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Questions on Matter Waves and Special Relativity, the kind your examinations ask. Solve one on paper. Then tell the book how it went. The book believes you, and it uses your answer to plan your revision.

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Radiation Pressure and Matter Waves

21 questions · after Lesson 2, Electrons Diffract: Davisson and Germer

Force of a light beam

Q1
Take \(h = 6.6 \times 10^{-34}\) J s, \(c = 3 \times 10^{8}\) m/s, \(e = 1.6 \times 10^{-19}\) C; \(1\) nN \(= 10^{-9}\) N. A \(6\) W beam falls normally on a surface.
  1. The surface absorbs all the light. Find the force on the surface.
  2. The surface is a perfect mirror. Find the force now.
How did it go?
Q2
Light of wavelength \(660\) nm falls normally on a mirror. Each second \(10^{20}\) photons are reflected.
  1. Find the momentum of one photon.
  2. Find the change in momentum of one photon on reflection.
  3. Find the force on the mirror.
How did it go?
Q3
A beam of power \(3\) W falls on a perfectly absorbing plate. The beam makes \(60^\circ\) with the normal to the plate.
  1. Find the momentum delivered per second, and the direction of the force.
  2. Find the components of the force normal to the plate and along the plate.
How did it go?
Q4
The plate of Question 3 is replaced by a perfect mirror. The beam still makes \(60^\circ\) with the normal. Find the force on the mirror and state its direction. Why is there no force along the mirror?
How did it go?
Q5
A \(3\) W beam falls normally on a plate that reflects \(60\%\) and absorbs the rest. Find the force on the plate.
How did it go?
Q6
A wide parallel beam of intensity \(300\) W/m\(^2\) falls on a large black surface at \(60^\circ\) to the normal.
  1. Show that the pressure on the surface is \(\frac{I}{c}\cos^2\theta\). Where does each \(\cos\theta\) come from?
  2. Find the pressure.
How did it go?
Q7
A \(6\) W beam meets a plate at \(60^\circ\) to the normal, as shown. The plate reflects half the light and absorbs the rest.
  1. Find the normal force from the absorbed part and from the reflected part.
  2. Find the total force normal to the plate and the force along the plate.
Beam of 6 W at 60 degrees to the normal, half reflected
How did it go?

de Broglie wavelength

Q8
A cricket ball of mass \(0.2\) kg moves at \(33\) m/s.
  1. Find its de Broglie wavelength.
  2. Why do we never see the wave nature of a cricket ball?
How did it go?
Q9
An electron at rest is accelerated through \(V\) volt. Its de Broglie wavelength is \(\lambda = \frac{12.27}{\sqrt{V}}\) Å.
  1. Find \(\lambda\) for \(V = 100\) V.
  2. Find \(\lambda\) for \(V = 10^4\) V.
  3. How must \(V\) change to halve \(\lambda\)?
How did it go?
Q10
A particle of mass \(m\) has kinetic energy \(K\).
  1. Show that its de Broglie wavelength is \(\lambda = \frac{h}{\sqrt{2mK}}\).
  2. An electron gains \(K = eV\) from a potential difference \(V\). Show that \(\lambda = \frac{h}{\sqrt{2meV}}\).
  3. With \(m = 9.1 \times 10^{-31}\) kg and \(h = 6.63 \times 10^{-34}\) J s, check that \(\frac{h}{\sqrt{2me}} \approx 12.3\) Å V\(^{1/2}\).
How did it go?
Q11
Find the de Broglie wavelength of an electron of kinetic energy
  1. \(150\) eV,
  2. \(600\) eV.
How did it go?
Q12
A proton is \(1836\) times heavier than an electron. Find the ratio \(\lambda_e : \lambda_p\) of their de Broglie wavelengths when the two particles have
  1. the same speed,
  2. the same kinetic energy,
  3. the same momentum.
How did it go?
Q13
A photon and an electron both have wavelength \(1\) Å. Take \(hc = 12400\) eV Å.
  1. Find the energy of the photon in eV.
  2. Find the kinetic energy of the electron in eV.
  3. Which one carries more energy, and roughly how many times more?
How did it go?
Q14
An electron starts from rest at A and reaches B, as shown. Its mass is \(9.1 \times 10^{-31}\) kg.
  1. Find the kinetic energy of the electron at B in eV and in joule.
  2. Find its speed at B.
  3. Find its de Broglie wavelength at B.
Electron released from rest at plate A at 0 V moving to plate B at 400 V
How did it go?

