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## New answers tagged gauge-theory

4

A gauge theory in the broadest sense is a theory with an action that has gauge symmetries parametrized by smooth functions of spacetime $\epsilon(x)$, i.e. the theory is invariant under infinitesimal changes of the coordinates/fields as $$\delta \phi = R\epsilon(x) + R^\mu \partial_\mu\epsilon(x) + R^{\mu\nu}\partial_\mu\partial_\nu \epsilon(x) + \dots$$ and ...

2

OK, I collect my comments since their obviousness is evidently not unassailable. You are exactly right that in my mind gauge and local are synonyms when used for symmetries, and "gauging" meant something like "localizing". ... "local symmetry", "gauge symmetry" and "local gauge symmetry" all mean the same ...

0

A global gauge symmetry means that the gauge group acts everywhere in the same way. We say it acts in a rigid fashion. Whilst a local gauge symmetry means that the gauge group acts in a position dependent fashion. We say a global gauge symmetry is gauged when it is made to depend in a position dependent fashion, that is in a local fashion. So we have a ...

6

You have touched on a point here which, in my experience, often gets glossed over, mentioned offhand, or mentioned indirectly (meaning it would be hard to realize it's the same point being mentioned without already knowing the answer) in first treatments of QFT. You may have heard it mentioned at some point that the modern perspective on gauge symmetry is ...

3

I don't think this is true, $\pi_5(G)$ has little to do with anomalies, at least not in any direct way. The general statement is: triangle anomalies for a given symmetry $G$, in $d$ dimensions, are classified by the free part of $\Omega_{d+2}(G)$. Here $\Omega_n(G)$ denotes the cobordism group of $G$, namely the collection of $n$ dimensional manifolds $M_n$ ...

2

Classically speaking, gauge fields are connections on principle $G$ bundles. Matter fields, on the other hand, are sections of associated bundles. To construct an associated bundle, you must choose a representation of $G$. For instance, if $G = U(1)$, then this amounts to choosing an integer. When you construct the associated bundle, this integer is the ...

4

The Dirac operator $D$ is self adoint on a dense subset of the Hilbert space, it has a complete set of $V$-valued eigenfunctions $\varphi_n(x)$ with real eigenvalues $\lambda_n$. As a consequence one can define $\exp\{-tD^\dagger D\}$ on the entire Hilbert space by the integral kernel $$K_t(x,x')=\exp\{-tD^\dagger D\}_{xx'}=\sum_n \varphi_n(x) e^{-t\... 4 Being a gauge theory and being an effective theory are completely orthogonal concepts. An effective quantum field theory is a theory that is only valid up to some energy scale. These theories are often non-renormalizable, but since they possess a physical meaningful energy cutoff, this is not a problem. Conversely, a (candidate for) a "fundamental" ... 3 A lot of times in theoretical physics, there is a gap between the theoretical and mathematical framework, and the underlying physical assumptions. Before getting to gauge theory, let's consider the idea of curved spacetime (which is actually quite similar but involves a less abstract space so is perhaps a bit easier to think about). What physical motivation ... 2 If you compacify to a torus then, in Cartesian coordinates, the spin connection vanishes and so is irrelevent. If you compactify to a sphere, as Fujikawa suggests, it is far less obvious that \hat A(TM) is not needed. That it plays no role is because \hat A(TM) is a genus and so cobordism invariant. This means that the curvature contribution to the ... 0 This is actually more general than just diffeomorphisms, but it is a but more intuitive there since we are so used to coordinate transformations. For any quantity, one can simply decide to measure it in different units, different scale, or shift the scale. This doesn't change physical properties in any way, and in this sense corresponds to a gauge ... 2 If you insist on not breaking one type of terms in the Hamiltonian - say, the plaquette constraints - then the remaining theory is a Z_2 gauge theory with the plaquette constraints as the gauge constraints. Thus, within this subspace where the plaquette constraints are not violated, the theory behaves just as a gauge theory. But this is no longer true when ... 2 The reason for this is that Gauß' law is not an equation of motion, but a constraint. The Lagrangian$$ L = -\frac{1}{4}\int F^{\mu\nu}F_{\mu\nu}\mathrm{d}^4 x $$gives us the canonical momenta \pi^\mu = F^{\mu0} and hence a primary constraint \pi^0\approx 0 (\approx means an equality that hold on the constraint surface/upon use of the equations of ... 0 Let's assume O acts on complex valued functions. We can improve the notation by setting \langle x|\psi\rangle:=\psi(x), \langle\psi|x\rangle:=\overline{\psi(x)} (complex conjugate) and |n\rangle:=\psi_n. We can obtain the result from the title by introducing the plane wave basis defined by \langle x|k\rangle=\mathrm{e}^{\mathrm{i}kx} and using the ... 1 Let P\to M be a principal G-bundle with a representation \rho\colon G\to\mathrm{GL}(V). The "extra term" is the endomorphism O\colon C^{\infty}(M,\Delta\otimes V)\to C^{\infty}(M,\Delta\otimes V) defined by O(\psi)=[\gamma^k,\gamma^l]\cdot\{\nabla_k,\nabla_l\}(\psi)=\sum_{k,l}[\gamma^k,\gamma^l]\cdot\{\nabla_k,\nabla_l\}(\... 3 You cannot reuse a free index as a dummy index, so \frac12h\eta_{\mu\nu}\equiv\frac12h^\alpha{}_\alpha\eta_{\mu\nu}\ne\frac12h_{\nu\mu} Verify for yourself that the residual gauge transformation acts on the polarisation tensor as a_{\mu\nu}\to a_{\mu\nu}+i(k_\mu B_\nu+k_\nu B_\mu-k^\sigma B_\sigma\eta_{\mu\nu}). Contracting,$$ \eta^{\mu\nu}a_{\mu\nu}\...

