Condensed Matter Physics
Condensed matter physics asks what happens when you bring 10²³ atoms together and let them settle. The answer is almost never the sum of the parts — order, rigidity, conduction, and magnetism are collective properties that no single atom possesses.
The starting point is structure. Most solids are crystals — atoms arranged on a periodic lattice — and that periodicity is the single fact from which nearly everything else follows. Choose a unit cell and a basis, and the reciprocal lattice hands you the natural language for waves inside the solid.
Periodicity reshapes the electrons. In a periodic potential the allowed energies collect into bands separated by gaps, and where the last electrons land — mid-band or at a band edge — decides whether a material is a metal, an insulator, or a semiconductor.
The lattice itself is never still. Its atoms vibrate in collective normal modes, and quantizing those modes gives phonons — the particle-like carriers of sound and heat that also scatter electrons and set a metal's resistance.
Before bands, the crudest model already carries a metal a long way: treat the conduction electrons as a free gas. Pauli exclusion stacks them into momentum space up to the Fermi energy, and the heat capacity, magnetism, and transport of a metal all trace back to what happens at that surface.
From this foundation the subject fans out: semiconductors and the doped junctions that make devices, dielectrics and ferroelectrics, and the several distinct origins of magnetism in solids.
The dramatic finale is superconductivity — below a critical temperature, electrons bind into Cooper pairs, resistance vanishes, and the material expels magnetic flux entirely, a purely quantum effect made visible at human scale.
Throughout, one move recurs: find the symmetry, count the states, and let the collective behavior emerge. The course follows Kittel, Ashcroft & Mermin, and Simon, ending in the low-dimensional physics of nanostructures and graphene.