---
title: "Introduction to Quantum Physics"
book: "University Physics — Year 1"
subject: physics
language: en
chapter: 30
exercises: 12
source: https://one-course.com/books/physics/3/en/chapter/30-introduction-to-quantum-physics
---

# Chapter 30 — Introduction to Quantum Physics

Shine ultraviolet light on a clean metal and electrons fly out at once, with an energy that depends on the colour of the light and not at all on its brightness; shine red light and nothing comes out however bright the lamp. Send electrons one by one through two slits and they land as dots, each in one place — and the dots build up, over thousands, into the fringes of a wave. Neither fact fits the physics of the first twenty-nine chapters. This last chapter introduces the ideas that do fit them: light comes in quanta, the photons; matter has a wavelength; what propagates is an [amplitude](https://one-course.com/books/physics/3/en/chapter/5-signal-propagation-travelling-and-standing-waves#def-b1-wave-propagation-signal) whose square is a probability; position and momentum cannot both be sharp; and a confined particle can only have certain energies — which is why atoms have sizes, spectra have lines, and a grain of semiconductor a few nanometres across glows in a colour set by its diameter.

## 30.1 The photon

**Theorem 30.1 (Planck–Einstein relations).**

Light of frequency $\nu$ and wavelength $\lambda$ exchanges energy with matter only in quanta, the *photons*, of energy and momentum

$$
E = h\nu = \frac{hc}{\lambda} , \qquad p = \frac{h}{\lambda} = \frac{E}{c} ,
$$

with *[Planck’s constant](#thm-b1-quantum-introduction-photon)* $h = 6.626 \times 10^{-34}\,\mathrm{J}\,\mathrm{s}$ ($\hbar = h/2\pi =
1.055 \times 10^{-34}\,\mathrm{J}\,\mathrm{s}$). Useful: $hc = 1240\,\mathrm{eV}\,\mathrm{nm}$ — a photon of $620\,\mathrm{nm}$ carries $2\,\mathrm{eV}$.

**Proof.** *Admitted at this level.* ∎

**Proposition 30.2 (The photoelectric effect).**

Light falling on a metal of *[work function](#prop-b1-quantum-introduction-photoelectric)* $W$ (the energy binding its least-bound electrons, a few eV) extracts electrons of maximal [kinetic energy](https://one-course.com/books/physics/3/en/chapter/13-work-energy-and-potential-energy#thm-b1-work-and-energy-ke)

$$
E_{k,\max} = h\nu - W ,
$$

hence only above the *threshold* $\nu_0 = W/h$, instantly, with an energy independent of the intensity; the intensity fixes the *number* of electrons per second. The *[stopping potential](#prop-b1-quantum-introduction-photoelectric)* $V_s$ that just cancels the current measures $E_{k,\max} = eV_s$, and the plot of $V_s$ against $\nu$ is a straight line of slope $h/e$ — how Millikan measured $h$.

**Proof.** Each photon is absorbed by one electron, which keeps $h\nu - W$ at best; a wave would deliver energy continuously to every electron, the energy would grow with intensity, and a weak light would need hours to accumulate $W$ on one atom ([Problem 30.1](#pb-b1-quantum-introduction-1)) — none of which is observed. Einstein’s interpretation (1905) is admitted as the law. ∎

![Left: the photoelectric cell — light frees electrons from the cathode; a reverse voltage V_s just sufficient to stop them measures their maximal energy. Right: the stopping potential against frequency is a straight line for every metal, of slope h/e; the intercept gives the work function, the threshold the minimum frequency.](https://one-course.com/images/onecourse/chapters/physics-3/b1-quantum-introduction/fig-d4a128949e7f.svg)

![Left: the photoelectric cell — light frees electrons from the cathode; a reverse voltage V_s just sufficient to stop them measures their maximal energy. Right: the stopping potential against frequency is a straight line for every metal, of slope h/e; the intercept gives the work function, the threshold the minimum frequency.](https://one-course.com/images/onecourse/chapters/physics-3/b1-quantum-introduction/fig-a4cb5d9de2ff.svg)

*Left: the photoelectric cell — light frees electrons from the cathode; a reverse [voltage](https://one-course.com/books/physics/3/en/chapter/6-dc-circuits-kirchhoffs-laws-and-theorems#def-b1-dc-circuits-voltage) $V_s$ just sufficient to stop them measures their maximal energy. Right: the [stopping potential](#prop-b1-quantum-introduction-photoelectric) against frequency is a straight line for every metal, of slope $h/e$; the intercept gives the [work function](#prop-b1-quantum-introduction-photoelectric), the threshold the minimum frequency.*

**Example 30.3 (Orders of magnitude).**

A visible photon: $2\,\mathrm{eV}$; an X-ray photon of $0.1\,\mathrm{nm}$: $12\,\mathrm{keV}$; a radio photon at $100\,\mathrm{MHz}$: $4 \times 10^{-7}\,\mathrm{eV}$. A $1\,\mathrm{mW}$ red laser emits $10^{-3}/(3.1 \times 10^{-19}) = 3 \times 10^{15}$ photons per second; a radio antenna picking up $1\,\mathrm{pW}$ at $100\,\mathrm{MHz}$ receives $10^{13}$ per second — so many, so small, that the wave description is exact for every purpose; the [eye](https://one-course.com/books/physics/3/en/chapter/4-optical-instruments-and-the-eye#def-b1-optical-instruments-eye), by contrast, can register a flash of a hundred photons. The quantum nature of light shows when photons are few or energetic: photoelectric cells, X-ray detectors, the grain of a faint photograph.

**Remark 30.4 (Compton scattering).**

A photon bouncing off a free electron transfers momentum like a billiard ball: its wavelength grows by $\Delta\lambda = \frac{h}{m_ec}(1 -
\cos\theta)$, with $h/m_ec = 2.43\,\mathrm{pm}$ (admitted — a relativistic collision, Year 2). Invisible for light ($\Delta\lambda/\lambda \sim 10^{-5}$), it is a $20\%$ effect for X-rays, and was the experiment that convinced the sceptics (1923) that the photon carries momentum $h/\lambda$.

## 30.2 Matter waves

**Theorem 30.5 (de Broglie).**

A particle of momentum $p$ propagates as a wave of wavelength

$$
\lambda = \frac{h}{p} ,
$$

and shows diffraction and interference accordingly: electrons on a crystal (Davisson and Germer, 1927), through two slits (Jönsson, 1961), neutrons, atoms, and molecules of sixty carbon atoms. For an electron accelerated by $U$, $\lambda = h/\sqrt{2m_eeU} = 1.23\,\mathrm{nm}/\sqrt{U/\mathrm{V}}$.

