Plain-text extraction hides a useful ambiguity: g2 may denote g2(μ), the square of a generic Yang–Mills coupling, or g2(μ), the Standard Model coupling carrying an SU(2)L label. Both readings will be developed here, beginning with the general theory and ending with the weak coupling

μdg2dμ=−196g2316π2+O(g25).

The coefficient 19/6 combines the SU(2)L gauge-and-ghost sector, three generations of left-handed quark and lepton doublets, and one complex Higgs doublet. Changing that content changes the coefficient. Crossing a mass threshold changes it again.

At one loop, the ultraviolet divergence maps a gauge group and its charged field content to a definite beta-function coefficient.

Part I. The one-loop calculation

1. Why the coupling appears to move

Consider a compact simple gauge group G, with Hermitian generators Ta. It is convenient to place the coupling in front of the Yang–Mills action:

SYM=12g02∫d4xtrFμνFμν,

where

Fμν=∂μAν−∂νAμ−i[Aμ,Aν].

In this convention Aμ contains no explicit g0. Rescale the field as

Aμ=g0Aμ.

Then

Fμν=g0(∂μAν−∂νAμ−ig0[Aμ,Aν]),

and the action has a canonically normalized quadratic term, a cubic vertex proportional to g0, and a quartic vertex proportional to g02. A diagram with one additional loop carries an additional factor of g02/(16π2), apart from group factors and logarithms. This is why g2, rather than g, is the natural loop-counting parameter.

Classically, g0 is a number written in the action. Quantum mechanically, loop integrals sample arbitrarily large momenta. A regulator introduces a scale, and the counterterm used to remove the regulator depends on the scale at which the renormalized coupling is defined. The bare parameter remains fixed while the renormalized parameter changes:

g0=μϵZg(g,ϵ)g(μ),d=4−2ϵ.

The beta function is the response required to keep g0 fixed:

β(g)≡μdgdμ|g0.

No physical law says that an observable changes because we renamed an arbitrary subtraction scale. A scattering amplitude depends on external momenta and masses. Its explicit logarithms of p/μ cancel the implicit μ dependence of g(μ) order by order. The renormalization group arranges that cancellation and resums large logarithms.

For an n-point renormalized Green function, the statement takes the Callan–Symanzik form

[μ∂∂μ+β(g)∂∂g+nγ(g)]Γ(n)=0,

where γ is the field anomalous dimension. Only the combination of g(μ) with the explicit momentum logarithms in an observable is independent of μ.

2. What one loop has to calculate

At one loop, the gauge coupling is determined by the ultraviolet divergence multiplying the gauge-invariant operator

12trFμνFμν.

One can compute several vertex and propagator counterterms and use Slavnov–Taylor identities to combine them. The background-field method is cleaner for our purpose because it keeps gauge invariance under transformations of a slowly varying background field manifest.

Split the gauge potential into a background and a fluctuation,

Aμ=A¯μ+aμ,

and define the background covariant derivative

D¯μX=∂μX−i[A¯μ,X].

The background is held fixed and supplies the external legs; the path integral is performed over the quantum fluctuation aμ. Choose the background-covariant gauge

D¯μaμ=0.

After adding the gauge-fixing term, the quadratic Euclidean action has the schematic form

S(2)=12g02∫ddxaμ(Δ1)μνaν+1g02∫ddxc¯Δ0c,

with

(Δ1)μν=−D¯2δμν−2ad(F¯μν),Δ0=−D¯2.

Factors of i in the spin term depend on whether the generators and Euclidean continuation are defined with Hermitian or anti-Hermitian conventions. The coefficient extracted from the final gauge-invariant divergence does not depend on that choice.

The one-loop effective action is therefore

Γ(1)[A¯]=12Trln⁡Δ1−Trln⁡Δ0.

The factor 1/2 belongs to a Gaussian integral over a real vector field. The minus sign belongs to the Grassmann ghost determinant. The trace runs over momentum, Lorentz, and adjoint group indices.

