
Explore finite matrix representations of angular momentum in a fixed j subspace; J^2 = j(j+1) hbar^2 and Jz are diagonal, while Jx and Jy come from J±.
We derive the non relativistic limit of Dirac equation for hydrogen, yielding a Schrödinger-like equation with kinetic energy corrections, including spin-orbit coupling, Thomas precession, and the Darwin term.
Derive the Dirac equation solutions for a free particle at rest, revealing positive and negative energy spinors and spin up/down states along a quantization axis.
Derive the Dirac Hamiltonian from the equation, identify the momentum pi, and demonstrate that the Hamiltonian commutes with total angular momentum Jz by showing that [H, Lz] and [H, Sz] cancel.
Show that the commutator [K, J] vanishes, with J as the total angular momentum and Kay as its spin component, using gamma matrices and sigma operators.
Apply the Dirac equation to hydrogen with an electromagnetic field, recasting it into a Hamiltonian form and relating energy to V(r), p, and sigma matrices.
Recast the Dirac equation for hydrogen part 4 using the K operator to separate angular and radial parts and derive two coupled radial equations for g and f.
Postulate forms for F and G in the Dirac equation for hydrogen, derive recurrence relations and a determinant condition to fix allowed solutions, and select the positive s solution.
Derive the relativistic energy spectrum for hydrogen-like atoms by enforcing a terminating Dirac equation series and applying recursion relations. This yields the exact relativistic energy expression for hydrogen-like atoms.
Derive the relativistic hydrogen energy spectrum from quantum numbers of the four commuting operators and the radial equation, then recover the non relativistic limit for small Z alpha.
Explore how Rutherford's experiments sparked the shift from planetary atom models to quantum mechanics, introducing Bohr's hydrogen-like energy levels and the Schrödinger equation for a step-by-step derivation.
Describe a hydrogen-like two-particle system with electron and proton, deriving a Hamiltonian with reduced mass mu and a Coulomb-like potential V(r) = - Z e^2 / a_h.
Analyze the radial Schrödinger equation via separation of variables, relate chi(r)=e^{-r/2} q(r), and study large‑r behavior to obtain a differential equation for q and the discrete energy spectrum.
Explore the Rodrigues formula for Legendre polynomials, prove P_l(1)=1, and derive the Legendre differential equation through induction and derivative operators.
Analyze the generalized Legendre polynomials P_ml, their Rodrigo's formula, derivative relations, and the m to −m symmetry, within the differential equation with 1−x^2 terms and large-x behavior.
Show how generalized Legendre polynomials are orthogonal on [-1,1], deriving the normalization constant h_{m l} and delta_{l l'} via Rodrigo's formula and integration by parts.
Prove the addition theorem for spherical harmonics by expanding the delta distribution, using completeness, Legendre polynomials, and the angle gamma between Ω and Ω′ to relate Ω and Ω′.
This is a course on Relativistic Quantum Mechanics. Why did I create this new course even if there is already a course on Quantum Mechanics and Quantum Field Theory? The answer is simple: the main reason is that I am passionate about these topics, but another reason is the fact that my previous course on QM and QFT already contained roughly 40 hours of content, so it would have been too "chaotic" if I added another 10 hours of content.
Besides, this course is developed on its own (even if we do not start from scratch). In fact, the topics covered here are not covered in the other course. Here we start from some commutation relations regarding angular momentum, from which we derive the concept of spin. It is therefore recommended to have a prerequisite knowledge of operators and commutators, and how the latter are related to the possibility of measuring two physical quantities simultaneously.
After a first part on angular momentum (in particular, intrinsic angular momentum), we use the concepts therein developed to construct the Dirac equation. We will see that the concept of spin is naturally incorporated into the relativistic theory.
Once we have the Dirac equation, we will start solving it in the case of a free particle, and we also derive conserved quantities from it (the Hamiltonian, current, etc.).
From other commutation relations that we derive, we finally find the spectrum of the hydrogen atom in the relativistic case, and compare it with the non-relativistic solution.