**Proof.** *Admitted at this level.* ∎

**Example 30.6 (Why we never saw it).**

An electron of $100\,\mathrm{eV}$: $\lambda = 0.12\,\mathrm{nm}$, the spacing of atoms in a crystal — hence the diffraction, and the electron [microscope](https://one-course.com/books/physics/3/en/chapter/4-optical-instruments-and-the-eye#def-b1-optical-instruments-microscope). A thermal neutron ($0.025\,\mathrm{eV}$): $0.18\,\mathrm{nm}$. A ball of $1\,\mathrm{g}$ at $1\,\mathrm{m}/\mathrm{s}$: $\lambda = 7 \times 10^{-31}\,\mathrm{m}$, $10^{20}$ times smaller than a nucleus: no slit, no crystal could ever diffract it. The wave nature of matter is universal; its wavelength is what makes it visible only for the light and the slow.

**Proposition 30.7 (Single particles build the fringes).**

Electrons sent one at a time through two slits (Tonomura, 1989) each make a single dot on the screen, at a place that cannot be predicted; the dots accumulate into the two-slit interference pattern of a wave of wavelength $h/p$. Closing one slit erases the fringes — the pattern is not made by electrons interfering with each other, but by each electron’s wave passing through both slits. Detecting which slit a particle went through also erases the fringes.

**Proof.** *Admitted at this level.* ∎

![Electrons one at a time through two slits. Each arrives as a dot somewhere (left, top); the dots pile up where the two-slit wave is intense (left, bottom), following the probability density | |2 of the amplitude that passed through both slits (right). The pattern is the same for photons, neutrons and molecules.](https://one-course.com/images/onecourse/chapters/physics-3/b1-quantum-introduction/fig-72b1ca13a53f.svg)

![Electrons one at a time through two slits. Each arrives as a dot somewhere (left, top); the dots pile up where the two-slit wave is intense (left, bottom), following the probability density | |2 of the amplitude that passed through both slits (right). The pattern is the same for photons, neutrons and molecules.](https://one-course.com/images/onecourse/chapters/physics-3/b1-quantum-introduction/fig-1e4e31a0d992.svg)

*Electrons one at a time through two slits. Each arrives as a dot somewhere (left, top); the dots pile up where the two-slit wave is intense (left, bottom), following the [probability density](#def-b1-quantum-introduction-wavefunction) $|\psi|^2$ of the [amplitude](https://one-course.com/books/physics/3/en/chapter/5-signal-propagation-travelling-and-standing-waves#def-b1-wave-propagation-signal) that passed through both slits (right). The pattern is the same for photons, neutrons and molecules.*

## 30.3 Amplitudes, probabilities, and the uncertainty principle

**Definition 30.8 (Wavefunction).**

The state of a particle is described by a *wavefunction* $\psi(x, t)$ (complex), such that $|\psi(x, t)|^2\,\dd x$ is the probability of finding the particle between $x$ and $x + \dd x$ when one looks: $|\psi|^2$ is a *probability density*, and $\int|\psi|^2\dd x =
1$. [Amplitudes](https://one-course.com/books/physics/3/en/chapter/5-signal-propagation-travelling-and-standing-waves#def-b1-wave-propagation-signal) add (superposition): if two paths lead to the same point, $\psi = \psi_1 + \psi_2$ and $|\psi|^2 = |\psi_1|^2 + |\psi_2|^2 +
2\,\mathrm{Re}(\psi_1^\ast\psi_2)$ — the last term is the interference. A measurement gives one of the possible results, at random with the probabilities the [amplitudes](https://one-course.com/books/physics/3/en/chapter/5-signal-propagation-travelling-and-standing-waves#def-b1-wave-propagation-signal) prescribe, and leaves the particle in the state found.

**Remark 30.9 (What is waving).**

$\psi$ is not a physical field like $\vect E$: it is not measured, only its square is, and it describes our best possible knowledge of where the particle will be found. A single electron is not spread over the screen; it is detected whole, at one point; what is spread is the probability. This is the content of the theory, and it has never failed a test.

**Theorem 30.10 (Heisenberg’s uncertainty principle).**

The position and the momentum of a particle along the same axis cannot both be sharply defined: their standard deviations in any state obey

$$
\Delta x\,\Delta p_x \geq \frac{\hbar}{2} .
$$

A particle confined to a region of size $\ell$ therefore has a momentum spread of at least $\hbar/2\ell$, hence a [kinetic energy](https://one-course.com/books/physics/3/en/chapter/13-work-energy-and-potential-energy#thm-b1-work-and-energy-ke) of order $\hbar^2/2m\ell^2$ that no cooling can remove: confinement costs energy.

**Proof.** *Admitted at this level.* ∎

**Example 30.11 (The size of the hydrogen atom).**

An electron within $r$ of the proton has $p \gtrsim \hbar/r$ and energy $E(r) \approx \dfrac{\hbar^2}{2m_er^2} - \dfrac{e^2}{4\pi\varepsilon_0r}$: the first term blows up if $r$ shrinks, the second if it grows. $\dd E/\dd r = 0$ at

$$
a_0 = \frac{4\pi\varepsilon_0\hbar^2}{m_ee^2} = 53\,\mathrm{pm} , \qquad
E(a_0) = -\frac{m_ee^4}{2(4\pi\varepsilon_0)^2\hbar^2} = -13.6\,\mathrm{eV} :
$$

the *[Bohr radius](#ex-b1-quantum-introduction-hsize)* and the ionization energy of hydrogen, to the last digit. Classical physics could not explain why the electron does not spiral into the nucleus (it radiates) nor why all atoms of an element are identical; the uncertainty principle answers both in one line: the atom is as small as it can be without the [kinetic energy](https://one-course.com/books/physics/3/en/chapter/13-work-energy-and-potential-energy#thm-b1-work-and-energy-ke) exceeding the binding.

## 30.4 Quantization of energy

**Proposition 30.12 (Particle in a box).**

A particle of mass $m$ confined between two impenetrable walls a distance $L$ apart has, like Melde’s string ([Chapter 5](https://one-course.com/books/physics/3/en/chapter/5-signal-propagation-travelling-and-standing-waves#ch-b1-wave-propagation)), only the [standing waves](https://one-course.com/books/physics/3/en/chapter/5-signal-propagation-travelling-and-standing-waves#thm-b1-wave-propagation-standing) $\lambda_n = 2L/n$, hence only the momenta $p_n = nh/2L$ and the energies

$$
E_n = \frac{n^2h^2}{8mL^2} , \qquad n = 1, 2, 3, \ldots
$$

with [wavefunctions](#def-b1-quantum-introduction-wavefunction) $\psi_n(x) \propto \sin(n\pi x/L)$. The energy is *quantized*; the lowest, the *[ground state](#prop-b1-quantum-introduction-box)* $E_1 > 0$, is the confinement energy of the uncertainty principle made exact; the particle jumps between levels by absorbing or emitting a photon of energy $h\nu = E_p - E_n$.