2.1 The two pieces inside the vector operator

The term −D¯2δμν treats each Lorentz component like a covariant scalar. The second term couples the spin-one fluctuation directly to the background curvature. In a heat-kernel calculation these two structures generate contributions with opposite signs. Tong describes them as diamagnetic and paramagnetic pieces. The terminology gives useful intuition, provided it is not pushed too far.

The division of the answer among gauge-field diagrams, ghost diagrams, and individual polarizations depends on the gauge-fixing choice. The sum does not. What survives every correct calculation is

b0pure YM=113CA,

where CA=C2(G) is the adjoint quadratic Casimir.

Equivalently, minimal subtraction gives

Zg=1−1ϵ11CA6g216π2+O(g4).

Differentiating g0=μϵZgg while holding g0 fixed yields

β(g)=−11CA3g316π2+O(g5).

The negative sign gives asymptotic freedom: the coupling decreases as the energy scale increases. Gross and Wilczek, and independently Politzer, established this behavior in 1973; their original papers are Phys. Rev. Lett. 30, 1343 and Phys. Rev. Lett. 30, 1346.

3. Adding matter

Matter fields screen gauge charge. The calculation again reduces to functional determinants.

A massless complex scalar in a representation Rs contributes

Γs(1)=Trln⁡(−D2).

A Dirac fermion in a representation Rf gives

Γf(1)=−ln⁡det(iγμDμ).

Squaring the Dirac operator exposes its coupling to the field strength:

(iγμDμ)2=−D2−i4[γμ,γν]Fμν.

The spin term changes the coefficient relative to a collection of scalar components. The Grassmann determinant supplies the overall fermion sign. After the traces are evaluated, the general one-loop result is

b0=113CA−23∑Weyl fT(Rf)−13∑complex sT(Rs)

and

β(g)=−b016π2g3+O(g5).

The same formula can be written with Dirac fermions and real scalars:

b0=113CA−43∑Dirac fT(Rf)−16∑real sT(Rs).

One Dirac fermion equals two Weyl fermions. One complex scalar equals two real scalars. Mixing the counting conventions is a common source of factors of two.

Some particle-physics references define coefficients ba by

μdgadμ=ba16π2ga3.

In that convention

ba=−b0,a.

Thus “b2=−19/6” and “b0,2=19/6” are the same claim. Any numerical beta coefficient should be accompanied by its defining equation.

4. The group theory carried by a loop

Let TRa denote the generator in a representation R. We define the Dynkin index and the quadratic Casimir by

trR(TRaTRb)=T(R)δab,

and

TRaTRa=C2(R)1R.

Taking a trace of the second equation gives

d(R)C2(R)=d(G)T(R).

For SU(N) in the usual particle-physics normalization,

T(N)=12,CF=N2−12N,CA=N.

For an SU(2) representation with isospin j,

d(j)=2j+1,C2(j)=j(j+1),

and hence

T(j)=13j(j+1)(2j+1)=d(j)[d(j)2−1]12.

This gives

T(2)=12,T(3)=2,T(4)=5.

For a product representation Ra⊗Rb, a loop coupled to group factor Ga contains a copy for every state in Rb:

Ta(Ra⊗Rb)=Ta(Ra)d(Rb).

This is why a weak quark doublet carries a color multiplicity of three. One must not multiply once more by the two weak components. Their trace is already contained in T(2)=1/2.

The general formula and its higher-loop extension are organized systematically in Machacek and Vaughn, Nucl. Phys. B 222, 83 (1983).

5. Integrating the one-loop equation

The beta function becomes especially transparent when written for the inverse squared coupling:

ddln⁡μ(1g2)=−2β(g)g3=b08π2.

Therefore

1g2(μ)=1g2(μ0)+b08π2ln⁡μμ0

or

g2(μ)=g2(μ0)1+b0g2(μ0)8π2ln⁡(μ/μ0).