Davisson-Germer

Q15
In the Davisson and Germer experiment, accelerated electrons fall on a nickel crystal.
  1. What quantity is measured, and against what is it plotted?
  2. What did the experiment show about electrons?
How did it go?
Q16
In the experiment a strong peak appeared at an accelerating voltage of \(54\) V. For the nickel planes used, the crystal spacing is \(d = 0.91\) Å and the glancing angle of the peak is \(\theta = 65^\circ\). Take \(\sin 65^\circ = 0.906\).
  1. Find the de Broglie wavelength of the electrons from \(\lambda = \frac{12.27}{\sqrt{V}}\) Å.
  2. Find the wavelength from Bragg's rule \(2d\sin\theta = \lambda\) for the first order.
  3. What does the agreement between (i) and (ii) show?
How did it go?
Q17
The figure shows the number of scattered electrons per second against the scattering angle \(\phi\) at \(54\) V.
  1. Read the angle \(\phi\) of the peak.
  2. The glancing angle is \(\theta = 90^\circ - \phi/2\). Find \(\theta\).
  3. The voltage is raised to \(64\) V. Does the peak move to a smaller or a larger \(\phi\)? Why?
Scattered electron count against scattering angle at 54 V
How did it go?
Q18
Electrons of kinetic energy \(150\) eV fall on a crystal whose planes are \(d = 1.0\) Å apart.
  1. Find the glancing angle \(\theta\) of the first-order maximum from \(2d\sin\theta = \lambda\).
  2. The energy is raised to \(600\) eV. Find the new first-order angle. Take \(\sin 14.5^\circ = 0.25\).
How did it go?
Q19
The figure shows the apparatus.
  1. What does the voltage \(V\) on the gun decide about the electrons?
  2. What does the detector measure, and how is it moved?
  3. Why must the whole apparatus be in a vacuum?
  4. Why is a peak at one angle a sign of wave behaviour?
Davisson-Germer apparatus: gun, nickel crystal, detector at angle phi
How did it go?

Small situations

Q20
A perfectly reflecting solar sail of area \(100\) m\(^2\) faces the Sun, as shown. Sunlight of intensity \(1500\) W/m\(^2\) falls normally on it. Sail and load have mass \(100\) kg.
  1. Find the force of the sunlight on the sail.
  2. Find the acceleration of the sail.
  3. Find the speed gained in one day (\(86400\) s), starting from rest.
Perfectly reflecting solar sail of 100 square metres with a 100 kg payload
How did it go?
Q21
An electron and a photon both have wavelength \(1\) nm. Take \(hc = 1240\) eV nm.
  1. Find the momentum of each.
  2. Find the energy of the photon.
  3. Find the kinetic energy of the electron.
How did it go?

Special Relativity

24 questions · after Lesson 5, Mass, Momentum and Energy

Frames and postulates

Q22
Take \(c = 3 \times 10^{8}\) m/s throughout. What is an inertial frame of reference? Which of these frames are inertial?
  1. A train at a steady \(30\) m/s on a straight track.
  2. A car that is braking.
  3. A rotating merry-go-round.
How did it go?
Q23
State the two postulates of special relativity in your own words.
How did it go?
Q24
A lamp in a train flashes. A rides in the train and B stands on the platform. The train moves at speed \(v\).
  1. What speed does A measure for the light that moves forward?
  2. What speed does B measure for the same light? Which postulate decides this?
  3. A throws a ball forward at \(10\) m/s while the train moves at \(20\) m/s. What speed does B measure for the ball, approximately?
A lamp flashes inside a moving train; A is on the train, B on the platform
How did it go?
Q25
The rule "speeds simply add" works for the ball in Question 3 but fails for light. Why do we never notice this failure in daily life?
How did it go?

The Lorentz factor

Q26
The Lorentz factor is \(\gamma = \frac{1}{\sqrt{1 - v^2/c^2}}\). Find \(\gamma\) for
  1. \(v = 0.6c\),
  2. \(v = 0.8c\),
  3. \(v = 0.96c\).
How did it go?
Q27
Find the speed, as a fraction of \(c\), at which
  1. \(\gamma = 1.25\),
  2. \(\gamma = 2\).
How did it go?
Q28
The figure shows \(\gamma\) against \(v/c\).
  1. Read \(\gamma\) at \(v = 0.6c\) and at \(v = 0.8c\) from the dotted lines.
  2. Read the speed at which \(\gamma = 2\), roughly.
  3. Why does the curve rise without limit as \(v\) approaches \(c\)?
  4. For \(v\) below \(0.2c\), \(\gamma\) is almost exactly \(1\). What does this mean for everyday motion?
Lorentz factor gamma against v/c
How did it go?

