4.32 \times 10^{-4} J$$
Therefore, the energy stored in the capacitor is $4.32 \times 10^{-4}\mathrm{J}$.
Question.4[(d) (i)] .2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: When fully charged the space between the plates of the capacitor is filled with a dielectric with double the permittivity of a vacuum.
Calculate: the change in the energy stored in the capacitor.
▶️Answer/Explanation
Solution:
First, when the dielectric is inserted between the plates, the capacitance of the capacitor increases by a factor of 2. However, the charge $Q$ on the capacitor plates remains the same, since charge is conserved.
Therefore, the voltage $V$ across the capacitor decreases by a factor of 2, since $V=Q/C$ and $C$ has doubled.
Capacitance is proportional to
$\varepsilon: C=\varepsilon \frac{A}{d} \Rightarrow$
$C$ increases 2 times : $\mathrm{C}_ 2=2 \times 6.0 \times 10^{-6} \mathrm{~F}=12.0 \times 10^{-6} \mathrm{~F}$
$$
\begin{aligned}
& C=\frac{Q}{V} \Rightarrow V=\frac{Q}{C} \Rightarrow V \text { decreases } 2 \text { times :V}_ 2=12 / 2=6 \mathrm{~V} \\
& E_ 2=\frac{1}{2} C_ 2(\mathrm{~V}_ 2)^2=0.5 \times 12.0 \times 10^{-6} \times 6^2=2.2 \times 10^{-4} \mathrm{~J} \\
& \Delta V=E_ 2-E_ 1=2.2 \times 10^{-4} \mathrm{~J}-4.3 \times 10^{-4} \mathrm{~J}=-2.1 \times 10^{-4} \mathrm{~J}
\end{aligned}
$$
Question.4[(d) (ii)] .2019-May-Physics_paper_2__TZ2_HL
Topic:
Discuss: the reason , in terms of conservation of energy, the cause for the above change.
▶️Answer/Explanation
Solution:
The change in energy stored in the capacitor when the dielectric is inserted is due to the work done by the electric field in polarizing the dielectric material. When a dielectric material is placed between the plates of a capacitor, the electric field in the region between the plates is reduced, since the electric field inside the dielectric is weaker than in the surrounding space. This causes a reduction in the potential difference across the plates, which leads to a decrease in the energy stored in the capacitor.
However, the polarization of the dielectric material results in the formation of bound charges within the dielectric, which produce an opposing electric field that partially cancels the electric field of the charges on the capacitor plates. This results in an increase in the capacitance of the capacitor, since more charge can be stored at the same potential difference across the plates. Therefore, the work done by the electric field in polarizing the dielectric is partially converted into potential energy stored in the bound charges and partially into the energy stored in the capacitor plates. Overall, the total energy stored in the capacitor and dielectric system remains conserved.
Question.5[(a) (i)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: A proton moves along a circular path in a region of a uniform magnetic field. The magnetic field is directed into the plane of the page.
Label with arrows on the diagram the magnetic force F on the proton.
▶️Answer/Explanation
Solution:
To determine the direction of the magnetic force on the proton, we use the right-hand rule again, but this time with the fingers pointing in the direction of the proton’s velocity (tangent to the circular path), and the palm of the hand facing in the direction of the magnetic field (into the page). The thumb will then point in the direction of the magnetic force on the proton, which is towards the center of the circular path.
So, the arrow labeled “F” should point towards the center of the circle.
Question.5[(a) (ii)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: A proton moves along a circular path in a region of a uniform magnetic field. The magnetic field is directed into the plane of the page.
Label with arrows on the diagram velocity vector v of the proton.
▶️Answer/Explanation
Solution:
The velocity vector v of the proton is tangent to the circular path, and its direction is constantly changing as the proton moves along the circle. At any given point on the circle, the direction of the velocity vector is perpendicular to the direction of the radius vector pointing from the center of the circle to the proton’s position.
Therefore, the direction of the velocity vector v of the proton is tangential to the circle, and it points in the direction of motion. To label this on the diagram, we can draw an arrow tangent to the circle at the position of the proton, as shown below:
The arrow labeled “v” indicates the direction of the velocity vector of the proton at that particular point on the circle.