If α=g2/(4π), the same equation is

α−1(μ)=α−1(μ0)+b02πln⁡μμ0.

This explains the familiar plot of inverse gauge couplings as straight lines against ln⁡μ. The approximation remains one-loop even when the equation is solved exactly. The denominator resums the leading logarithms (g2ln⁡μ)n generated by repeated insertion of the one-loop result.

5.1 Translating the cutoff formula

Take μ0=ΛUV and call the coupling there g0. Then

1g2(μ)=1g02−b016π2ln⁡ΛUV2μ2.

For pure Yang–Mills, b0=11CA/3. This is the formula whose superscript was flattened into “g2” by the PDF extractor in Tong’s Gauge Theory notes.

5.2 The beta function of g2

If the quantity of interest is literally g2, then

βg2≡μdg2dμ=2gβ(g)=−b08π2g4+O(g6).

The sign is unchanged. Squaring the coupling does not create a new running law; it changes the coordinate used to describe the same flow.

6. Dimensional transmutation

When b0>0, the one-loop solution can be rewritten as

1g2(μ)=b08π2ln⁡μΛ,

where

Λ=μexp⁡[−8π2b0g2(μ)].

The dimensionless input g(μ) has been traded for a dimensionful scale Λ. This is dimensional transmutation. At one loop, differentiating the right-hand side with respect to μ gives zero.

The formal divergence at μ=Λ does not prove that the exact coupling has a pole. It announces that perturbation theory has reached its boundary. In QCD, the corresponding ΛMS― is a useful scheme-dependent scale, while hadron masses and cross sections are physical. Confinement and chiral symmetry breaking require nonperturbative physics beyond the one-loop beta function.

Part II. From model counting to electroweak running

7. Three quick theories

Pure SU(N) Yang–Mills has

b0=113N.

It is asymptotically free for every N≥2. The coupling is weak at short distance and grows toward the infrared.

An SU(Nc) theory with Nf Dirac fermions in the fundamental has

b0=113Nc−43NfT(Nc)=113Nc−23Nf.

Asymptotic freedom at one loop requires

Nf<112Nc.

For QCD, Nc=3. With six active quark flavors, b0=7. At lower energies the top, bottom, and charm quarks successively decouple, so the slope changes across their thresholds.

QED has CA=0. For Nf Dirac fermions of unit charge,

β(e)=Nf12π2e3+O(e5).

The coupling grows toward the ultraviolet. Matter screening is all that remains because an Abelian photon has no Yang–Mills self-interaction. The one-loop solution has a remote ultraviolet Landau pole. That pole says that QED alone cannot define a weakly coupled continuum theory to arbitrarily high energy; electroweak physics intervenes long before it becomes numerically relevant.

8. Computing the Standard Model weak coefficient

We now return to the genuinely subscripted coupling g2. Above the electroweak scale, the Standard Model gauge group is

SU(3)c×SU(2)L×U(1)Y.

Use the convention

μdgidμ=bi16π2gi3.

For SU(2)L, the gauge contribution is

b2gauge=−113CA=−223.

Only left-handed fermion doublets contribute. In each generation, the quark doublet QL has three color copies and the lepton doublet LL has one:

∑one generationT2(Rf)=3×12+1×12=2.

With three generations,

∑Weyl fT2(Rf)=6,

so

b2fermions=23×6=4.

The Standard Model Higgs is one complex doublet. It gives

b2Higgs=13T(2)=16.

Combining the sectors,

b2=−223+4+16=−196.

The count can be read at a glance:

Standard Model sectorcontribution to b2
SU(2)L gauge field and ghosts−22/3
three generations of QL+3
three generations of LL+1
one complex Higgs doublet+1/6
total−19/6

Right-handed quarks and charged leptons are weak singlets. Gauge-singlet right-handed neutrinos would also leave b2 unchanged. Their Yukawa couplings can affect gauge running only at higher loop order.

The one-loop Standard Model coefficients are

(b1,b2,b3)=(4110,−196,−7),

where

g1=53gY.

