Gauge Symmetry Principles
From global to local symmetries: The origin of forces
📺 Video Lectures
For comprehensive video lectures on gauge symmetry and gauge theories, see:
- • Susskind's Theoretical Minimum:Lectures 5-6 on Gauge Fields and Symmetry
Excellent intuitive explanation of gauge principle
- • Tobias Osborne QFT 2016:YouTube Playlist (18 lectures)
Covers both Abelian and non-Abelian gauge theories
- • David Tong QFT Lectures:Perimeter Institute (PIRSA)
Lecture notes available at www.damtp.cam.ac.uk/user/tong/qft.html
The Gauge Principle
The gauge principle is one of the most profound ideas in modern physics: forces arise from demanding that local symmetries be preserved.
This remarkable statement means that the electromagnetic, weak, and strong forces are not independent phenomena, but rather necessary consequences of requiring that the laws of physics remain invariant under local phase transformations.
Central Insight
Global symmetry + locality requirement → gauge fields (force carriers) must exist
1. Global vs Local Symmetries
Global U(1) Symmetry
Consider a complex scalar field with Lagrangian:
ℒ = (∂μφ)†(∂μφ) - m²φ†φThis is invariant under global U(1) transformation:
φ(x) → eiα φ(x)where α is a constant (same everywhere in spacetime). This symmetry leads to charge conservation via Noether's theorem.
Local U(1) Symmetry (Gauge Symmetry)
Now demand invariance under local transformations:
φ(x) → eiα(x) φ(x)Problem: The derivative term is NOT invariant:
∂μφ → eiα(x)(∂μφ + iφ ∂μα)The extra term iφ ∂μα breaks the symmetry!
The Solution: Introduce a Gauge Field
Key idea: Replace the ordinary derivative with a covariant derivative:
Dμ = ∂μ + ieAμ(x)where Aμ(x) is a new gauge field that transforms as:
Aμ(x) → Aμ(x) - (1/e) ∂μα(x)Then the covariant derivative transforms as:
Dμφ → eiα(x) DμφThe gauge field Aμ exactly cancels the unwanted term, restoring gauge invariance!
2. Physical Interpretation
What is the gauge field Aμ?
For U(1) gauge symmetry, Aμ is the photon field (electromagnetic potential).
The transformation Aμ → Aμ - ∂μΛ is exactly the familiar gauge transformation of electromagnetism.
The parameter e in the covariant derivative is the electric charge (e² = 4πα ≈ 1/137 in natural units).
The replacement ∂μ → Dμ = ∂μ + ieAμ is called minimal coupling - the simplest way to couple matter to gauge fields.
Profound Realization
The electromagnetic force is not an independent entity added to quantum mechanics. Rather, it is forced into existence by demanding local U(1) symmetry. The photon exists because we require gauge invariance!
3. The Gauge-Invariant Lagrangian
The complete gauge-invariant Lagrangian for a charged scalar field:
ℒ = (Dμφ)†(Dμφ) - m²φ†φ - (1/4)FμνFμνwhere the field strength tensor is:
Fμν = ∂μAν - ∂νAμThree pieces:
- 1. Matter kinetic term: (Dμφ)†(Dμφ)
Contains φ propagation + interaction with Aμ - 2. Mass term: -m²φ†φ
Mass of the charged scalar field - 3. Gauge field kinetic term: -(1/4)FμνFμν
Free propagation of the photon field (Maxwell's equations)
Key Property: Gauge Invariance
Under the transformations:
- • φ(x) → eiα(x) φ(x)
- • Aμ(x) → Aμ(x) - (1/e) ∂μα(x)
The entire Lagrangian ℒ remains unchanged. Fμν is automatically gauge-invariant because it involves differences of derivatives.
4. Equations of Motion
For the scalar field φ:
DμDμφ + m²φ = 0The gauge-covariant Klein-Gordon equation.
For the gauge field Aμ:
∂μFμν = jνwhere the current is:
jμ = ie[(Dμφ)†φ - φ†(Dμφ)]This is Maxwell's equation ∂μFμν = jν with source jμ. Gauge invariance automatically ensures current conservation: ∂μjμ = 0.
5. Why Gauge Symmetry Matters
🔒 Ensures Consistency
Gauge symmetry prevents unphysical longitudinal photon modes. Only 2 transverse polarizations propagate, as required by massless spin-1 particles.
⚖️ Current Conservation
Gauge invariance implies (via Noether) that electric charge is conserved. ∂μjμ = 0 follows automatically from the gauge structure.
🎯 Unification
The same principle (local gauge symmetry) explains electromagnetism, weak force, and strong force under different gauge groups: U(1), SU(2), SU(3).
🧮 Renormalizability
Gauge symmetry constrains the theory so severely that it becomes renormalizable, making quantum corrections calculable to arbitrary precision.
6. Preview: Non-Abelian Gauge Theory
U(1) gauge theory (electromagnetism) is Abelian: transformations commute. The real power of gauge theory emerges with non-Abelian groups like SU(2) and SU(3).
Key differences:
- • Multiple gauge fields:SU(2) has 3 gauge bosons (W¹, W², W³), SU(3) has 8 gluons
- • Non-commuting transformations:Gauge transformations don't commute: [Ta, Tb] = ifabcTc
- • Self-interactions:Gauge bosons carry "charge" and interact with each other (gluons interact with gluons!)
- • Asymptotic freedom:Coupling becomes weaker at high energies (QCD)
We'll develop non-Abelian gauge theory systematically in Chapter 3.
Summary
- ✓ Global symmetry φ → eiαφ leads to conserved charge (Noether)
- ✓ Local symmetry φ → eiα(x)φ requires introducing gauge field Aμ
- ✓ Covariant derivative Dμ = ∂μ + ieAμ transforms covariantly
- ✓ Field strength Fμν = ∂μAν - ∂νAμ is gauge-invariant
- ✓ Minimal coupling ∂μ → Dμ generates electromagnetic interactions
- ✓ Gauge invariance ensures current conservation and renormalizability
- ✓ This principle extends to SU(2)×U(1) (electroweak) and SU(3) (strong force)
Further Resources
- • Peskin & Schroeder - Section 15.1 (The Abelian Gauge Theory)
- • Srednicki - Chapters 54-56 (Gauge Symmetry)
- • Zee - Part III (Chapters III.1-III.3)
- • 't Hooft - "Gauge Theories of the Forces Between Elementary Particles" (Scientific American, 1980)