Question.5[(b) (i)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: The speed of the proton is $2.16 \times 10^6 \mathrm{~m} \mathrm{~s}^{-1}$ and the magnetic field strength is $0.042 \mathrm{~T}$. For this proton,
Calculate: in $m$, the radius of the circular path. Give your answer to an appropriate number of significant figures.
▶️Answer/Explanation
Solution:
The magnetic force $F$ on a charged particle moving with velocity $v$ in a magnetic field $B$ is given by the equation:
$$F = qvB\sin\theta$$
where $q$ is the charge of the particle, and $\theta$ is the angle between the velocity vector and the magnetic field vector. In this case, since the magnetic field is directed into the plane of the page, the angle between the velocity vector and the magnetic field vector is 90 degrees, and $\sin\theta = 1$.
The magnetic force provides the centripetal force needed to keep the proton moving in a circular path, so we can set the magnetic force equal to the centripetal force:
$$F = \frac{mv^2}{r}$$
where $m$ is the mass of the proton, and $r$ is the radius of the circular path.
Setting these two expressions for force equal to each other and solving for $r$, we get:
$$\frac{mv^2}{r} = qvB$$
Solving for $r$, we get:
$$r = \frac{mv}{qB}$$
Plugging in the given values for $m$, $v$, $q$, and $B$, we get:
$$r = \frac{(1.67 \times 10^{-27}\mathrm{~kg})(2.16 \times 10^6\mathrm{~m/s})}{(1.60 \times 10^{-19}\mathrm{~C})(0.042\mathrm{~T})} \approx 0.538 \mathrm{~m}$$
Rounding to an appropriate number of significant figures, we get:
$$r \approx \boxed{0.54 \mathrm{~m}}$$
Question.5[(b) (ii)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Calculate: in sec, the time for one full revolution.
▶️Answer/Explanation
Solution:
The time for one full revolution (period) can be found using the formula:
$$T = \frac{2\pi r}{v}$$
where $r$ is the radius of the circular path, and $v$ is the speed of the proton.
Plugging in the given values for $r$ and $v$, we get:
$$T = \frac{2\pi (0.54\mathrm{~m})}{2.16 \times 10^6\mathrm{~m/s}} =1.57 \times 10^{-6} \mathrm{~s}$$
Rounding to an appropriate number of significant figures, we get:
$$T \approx \boxed{1.6 \times 10^{-6} \mathrm{~s}}$$
Question.6(a) .2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: Deuterium, ${ }_1^2 \mathrm{H}$, undergoes fusion according to the following reaction.
$$
{ }_1^2 \mathrm{H}+{ }_1^2 \mathrm{H} \rightarrow{ }_1^3 \mathrm{H}+\mathrm{X}
$$
Identify: particle $X$.
▶️Answer/Explanation
Solution:
If we balance the equation for the fusion reaction of two deuterium nuclei, we get:
$${ }_1^2 \mathrm{H}+{ }_1^2 \mathrm{H} \rightarrow{ }_1^3 \mathrm{H}+{ }_{\mathrm{b}}^{\mathrm{a}} \mathrm{X}$$
where $\mathrm{a}$ and $\mathrm{b}$ are coefficients for the product $\mathrm{X}$. To balance the equation, we need to ensure that the total number of protons and neutrons is the same on both sides of the equation.
Balancing the top values gives:
$2+2=3+\mathrm{a}\Rightarrow \mathrm{a}=1$
Balancing the bottom values gives:
$1+1=1+\mathrm{b}\Rightarrow \mathrm{b}=1$
Thus, the balanced equation is:
$${ }_1^2 \mathrm{H}+{ }_1^2 \mathrm{H} \rightarrow{ }_1^3 \mathrm{H}+{ }_1^1 \mathrm{H}$$
The product $\mathrm{X}$ is a hydrogen nucleus, which is a proton, denoted by ${ }_1^1 \mathrm{H}$.
Question.6[(b) (i)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: The following data are available for binding energies per nucleon.
$$
\begin{aligned}
& { }_1^2 \mathrm{H}=1.12 \mathrm{MeV} \\
& { }_1^3 \mathrm{H}=2.78 \mathrm{MeV}
\end{aligned}
$$
Calculate: in $\mathrm{MeV}$, the energy released.
▶️Answer/Explanation
Solution:
To determine the energy released in the given fusion reaction, we need to calculate the difference in binding energies between the reactants and the products. The binding energy per nucleon is the energy required to separate the nucleus into its individual nucleons, so a larger binding energy per nucleon corresponds to a more stable nucleus.