**Proof.** $\psi$ must vanish at the walls (the particle cannot be there), so the wave fits a whole number of half-wavelengths in $L$ — the string condition; de Broglie gives $p$, and $E = p^2/2m$. That $\psi$ obeys a wave equation with these boundary conditions is admitted (the Schrödinger equation, Year 2). ∎

![Left: the three lowest states of a particle in a box — the wavefunctions are the standing waves of a string, the energies grow as n2, and the ground state is not at zero. Right: the levels of the hydrogen atom and its two first series of lines; each line is a photon of energy equal to the gap it bridges.](https://one-course.com/images/onecourse/chapters/physics-3/b1-quantum-introduction/fig-e856b32aaafb.svg)

![Left: the three lowest states of a particle in a box — the wavefunctions are the standing waves of a string, the energies grow as n2, and the ground state is not at zero. Right: the levels of the hydrogen atom and its two first series of lines; each line is a photon of energy equal to the gap it bridges.](https://one-course.com/images/onecourse/chapters/physics-3/b1-quantum-introduction/fig-cf6dfc3168fc.svg)

*Left: the three lowest states of a particle in a box — the [wavefunctions](#def-b1-quantum-introduction-wavefunction) are the [standing waves](https://one-course.com/books/physics/3/en/chapter/5-signal-propagation-travelling-and-standing-waves#thm-b1-wave-propagation-standing) of a string, the energies grow as $n^2$, and the [ground state](#prop-b1-quantum-introduction-box) is not at zero. Right: the levels of the [hydrogen atom](#prop-b1-quantum-introduction-hydrogen) and its two first series of lines; each line is a photon of energy equal to the gap it bridges.*

**Proposition 30.13 (The hydrogen atom).**

The electron of the [hydrogen atom](#prop-b1-quantum-introduction-hydrogen) has the discrete energies

$$
E_n = -\frac{13.6\,\mathrm{eV}}{n^2} , \qquad n = 1, 2, 3, \ldots ,
$$

$n = 1$ being the [ground state](#prop-b1-quantum-introduction-box) and $E \geq 0$ the ionized atom. Its spectrum consists of lines at $h\nu = E_p - E_n$: the Lyman series down to $n = 1$ (ultraviolet, $122\,\mathrm{nm}$ for $2 \to 1$), the Balmer series down to $n = 2$ (visible: $656\,\mathrm{nm}$, $486\,\mathrm{nm}$, $434\,\mathrm{nm}$, …), and so on. Bohr’s model (1913) obtains these energies by quantizing the [angular momentum](https://one-course.com/books/physics/3/en/chapter/15-angular-momentum#def-b1-angular-momentum-L) of a [circular orbit](https://one-course.com/books/physics/3/en/chapter/16-central-forces-planets-and-satellites#prop-b1-central-forces-effective), $m_evr = n\hbar$ ([Exercise 30.9](#exo-b1-quantum-introduction-9)); the full theory replaces orbits by [wavefunctions](#def-b1-quantum-introduction-wavefunction) but keeps the energies.

**Proof.** *Admitted at this level.* ∎

**Example 30.14 (Colours from size: the quantum dot).**

A nanocrystal of semiconductor a few nanometres across confines its electrons like a box: the smaller the crystal, the larger the confinement energy added to the semiconductor’s gap, the bluer the light it emits. Cadmium selenide dots of radius $2\,\mathrm{nm}$ glow blue, $3\,\mathrm{nm}$ yellow, $4\,\mathrm{nm}$ red — one material, colours chosen with a ruler ([Problem 30.1](#pb-b1-quantum-introduction-1)). Television screens use them.

**Remark 30.15 (What the rest of the theory adds).**

The Schrödinger equation makes the box, the atom and the molecule exact; it predicts that a particle can cross a barrier it has not the energy to climb (the *[tunnel effect](#rem-b1-quantum-introduction-rest)*, behind radioactivity and the scanning tunnelling [microscope](https://one-course.com/books/physics/3/en/chapter/4-optical-instruments-and-the-eye#def-b1-optical-instruments-microscope)); that identical particles are either sociable (bosons — hence the *laser*, where photons pile into one mode) or exclusive (fermions — hence the periodic table and the stiffness of matter); and that the spin of the electron is a [magnetic moment](https://one-course.com/books/physics/3/en/chapter/28-magnetostatics-field-forces-and-dipoles#def-b1-magnetostatics-moment) with no classical counterpart. All of it is Year 2 and beyond; all of it rests on the few ideas of this chapter.

## 30.5 Exercises

**Exercise 30.1 ★.**

Energy of a photon of: radio at $100\,\mathrm{MHz}$; light at $500\,\mathrm{nm}$; X-rays at $0.10\,\mathrm{nm}$; gamma rays of $1\,\mathrm{MeV}$ (give its wavelength). Number of photons per second from a $1.0\,\mathrm{mW}$ laser at $633\,\mathrm{nm}$.

**Solution of Exercise 30.1.**

$h\nu$: $100\,\mathrm{MHz}$: $6.6 \times 10^{-26}$ J $= 4.1 \times 10^{-7}\,\mathrm{eV}$; $500\,\mathrm{nm}$: $1240/500 = 2.5\,\mathrm{eV}$; $0.10\,\mathrm{nm}$: $12.4\,\mathrm{keV}$; $1\,\mathrm{MeV}$: $\lambda =
1240/10^6 = 1.2 \times 10^{-3}\,\mathrm{nm} = 1.2\,\mathrm{pm}$. Laser: $1240/633 = 1.96\,\mathrm{eV} =
3.1 \times 10^{-19}\,\mathrm{J}$, so $10^{-3}/3.1 \times 10^{-19} = 3.2 \times 10^{15}$ photons per second.

**Exercise 30.2 ★.**

Sodium, $W = 2.3\,\mathrm{eV}$: threshold wavelength; maximal [kinetic energy](https://one-course.com/books/physics/3/en/chapter/13-work-energy-and-potential-energy#thm-b1-work-and-energy-ke) and [stopping potential](#prop-b1-quantum-introduction-photoelectric) for $400\,\mathrm{nm}$ light; what changes if the intensity is doubled? and with $600\,\mathrm{nm}$ light?

**Solution of Exercise 30.2.**

$\lambda_0 = 1240/2.3 = 540\,\mathrm{nm}$. At $400\,\mathrm{nm}$, $h\nu = 3.1\,\mathrm{eV}$: $E_{k,\max} = 0.8\,\mathrm{eV}$, $V_s = 0.8\,\mathrm{V}$. Doubling the intensity doubles the current and leaves $V_s$ unchanged. At $600\,\mathrm{nm}$ ($2.07\,\mathrm{eV}$ $< W$): nothing, at any intensity.

