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Chapter 08

Identical particles and many-body basics

How exchange symmetry holds up the periodic table, metals and white dwarfs.

Sections
7
Finalised
7/7
Simulations
0
Estimated time
3 hours
  1. 8.1The identity principleClassical particles can be labelled; quantum particles cannot. Out of this innocent-looking difference grow the Pauli exclusion principle, the periodic table, and the pressure that holds up a white dwarf — this section digs out the root.
  2. 8.2Bosons and fermionsWho goes symmetric and who antisymmetric? Nature's answer has no exceptions: integer spin is symmetric (bosons), half-integer spin antisymmetric (fermions). This section constructs both kinds of wavefunction, introduces the Slater determinant, and states the spin–statistics theorem behind it all.
  3. 8.3The Pauli exclusion principleTwo fermions cannot occupy the same quantum state. It is not a repulsive force but a direct corollary of antisymmetry — yet it is enough to draw the periodic table, give atoms their volume, and hold a white dwarf up against gravity.
  4. 8.4The exchange interaction and its mark on spectraHelium's Hamiltonian contains no spin, yet its levels split into two ladders by spin. Exchange symmetry locks the Coulomb energy to the spin orientation, manufacturing an energy difference that "looks like a force but isn't" — and it unlocks the helium-spectrum puzzle and the ferromagnetism puzzle in one stroke.
  5. 8.5A first look at second quantizationThe term count of an antisymmetrized wavefunction explodes as N!, yet the information in it is just "how many particles in each state". The occupation-number representation compresses the determinant to one line, and creation and annihilation operators turn symmetry into algebra — the doorway to many-body physics and quantum field theory.
  6. 8.6The Hartree-Fock ideaWhen the 3N-dimensional Schrödinger equation won't budge, let each electron move alone in the "mean field" of the others — then let field and orbitals feed each other, iterating to self-consistency. Hartree–Fock is the many-body problem's first computable answer, and the foundation of quantum chemistry.
  7. 8.7Reduced density matrices and first steps in entanglementThe whole can be pure while a part is mixed — the partial trace turns that sentence into a computable operation. The reduced density matrix keeps the books on "how much the subsystem knows", and entanglement entropy puts a scale on entanglement for the first time.