The binding energies per nucleon for the reactants and the product are given as:
$${ }_1^2 \mathrm{H}=1.12 \mathrm{MeV}$$
$${ }_1^3 \mathrm{H}=2.78 \mathrm{MeV}$$
The total binding energy for two deuterium nuclei is:
$$E_1 = 2 \times 2 \times 1.12 \mathrm{MeV} = 4.48 \mathrm{MeV}$$
The total binding energy for the product tritium and the unspecified particle X is:
$$E_2 = 3 \times 2.78 \mathrm{MeV} = 8.34 \mathrm{MeV}$$
The energy released in the fusion reaction is the difference in binding energies, which is:
$$\Delta E = E_2 – E_1 = 8.34 \mathrm{MeV} – 4.48 \mathrm{MeV} = 3.86 \mathrm{MeV}$$
This means that 3.86 MeV of energy is released during the fusion reaction, and this energy is usually released in the form of kinetic energy of the product particles (tritium and the unspecified particle X) and gamma rays.
Question.6[(b) (ii)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Discuss: why, for the fusion reaction above to take place, the temperature of deuterium must be very high.
▶️Answer/Explanation
Solution:
The fusion reaction of two deuterium nuclei requires a high temperature because the positively charged nuclei must overcome their mutual electrostatic repulsion to get close enough together for the strong nuclear force to bind them together. The repulsion arises from the electromagnetic force between the positively charged protons in the nuclei. The closer the two nuclei are, the stronger the attractive strong nuclear force becomes and the more likely the nuclei are to fuse.
At high temperatures, the deuterium nuclei have a higher kinetic energy, which means they move faster and collide with more force. This higher collision energy can overcome the electrostatic repulsion and bring the nuclei close enough together for the strong nuclear force to bind them. The temperature required to achieve this is typically on the order of millions of degrees Kelvin.
In addition, at high temperatures, the deuterium exists in the form of a plasma, where the electrons are stripped away from the nuclei. This allows the positively charged nuclei to move freely and collide with each other, increasing the chances of fusion. Overall, the high temperature is necessary to provide the kinetic energy required to overcome the electrostatic repulsion between the nuclei and initiate the fusion process.
Question.6[(c) (i)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Particle $\mathrm{Y}$ is produced in the collision of a proton with a $\mathrm{K}^{-}$in the following reaction.
$$
\mathrm{K}^{-}+\mathrm{p}^{+} \rightarrow \mathrm{K}^0+\mathrm{K}^{+}+\mathrm{Y}
$$
The quark content of some of the particles involved are
$$
\mathrm{K}^{-}=\overline{\mathrm{u}} \mathrm{S} \quad \mathrm{K}^0=\mathrm{d} \overline{\mathrm{s}}
$$
Identify: for particle $Y$, the charge.
▶️Answer/Explanation
Solution:
Charge:
In the reaction $\mathrm{K}^{-}+\mathrm{p}^{+} \rightarrow \mathrm{K}^0+\mathrm{K}^{+}+\mathrm{Y}$, the total charge on the left-hand side is $-1+1=0$, while on the right-hand side, it is $0+1+Q_{\mathrm{Y}}$. Hence, the charge of particle $\mathrm{Y}$ is $Q_{\mathrm{Y}}= -1/e$.
Question.6[(c) (ii)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Identify: for particle $Y$, the strangeness.
▶️Answer/Explanation
Solution:
Strangeness:
The strangeness quantum number ($S$) is a conserved quantity in strong interactions. In the reaction, the strangeness on the left-hand side is $S_{\mathrm{LHS}}=-1$, and on the right-hand side, it is $S_{\mathrm{RHS}}=-1+1+S_{\mathrm{Y}}$. Since $S_{\mathrm{LHS}}=S_{\mathrm{RHS}}$, we have $-1=S_{\mathrm{Y}}-2$, which means that the strangeness of particle $\mathrm{Y}$ is $S_{\mathrm{Y}}=-3$.
Question.7 (a) .2019-May-Physics_paper_2__TZ2_HL
Given: The average temperature of ocean surface water is $289 \mathrm{~K}$. Oceans behave as black bodies.
Show: that the intensity radiated by the oceans is about $400 \mathrm{~W} \mathrm{~m}^{-2}$.