Without the grand-unified normalization, the hypercharge coefficient is bY=41/6. The U(1) normalization must be stated whenever different references are compared. The current Particle Data Group review of grand unification uses the GUT-normalized convention above.

9. How fast does g2 actually run?

The 2026 Particle Data Group grand-unification review uses the illustrative MS― inputs

α^−1(MZ)=127.930,sin2⁡θ^W(MZ)=0.23122.

Using the corresponding MS― definitions at MZ, the leading relation is

α2=α^sin2⁡θ^W,

so

α2−1(MZ)=α^−1(MZ)sin2⁡θ^W(MZ)≃29.580,

and

g2(MZ)=4πα2(MZ)≃0.6518.

With MZ=91.1879GeV, the one-loop solution is

α2−1(μ)=29.580+1912πln⁡μMZ.

It gives the following teaching-level extrapolation:

μα2−1(μ)g2(μ)
MZ29.5800.6518
1TeV30.7870.6389
106GeV34.2680.6056
1010GeV38.9100.5683
1016GeV45.8730.5234
2.435×1018GeV48.6430.5083

Across the table, the modest one-loop slope raises α2−1 by about 19. A logarithm needs many decades of energy to make an order-one change in g2, but a small change in the slope sustained over that interval produces a visible shift in a unification test.

The final row should not be treated as a precision Standard Model prediction at the reduced Planck scale. Two- and three-loop terms, electroweak matching, quark thresholds, and any new particles modify the curve. Quantum gravity may invalidate the field theory extrapolation near that scale. Precision studies use multi-loop running and matching, as in Buttazzo et al., rather than the single straight line above.

There is a further convention trap. The on-shell weak angle, the effective leptonic angle measured at the Z pole, and sin2⁡θ^W(MZ) in MS― are different renormalized quantities. One cannot insert whichever value is most familiar into the equation for an MS― coupling. The distinctions are tabulated in the current PDG electroweak review.

10. A massive field does not run forever

The formula for b0 was derived as if every field were massless. A particle of mass M contributes fully when the external scale is far above M and decouples from low-energy amplitudes when the scale is far below M. The original general statement is the Appelquist–Carazzone decoupling theorem.

There is a technical qualification. The MS― counterterm is mass independent, so a heavy field does not automatically disappear from an MS― beta function. One constructs an effective field theory (EFT) without the heavy field and matches its coupling to the full-theory coupling near μ=M.

Let

Δb=bfull−bEFT.

At leading logarithmic order, the relation can be written as

αEFT−1(μ)=αfull−1(μ)+Δb2πln⁡μM+δfinite.

For a simple fermion or scalar threshold, choosing μ=M removes the one-loop logarithm. Finite matching corrections can remain for broken gauge theories, nondegenerate spectra, particular mass definitions, and higher orders.

If μ0 lies below all new thresholds and μ lies above some masses Ma, the leading-log result is

αi−1(μ)=αi−1(μ0)−bilight2πln⁡μμ0−∑Ma<μΔbia2πln⁡μMa.

Every threshold changes the slope of the inverse coupling. The exact crossover is smooth in a physical amplitude; the stepwise EFT description reproduces it as a controlled expansion in powers of external momentum over Ma.

10.1 The electroweak threshold is structural

Below the weak scale, the Higgs expectation value breaks

SU(2)L×U(1)Y⟶U(1)EM.

The W and Z are massive and are eventually integrated out. The appropriate low-energy theory contains QCD and QED, plus higher-dimensional four-fermion and other operators. It does not contain an independent unbroken SU(2)L gauge field whose coupling can be run unchanged toward zero energy.

One can still quote a renormalized g2(μ) within the full Standard Model at a chosen scale. Connecting it to low-energy observables requires electroweak matching. Extrapolating the coefficient −19/6 below every weak threshold would confuse a convenient full-theory parameter with the active coupling of the low-energy EFT.

