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Unit 16: Quantum and Nuclear Physics

Light behaving like particles, matter behaving like waves, an atom that only glows at a few exact colors, and a nucleus trading mass for energy.

12 topics · 44 questions

Each topic is a path, not a menu: work down it in order and every question builds on the one above. Click any of them to watch the answer draw itself.

Blackbody Radiation

  1. How it worksHow did Planck's assumption that light energy comes in discrete packets finally explain a hot object's whole glow spectrum?
  2. Common mistakeWhy doesn't classical physics, which predicted infinite energy at short wavelengths, actually describe a hot object's real glow?
  3. Ties togetherHow does Planck's quantized light energy set up the very idea Einstein later used to explain the photoelectric effect?
Your turn1 of 2
Classical physics predicted that a hot object should radiate infinite energy at very short wavelengths, the 'ultraviolet catastrophe,' but real hot objects clearly don't. What resolved this contradiction?

The Photoelectric Effect

  1. How it worksHow does treating light as individual photons, each with energy set only by frequency, explain the photoelectric effect completely?
  2. Worked exampleFind the kinetic energy of an electron ejected by an 8 times 10 to the 14 Hz photon from a metal with a 2 eV work function.
  3. Common mistakeWhy isn't a photon's energy determined by how intense or bright the overall light beam happens to be?
  4. Going furtherWhat happens to the number of electrons ejected per second, as opposed to their energy, when the light's intensity is raised?
  5. Worked exampleFind the threshold frequency below which no electrons are ejected from a metal with a work function of 2.3 eV.
Your turn1 of 2
A metal has a work function of 2 eV. Write the kinetic energy of an ejected electron as a function of f, the photon frequency in units of 1014 Hz. Use h = 4.136x10−15 eV s.

The Compton Effect

  1. How it worksHow does treating a photon as a particle with momentum, colliding with an electron like a billiard ball, explain that wavelength shift?
  2. Worked exampleFind the wavelength shift of an X-ray photon scattered at 90 degrees off a free electron.
  3. Ties togetherHow does the Compton effect confirm the very same particle picture of light the photoelectric effect first suggested?
Your turn1 of 2
Find the wavelength shift of an X-ray photon scattered at 121 degrees off a free electron. Use h/(me c) = 2.43x10−12 m.

The Bohr Model of the Hydrogen Atom

  1. How it worksHow did Bohr's model quantize the electron's allowed orbits into discrete energy levels to explain hydrogen's spectral lines?
  2. Worked exampleFind the energy of a photon emitted when a hydrogen electron drops from the n=3 level to the n=2 level.
  3. Common mistakeWhy doesn't a hydrogen electron sitting in an allowed Bohr orbit continuously radiate energy and spiral into the nucleus?
  4. Going furtherWhat happens to the spacing between hydrogen's energy levels as the quantum number n keeps getting larger?
Your turn1 of 2
Find the energy of a photon emitted when a hydrogen electron drops from the n=5 level to the n=2 level.

De Broglie Matter Waves

  1. How it worksHow does de Broglie's hypothesis assign every moving particle a wavelength set by its own momentum?
  2. Worked exampleFind the de Broglie wavelength of an electron moving at 2 times 10 to the 6 m/s.
  3. Going furtherWhat happens to a thrown baseball's de Broglie wavelength compared to an electron's, given its far larger mass?
Your turn1 of 2
Find the de Broglie wavelength of an electron moving at 7 times 106 m/s. Use h = 6.626x10−34 J s and electron mass m = 9.11x10−31 kg.

Wave-Particle Duality

  1. How it worksHow does each individual photon land at a random spot while the pattern accumulated over many photons reveals wave interference?
  2. Worked exampleFind how a double-slit setup's slit separation and screen distance should be chosen to show visibly separated fringes for electrons of a given de Broglie wavelength.
  3. Common mistakeWhy doesn't watching a single photon land on the screen ever look anything like a wave striking that screen?
  4. Ties togetherHow does this single-photon buildup connect de Broglie's matter waves directly back to Young's original light experiment?
Your turn1 of 2
Photons are fired through a double slit one at a time, so far apart that only one photon is ever in the apparatus at once. Over a long exposure, does an interference pattern still build up on the screen?

