What is Quantum Mechanics? (joke video)

Spinors for Beginners 19: Tensor Product Representations of su(2) [Clebsch-Gordan coefficients]

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Spinors for Beginners 18: Irreducible Representations of SU(2) (Ladder Operators)

Spinors for Beginners 17: The spin 1/2 representations of SU(2) and SL(2,C)

Spinors for Beginners 16: Lie Groups and Lie Algebras

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Spinors for Beginners 15: Nilpotents, Fermions, and Maximally Isotropic Subspaces

Spinors for Beginners 14: Minimal Left Ideals (and Pacwoman Property)

Spinors for Beginners 13: Ideals and Projectors (Idempotents)

Spinors for Beginners 12: How the Spin Group Generalizes Quaternions to any Dimension

Spinors for Beginners 10: SU(2) double covers SO(3) [ SL(2,C) double covers SO+(1,3) ]

Spinors for Beginners 11: What is a Clifford Algebra? (and Geometric, Grassmann, Exterior Algebras)

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Spinors for Beginners 6.1 - Equivalence of Quaternions, Sigma Matrices, and SU(2)

Spinors for Beginners 9: Pauli Spinors vs Weyl Spinors vs Dirac Spinors

What Is Voltage? (joke video)

Spinors for Beginners 8: Are the Pauli Matrices also Vectors? (Intro to Spinor Spaces)

Spinors for Beginners 7: Square Root of a Vector (factoring vector into spinors)

Spinors for Beginners 6: Pauli Vectors and Pauli Matrices

Spinors for Beginners 5: The Flagpole and Complex Projective Line (CP1)

Spinors for Beginners 4: Quantum Spin States (Stern-Gerlach Experiment)

Spinors for Beginners 3: Polarizations and SU(2) Matrices [and O(3), SO(3), U(2)]

Spinors for Beginners 2: Jones Vectors and Light Polarization

Spinors for Beginners 1: Introduction (Overview +Table of Contents for video series)

Tensors for Beginners 1: Forward and Backward Transformations (REMAKE)

Relativity 110d: Cosmology - FLRW Geodesics, Cosmological Redshift, Horizons, Comoving Coordinates

Relativity 110f: Cosmology - Friedmann Equations Derivation + Universe Evolution Models (FINALE)

Relativity 110b: Cosmology - FLRW Metric Derivation (3 possible geometries)

Relativity 108e: Schwarzschild Metric - Gravitational Redshift / Blueshift (via covector fields)