11. New electroweak multiplets

The one-loop effect of new matter can be read directly from its SU(2) isospin. For a colorless isospin-j multiplet,

Δb2Weyl=23T(j),Δb2Dirac=43T(j),

and

Δb2complex scalar=13T(j),Δb2real scalar=16T(j).

If the multiplet also transforms under color, multiply by the dimension of its color representation. Some examples are:

new colorless fieldT2Δb2
complex scalar doublet1/21/6
Weyl fermion doublet1/21/3
Dirac fermion doublet1/22/3
real scalar triplet21/3
complex scalar triplet22/3
Majorana fermion triplet24/3
Dirac fermion triplet28/3
complex scalar quartet55/3

Matter makes b2 less negative. Five additional colorless Dirac doublets give

b2=−196+5(23)=16.

The weak coupling then loses asymptotic freedom at one loop. Nineteen additional complex scalar doublets make b2=0 exactly at this order.

For b2>0, the formal one-loop Landau scale is

ΛL=μ0exp⁡[8π2b2g22(μ0)].

This estimate becomes unreliable if a new threshold, a sizeable two-loop term, a Yukawa coupling, or a fixed point appears first. Large representations introduce a second warning sign: the relevant expansion parameter can be g22C2(R)/(16π2), which may cease to be small well below the naive pole.

11.1 A beta function does not certify a consistent spectrum

The table accepts any representation as bookkeeping input. A chiral gauge theory must also satisfy its anomaly constraints. Local cubic and mixed anomalies restrict hypercharges and representations. SU(2) has an additional global obstruction: an odd number of left-handed fundamental doublets is inconsistent, even though the perturbative cubic SU(2) anomaly vanishes. More generally, for the original Witten anomaly on a spin manifold, the fermion representations must obey

∑f2T(Rf)=0(mod2).

The fundamental has 2T(2)=1, which gives the familiar even-doublet rule. This is the Witten SU(2) anomaly.

The Standard Model has twelve left-handed weak doublets when color copies are counted, so the number is even. Adding one isolated Weyl doublet would spoil that consistency. A vectorlike Dirac doublet contains two Weyl doublets and avoids the global anomaly, though its hypercharge assignments must still be checked.

Running tells us how an allowed theory changes with scale. It does not decide whether the proposed field content defines an allowed quantum theory in the first place.

12. Two Higgs doublets and supersymmetry

An additional complex Higgs doublet contributes 1/6 to b2. With GUT-normalized hypercharge, the two-Higgs-doublet model (2HDM) has

(b1,b2,b3)2HDM=(215,−3,−7).

The one-loop gauge coefficients do not care whether the Yukawa sector is type I, II, X, or Y. Those variants use the same gauge representations. Their different Yukawa assignments enter the gauge beta functions at two loops.

The minimal supersymmetric Standard Model (MSSM) changes the counting more substantially. For an N=1 supersymmetric gauge theory,

b=−3CA+∑chiral multipletsT(R).

For SU(2)L, the vector multiplet gives −6. Each of three generations contributes

3×T(2)+T(2)=2

from Q and L, and the two Higgs chiral multiplets contribute one more unit in total. Thus

b2MSSM=−6+3×2+1=1.

The full MSSM vector is

(b1,b2,b3)MSSM=(335,1,−3).

Above the superpartner thresholds, g2 grows rather than shrinks toward the ultraviolet. The change in sign is modest enough that the coupling remains perturbative up to the usual grand-unification scale. A detailed supersymmetric calculation is normally performed in DR― rather than MS―; precision work includes the scheme conversion and nondegenerate superpartner thresholds. A useful entry point is Martin’s Supersymmetry Primer.

13. Why three straight lines became evidence for unification

At one loop,

αi−1(μ)=αi−1(MZ)−bi2πln⁡μMZ.

If the three couplings meet at one scale, their measured separations and their slopes must obey

Rexp≡α2−1−α3−1α1−1−α2−1=b2−b3b1−b2.