The Quantum Atom and the Periodic Table

  1. How it worksHow do allowed electron shells and the exclusion principle together build up the periodic table one element at a time?
  2. Common mistakeWhy isn't an atom's electron structure just every electron falling into the single lowest energy state at once?
  3. Going furtherWhat happens to an atom's chemical behavior once its outermost electron shell is completely filled?
Your turn1 of 2
Why can't two electrons inside the same atom ever occupy exactly the same quantum state?

Nuclear Structure and Binding Energy

  1. How it worksHow does a nucleus's missing mass convert, through E equals m c squared, into the binding energy holding it together?
  2. Worked exampleFind the binding energy of a nucleus with a mass defect of 0.03 atomic mass units.
  3. Common mistakeWhy doesn't a stable nucleus fly apart under the mutual electric repulsion between all its own protons?
  4. Going furtherWhat happens to the binding energy per nucleon as you move from light nuclei up toward iron on the periodic table?
Your turn1 of 2
Find the binding energy of a nucleus with a mass defect of 7 times 0.01 atomic mass units. Use 1 amu = 931.5 MeV/c2.

Radioactivity and Decay Modes

  1. How it worksHow do alpha, beta, and gamma decay each change a nucleus's mass and charge in their own distinct way?
  2. Worked exampleFind the resulting element and mass number after a uranium-238 nucleus undergoes alpha decay.
  3. Common mistakeWhy isn't beta decay simply an electron that was already sitting inside the nucleus being ejected outward?
  4. Going furtherWhat happens to a nucleus's identity as it moves through a whole chain of alpha and beta decays in a row?
  5. Worked exampleFind the resulting element and mass number after a carbon-14 nucleus undergoes beta-minus decay.
Your turn1 of 2
A nucleus with mass number 235 and atomic number 90 undergoes alpha decay. Find the atomic number of the resulting nucleus.

Half-Life and the Radioactive Decay Law

  1. How it worksHow does a constant decay probability per atom produce a smooth exponential decline across a whole sample?
  2. Worked exampleFind how much of a 100 gram sample with a 5 year half-life remains after 20 years.
  3. Worked exampleFind the decay constant of an isotope with a half-life of 8 days.
  4. Going furtherWhat happens to a radioactive sample's decay rate as more and more of that sample decays away over time?
Your turn1 of 2
A sample of 142 grams has a half-life of 7 years. Write the amount remaining as a function of t, the elapsed time in years.

Nuclear Fission

  1. How it worksHow does a neutron striking a uranium-235 nucleus split it into two smaller nuclei plus free neutrons that keep the reaction going?
  2. Worked exampleFind the energy released by a fission event with a mass defect of 0.2 atomic mass units.
  3. Ties togetherHow does nuclear fission release energy from the very same binding-energy-per-nucleon curve you'd use to compare element stability?
Your turn1 of 2
Find the energy released by a fission event with a mass defect of 4 times 0.1 atomic mass units. Use 1 amu = 931.5 MeV/c2.

Nuclear Fusion

  1. How it worksHow does fusing light nuclei like hydrogen into helium release energy from the opposite end of the same binding-energy curve fission uses?
  2. Common mistakeWhy does building a working fusion reactor on Earth turn out to be so much harder than sustaining fusion inside the Sun's core?
  3. Ties togetherHow do fission and fusion end up releasing energy from opposite ends of the very same binding-energy-per-nucleon curve?
Your turn1 of 2
The Sun continuously fuses hydrogen into helium in its core, releasing energy for billions of years. Why is building a controlled, net-energy-positive fusion reactor on Earth so much harder than what happens naturally inside the Sun?