Yang-Mills Equations
Prerequisites: Gauge Models. Full path (17 pages)
see also Gauge Models and Gauge Symmetry
Intuitive
The Yang-Mills equations generalize the Maxwell equations. In electromagnetism there is one kind of charge, electric charge, and the field that charges create, the electromagnetic field, is itself uncharged. In classical electromagnetism, two light beams pass through each other without noticing each other. This is why the Maxwell equations are linear.
The strong and the weak interaction work with a richer kind of charge. In the strong interaction a quark carries one of three "colors", and the interaction can change a quark's color. Instead of one photon there are several force particles, eight gluons in the case of the strong interaction, and these carry color charge themselves. So the field acts as a source of itself: gluons attract and scatter other gluons. In the equations this shows up as extra terms in which the field appears multiplied by itself, which makes the Yang-Mills equations nonlinear. Mathematically, the extra terms exist because the symmetry transformations behind the theory are described by matrices that do not commute, so the order in which two transformations are applied matters.
The self-interaction has large consequences in the quantum theory. For the strong interaction, the force becomes weak at very short distances (asymptotic freedom) and strong at large distances, which is the accepted explanation of why quarks and gluons are never seen in isolation, although a proof is missing. Proving that the quantum theory of pure Yang-Mills fields has a mass gap, meaning that its lightest states have a nonzero mass, is an open problem.
L=1/4g²∫TrF∧∗F
Concrete
Derivation of the Yang-Mills equation from the Yang-Mills Lagrangian
Let L=−41FaμνFμνa and Aaμ be real functions.
The Euler-Lagrange equations for L=L(Aμ,∂νAμ) are ∂ν(∂(∂νAaμ)L)=∂Aaμ∂L
Then
∂Aaμ∂Fdμν=−gfdacAcν∂Aaμ∂Fμνd=−gfdacAcνgμμgνν∂Aaμ∂L=21gfabcAbνFμνc∂(∂νAaμ)∂Fdμν=−δad∂(∂νAaμ)∂Fμνd=δad(gμνgνμ−gμμgνν)∂(∂νAaμ)∂L=21Fμνa
Directly computing ∂Aaμ∂Fdμν=∂Aaμ∂(−gfdbcAbμAcν)=−gδabfdbcAcν=−gfdacAcν
∂Aaμ∂Fμνd=∂Aaμ∂(−gfdbcAμbAνc)=∂Aaμ∂(−gfdbcgμαAbαAνc)=−gfdacgμαδαμδabAνc=−gfdacAνcgμμ=−gfdacgναAcαgμμ=−gfdacAcνgμμgνν
∂Aaμ∂L=−41((∂Aaμ∂Fdμν)Fμνd+Fdμν(∂Aaμ∂Fμνd))
=41gfdac(AcνFμνd+FdμνAcνgμμgνν)=41gfdac(AcνFμνd+AcνgμαgνβFdαβ)=41gfdac(AcνFμνd+AcνFμνd)=21gfdacAcνFμνd=21gfacdAcνFμνd=21gfabcAbνFμνc
∂(∂νAaμ)∂Fdμν=∂(∂νAaμ)∂(∂μAdν−∂νAdμ)=−δad
∂(∂νAaμ)∂Fμνd=∂(∂νAaμ)∂(∂μAνd−∂νAμd)=∂(∂νAaμ)∂(gμαgνβ(∂αAdβ−∂βAdα))=gμαgνβδadδμβδνα−gμαgνβδadδνβδμα=−δad(gμνgνμ−gμμgνν)
∂(∂νAaμ)∂L=−41(−δadFμνd−gμμgννδadFdμν)=41(Fμνa+gμαgνβFaαβ)=41(Fμνa+gμαgνβFaαβ)=41(Fμνa+Fμνa)=21Fμνa
Abstract
The Yang-Mills equations can be expressed with the Hodge star operator as dA∗F=0F=dA+A∧A where dA is the gauge-covariant extension of the exterior derivative. The curvature also satisfies the Bianchi identity dAF=0, which holds for every A. The gauge field A is a one-form A(x)=Aμa(x)tadxμ with the values on the Lie algebra of a compact simple Lie group G. The curvature is a two-form F=dA+A∧AF=21Fμνatadxμ∧dxνFμνa=∂μAνa−∂νAμa+fabcAμbAνc with [ta,tb]=fabctc and the coupling constant g absorbed into A.
Why is it interesting?
In physics, of course, Maxwell's equations of electromagnetism are linear partial differential equations. Their counterparts, the famous Yang-Mills equations, are non-linear equations which are supposed to govern the forces involved in the structure of matter. The equations are non-linear, because the Yang-Mills equations are essentially matrix versions of Maxwell's equations, and the fact that matrices do not commute is what produces the non-linear term in the equations.
The Aleph of Space by Luciano Boi
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