Using αs(MZ)≃0.1180 together with the electroweak inputs above gives

Rexp≃0.717.

The slope ratios are

theory above the weak threshold(b2−b3)/(b1−b2)
Standard Model0.528
two-Higgs-doublet model0.556
MSSM0.714

One additional Higgs doublet moves the slopes toward the measured ratio but does not make them meet. The MSSM value 0.714 lies close to Rexp≃0.717 in this one-loop treatment. Its couplings meet near

MG≃2×1016GeV,αG−1≃24.3.

This is evidence about relative slopes, not a direct observation of a grand-unified gauge boson. The current PDG GUT review emphasizes the required qualifications: two-loop evolution, weak-scale and supersymmetric thresholds, MS― to DR― conversion, and GUT-scale thresholds all matter in a precision fit. The minimal Standard Model misses exact unification; supersymmetric spectra can achieve it accurately, but the result depends on their masses.

A degenerate complete GUT multiplet gives equal one-loop shifts to the canonically normalized bi. It changes the unified coupling while leaving bi−bj and the one-loop meeting scale unchanged. Splitting the multiplet masses generates unequal threshold logarithms and can move the apparent intersection.

Part III. Beyond the isolated one-loop coefficient

14. At two loops, g2 stops running alone

The independence of the three gauge equations is a one-loop property. In the Standard Model, with g1=5/3gY, the next term for g2 is

βg2=−196g2316π2+g23(16π2)2[910g12+356g22+12g32−32Tr(Yu†Yu)−32Tr(Yd†Yd)−12Tr(Ye†Ye)]+⋯.

The strong coupling enters through quarks carrying both color and weak isospin. Hypercharge enters through fields carrying both Y and weak isospin. Yukawa couplings enter because the same matter propagators are dressed by Higgs interactions. The Higgs quartic does not enter a gauge beta function at two loops; it first appears at three loops.

Once these terms are retained, all gauge, Yukawa, and scalar equations must be solved as a coupled system. The general two-loop organization goes back to Machacek and Vaughn. The Standard Model gauge functions are known through higher orders; Mihaila, Salomon, and Steinhauser computed the three-loop gauge contributions including Yukawa and Higgs-sector effects.

Two-loop corrections are small over a short interval when every coupling is perturbative. Across many decades, small local corrections accumulate. A unification analysis that quotes percent-level intersections while using only one-loop slopes has assigned more precision than the calculation contains.

15. When two loops create a fixed point

Consider SU(Nc) with Nf Dirac fundamental fermions and write

β(g)=−g316π2β0−g5(16π2)2β1+O(g7),

where

β0=113Nc−23Nf,

and

β1=343Nc2−(103Nc+2CF)Nf.

Take Nf just below 11Nc/2. Then β0 is positive and small, while β1 is negative. The two terms balance at

g∗216π2=−β0β1.

The flow approaches this value in the infrared. Because g∗2 can be made parametrically small by choosing Nf close to the loss of asymptotic freedom, the fixed point is perturbatively controlled. This is the Banks–Zaks mechanism, building on the two-loop analysis of Caswell and developed in Banks and Zaks.

For SU(3) with Nf=16,

β0=13,β1=−3023,

so

α∗=g∗24π≃0.0416.

At this order, the zero is the perturbative signal of an interacting infrared conformal field theory. Moving to smaller Nf strengthens the fixed point until perturbation theory can no longer locate the lower edge of the conformal window reliably. A one-loop coefficient can tell us where asymptotic freedom ends; it cannot determine the entire infrared phase diagram.

16. What is universal, and what belongs to a scheme

The one-loop coefficient b0 is independent of the gauge-fixing parameter and of ordinary analytic changes of renormalization scheme. It is also insensitive to Yukawa and scalar self-couplings. Those facts make it unusually robust.