▶️Answer/Explanation
Solution:
The intensity of radiation emitted by a blackbody at temperature $T$ can be calculated using the Stefan-Boltzmann law:
$$
I=\sigma T^{4},
$$
where $\sigma=5.67 \times 10^{-8} \mathrm{~W~m^{-2}~K^{-4}}$ is the Stefan-Boltzmann constant.
Substituting the given temperature $T=289 \mathrm{~K}$, we get:
$$
I=\sigma T^{4} = 5.67 \times 10^{-8} \mathrm{~W~m^{-2}~K^{-4}} \times (289 \mathrm{~K})^{4} \approx 396 \mathrm{~W~m^{-2}}
$$
Therefore, the intensity radiated by the oceans is about $400 \mathrm{~W~m^{-2}}$ (rounded to two significant figures).
Question.7 (b) .2019-May-Physics_paper_2__TZ2_HL
Explain: why some of this radiation is returned to the oceans from the atmosphere.
▶️Answer/Explanation
Solution:
The radiation emitted by the oceans is mostly in the form of long-wavelength infrared radiation, which can be absorbed by certain atmospheric gases such as water vapor, carbon dioxide, and methane. These gases are known as greenhouse gases because they trap some of the infrared radiation and prevent it from escaping to space. As a result, some of the radiation emitted by the oceans is absorbed by the atmosphere and re-radiated back towards the surface of the Earth.
This phenomenon is known as the greenhouse effect, and it is important for regulating the Earth’s temperature. Without the greenhouse effect, the Earth’s surface would be much colder than it is today, and life as we know it would not be able to survive. However, human activities have increased the concentration of greenhouse gases in the atmosphere, leading to an enhanced greenhouse effect and global warming.
Question.7[(c) (i)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: The intensity in (b) returned to the oceans is $330 \mathrm{~W} \mathrm{~m}^{-2}$. The intensity of the solar radiation incident on the oceans is $170 \mathrm{~W} \mathrm{~m}^{-2}$.
Calculate: the additional intensity that must be lost by the oceans so that the water temperature remains constant.
▶️Answer/Explanation
Solution:
In order for the water temperature to remain constant, the intensity of radiation emitted by the oceans must equal the sum of the intensity of solar radiation absorbed by the oceans, plus the intensity of radiation absorbed from the atmosphere and re-radiated back towards the surface. Mathematically, we can express this as:
$$ I_{\text{emitted}} = I_{\text{solar}} + I_{\text{atmospheric}} $$
We are given that $I_{\text{emitted}} = 400 \mathrm{~W/m^2}$ and $I_{\text{atmospheric}} = 330 \mathrm{~W/m^2}$, and $I_{\text{solar}} = 170 \mathrm{~W/m^2}$. Substituting these values into the equation, we have:
$$ 400 \mathrm{~W/m^2} = 170 \mathrm{~W/m^2} + 330 \mathrm{~W/m^2} + \Delta I $$
Simplifying, we get:
$$ \Delta I = 400 \mathrm{~W/m^2} – 170 \mathrm{~W/m^2} – 330 \mathrm{~W/m^2} = -100 \mathrm{~W/m^2} $$
Therefore, an additional intensity of $100 \mathrm{~W/m^2}$ must be lost by the oceans so that the water temperature remains constant. This means that the oceans must emit $100 \mathrm{~W/m^2}$ more radiation than they absorb from both the sun and the atmosphere.
Question.7 (c).2019-May-Physics_paper_2__TZ2_HL
Topic:
Suggest: a mechanism by which the additional intensity can be lost.
▶️Answer/Explanation
Solution:
There are several mechanisms by which the additional intensity can be lost from the oceans to the environment, including:
1. Conduction: Heat can be conducted from the warmer ocean surface to the cooler atmosphere and to deeper layers of the ocean.
2. Convection: Warmer surface water can mix with cooler water below, transferring heat to deeper layers of the ocean.
3. Evaporation: Heat is absorbed when water evaporates from the ocean surface, carrying heat away from the surface.
4. Radiation: Oceans can also radiate heat back into space, especially at higher altitudes where the atmosphere is thinner and there is less absorption and re-emission of infrared radiation.
These processes collectively help to maintain the Earth’s energy balance and prevent the oceans from overheating.
