The Dirac Field
Relativistic quantum theory of spin-1/2 particles
Video Lecture
Lecture 13: Introducing the Dirac Equation - MIT 8.323
Classical Dirac field theory and spinor structure (MIT QFT Course)
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Video Lecture
What is the Dirac Equation β Dirac Equation Explained
Accessible overview of the Dirac equation in relativistic quantum mechanics
π‘ Tip: Watch at 1.25x or 1.5x speed for efficient learning. Use YouTube's subtitle feature if available.
π Related Topics
- β’ Lagrangian Formalism Page 7 - Original location of this content
- β’ Dirac Quantization (Part II) - Quantization with anticommutators
- β’ Spin 1/2 (QM) - Prerequisite spinor concepts
5.1 The Dirac Equation
To describe spin-1/2 particles (electrons, quarks, neutrinos), we need a spinor field Ο(x). The Dirac field is a 4-component complex object:
The Dirac Lagrangian is:
where:
- $\bar{\psi} = \psi^\dagger \gamma^0$ is the Dirac adjoint
- Ξ³ΞΌ are the Dirac gamma matrices (4Γ4 matrices)
- m is the fermion mass
- We use natural units with β = c = 1
Gamma Matrices
The gamma matrices satisfy the Clifford algebra:
where { , } denotes the anticommutator. In the Dirac (standard) representation:
where Οi are the Pauli matrices.
5.2 Deriving the Dirac Equation
Treating Ο and $\bar{\psi}$ as independent fields, the Euler-Lagrange equation for $\bar{\psi}$ gives:
This is the Dirac equation. Multiplying by (iΞ³Ξ½βΞ½ + m):
Using the Clifford algebra:
Therefore each component satisfies the Klein-Gordon equation:
But the Dirac equation is first-order in time, unlike Klein-Gordon. This allows for a positive-definite probability density.
5.3 Dirac Adjoint and Conserved Current
Varying with respect to Ο gives the adjoint Dirac equation:
or equivalently:
Probability Current
Multiplying the Dirac equation by $\bar{\psi}$ from the left and the adjoint equation by Ο from the right, then adding:
Therefore the Dirac current:
is conserved: βΞΌjΞΌ = 0. The time component:
is positive definite, solving the negative probability problem of the Klein-Gordon equation!
5.4 Global U(1) Symmetry
The Dirac Lagrangian is invariant under the global phase transformation:
where Ξ± is a constant. This U(1) symmetry leads to the conserved current jΞΌ = $\bar{\psi}\gamma^\mu \psi$ by Noether's theorem.
The conserved charge:
is the total fermion number (electric charge for electrons).
Lorentz Invariance
Under a Lorentz transformation Ξ, the Dirac field transforms as:
where S(Ξ) is a 4Γ4 matrix representation of the Lorentz group satisfying:
This ensures the Dirac Lagrangian is Lorentz invariant. Spinors transform under the (1/2, 0) β (0, 1/2) representation of the Lorentz group.
5.5 Energy-Momentum Tensor for Dirac Field
The canonical energy-momentum tensor is:
For the Dirac Lagrangian:
Therefore:
This is not symmetric. The symmetric (Belinfante) tensor is:
where $\overleftrightarrow{\partial}^\nu = \overrightarrow{\partial}^\nu - \overleftarrow{\partial}^\nu$.
Hamiltonian
The Hamiltonian density is:
Using the Dirac equation, this can be rewritten as:
The energy density is:
Total energy:
π― Key Concepts: The Dirac Field
- β’ Dirac Lagrangian: $\mathcal{L} = \bar{\psi}(i\gamma^\mu \partial_\mu - m)\psi$
- β’ Dirac equation: (iΞ³ΞΌβΞΌ - m)Ο = 0 (first-order in time)
- β’ Clifford algebra: {Ξ³ΞΌ, Ξ³Ξ½} = 2gΞΌΞ½
- β’ Conserved current: jΞΌ = $\bar{\psi}\gamma^\mu \psi$
- β’ Positive probability: Ο = Οβ Ο β₯ 0 (solves Klein-Gordon problem)
- β’ U(1) symmetry: Global phase invariance β charge conservation
- β’ Spinor representation: (1/2, 0) β (0, 1/2) of Lorentz group
- β’ Energy-momentum tensor: TΞΌΞ½ = i ΟΜΞ³ΞΌβΞ½Ο (not symmetric)
π What's Next?
Now that you understand the classical Dirac field, you're ready for:
- β’ Part II: Dirac Quantization - Anticommutators and fermion creation operators
- β’ Spin-Statistics Theorem - Why fermions need anticommutators
- β’ Energy-Momentum Tensor Chapter - General theory and other field examples
Runnable Simulations
Dirac Gamma Matrix Algebra Verification
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Dirac Equation Energy-Momentum Relation
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