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10 videos · 3 h 33 min
Lecture · YouTube
Physics Explained
A long, mathematically honest lecture: it builds two-particle wavefunctions in a box, separates fermions from bosons, derives the exclusion principle, and then calculates the quantum pressure that makes solids resist compression. Ideal after the lesson, when you want the reasoning behind sections 2 and 6.
Explainer · YouTube
PBS Space Time
Matt O'Dowd connects the spin you met in chapter 17 to the fact that all electrons are identical, and shows why that combination keeps you from falling through your chair. A good bridge into next chapter's bosons and fermions.
Explainer · YouTube
Sixty Symbols
Brian Cox ruffled feathers with a TV lecture that touched on the Pauli exclusion principle, and two of the channel's scientists weigh in. Use it to test section 1's fine print: 'the same quantum state' means the complete state, spatial wavefunction and spin together, so ask how far the rule really reaches between electrons in different atoms.
Explainer · YouTube
Parth G
Parth G sets out the basic mathematics behind why electrons are arranged in shells, with the exclusion principle doing the work: the seat-counting at the heart of section 2. As he counts, check his numbers against 2 × (2l + 1) electrons per subshell and 2n² per shell.
Lecture · YouTube
Nicola Spaldin
A lecture by ETH Zürich materials theorist Nicola Spaldin, posted on her own channel rather than a university one: an introduction to the quantum-mechanical exchange interaction using the first excited state of helium, where the two electrons' spins can be parallel or opposite. It is the machinery behind Hund's rule in section 4; keep the section's caveat in mind that in real atoms much of the gain comes from reduced screening.
Explainer · YouTube
The Science Asylum
Nick Lucid shows how the different sections of the periodic table are governed by electron orbitals and quantum spin, in about seven minutes. A quick visual check of section 5's claim that the table's blocks and row lengths are exclusion bookkeeping.
Interview · YouTube
Web of Stories - Life Stories of Remarkable People
Freeman Dyson, in his own words, tells a story from the work on the stability of matter, the result from section 6 that showed exclusion is what keeps ordinary matter from collapsing. The next clip in his series (107/157) continues with Lieb and Thirring cleaning up his proof.
Explainer · YouTube
The Science Asylum
Nick Lucid on white dwarfs as degenerate matter, packed so tightly that there is no room left for atoms. A friendly run-up to section 7's Earth-sized star holding about a Sun's mass, before the Chandrasekhar derivation.
Explainer · YouTube
Physics Explained
A simplified, step-by-step derivation of the Chandrasekhar limit for white dwarfs, close to fifty minutes long. Work it alongside worked example 3: the limit exists only because the fastest electrons turn relativistic, so look for the point where that assumption enters.
Lecture · MIT
MIT OpenCourseWare · Barton Zwiebach
A 20-minute MIT 8.06 segment in which Barton Zwiebach introduces identical particles and the exchange degeneracy they create: when particles cannot be told apart, a two-particle state has no unique label. It is rigorous background to section 2's minus-sign callout; later segments of the same course (L23.4 on symmetric and antisymmetric states of N particles, then the symmetrization postulate) resolve the ambiguity, which chapter 19 takes up.