Question.8 (a).2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: Monochromatic coherent light is incident on two parallel slits of negligible width a distance $d$ apart. A screen is placed a distance $D$ from the slits. Point $\mathrm{M}$ is directly opposite the midpoint of the slits.
Initially the lower slit is covered and the intensity of light at $\mathrm{M}$ due to the upper slit alone is $22 \mathrm{Wm}^{-2}$. The lower slit is now uncovered.
Deduce:, in $\mathrm{Wm}^{-2}$, the intensity at $\mathrm{M}$.
▶️Answer/Explanation
Solution:
When both slits are open, there will be interference between the waves from each slit, resulting in a pattern of bright and dark fringes on the screen. At the location of $\mathrm{M}$, constructive interference occurs when the path difference between the waves from each slit is equal to an integer number of wavelengths.
Initially, when only the upper slit is open, the intensity at $\mathrm{M}$ is $22 \mathrm{Wm}^{-2}$. When the lower slit is also open, the waves from both slits interfere constructively at $\mathrm{M}$, so the amplitude at $\mathrm{M}$ doubles. Since intensity is proportional to the square of the amplitude, the intensity at $\mathrm{M}$ increases by a factor of $(2)^2=4$. Therefore, the intensity at $\mathrm{M}$ with both slits open is $22 \mathrm{Wm}^{-2} \times 4 = 88 \mathrm{Wm}^{-2}$.
Question.8 (b).2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: $\mathrm{P}$ is the first maximum of intensity on one side of M. The following data are available.
$$
\begin{aligned}
d & =0.12 \mathrm{~mm} \\
D & =1.5 \mathrm{~m} \\
\text { Distance MP } & =7.0 \mathrm{~mm}
\end{aligned}
$$
Calculate:, in $\mathrm{nm}$, the wavelength $\lambda$ of the light.
▶️Answer/Explanation
Solution:
For the first maximum, the path difference between the two waves from the slits is $\Delta x = d\sin\theta$, where $\theta$ is the angle between the incident direction and the direction to the maximum. For small angles $\sin\theta \approx \theta$, and we have $\Delta x \approx d\theta$. The condition for constructive interference at the first maximum is then $\Delta x = m\lambda$, where $m$ is an integer. For the first maximum $m=1$, so we have$$
d\theta = \lambda.
$$
The angle $\theta$ is given by $\tan\theta = \frac{MP}{D}$, so we can write
$$
\lambda = d \tan\theta \approx d\frac{MP}{D}.
$$
Substituting the given values we find
$$
\lambda \approx 0.12 \times 10^{-3} \times \frac{7.0 \times 10^{-3}}{1.5} \approx 560 \mathrm{~nm}.
$$
Question.8[(c) (i)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: The width of each slit is increased to $0.030 \mathrm{~mm} . D, d$ and $\lambda$ remain the same.
Discuss: why, after this change, the intensity at $P$ will be less than that at $M$.
▶️Answer/Explanation
Solution:
After the increase in slit width, the single-slit diffraction pattern will become wider, causing the overlapping central maximums to become less intense. This will result in a decrease in the intensity at $P$, which corresponds to the first maximum on one side of $M$.
Question.8 [(c) (ii)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Show: that, due to single slit diffraction, the intensity at a point on the screen a distance of $28 \mathrm{~mm}$ from $\mathrm{M}$ is zero.
▶️Answer/Explanation
Solution:
$\theta=\frac{\lambda}{b} ; \theta$ – angle between first minimum and central maximum, $\lambda$ – wavelength, $b$ – slit width.
$\mathrm{b}=0.030 \mathrm{~mm}=0.030 \times 10^{-3}=>\theta=\frac{\lambda}{b}=\left(5.6 \times 10^{-7}\right) / 0.030 \times 10^{-3}=0.01867 \mathrm{rad}$
$\tan \theta=\frac{X}{1.5 m} \Rightarrow X=1.5 \mathrm{~m} \times \tan \theta=1.5 \mathrm{~m} \times \tan (0.01867 \mathrm{rad})=28.0 \mathrm{~mm}$ (( change calculator to radians ” mode $”))$
Question.9[(a) (i)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: A planet of mass $m$ is in a circular orbit around a star. The gravitational potential due to the star at the position of the planet is $V$.