Time dilation

Q29
A muon at rest lives for \(2.2\ \mu\)s on average. Muons made high in the atmosphere move at \(0.96c\).
  1. Find the average lifetime of these muons as measured from the ground.
  2. Find the distance a muon travels in this time.
  3. How far would it travel if there were no time dilation?
How did it go?
Q30
A clock on a spaceship moving at \(0.6c\) shows that \(1\) hour has passed. How much time has passed for observers on Earth?
How did it go?
Q31
An astronaut's heart beats \(60\) times per minute, as measured by the astronaut. The spaceship passes Earth at \(0.8c\). How many beats per minute does an observer on Earth count?
How did it go?
Q32
Two events happen at the same place in a frame S. A clock at rest in S measures the time between them as \(\Delta t_0\), the proper time.
  1. Is the time between the same two events measured in any other frame longer or shorter than \(\Delta t_0\)?
  2. A muon is created and later decays. In which frame is the time between these two events the proper time?
How did it go?
Q33
A light clock has two mirrors a distance \(d\) apart. One tick is the flash going from the lower mirror to the upper one.
  1. For the clock at rest, write the time \(\Delta t_0\) of one tick.
  2. In a frame where the clock moves at \(v\), the flash travels along the slant. Use Pythagoras to show that \(\Delta t = \gamma\,\Delta t_0\).
Light clock at rest and as seen from a frame where it moves
How did it go?

Length contraction

Q34
A rod has proper length \(5\) m. It moves along its length at \(0.8c\). Find its length as measured by an observer at rest.
How did it go?
Q35
A spaceship is \(100\) m long and \(20\) m wide when at rest. It passes Earth at \(0.6c\), moving along its length.
  1. Find the length and the width measured from Earth.
  2. Which dimension changes, and why not the other?
How did it go?
Q36
A rides in a train car and measures its length as \(60\) m. The car passes B, who stands on the ground, at \(0.6c\).
  1. Who measures the proper length of the car? Why?
  2. Find the length of the car measured by B.
  3. B holds a metre stick along the track. Find its length as measured by A.
Train car of proper length 60 m passing observer B at 0.6c
How did it go?
Q37
Return to the muon of Question 8. In the muon's own frame it lives for only \(2.2\ \mu\)s.
  1. The ground is \(2263\) m below the muon in the ground frame. Find this distance in the muon's frame.
  2. Show that in its own frame the muon can still reach the ground.
How did it go?

Mass, momentum and energy

Q38
The rest mass of an electron is \(9.1 \times 10^{-31}\) kg. Find its rest energy \(m_0c^2\) in joule and in MeV. Take \(1\) eV \(= 1.6 \times 10^{-19}\) J.
How did it go?
Q39
Find the energy released if \(1\) g of matter is fully converted into energy. Express the answer in joule and in kilowatt hours (\(1\) kWh \(= 3.6 \times 10^{6}\) J).
How did it go?
Q40
An electron moves at \(0.8c\).
  1. Find its relativistic momentum \(p = \gamma m_0 v\).
  2. Find the classical value \(m_0 v\). What is the ratio of the two?
How did it go?
Q41
Take the rest energy of an electron as \(0.5\) MeV. The electron moves at \(0.6c\).
  1. Find its total energy \(E = \gamma m_0 c^2\).
  2. Find its kinetic energy \(K = E - m_0c^2\).
  3. Compare \(K\) with the classical value \(\frac{1}{2}m_0 v^2\), written in terms of \(m_0c^2\).
How did it go?
Q42
A particle has rest energy \(m_0c^2 = 3\) MeV and momentum \(p\) such that \(pc = 4\) MeV.
  1. Use \(E^2 = (pc)^2 + (m_0c^2)^2\) to find the total energy \(E\).
  2. Find the kinetic energy.
  3. Find \(\gamma\) and hence the speed of the particle.
How did it go?
Q43
The figure shows kinetic energy against \(v/c\) for a particle, in units of \(mc^2\). One curve is the classical \(\frac{1}{2}mv^2\), the other the relativistic \((\gamma - 1)mc^2\).
  1. Which curve, P or Q, is relativistic? Give the reason.
  2. Find the value of each curve at \(v = 0.8c\) by calculation.
  3. Why does curve P rise without limit near \(v = c\)?
Kinetic energy against v/c, classical and relativistic curves
How did it go?
Q44
A photon has zero rest mass. Use \(E^2 = (pc)^2 + (m_0c^2)^2\) to show that its momentum is \(p = E/c\). Find \(p\) for a photon of energy \(2\) eV.
How did it go?
Q45
Use the formulas for \(\gamma\), \(p\) and \(E\) to explain why no object with rest mass can be accelerated to the speed of light.
How did it go?