0

Think of the $\psi$'s as being a some spinor $u\in\mathbb{C}^4$ of functions $f:\mathbb{R}^4\rightarrow \mathbb{C}$, which is again the space where the Lie algebra acts, not the Lie algebra itself. So think that $$\psi(x)\propto e^{i k x} u_s$$ Now notice equation (1) still has a trace, which is the trace over possible remaining index $s$, in this case the ...

1

You are probably confused because of the muddled notation such as $|\psi(x)\rangle$. Indeed I remember being confused when I first read Fujikawa's account. Let's do it with proper Dirac notation: Firstly the LHS $$\sum_n \langle \psi_n(x)|O(\psi_n(x)\rangle$$ is to be interpreteted as $$\sum_n\langle \psi_n|x\rangle \langle x|\hat O|\psi_n\rangle$$ ...

4

As the three-form $(g^{-1} dg)^3$ is proportional to the Haar volume form on ${\rm SU}(2)$, and there is a tacit pull-back of this to $S^3$, the quantity $Q/24 \pi^2$ will be the integer winding number (Brouwer degree) of the map $g: S^3 \to {\rm SU}(2)\equiv S^3$.

2

Well you have seen the Faddeev–Popov method for gauge fields because it is designed to help with the path integral in a gauge theory; namely with summing over equivalent gauge configurations. If you don't have a gauge symmetry you don't have a problem to try to solve with Faddeev–Popov to begin with. Now, in your case you have a global $\mathrm{SO}(2)$ ...

9

In the Lorenz gauge $\vec{\nabla}\cdot\vec{A}+\frac{1}{c^2}\frac{\partial V}{\partial t}=0$, the Maxwell equations in terms of the potentials are, for $V$: $$-\frac{1}{c^2}\frac{\partial^2V}{\partial t^2}+\nabla^2V=-\frac{\rho}{\epsilon_0},\tag{1}$$ where $\rho=\rho(\vec{x},t)$ is the charge distribution. The general solution to this is $$V(\vec{x},t)=V_0(\... 9 the time of the density corresponds to the scalar potential. This is not correct, precisely because of causality considerations. If the charge distribution is time-dependent, the potential at time t will instead depend on the configuration at some retarded time, t_r=t-\frac{|\boldsymbol{r}-\boldsymbol{r}'|}{c}. 2 There is no relation at all between the particle fields \phi that are sections of associated bundles and the gauge field A. A is the field of the gauge bosons, \phi is a field of a particle charged under the interaction with that boson. The Standard Model does not contain particles charged in the adjoint of some gauge group, so there is no analogue ... 1 It seems you are essentially asking two questions which aren't really related. One of the two can be phrased as: given a Lie algebra-valued 1-form A (whether it's a connection or not is irrelevant to this question), does there exist a spacetime vector field v such that on some patch U of spacetime we may obtain A(v)=\phi for an arbitrary Lie algebra-... 1 The trace in those formulae is simply the trace over the group indices of the field strength tensor F, you are free to compute it in whichever basis you want, since the trace is an invariant, however the extra structure of an inner-product is not needed only matricial algebra. So once you have a representation \rho and a basis, \{T_a\} for the vector ... 0 Here's what should be the mathematically rigorous statement and proof: Let \rho_*\colon g\to\mathrm{End}(V) be the Lie algebra homomorphism induced by the Lie group homomorphism \rho\colon G\to\mathrm{GL}(V). Consider the right action \begin{equation*} \mathrm{End}(V)\times V\ni(A,v)\mapsto A\cdot v:=A(v)\in V. \end{equation*} If A\in C^{\infty}(U,g)... 3 The field strength F is \mathfrak{g}-valued. In that case if X^a is a basis of the Lie algebra we can write$$F=\dfrac{1}{2}F_{\mu\nu}^a dx^\mu\wedge dx^\nu \otimes X^a.$$In particular, given any representation R:G\to {\rm GL}(V) of G on the vector space V, we have the derived representation dR:\mathfrak{g}\to {\rm End}(V) of the Lie algebra, ... 8 Not that much notation, but probably not less true either:$$[\partial_\mu+A_\mu,\partial_\nu+A_\nu]\psi=(\partial_\mu+A_\mu)(\partial_\nu+A_\nu)\psi-(\partial_\nu+A_\nu)(\partial_\mu+A_\mu)\psi==\partial_\mu\partial_\nu\psi+A_\mu\partial_\nu\psi+\partial_\mu (A_\nu\psi)+A_\mu A_\nu\psi-\partial_\nu\partial_\mu\psi-A_\nu\partial_\mu\psi-\partial_\nu (A_\...

1

The easiest way to check the antisymmetry of $F$ is to write it as $$\mathcal{F}_{\mu \nu} = \partial_\mu \mathcal{A}_\nu - \partial_\nu \mathcal{A}_\mu + [ \mathcal{A}_\mu , \mathcal{A}_\nu]$$ This is manifestly antisymmetric, because the commutator is antisymmetric. Note then that \begin{align} [ \mathcal{A}_\mu , \mathcal{A}_\nu] &= [A_\mu^a T_a, A_\...

3

Do you know any other book containing the derivation of (1)? I would prefer a proper mathematical derivation, but all additional references would help. Here's one in the "additional references" category: Fujikawa and Suzuki (2004), Path Integrals and Quantum Anomalies, Oxford University Press. It includes detailed derivations of chiral anomalies ...

2

You can try the proof by Getzler: "A short proof of the local Atiyah-Singer Index theorem" Topology, Vol 25, pages 111-117 (1986). That give the general case, including curved space, and in any dimension.

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