Show: that the total energy of the planet is given by the equation shown.
$$
E=\frac{1}{2} m V
$$
▶️Answer/Explanation
Solution:
The potential energy of a planet in a circular orbit around a star is given by:
$$U=-\frac{GMm}{r}$$
where $M$ is the mass of the star, $r$ is the distance between the planet and the star, and $G$ is the gravitational constant. Since the planet is in a circular orbit, its kinetic energy is given by:
$$K=\frac{1}{2}mv^2$$
where $v$ is the speed of the planet.
The total energy of the planet is the sum of its kinetic and potential energies:
$$E=K+U$$
Using the fact that the planet is in a circular orbit, we can relate the speed $v$ to the distance $r$:
$$v=\frac{2\pi r}{T}$$
where $T$ is the period of the planet’s orbit.
Substituting this expression for $v$ into the equation for kinetic energy and using the equation for potential energy, we get:
$$\begin{aligned}
E&=\frac{1}{2}mv^2-\frac{GMm}{r}\\
&=\frac{1}{2}m\left(\frac{2\pi r}{T}\right)^2-\frac{GMm}{r}\\
&=\frac{4\pi^2}{2T^2}mr^2-\frac{GMm}{r}\\
&=\frac{2\pi^2}{T^2}mr^2-\frac{GMm}{r}
\end{aligned}$$
Now, we use the fact that the period of a circular orbit is related to the distance between the planet and the star by:
$$T=\frac{2\pi r}{v}=\frac{2\pi r}{\sqrt{GM/r}}=\frac{2\pi}{\sqrt{GM}}r^{3/2}$$
Substituting this expression for $T$ into the equation for $E$, we get:
$$E=\frac{2\pi^2}{\left(\frac{2\pi}{\sqrt{GM}}r^{3/2}\right)^2}mr^2-\frac{GMm}{r}=\frac{1}{2}m\left(\frac{GM}{r}\right)-\frac{GMm}{r}=\frac{1}{2}mV$$
Therefore, the total energy of the planet is given by $E=\frac{1}{2}mV$.
Question.9[(a) (ii)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: Suppose the star could contract to half its original radius without any loss of mass.
Discuss: the effect, if any, this has on the total energy of the planet.
▶️Answer/Explanation
Solution:
The gravitational potential at the position of the planet depends only on the mass of the star and not on its radius. Therefore, if the star were to contract to half its original radius while keeping the same mass, the gravitational potential at the position of the planet would remain unchanged.
As a result, the total energy of the planet, which is given by $E=\frac{1}{2}mV$, would also remain unchanged, since both $m$ and $V$ would be constant. So the contraction of the star would have no effect on the total energy of the planet.
Question.9(b) .2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: The diagram shows some of the electric field lines for two fixed, charged particles $X$ and $Y$.
The magnitude of the charge on $X$ is $Q$ and that on $Y$ is $q$. The distance between $X$ and $Y$ is $0.600 \mathrm{~m}$. The distance between $P$ and $Y$ is $0.820 \mathrm{~m}$.
At $P$ the electric field is zero.
Calculate: to one significant figure, the ratio $\frac{Q}{q}$.
▶️Answer/Explanation
Solution:
Using Coulomb’s law, the electric field at a distance $r$ from a point charge $Q$ is given by $E=kQ/r^2$, where $k$ is the Coulomb constant. At point $P$, the electric field due to charges $X$ and $Y$ are equal in magnitude but opposite in direction. Thus, we have:
$$
k\frac{Q}{(0.600+0.820)^2}=k\frac{q}{0.820^2}
$$
Simplifying this expression gives:
$$
\frac{Q}{q}=\frac{(0.600+0.820)^2}{0.820^2}=3.00
$$
Therefore, to one significant figure, the ratio $Q/q$ is 3.
Question.10(a).2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: A small magnet is dropped from rest above a stationary horizontal conducting ring. The south (S) pole of the magnet is upwards.
While the magnet is moving towards the ring,
State: why the magnetic flux in the ring is increasing.
▶️Answer/Explanation
Solution:
The magnetic flux through the ring is given by the equation $\Phi=B A \cos \theta$, where $B$ is the magnetic field, $A$ is the area of the ring, and $\theta$ is the angle between the magnetic field and the normal to the ring. As the magnet approaches the ring, the magnetic field through the ring increases, since the magnetic field due to the magnet is increasing in strength as it gets closer to the ring. Therefore, the magnetic flux through the ring is increasing.
