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Effective Field Theory & Curing UV Divergence |
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| May7-08, 05:00 AM | #1 |
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Effective Field Theory & Curing UV Divergence
Effective field theory arrives at the right conclusions, that I think
are for the wrong reasons. Its point of view is that because that the quantum theory is broken which is rooted in a classical field theory that possesses the Lorentz relations (for electromagnetism) or, more generally, rooted in the classical field theory with a Lagrangian quadratic in the field velocities with constant quadratic coefficients; then this broken condition means that it is actually an effective low energy limit of a high energy theory (and one that may not even be a field theory at all), when all is said and done. Nonetheless, we can seal off the low energy level from the high energy level and treat the effective field theory in a quasi-self-contained fashion by simply asking the question: what is the most general Lagrangian consistent with spacetime and gauge symmetries? In contrast, Maxwell's resolution of the divergence problem -- and its modern-day descendant -- pays no need to the issue of quantum theory at all. It says: let's pose the same question of the CLASSICAL field theory, instead. The modern-day extension of this idea goes one step further: it says that maybe if we just start out with the right classical theory, in the first place, then we can resolve the divergence issue at its root -- at the classical level -- and THEN move on to a quantum theory that is in a proper state of repair. The final point reached is precisely the same as that of effective field theory: we are once again at the point of asking what the most general Lagrangian is that is consistent with spacetime and gauge symmetries. Except that: (a) we're reaching this point along the right path now from the right direction; and (b) we no longer regard the result as an "effective field theory", but rather the ACTUAL field theory. In the case of electromagnetism, this leads to a Lagranian L = L(I, J) as a function of the Lorentz invariants I = 1/2 (E^2 - B^2 c^2) and J = E.B. The coefficients, epsilon = dL/dI and theta = dL/dJ then play a central role in the field theory. The first coefficient, epsilon, is none other than the cornerstone of Maxwell's theory of the universal dielectric medium. Not only does he employ the device of epsilon to remove the self-energy and self-force divergence from the classical theory, but he bases his whole idea on it of the vacuum as an active medium with a structure described by epsilon. At the end of Chapter 1 in his treatise he points out that we should now be seeking to find what structure and dynamics epsilon conforms to, if we want to get a deeper understanding of electromagnetism that goes beyond the field law. Unfortunately, theta never entered Maxwell's considerations because -- when all is said and done -- Maxwell did NOT explore the issue of what the most general field theory is that is consistent with the underlying spacetime symmetry. Under the Galilei group, the most general field theory that possesses Maxwell's universal velocity vector G is given by the following constitutive law: D = epsilon (E + G x B) + theta B, B/mu = H - G x D + theta E where epsilon, mu and theta are indepdendent coefficients. In the absence of G, the most general law that can be stated is only of the form: D = theta B, B - theta E = mu H. One needs G in order to account for the dielectric coefficient. Thus, Maxwell's theory of the dielectric medium was inextricably mixed up with an otherwise independent theory of the vacuum as a universal reference medium. So, when Lorentz substituted the Lorentz group for the Galilei group, he not only threw out the velocity vector G, but also eliminated epsilon and wrote: D = epsilon_0 E, B = mu_0 H, epsilon_0 mu_0 = 1/c^2. But, if you were to ask what the MOST GENERAL Lorentz-invariant constitutive law for the vacuum is, you get the following: D = epsilon E + theta B, H = epsilon c^2 B - theta E where epsilon = epsilon(I, J) and theta = theta(I, J) are otherwise arbitrary functions of the Lorentz invariants. In it, light propagation is already accounted for. The null field is characterized by I = 0 = J. Without loss of generality, we can set theta(0, 0) = 0, since theta is already only given up to an additive constant (a residue of complexion symmetry). Defining epsilon_0 = epsilon(0, 0), one arrives at the following dynamics for a null field: E^2 = B^2 c^2, E.B = 0, D = epsilon_0 E, B = mu_0 H, epsilon_0 mu_0 = 1/c^2. Substituting in source-free Maxwell's equations del.D = 0 = del.B, del x E + dB/dt = 0 = del x H - dD/dt yields the wave equations for all the fields: ((1/c)^2 (d/dt)^2 - del^2) { E, B, D, H } = 0. This applies generally for ABELIAN gauge fields, where the only Lorentz invariants are I and J ... except that here I and J are GxG matrices, where G is the dimension of the underlying gauge group. the coefficients epsilon = dL/dI then become, up to factors of c, the components of the gauge group metric k. In particular, k = epsilon c. It is not necessarily the case, however, for NON-ABELIAN gauge fields, since one also has cubic Lorentz invariants in spacetimes of dimension 4 or greater. These need not be 0, so that the constitutive coefficients need not be at their asymptotic values, even for null fields. There is a much more complicated classification by invariants even for the SU(2) field, and one is no longer talking about a mere 3-way split into (0 vs. null vs. non-null). |
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