The numerical value of a renormalized coupling at a quoted scale is scheme dependent. A finite redefinition

g′=g+cg316π2+O(g5)

changes higher-order beta coefficients while leaving the one-loop term intact. For a single coupling, the two-loop coefficient is also unchanged under such an analytic redefinition. With several coupled gauge and Yukawa parameters, scheme changes act on the full vector field of beta functions, and comparisons require all conventions to be transformed consistently.

The scale Λ obtained by dimensional transmutation is scheme dependent by a multiplicative constant. A physical mass gap or cross section is not. The relation between the two contains nonperturbative information.

The running coupling itself is therefore not an observable in isolation. Experiments determine cross sections, decay rates, asymmetries, and potential energies. A renormalization prescription extracts g(μ) from those data. Another prescription extracts a different number and supplies different perturbative coefficients, while predicting the same observable when calculated consistently.

For electroweak theory, the tree-level identities

e=g2sin⁡θW=gYcos⁡θW

and

1e2=1g22+1gY2

are useful definitions at leading order. Beyond tree level, the weak angle and the couplings must share a stated scheme and matching prescription. Mixing an on-shell angle with MS― couplings breaks that consistency.

17. Domain of validity

The one-loop equation is controlled only while every relevant loop parameter remains small, the field content is fixed, and the symmetry phase has been stated. A threshold requires matching to a new effective theory. A long extrapolation may require higher-loop gauge, Yukawa, and scalar running even when the coupling never becomes large.

Within those limits, the calculation establishes four precise facts. A non-Abelian gauge field contributes with the sign required for ultraviolet asymptotic freedom. Matter screens that effect in amounts fixed by Dynkin indices. The inverse squared coupling runs linearly with ln⁡μ between thresholds. A dimensionless coupling can generate a physical scale through dimensional transmutation.

The same calculation does not establish confinement, a mass gap, exact gauge unification, or a physical Landau singularity. It does not make g(μ) scheme independent. Those questions require EFT matching, higher loops, nonperturbative methods, or experimental input.

Part IV. Problems and references

18. Problems

Problem 1: recover the cutoff expression

Start from

β(g)=−b016π2g3.

Derive the beta function for g2, integrate it between ΛUV and μ, and recover the logarithm of ΛUV2/μ2. Explain why a factor of two moves when the logarithm is squared.

Solution

Since μdg2/dμ=2gβ(g),

μdg2dμ=−b08π2g4.

It follows that

ddln⁡μ1g2=b08π2.

Integrating from ΛUV to μ gives

1g2(μ)=1g2(ΛUV)−b08π2ln⁡ΛUVμ.

Because ln⁡(Λ2/μ2)=2ln⁡(Λ/μ), this is

1g2(μ)=1g02−b016π2ln⁡ΛUV2μ2.

Problem 2: count b2 without double counting

Compute the Standard Model b2 using Weyl fermions and complex scalars. Repeat the calculation by grouping the fermions as much as possible into Dirac fields. Identify why the second route is awkward before electroweak symmetry breaking.

Solution

The Weyl count is

b2=−113(2)+23[3gen(3color12+12)]+1312=−196.

The unbroken Standard Model is chiral. A left-handed weak doublet and its right-handed partners do not transform in the same SU(2)L representation, so they do not form a Dirac representation of the weak gauge group. Grouping particles into massive Dirac fermions is natural only after symmetry breaking, precisely where the unbroken-theory beta coefficient must be connected to a different EFT by matching. The Weyl formula respects the ultraviolet gauge representations directly.

Problem 3: insert one threshold

Add a colorless vectorlike Dirac weak doublet of mass M=10TeV. Use α2−1(MZ)=29.580 and stepwise one-loop running to estimate g2(1010GeV). Compare with the Standard Model value in the table.

Solution

Below M, b2=−19/6. Above M, the Dirac doublet adds 2/3, so

b2high=−196+23=−52.

Therefore

α2−1(1010GeV)=29.580−−19/62πln⁡104MZ−−5/22πln⁡1010104≃37.44.

Thus

g2(1010GeV)≃4π37.44≃0.579.