Question.10(b).2019-May-Physics_paper_2__TZ2_HL
Topic:
Sketch:, using an arrow on Diagram 2, the direction of the induced current in the ring.
▶️Answer/Explanation
Solution:
the current must be counterclockwise in diagram 2
Question.10(c).2019-May-Physics_paper_2__TZ2_HL
Topic:
Deduce: the direction of the magnetic force on the magnet.
▶️Answer/Explanation
Solution:
The magnetic force on the magnet is given by the equation:
$\vec{F} = q\vec{v} \times \vec{B}$
where $q$ is the charge of the moving particles (in this case, the magnet), $\vec{v}$ is its velocity, and $\vec{B}$ is the magnetic field.
In this case, the magnet is moving towards the ring and the magnetic field is generated by the ring. As the magnet gets closer to the ring, the magnetic flux through the ring increases, as we found in part (a).
The magnetic field generated by the ring is directed perpendicular to the plane of the ring and in a direction that opposes the change in magnetic flux. Therefore, the magnetic field is directed downwards and increasing as the magnet approaches the ring.
The velocity of the magnet is initially downwards, and as it approaches the ring, it is directed towards the center of the ring. Thus, the direction of the velocity vector changes from downwards to towards the center of the ring.
Therefore, the direction of the magnetic force is perpendicular to both the velocity vector and the magnetic field vector and is directed out of the page.
Question.7[(a) (i)].2019-May-Physics_paper_2__TZ1_HL
Topic:
Given: The Moon has no atmosphere and orbits the Earth. The diagram shows the Moon with rays of light from the Sun that are incident at $90^{\circ}$ to the axis of rotation of the Moon. A black body is on the Moon’s surface at point A.
Show: that the maximum temperature that this body can reach is $400 \mathrm{~K}$. Assume that the Earth and the Moon are the same distance from the Sun.
▶️Answer/Explanation
Solution:
$\begin{aligned} & P=e \sigma A T^4, \sigma=5.67 \times 10^{-8} \\ & T=\left(\frac{P}{e \sigma A}\right)^{1 / 4} ; \text { Stefan-Boltzmann constant : } \sigma=5.67 \times 10^{-8}, \\ & \text { equilibrium hence intensity of emission: }(P / A)=S=1.36 \times 10^3 \mathrm{Wm}^{-2} \text { (solar constant); } \\ & T=\left(\frac{1.36 \times 10^3}{5.67 \times 10^{-8}}\right)^{1 / 4} \\ & T=393 \mathrm{~K}=400 \mathrm{~K}\end{aligned}$
Question.11(a) .2019-May-Physics_paper_2__TZ2_HL
Topic:
Discuss: why de Broglie’s hypothesis is not consistent with Bohr’s conclusion that the electron’s orbit in the hydrogen atom has a well defined radius.
▶️Answer/Explanation
Solution:
De Broglie’s hypothesis suggests that particles, including electrons, exhibit wave-like behavior. According to this hypothesis, electrons in the hydrogen atom would have a wavelength associated with them, given by $\lambda = h/p$, where $h$ is Planck’s constant and $p$ is the momentum of the electron. This implies that the electron’s position is not well-defined, but rather spread out over a region of space determined by the wavelength of the electron.
On the other hand, Bohr’s model of the hydrogen atom assumes that the electron orbits the nucleus in a well-defined circular path, with a radius determined by the electron’s energy. This is inconsistent with de Broglie’s hypothesis, as it implies that the electron’s position is well-defined, and not spread out over a region of space determined by the electron’s wavelength. Therefore, de Broglie’s hypothesis is not consistent with Bohr’s conclusion that the electron’s orbit in the hydrogen atom has a well-defined radius.
Question.11[(b) (i)].2019-May-Physics_paper_2__TZ2_HL
Topic:
In an experiment to determine the radius of a carbon-12 nucleus, a beam of neutrons is scattered by a thin film of carbon-12. The graph shows the variation of intensity of the scattered neutrons with scattering angle. The de Broglie wavelength of the neutrons is $1.6 \times 10^{-15} \mathrm{~m}$.
Calculate: using the graph, the radius of a carbon-12 nucleus.