**Exercise 30.3 ★.**

[De Broglie wavelength](#thm-b1-quantum-introduction-debroglie) of an electron of $100\,\mathrm{eV}$, of $1.0\,\mathrm{keV}$; of a neutron of $0.025\,\mathrm{eV}$; of a $1\,\mathrm{g}$ ball at $1\,\mathrm{m}/\mathrm{s}$. Which of these can be diffracted by a crystal ($0.2\,\mathrm{nm}$ spacing)?

**Solution of Exercise 30.3.**

Electron: $1.23/\sqrt{100} = 0.12\,\mathrm{nm}$; at $1\,\mathrm{keV}$: $0.039\,\mathrm{nm}$. Neutron: $E = 4.0 \times 10^{-21}\,\mathrm{J}$, $p = \sqrt{2m_nE} = 3.7 \times 10^{-24}\,\mathrm{kg}\,\mathrm{m}/\mathrm{s}$, $\lambda = h/p = 0.18\,\mathrm{nm}$. Ball: $6.6 \times 10^{-34}/10^{-3} = 7 \times 10^{-31}\,\mathrm{m}$. The first three have $\lambda$ of the order of the atomic spacing and are diffracted (electron, neutron and X-ray crystallography); the ball never.

**Exercise 30.4 ★.**

An electron in a box of $1.0\,\mathrm{nm}$: $E_1$, $E_2$, wavelength of the photon emitted from $2 \to 1$. A proton in a box of $5\,\mathrm{fm}$ (a nucleus): $E_1$ in $\mathrm{MeV}$.

**Solution of Exercise 30.4.**

$E_1 = h^2/8m_eL^2 = 4.39 \times 10^{-67}/(8 \times 9.11 \times 10^{-31} \times 10^{-18}) =
6.0 \times 10^{-20}\,\mathrm{J} = 0.38\,\mathrm{eV}$, $E_2 = 4E_1 = 1.5\,\mathrm{eV}$; photon $1.13\,\mathrm{eV}$, $\lambda = 1240/1.13 = 1.1\,\text{µ}\mathrm{m}$ (near infrared). Proton in $5\,\mathrm{fm}$: $4.39 \times 10^{-67}/(8 \times 1.67 \times 10^{-27} \times 25 \times 10^{-30}) =
1.3 \times 10^{-12}\,\mathrm{J} = 8\,\mathrm{MeV}$ — the scale of nuclear energies, from confinement alone.

**Exercise 30.5 ★★.**

[Stopping potentials](#prop-b1-quantum-introduction-photoelectric) measured for a metal: $0.40\,\mathrm{V}$ at $6.0 \times 10^{14}\,\mathrm{Hz}$, $1.23\,\mathrm{V}$ at $8.0 \times 10^{14}\,\mathrm{Hz}$, $2.05\,\mathrm{V}$ at $1.0 \times 10^{15}\,\mathrm{Hz}$. Deduce $h$ (with $e$ known) and the [work function](#prop-b1-quantum-introduction-photoelectric); threshold wavelength; which metal could it be (caesium $2.1\,\mathrm{eV}$, potassium $2.3\,\mathrm{eV}$, zinc $4.3\,\mathrm{eV}$)?

**Solution of Exercise 30.5.**

Slope $(2.05 - 0.40)/(4.0 \times 10^{14}) = 4.1 \times 10^{-15}\,\mathrm{V}\,\mathrm{s}$, $h = e \times 4.1 \times
10^{-15} = 6.6 \times 10^{-34}\,\mathrm{J}\,\mathrm{s}$. $W = h\nu - eV_s = 2.48 - 0.40 = 2.1\,\mathrm{eV}$, threshold $\lambda_0 = 1240/2.1 = 600\,\mathrm{nm}$: caesium.

**Exercise 30.6 ★★.**

Compton: an X-ray photon of $10\,\mathrm{pm}$ scatters at $90{}^{\circ}$ off an electron. New wavelength; energies of the photon before and after; energy given to the electron. Relative shift for $500\,\mathrm{nm}$ light — why Compton needed X-rays.

**Solution of Exercise 30.6.**

$\Delta\lambda = 2.43\,\mathrm{pm}$: $\lambda' = 12.4\,\mathrm{pm}$. Before: $1240/0.010 =
124\,\mathrm{keV}$; after: $1240/0.0124 = 100\,\mathrm{keV}$; the electron takes $24\,\mathrm{keV}$. For light, $\Delta\lambda/\lambda = 2.4 \times 10^{-12}/5 \times 10^{-7} = 5 \times
10^{-6}$: unmeasurable in 1923 — X-rays made the shift a $25\%$ effect.

**Exercise 30.7 ★★.**

*Jönsson’s experiment.* Electrons of $50\,\mathrm{keV}$ (use $p =
\sqrt{2m_eE}$), two slits $2.0\,\text{µ}\mathrm{m}$ apart, screen at $35\,\mathrm{cm}$. Wavelength; [fringe spacing](https://one-course.com/books/physics/3/en/chapter/5-signal-propagation-travelling-and-standing-waves#ex-b1-wave-propagation-young); why a magnifying electron [lens](https://one-course.com/books/physics/3/en/chapter/3-mirrors-and-thin-lenses#def-b1-mirrors-thin-lenses-lens) was needed. In Tonomura’s version one electron at a time crosses the apparatus: what does the screen show after 10, after $10^5$ electrons, and what does that teach?

**Solution of Exercise 30.7.**

$p = \sqrt{2 \times 9.11 \times 10^{-31} \times 5 \times 10^4 \times 1.6 \times 10^{-19}} =
1.2 \times 10^{-22}\,\mathrm{kg}\,\mathrm{m}/\mathrm{s}$, $\lambda = 5.5\,\mathrm{pm}$ (relativity corrects it to $5.4\,\mathrm{pm}$); [fringe spacing](https://one-course.com/books/physics/3/en/chapter/5-signal-propagation-travelling-and-standing-waves#ex-b1-wave-propagation-young) $\lambda D/d = 5.5 \times 10^{-12} \times 0.35/2 \times 10^{-6}
= 1\,\text{µ}\mathrm{m}$: invisible to the [eye](https://one-course.com/books/physics/3/en/chapter/4-optical-instruments-and-the-eye#def-b1-optical-instruments-eye), hence the magnifying [lens](https://one-course.com/books/physics/3/en/chapter/3-mirrors-and-thin-lenses#def-b1-mirrors-thin-lenses-lens). Ten electrons: ten dots, apparently at random; $10^5$: the fringes. Each electron lands at one point; the *probability* of landing follows the two-slit wave — a single electron’s wave goes through both slits.