The Standard Model-only value is about 0.568. The extra matter screens the gauge contribution, so g2 decreases more slowly toward the ultraviolet.

Problem 4: test one-loop unification without finding the meeting scale

Show that exact one-loop unification implies

α2−1−α3−1α1−1−α2−1=b2−b3b1−b2.

Evaluate the right-hand side for the Standard Model and the MSSM. Why is this ratio insensitive to the assumed unified coupling and unification scale?

Solution

If all three couplings equal αG at MG, then

αi−1(MZ)=αG−1+bi2πln⁡MGMZ.

Subtracting two equations eliminates αG−1. Taking a ratio of two differences also eliminates ln⁡(MG/MZ). For the Standard Model,

−19/6+741/10+19/6=115/30218/30≃0.528.

For the MSSM,

1+333/5−1=428/5=57≃0.714.

The experimental ratio is about 0.717, before precision threshold and higher-loop corrections.

Problem 5: locate a perturbative Banks–Zaks point

For SU(3) with Nf=16 fundamental Dirac fermions, compute b0, b1, and α∗. Then estimate the expansion parameter and explain why the result is more trustworthy than the same formula at Nf=9.

Solution

For SU(3), CF=4/3, so

b0=11−23Nf,b1=102−383Nf.

At Nf=16,

b0=13,b1=−3023.

The fixed point satisfies

g∗216π2=−b0b1=1302,

and therefore

α∗=g∗24π=4π302≃0.0416.

The loop parameter is about 0.0033, so higher loops are plausibly controlled. At Nf=9, the candidate fixed point is much stronger. Higher-loop and nonperturbative effects can shift or remove a fixed point inferred from a low-order truncation, so the two-loop answer alone cannot locate the lower edge of the conformal window.

19. Further reading

  1. David Tong, Gauge Theory, Chapter 2. Sections 2.4 and 2.7 motivate the pure Yang–Mills result, the background-field computation, matter contributions, and QCD-like infrared phases.
  2. D. J. Gross and F. Wilczek, “Ultraviolet Behavior of Non-Abelian Gauge Theories”. One of the two original 1973 discoveries of asymptotic freedom.
  3. H. D. Politzer, “Reliable Perturbative Results for Strong Interactions?”. The independent companion result.
  4. M. E. Machacek and M. T. Vaughn, “Two-Loop Renormalization Group Equations in a General Quantum Field Theory”. The systematic general framework for gauge theories with fermions and scalars.
  5. Particle Data Group, “Grand Unified Theories”. Current conventions, Standard Model and MSSM coefficients, thresholds, and the status of precision unification.
  6. T. Appelquist and J. Carazzone, “Infrared Singularities and Massive Fields”. The foundational decoupling theorem behind threshold EFTs.
  7. L. N. Mihaila, J. Salomon, and M. Steinhauser, “Gauge Coupling Beta Functions in the Standard Model to Three Loops”. A concise route from the one-loop coefficients to modern high-order running.
  8. J. Brod and Z. Polonsky, “Two-loop Beta Function for Complex Scalar Electroweak Multiplets”. A useful extension when large SU(2) scalar representations or minimal-dark-matter multiplets are added.
  9. T. Banks and A. Zaks, “On the Phase Structure of Vector-Like Gauge Theories with Massless Fermions”. The perturbative infrared fixed point near the loss of asymptotic freedom.

20. The compact answer

For a simple gauge group with Weyl fermions and complex scalars,

β(g)=−g316π2[113CA−23∑fT(Rf)−13∑sT(Rs)]+O(g5).

The corresponding running of the squared coupling is

μdg2dμ=−b08π2g4+O(g6),

with solution

1g2(μ)=1g2(μ0)+b08π2ln⁡μμ0.

For the Standard Model SU(2)L coupling,

b0,2=223−4−16=196,

so g2 decreases logarithmically toward the ultraviolet. The coefficient remains 19/6 only while the active theory is the unbroken Standard Model with its stated field content. Threshold matching is required whenever the active field content changes.