▶️Answer/Explanation
Solution:
$sin \theta=\frac{\lambda}{D} \Rightarrow$ ( First minimum of an electron diffraction pattern around a circular object.$D$ – nuclear diameter, $\lambda$-de Broglie wavelength of the electrons)
$$
\lambda=1.6 \times 10^{-15} \mathrm{~m}, \theta=17^0
$$
Rewriting and substituting values: $D=\frac{\lambda}{\sin \theta}=1.6 \times 10^{-15} \mathrm{~m} / \sin 17^0=5.47 \times 10^{-15} \mathrm{~m}$
Radius $=\mathrm{D} / 2=5.47 \times 10^{-15} \mathrm{~m} / 2=2.74 \times 10^{-15} \mathrm{~m}=2.7 \times 10^{-15} \mathrm{~m}$
Question.11[(b) (ii)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: The ratio $\frac{\text { volume of a nucleus of mass number } A}{\text { volume of a nucleon }}$ is approximately $A$.
Discuss: on this observation by reference to the strong nuclear force.
▶️Answer/Explanation
Solution:
The strong nuclear force is a very short-range force that acts between nucleons (protons and neutrons) in the nucleus. The force is attractive at close range and holds the nucleus together. However, at distances beyond a few femtometers, the force becomes repulsive. This is because the nucleons are so close together that they begin to experience the strong nuclear force from neighboring nucleons. The repulsive force acts to prevent the nucleus from collapsing under the strong attractive force.
As the mass number $A$ of the nucleus increases, the number of nucleons in the nucleus increases. This means that the volume of the nucleus also increases, as more nucleons must be packed together in a small space. However, the strong nuclear force still acts between these nucleons, and the repulsive force that arises at short distances also increases as more nucleons are added. As a result, the ratio of the volume of the nucleus to the volume of a nucleon increases approximately linearly with the mass number $A$. This reflects the fact that the strong nuclear force is able to overcome the repulsive force and hold the nucleus together up to a certain point, beyond which the repulsive force becomes too great and the nucleus becomes unstable.
Question.11[(c) (i)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Given: A pure sample of copper-64 has a mass of $28 \mathrm{mg}$. The decay constant of copper-64 is $5.5 \times 10^{-2}$ hour $^{-1}$.
Calculate:, in $\mathrm{Bq}$, the initial activity of the sample.
▶️Answer/Explanation
Solution:
We know that capacitance, $C$ is given by:
$$C = \frac{Q}{V}$$
where $Q$ is the charge stored and $V$ is the potential difference across the capacitor.
The potential difference $V$ is given by:
$$V = Ed$$
where $E$ is the electric field strength and $d$ is the distance between the plates.
Thus, we have:
$$Q = CV = CEd$$
Substituting the given values, we get:
$$Q = (68 \times 10^{-9})\cdot (1.5 \times 10^6)\cdot (55 \times 10^{-6}) = 5.6 \times 10^{-6} \mathrm{~C}$$
Therefore, the maximum charge that can be stored on the capacitor is $5.6 \times 10^{-6} \mathrm{~C}$.
Question.11[(c) (ii)].2019-May-Physics_paper_2__TZ2_HL
Topic:
Calculate:, in hours, the time at which the activity of the sample has decreased to one-third of the initial activity.
▶️Answer/Explanation
Solution:
Sure! Using your method:
At $t = 0$, the activity of the sample is $A_0 = 4.0 \times 10^{15} \mathrm{~Bq}$.
Let $t_\frac{1}{3}$ be the time at which the activity of the sample has decreased to one-third of the initial activity.
We have:
$$\frac{A}{A_0} = \left(\frac{1}{3}\right)$$
Taking the natural logarithm of both sides:
$$\ln\left(\frac{A}{A_0}\right) = \ln\left(\frac{1}{3}\right)$$
Using the relation $A = A_0 e^{-\lambda t}$:
$$\ln\left(e^{-\lambda t}\right) = -\lambda t = \ln\left(\frac{1}{3}\right)$$
Solving for $t$:
$$t = \frac{\ln\left(\frac{1}{3}\right)}{-\lambda} = \frac{\ln(3)}{\lambda}\left(\lambda=5.5 \times 10^{-2} \text { hour }^{-1}\right)\approx 20 \mathrm{~hours}$$
Therefore, the time at which the activity of the sample has decreased to one-third of the initial activity is approximately 20 hours.