**Exercise 30.8 ★★.**

Minimum [kinetic energy](https://one-course.com/books/physics/3/en/chapter/13-work-energy-and-potential-energy#thm-b1-work-and-energy-ke), from the uncertainty principle, of: an electron confined to $0.1\,\mathrm{nm}$ (an atom); an electron confined to $5\,\mathrm{fm}$ (a nucleus — use $E \approx pc$ if the result is relativistic, and conclude whether nuclei can contain electrons); a dust grain of $1\,\text{µ}\mathrm{g}$ localized to $1\,\text{µ}\mathrm{m}$ (give $\Delta v$).

**Solution of Exercise 30.8.**

Atom: $\Delta p \geq \hbar/2\Delta x = 5.3 \times 10^{-25}\,\mathrm{kg}\,\mathrm{m}/\mathrm{s}$, $E \sim \Delta p^2/2m_e =
1.5 \times 10^{-19}\,\mathrm{J} \approx 1\,\mathrm{eV}$: the right scale. Nucleus: $\Delta p \geq
1.1 \times 10^{-20}\,\mathrm{kg}\,\mathrm{m}/\mathrm{s}$; $\Delta p^2/2m_e$ would be $400\,\mathrm{MeV}$, far above $m_ec^2$, so use $E \approx \Delta p\,c = 3 \times 10^{-12}\,\mathrm{J} = 20\,\mathrm{MeV}$: no force in the nucleus could hold an electron that energetic — nuclei contain no electrons (beta electrons are created when emitted). Grain: $\Delta v \geq
\hbar/2m\Delta x = 1.05 \times 10^{-34}/(2 \times 10^{-9} \times 10^{-6}) = 5 \times 10^{-20}\,\mathrm{m}/\mathrm{s}$: irrelevant.

**Exercise 30.9 ★★.**

*Bohr’s model.* Electron on a [circular orbit](https://one-course.com/books/physics/3/en/chapter/16-central-forces-planets-and-satellites#prop-b1-central-forces-effective) of radius $r$ round a proton: (a) speed and energy as functions of $r$ (Coulomb dynamics, [Chapter 16](https://one-course.com/books/physics/3/en/chapter/16-central-forces-planets-and-satellites#ch-b1-central-forces)); (b) impose $m_evr = n\hbar$ and deduce $r_n = n^2a_0$, $E_n = E_1/n^2$ with $a_0$ and $E_1$ as in [Example 30.11](#ex-b1-quantum-introduction-hsize); (c) $v_1$ and $v_1/c$; (d) wavelengths of Lyman $\alpha$ ($2 \to 1$) and of H$\alpha$ ($3 \to 2$); (e) show that the orbit $n$ holds exactly $n$ [de Broglie wavelengths](#thm-b1-quantum-introduction-debroglie).

**Solution of Exercise 30.9.**

(a) $m_ev^2/r = e^2/4\pi\varepsilon_0r^2$: $v = \sqrt{e^2/4\pi\varepsilon_0m_er}$, $E =
\tfrac12m_ev^2 - e^2/4\pi\varepsilon_0r = -e^2/8\pi\varepsilon_0r$. (b) $m_evr = n\hbar$ and $m_ev^2r = e^2/4\pi\varepsilon_0$: divide the square of the first by the second: $m_er = n^2\hbar^2 \cdot 4\pi\varepsilon_0/e^2$, $r_n = n^2a_0$, and $E_n = -e^2/8\pi\varepsilon_0n^2a_0
= E_1/n^2$ with $a_0 = 52.9\,\mathrm{pm}$, $E_1 = -13.6\,\mathrm{eV}$. (c) $v_1 =
\hbar/m_ea_0 = 2.19 \times 10^{6}\,\mathrm{m}/\mathrm{s}$, $v_1/c = 1/137$. (d) $2 \to 1$: $\tfrac34 \times
13.6 = 10.2\,\mathrm{eV}$, $122\,\mathrm{nm}$; $3 \to 2$: $(\tfrac14 - \tfrac19) \times 13.6 =
1.89\,\mathrm{eV}$, $656\,\mathrm{nm}$. (e) $\lambda_n = h/m_ev_n = nh/m_ev_1 = 2\pi na_0$ (since $m_ev_1a_0 = \hbar$), and $2\pi r_n = 2\pi n^2a_0 = n\lambda_n$.

**Exercise 30.10 ★★★.**

*Hydrogen-like systems.* (a) For a nucleus of charge $Ze$ show $E_n = -Z^2 \times 13.6\,\mathrm{eV}/n^2$ and $r_n = n^2a_0/Z$: ionization energy of He$^+$ and of the last electron of uranium ($Z = 92$; comment). (b) Muonic hydrogen: the muon has $207$ times the electron’s mass: radius and ground energy; wavelength of its Lyman $\alpha$ line; why it is used to measure the size of the proton (radius $0.84\,\mathrm{fm}$). (c) Positronium (electron and positron, equal masses): show that the [reduced mass](https://one-course.com/books/physics/3/en/chapter/19-systems-of-points-introduction-to-rigid-bodies#prop-b1-systems-of-points-twobody) halves the energies: its Lyman $\alpha$.

**Solution of Exercise 30.10.**

(a) Replace $e^2$ by $Ze^2$: $a_0 \to a_0/Z$, $E_1 \to Z^2E_1$. He$^+$: $54.4\,\mathrm{eV}$. U$^{91+}$: $92^2 \times 13.6 = 115\,\mathrm{keV}$ — but $v_1 = Z\alpha c
= 0.67c$: the non-relativistic model is only indicative there. (b) $a_0/207
= 256\,\mathrm{fm}$, $E_1 = 207 \times 13.6 = 2.8\,\mathrm{keV}$; Lyman $\alpha$: $2.1\,\mathrm{keV}$, $\lambda = 0.59\,\mathrm{nm}$ (X-rays). The muon’s orbit is only $300$ proton radii: its levels shift measurably with the proton’s size, which is how the proton radius was re-measured (2010). (c) The two particles orbit their common centre: the [reduced mass](https://one-course.com/books/physics/3/en/chapter/19-systems-of-points-introduction-to-rigid-bodies#prop-b1-systems-of-points-twobody) $m_e/2$ halves every energy: $E_1 = -6.8\,\mathrm{eV}$, Lyman $\alpha$ at $5.1\,\mathrm{eV}$, $243\,\mathrm{nm}$.

**Exercise 30.11 ★★★.**

*[Quantum dots](#ex-b1-quantum-introduction-dot).* In a spherical nanocrystal of radius $R$ the confinement energy of a particle of effective mass $m^\ast$ is $h^2/8m^\ast R^2$ (admitted). CdSe: gap $E_g = 1.74\,\mathrm{eV}$, $m_e^\ast =
0.13\,m_e$, $m_h^\ast = 0.45\,m_e$ (the “hole” left by the excited electron also confines). (a) Emitted photon energy $E_g + E_e + E_h$ and wavelength for $R = 2.0\,\mathrm{nm}$, $3.0\,\mathrm{nm}$, $4.0\,\mathrm{nm}$; colours. (b) Radius for emission at $520\,\mathrm{nm}$ (green). (c) Why does bulk CdSe emit at $713\,\mathrm{nm}$ only? (d) A $10\,\%$ spread in radius in a batch: spread in wavelength at $3\,\mathrm{nm}$.

