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Gravity and Strings

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8.7 Electric-magnetic duality 249<br />

dynamical electric (only) charges. It is necessary to introduce magnetic sources that can<br />

be rotated into the electric ones in order to maintain duality invariance of the Maxwell<br />

equations. We have already seen in Eq. (8.133) that electric–magnetic duality needs the<br />

introduction of magnetic charges into which electric charges can transform. By definition,<br />

then, the magnetic charge is given by25 :<br />

<br />

p ≡˜q = d 2 S · ˜ <br />

E =<br />

S 2 ∞<br />

S 2 ∞<br />

d 2 <br />

S · B =−<br />

S2 F. (8.144)<br />

∞<br />

The simplest electric-charge distribution is a point-like electric charge <strong>and</strong> its dual is a<br />

magnetic point-like charge, which should be given by a magnetic field obeying<br />

∇ · B = p δ (3) (x3), (8.145)<br />

which is the Dirac monopole equation for the vector potential.<br />

Introducing magnetic sources to preserve electric–magnetic duality is, however, a very<br />

dangerous move: the Bianchi identity is not satisfied at the locations of the magnetic sources<br />

<strong>and</strong> there the vector potential, the true dynamical field, cannot be defined or, more precisely,<br />

it cannot be defined everywhere: it will have singularities. This may not be as bad as it looks<br />

at first sight, because, after all, the electrostatic potential is not defined at the location of<br />

an electric point-like charge, either. It depends on how bad the singularities of the vector<br />

field are. In the electric case, it is quite benign, since the singularity affects only the particle<br />

that gives rise to the field. Let us see what happens with the vector potential of a point-like<br />

magnetic monopole. First, we have to find it.<br />

Knowing that<br />

2 1<br />

∇<br />

|x3| =−4πδ(3) (x3), (8.146)<br />

we find that the magnetic field is given by<br />

B =− p<br />

∇<br />

1<br />

, (8.147)<br />

4π |x3|<br />

which implies, due to B = ∇ × A, for the Dirac monopole equation<br />

∇ × A =− p<br />

∇<br />

1<br />

, (8.148)<br />

4π |x3|<br />

or, defining, to simplify matters f =−(4π/p) A, the following, st<strong>and</strong>ard form:<br />

1<br />

∂m fn − ∂n fm = ɛmnp∂p . (8.149)<br />

|x3|<br />

25 We work again in the st<strong>and</strong>ard units of the beginning of Section 8.2.1 <strong>and</strong> in flat spacetime. At the end of<br />

this section we will say which changes have to be made when using our normalization Eq. (8.58).

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