Ultraviolet Divergences
When loop integrals blow up at high momentum
πCourse Connections
1.1 The Problem: Infinite Quantum Corrections
In Part IV, we calculated radiative corrections in QED and encountered a disturbing phenomenon:loop diagrams produce infinite integrals. Consider the simplest one-loop correction to the photon propagator (vacuum polarization):
Vacuum Polarization Diagram:
~~~~~~~>~~~~~~~
| |
eβ» eβΊ
| |
<~~~~~~Ξ³~~~~~~~>
Virtual electron-positron loop contributes to photon self-energy
The amplitude involves an integral over the loop momentum k:
At large momentum k β β, the numerator behaves like kΒ² while the denominator goes like kβ΄, giving:
The integral diverges logarithmically as we take the cutoff Ξ β β!
π‘Why do we integrate to infinity?
In quantum field theory, virtual particles can have any momentum k, no matter how large. The integral β«dβ΄k sums over all possible virtual particle configurations.
High momentum k corresponds to short distances Ξx ~ 1/k. Ultraviolet (UV) divergences signal our ignorance of physics at arbitrarily short distances - perhaps new physics appears at some scale!
1.2 Degree of Divergence: Power Counting
How badly does a Feynman diagram diverge? The superficial degree of divergence D tells us. For a diagram with:
- L = number of loops
- I_B = number of internal boson lines
- I_F = number of internal fermion lines
- E_B = number of external boson lines
- E_F = number of external fermion lines
- V = number of vertices
In d spacetime dimensions, the degree of divergence is:
For d = 4 dimensions, using topological relations between loops, vertices, and propagators:
Interpretation of D:
- D > 0: Superficially divergent (power-law divergence: Ξ^D)
- D = 0: Logarithmically divergent (~ ln Ξ)
- D < 0: Superficially convergent
1.3 Examples in Οβ΄ Theory
Consider scalar Οβ΄ theory with interaction β_int = (Ξ»/4!)Οβ΄. Let's analyze key diagrams:
(a) Vacuum Bubble
E_B = 0 external lines
(b) Tadpole (1-point function)
E_B = 1 external line
(c) Self-Energy (2-point function)
E_B = 2 external lines
(d) Vertex Correction (4-point function)
E_B = 4 external lines
(e) Higher-Point Functions (n β₯ 6)
E_B β₯ 6 external lines
Key Observation:
In Οβ΄ theory, only a finite number of diagram types are superficially divergent (vacuum, tadpole, 2-point, 4-point). This makes the theory renormalizable - we only need a finite number of counterterms!
1.4 Divergences in QED
In QED, we have both photons (spin-1) and electrons (spin-1/2). The three key divergent diagrams are:
1. Photon Self-Energy (Vacuum Polarization)
Virtual eβΊeβ» pairs modify the photon propagator. Degree of divergence:
Actually only logarithmically divergent due to gauge invariance (Ward identity constrains the form).
2. Electron Self-Energy
Virtual photon emission/absorption modifies the electron propagator:
Superficially convergent, but contains logarithmic subdivergences!
3. Vertex Correction
Virtual photon exchange corrects the Ξ³-e-e vertex:
Logarithmically divergent. This correction gives the anomalous magnetic moment of the electron!
1.5 Subdivergences and Overlapping Divergences
Power counting only identifies superficial divergences. A diagram with D < 0 can still diverge if it contains divergent subdiagrams!
Example: Two-Loop Self-Energy
Consider a two-loop scalar propagator correction. The overall diagram has D < 0, but the internal one-loop subdiagrams have D = 2 (quadratically divergent).
These subdivergences must be handled systematically using the BPHZ renormalization prescription (Bogoliubov-Parasiuk-Hepp-Zimmermann).
1.6 Renormalizability
A theory is renormalizable if only a finite number of coupling constants need counterterms (to all orders in perturbation theory).
Classification by Mass Dimension:
In d = 4 dimensions, operators have mass dimension [πͺ]. The coupling constant g in gπͺ has dimension [g] = 4 - [πͺ]:
- [g] > 0: Super-renormalizable (e.g., ΟΒ³ in d=6)
- [g] = 0: Renormalizable (e.g., Οβ΄, QED, QCD, Yang-Mills)
- [g] < 0: Non-renormalizable (e.g., Fermi theory, General Relativity)
Standard Model is Renormalizable!
The entire Standard Model (QED + weak + QCD) is renormalizable. This is why it's so successful: a finite number of measurements (e, m_e, m_ΞΌ, Ξ±_s, etc.) determines infinitely many predictions.
1.7 Types of Divergences
UV (Ultraviolet)
- β’ From high momentum k β β
- β’ Short distance Ξx β 0
- β’ Fixed by renormalization
- β’ Examples: All loop diagrams
IR (Infrared)
- β’ From low momentum k β 0
- β’ Long distance Ξx β β
- β’ From massless particles (photons)
- β’ Resolved by Bloch-Nordsieck theorem
In this course, we focus on UV divergences and renormalization. IR divergences are handled separately (soft photon resummation, jets in QCD, etc.).
π― Key Takeaways
- Loop integrals in QFT often diverge at high momentum (UV divergences)
- Superficial degree of divergence: D = 4 - E_B - (3/2)E_F in d = 4
- D > 0: power divergence; D = 0: log divergence; D < 0: convergent
- Renormalizable theories: finite # of divergent diagram types
- Οβ΄, QED, QCD are renormalizable; Fermi theory is not
- Subdivergences require careful treatment (BPHZ prescription)
- UV divergences signal our ignorance of short-distance physics
- Next: How to regulate these infinities and make sense of them!