**Solution of Exercise 30.11.**

(a) $h^2/8m_e = 6.02 \times 10^{-38}\,\mathrm{J}\,\mathrm{m}^{2}$. $R = 2\,\mathrm{nm}$: $E_e = 6.02 \times 10^{-38}/
(0.13 \times 4 \times 10^{-18}) = 0.72\,\mathrm{eV}$, $E_h = 0.21\,\mathrm{eV}$, total $1.74 +
0.93 = 2.67\,\mathrm{eV}$, $464\,\mathrm{nm}$: blue. $3\,\mathrm{nm}$: confinement $\times4/9$, $2.15\,\mathrm{eV}$, $577\,\mathrm{nm}$: yellow. $4\,\mathrm{nm}$: $\times1/4$, $1.97\,\mathrm{eV}$, $629\,\mathrm{nm}$: red. (b) $520\,\mathrm{nm}$ is $2.38\,\mathrm{eV}$: confinement $0.65\,\mathrm{eV}$ $= 0.93 \times (2/R)^2$, $R = 2.4\,\mathrm{nm}$. (c) No confinement: $E_g$ alone, $713\,\mathrm{nm}$. (d) $\delta E = -2 \times 0.1 \times 0.41 = -0.08\,\mathrm{eV}$, $4\%$ of $2.15\,\mathrm{eV}$: about $20\,\mathrm{nm}$ of spread — pure colours need monodisperse batches.

**Exercise 30.12 ★★★.**

*Zero-point energy.* (a) For a [harmonic oscillator](https://one-course.com/books/physics/3/en/chapter/14-mechanical-oscillators-damping-and-resonance#def-b1-oscillators-resonance-harmonic) $E = p^2/2m +
\tfrac12m\omega^2x^2$, take $\Delta x\,\Delta p = \hbar/2$ and minimize $E \approx
\Delta p^2/2m + \tfrac12m\omega^2\Delta x^2$ over $\Delta x$: show $E_{\min} = \hbar\omega/2$ (the exact ground energy). (b) The H$_2$ molecule vibrates at $\omega =
8.3 \times 10^{14}\,\mathrm{rad}/\mathrm{s}$: zero-point energy in eV, and the lowest temperature at which its vibration is “thermal” ($k_BT \sim \hbar\omega$). (c) Liquid helium never freezes at atmospheric pressure: estimate the zero-point energy of a helium atom localized to $\Delta x = 0.05\,\mathrm{nm}$ (a fraction of the interatomic distance) in a crystal, and compare with its binding energy in the solid, about $1\,\mathrm{meV}$. (d) Compare the box formula $E_1 = h^2/8mL^2$ with the uncertainty bound for $\Delta x = L/2$: which is larger, and why must it be?

**Solution of Exercise 30.12.**

(a) $E(\Delta x) = \hbar^2/8m\Delta x^2 + \tfrac12m\omega^2\Delta x^2$; zero derivative at $\Delta x^2 = \hbar/2m\omega$, where both terms equal $\hbar\omega/4$: $E_{\min} =
\hbar\omega/2$. (b) $\tfrac12 \times 1.055 \times 10^{-34} \times 8.3 \times 10^{14} = 4.4 \times 10^{-20}\,\mathrm{J}
= 0.27\,\mathrm{eV}$; $T \sim \hbar\omega/k_B = 6300\,\mathrm{K}$ — at room temperature the vibration is frozen in its [ground state](#prop-b1-quantum-introduction-box). (c) $\Delta p = \hbar/2\Delta x =
1.05 \times 10^{-24}\,\mathrm{kg}\,\mathrm{m}/\mathrm{s}$, $E = \Delta p^2/2m_{\mathrm{He}} = 1.1 \times 10^{-48}/1.33 \times
10^{-26} = 8 \times 10^{-23}\,\mathrm{J} = 0.5\,\mathrm{meV}$: half the binding — the atoms cannot sit still enough to crystallize; helium stays liquid down to absolute zero unless squeezed ($25\,\mathrm{bar}$). (d) $E_1 = \pi^2\hbar^2/2mL^2$ against $\hbar^2/2mL^2$: ten times larger, as it must be — the bound is a lower limit, and the box state has $\Delta x \approx 0.18L$, not $L/2$.

![The visible emission spectrum of hydrogen: the Balmer lines at 656\, nm, 486\, nm, 434\, nm and 410\, nm, each a jump down to n = 2.](https://one-course.com/images/onecourse/chapters/physics-3/b1-quantum-introduction/img-ba97c5e0ee08.jpg)

*The visible emission spectrum of hydrogen: the Balmer lines at $656\,\mathrm{nm}$, $486\,\mathrm{nm}$, $434\,\mathrm{nm}$ and $410\,\mathrm{nm}$, each a jump down to $n = 2$.*

![Quantum dots of one material in vials: the smaller the nanocrystal, the larger the confinement energy and the bluer the light — colour chosen by size.](https://one-course.com/images/onecourse/chapters/physics-3/b1-quantum-introduction/img-7f970193e5ad.jpg)

*[Quantum dots](#ex-b1-quantum-introduction-dot) of one material in vials: the smaller the nanocrystal, the larger the confinement energy and the bluer the light — colour chosen by size.*

## 30.6 Problem: The hydrogen spectrum and a quantum dot

**Problem 30.1.**

Weekend problem — measuring $h$ with light and a voltmeter, building the hydrogen atom from three constants, and choosing the colour of a crystal with its size

Constants: $h = 6.626 \times 10^{-34}\,\mathrm{J}\,\mathrm{s}$, $\hbar = 1.055 \times 10^{-34}\,\mathrm{J}\,\mathrm{s}$, $c =
3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s}$, $e = 1.602 \times 10^{-19}\,\mathrm{C}$, $m_e = 9.11 \times 10^{-31}\,\mathrm{kg}$, $1/4\pi\varepsilon_0 = 8.99 \times 10^{9}\,\mathrm{SI}$, $hc = 1240\,\mathrm{eV}\,\mathrm{nm}$.

**Part I — Measuring [Planck’s constant](#thm-b1-quantum-introduction-photon).** A potassium photocathode is lit with monochromatic light; the [stopping potential](#prop-b1-quantum-introduction-photoelectric) is measured: $0.30\,\mathrm{V}$ at $6.0 \times 10^{14}\,\mathrm{Hz}$, $0.69\,\mathrm{V}$ at $7.0 \times 10^{14}\,\mathrm{Hz}$, $1.13\,\mathrm{V}$ at $8.0 \times 10^{14}\,\mathrm{Hz}$, $1.50\,\mathrm{V}$ at $9.0 \times 10^{14}\,\mathrm{Hz}$, $2.36\,\mathrm{V}$ at $1.1 \times 10^{15}\,\mathrm{Hz}$.

1. Describe the cell and explain why a reverse [voltage](https://one-course.com/books/physics/3/en/chapter/6-dc-circuits-kirchhoffs-laws-and-theorems#def-b1-dc-circuits-voltage) can stop the current, and what $eV_s$ measures.
2. Write Einstein’s relation and say what the slope and the intercept of $V_s(\nu)$ give.
3. From the data (a linear fit, or the two extreme points), deduce $h$ ; compare with the accepted value.
4. [Work function](#prop-b1-quantum-introduction-photoelectric) of potassium in eV; threshold frequency and wavelength; could a red laser pointer extract electrons?
5. The lamp’s intensity is doubled: what happens to $V_s$ , to the current? Why is this incompatible with a purely wave picture?
6. Classical estimate: a light of $1\,\text{µ}\mathrm{W}/\mathrm{m}^{2}$ falls on the metal; an atom offers an area of about $1 \times 10^{-20}\,\mathrm{m}^{2}$ : how long would it take to accumulate $2.2\,\mathrm{eV}$ on one atom? What is observed instead?

**Part II — Bohr’s [hydrogen atom](#prop-b1-quantum-introduction-hydrogen).**

7. An electron on a [circular orbit](https://one-course.com/books/physics/3/en/chapter/16-central-forces-planets-and-satellites#prop-b1-central-forces-effective) of radius $r$ round a fixed proton: speed $v(r)$ and [mechanical energy](https://one-course.com/books/physics/3/en/chapter/13-work-energy-and-potential-energy#thm-b1-work-and-energy-em) $E(r)$ .
8. Bohr’s condition $m_evr = n\hbar$ : show $r_n = n^2a_0$ and give $a_0 = 4\pi\varepsilon_0\hbar^2/m_ee^2$ numerically.
9. $E_n = E_1/n^2$ with $E_1 = -m_ee^4/[2(4\pi\varepsilon_0)^2\hbar^2]$ ; numerical value in eV.
10. Speed on the first orbit and the ratio $v_1/c$ (the fine-structure constant $\alpha \approx 1/137$ ).
11. Wavelengths of the lines $2 \to 1$ (Lyman $\alpha$ ), $3 \to 2$ and $4 \to 2$ (Balmer H $\alpha$ , H $\beta$ ): which are visible?
12. Show that $1/\lambda = R_H(1/n^2 - 1/p^2)$ and compute the Rydberg constant $R_H$ ; the shortest Balmer wavelength.
13. Ionization energy of hydrogen from the [ground state](#prop-b1-quantum-introduction-box) ; wavelength of the photon that just ionizes it.
14. De Broglie: show that the circumference of orbit $n$ is $n$ wavelengths — Bohr’s condition is a standing-wave condition.
15. Two things the model gets wrong, one thing it gets exactly right, and what replaces the orbit in the full theory.

**Part III — The [quantum dot](#ex-b1-quantum-introduction-dot).** A CdSe nanocrystal of radius $R$ confines an excited electron (effective mass $m_e^\ast = 0.13\,m_e$) and the hole it leaves ($m_h^\ast = 0.45\,m_e$); the confinement energy of each in a sphere of radius $R$ is $h^2/8m^\ast R^2$ (admitted); the gap of bulk CdSe is $E_g = 1.74\,\mathrm{eV}$.

16. Derive the energies $E_n = n^2h^2/8mL^2$ of a particle in a one-dimensional box from the standing-wave condition, and comment on the analogy with the sphere formula.
17. Confinement energies of the electron and of the hole for $R = 2.0\,\mathrm{nm}$ .
18. Energy and wavelength of the emitted photon for $R = 2.0\,\mathrm{nm}$ , $3.0\,\mathrm{nm}$ and $4.0\,\mathrm{nm}$ ; colours.
19. Explain in one sentence why smaller dots are bluer.
20. Check the [order of magnitude](https://one-course.com/books/physics/3/en/chapter/1-units-dimensions-and-measurement#def-b1-units-dimensions-oom) with the uncertainty principle: $\Delta p \sim \hbar/R$ for the electron at $R = 2\,\mathrm{nm}$ , and the [kinetic energy](https://one-course.com/books/physics/3/en/chapter/13-work-energy-and-potential-energy#thm-b1-work-and-energy-ke) it implies.
21. A dot emits $1.0\,\mathrm{nW}$ at $577\,\mathrm{nm}$ : photons per second.

**Part IV — Counting quanta.**

22. Photons per second from a $1.0\,\mathrm{mW}$ laser at $633\,\mathrm{nm}$ .
23. The dark-adapted [eye](https://one-course.com/books/physics/3/en/chapter/4-optical-instruments-and-the-eye#def-b1-optical-instruments-eye) detects a flash of about $100$ photons at $500\,\mathrm{nm}$ arriving within $0.1\,\mathrm{s}$ : the corresponding power.
24. An FM antenna receives $1.0\,\mathrm{pW}$ at $100\,\mathrm{MHz}$ : photons per second; is there any hope of detecting them one by one?
25. Sum up: from $h$ , $e$ , $m_e$ alone, which three quantities of the atomic world did this problem produce, and with which magnitudes?

**Solution of Problem 30.1.**

**1.** Light frees electrons from the cathode with various energies; held at $-V_s$, the anode repels them and only those with $E_k > eV_s$ arrive. The current vanishes when $eV_s = E_{k,\max}$.

**2.** $eV_s = h\nu - W$: slope $h/e$, intercept $-W/e$; $V_s = 0$ at the threshold $\nu_0 = W/h$.

**3.** Extreme points: $(2.36 - 0.30)/(5.0 \times 10^{14}) = 4.12 \times 10^{-15}\,\mathrm{V}\,\mathrm{s}$, $h = 1.602 \times 10^{-19} \times 4.12 \times 10^{-15} = 6.60 \times 10^{-34}\,\mathrm{J}\,\mathrm{s}$ (a fit on all five gives $6.62$): within $0.5\%$ of $6.626 \times 10^{-34}$.

**4.** $W = h\nu - eV_s = 2.47 - 0.30 = 2.2\,\mathrm{eV}$; $\nu_0 = W/h =
5.3 \times 10^{14}\,\mathrm{Hz}$, $\lambda_0 = 1240/2.2 = 560\,\mathrm{nm}$. A red pointer ($650\,\mathrm{nm}$, $1.9\,\mathrm{eV}$) extracts nothing.

**5.** $V_s$ unchanged, current doubled: twice the photons, each of the same energy. A wave would give each electron more energy with more intensity, and a threshold in intensity rather than in frequency.

**6.** $10^{-6} \times 10^{-20} = 1 \times 10^{-26}\,\mathrm{W}$ on the atom; $2.2\,\mathrm{eV}$ $=
3.5 \times 10^{-19}\,\mathrm{J}$ takes $3.5 \times 10^7$ s — a year. Emission is observed within nanoseconds: the energy arrives in whole quanta.

**7.** $m_ev^2/r = e^2/4\pi\varepsilon_0r^2$: $v = \sqrt{e^2/4\pi\varepsilon_0m_er}$; $E =
\tfrac12m_ev^2 - e^2/4\pi\varepsilon_0r = -e^2/8\pi\varepsilon_0r$.

**8.** $(m_evr)^2 = n^2\hbar^2$ and $m_ev^2r = e^2/4\pi\varepsilon_0$: $r_n = n^2 \cdot
4\pi\varepsilon_0\hbar^2/m_ee^2 = n^2a_0$, $a_0 = (1.055 \times 10^{-34})^2/(8.99 \times 10^9
\times 9.11 \times 10^{-31} \times 2.57 \times 10^{-38}) = 52.9\,\mathrm{pm}$.

**9.** $E_n = -e^2/8\pi\varepsilon_0r_n = -m_ee^4/2(4\pi\varepsilon_0)^2\hbar^2n^2$; $E_1 =
-2.31 \times 10^{-28}/(2 \times 5.29 \times 10^{-11}) = -2.18 \times 10^{-18}\,\mathrm{J} = -13.6\,\mathrm{eV}$.

**10.** $v_1 = \hbar/m_ea_0 = 2.19 \times 10^{6}\,\mathrm{m}/\mathrm{s}$; $v_1/c = 7.3 \times 10^{-3} =
1/137$.

**11.** $2 \to 1$: $10.2\,\mathrm{eV}$, $122\,\mathrm{nm}$ (ultraviolet); $3 \to 2$: $1.89\,\mathrm{eV}$, $656\,\mathrm{nm}$ (red); $4 \to 2$: $2.55\,\mathrm{eV}$, $486\,\mathrm{nm}$ (blue-green): the Balmer lines are the visible ones.

**12.** $hc/\lambda = |E_1|(1/n^2 - 1/p^2)$: $R_H = |E_1|/hc = 13.6/1240 =
1.097 \times 10^{-2}\,\mathrm{nm}^{-1} = 1.097 \times 10^{7}\,\mathrm{m}^{-1}$. Balmer limit ($p \to \infty$): $\lambda = 4/R_H = 365\,\mathrm{nm}$.

**13.** $13.6\,\mathrm{eV}$; $\lambda = 1240/13.6 = 91\,\mathrm{nm}$.

**14.** $v_n = v_1/n$, $\lambda_n = h/m_ev_n = nh/m_ev_1 = 2\pi na_0$ (as $m_ev_1a_0
= \hbar$); $2\pi r_n = 2\pi n^2a_0 = n\lambda_n$: the orbit carries $n$ whole waves — Bohr’s rule is a standing-wave rule.

**15.** Wrong: the electron has no orbit (it would radiate; the [ground state](#prop-b1-quantum-introduction-box) has zero [angular momentum](https://one-course.com/books/physics/3/en/chapter/15-angular-momentum#def-b1-angular-momentum-L)) and the model fails for any atom with two electrons. Right: the hydrogen levels, hence every line of its spectrum. The orbit is replaced by a [wavefunction](#def-b1-quantum-introduction-wavefunction), a probability cloud of size $\sim n^2a_0$.

**16.** [Standing waves](https://one-course.com/books/physics/3/en/chapter/5-signal-propagation-travelling-and-standing-waves#thm-b1-wave-propagation-standing): $L = n\lambda/2$, $p_n = h/\lambda_n = nh/2L$, $E_n =
p_n^2/2m = n^2h^2/8mL^2$. The sphere formula is the same with $L \to R$: the [ground state](#prop-b1-quantum-introduction-box) fits half a wavelength in the radius.

**17.** $E_e = 6.02 \times 10^{-38}/(0.13 \times 4 \times 10^{-18}) = 0.72\,\mathrm{eV}$; $E_h = 0.13/0.45 \times 0.72 = 0.21\,\mathrm{eV}$.

**18.** $R = 2\,\mathrm{nm}$: $1.74 + 0.93 = 2.67\,\mathrm{eV}$, $464\,\mathrm{nm}$, blue; $3\,\mathrm{nm}$: $2.15\,\mathrm{eV}$, $577\,\mathrm{nm}$, yellow; $4\,\mathrm{nm}$: $1.97\,\mathrm{eV}$, $629\,\mathrm{nm}$, red.

**19.** The confinement energy grows as $1/R^2$: a smaller box lifts the levels, the photon is more energetic, the light bluer.

**20.** $\Delta p \sim \hbar/R = 5.3 \times 10^{-26}\,\mathrm{kg}\,\mathrm{m}/\mathrm{s}$, $E \sim \Delta p^2/2m_e^\ast =
1.2 \times 10^{-20}\,\mathrm{J} = 0.07\,\mathrm{eV}$: the right order (the exact coefficient $\pi^2/2$ and the cruder $\Delta p$ account for the factor ten).

**21.** $1240/577 = 2.15\,\mathrm{eV} = 3.4 \times 10^{-19}\,\mathrm{J}$: $10^{-9}/3.4 \times 10^{-19}
= 2.9 \times 10^9$ photons per second.

**22.** $10^{-3}/(1.96 \times 1.6 \times 10^{-19}) = 3.2 \times 10^{15}$ per second.

**23.** $100 \times 2.48 \times 1.6 \times 10^{-19} = 4 \times 10^{-17}\,\mathrm{J}$ in $0.1\,\mathrm{s}$: $4 \times 10^{-16}\,\mathrm{W}$.

**24.** $h\nu = 6.6 \times 10^{-26}\,\mathrm{J}$: $1.5 \times 10^{13}$ photons per second — and each is $10^5$ times smaller than the thermal energy $k_BT$ of the antenna: no hope, and no need; the wave picture is exact there.

**25.** The size of atoms, $a_0 = 53\,\mathrm{pm}$; their energy scale, $13.6\,\mathrm{eV}$ (hence eV photons, chemistry, the visible spectrum); and the speed of their electrons, $\alpha c \approx 2 \times 10^{6}\,\mathrm{m}/\mathrm{s}$ — all three from $h$, $e$ and $m_e$ (and $\varepsilon_0$), with nothing adjusted.