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Notes on Relativity and Cosmology - Physics Department, UCSB

Notes on Relativity and Cosmology - Physics Department, UCSB

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2.1. THE BASICS OF E & M 47<br />

(moving charges) when that current is in a vacuum 3 . The key point here is that<br />

both of the numbers are things that had been measured in the laboratory l<strong>on</strong>g<br />

before Maxwell or anybody else had ever thought of ‘electromagnetic waves.’<br />

−12 C2<br />

−7 Ns2<br />

Their values were ǫ 0 = 8.854 × 10<br />

Nm<br />

<strong>and</strong> µ 2 0 = 4π × 10<br />

C<br />

. 2<br />

Anyway, this other Equati<strong>on</strong> of Maxwell’s looks like:<br />

∂E<br />

∂t = ǫ 0µ 0<br />

∂B<br />

∂x . (2.2)<br />

Now, to underst<strong>and</strong> how the waves come out of all this, it is useful to take the<br />

derivative (<strong>on</strong> both sides) of equati<strong>on</strong> (2.1) with respect to time. This yields<br />

some sec<strong>on</strong>d derivatives:<br />

∂ 2 B<br />

∂t 2 = ∂2 E<br />

∂x∂t<br />

(2.3)<br />

Note that <strong>on</strong> the right h<strong>and</strong> side we have taken <strong>on</strong>e derivative with respect to<br />

t <strong>and</strong> <strong>on</strong>e derivative with respect to x.<br />

Similarly, we can take a derivative of equati<strong>on</strong> (2.2) <strong>on</strong> both sides with respect<br />

to x <strong>and</strong> get:<br />

∂ 2 B<br />

∂x 2 = (ǫ 0µ 0 ) ∂2 E<br />

∂x∂t . (2.4)<br />

Here, I have used the interesting fact that it does not matter whether we first<br />

∂ ∂<br />

differentiate with respect to x or with respect to t:<br />

∂t ∂x E = ∂ ∂<br />

∂x ∂t E.<br />

Note that the right h<strong>and</strong> sides of equati<strong>on</strong>s (2.3) <strong>and</strong> (2.4) differ <strong>on</strong>ly by a factor<br />

of ǫ 0 µ 0 . So, I could divide equati<strong>on</strong> (2.4) by this factor <strong>and</strong> then subtract it<br />

from (2.3) to get<br />

∂ 2 B<br />

∂t 2 − 1 ∂ 2 B<br />

ǫ 0 µ 0 ∂x 2 = 0 (2.5)<br />

This is the st<strong>and</strong>ard form for a so-called ‘wave equati<strong>on</strong>.’ To underst<strong>and</strong> why,<br />

let’s see what happens if we assume that the magnetic field takes the form<br />

B = B 0 sin(x − vt) (2.6)<br />

for some speed v. Note that equati<strong>on</strong> (2.6) has the shape of a sine wave at any<br />

time t. However, this sine wave moves as time passes. For example, at t = 0<br />

the wave vanishes at x = 0. On the other h<strong>and</strong>, at time t = π/2v, at x = 0 we<br />

3 Charges <strong>and</strong> currents placed in water, ir<strong>on</strong>, plastic, <strong>and</strong> other materials are associated<br />

with somewhat different values of electric <strong>and</strong> magnetic fields, described by parameters ǫ <strong>and</strong><br />

µ that depend <strong>on</strong> the materials. This is due to what are called ‘polarizati<strong>on</strong> effects’ within the<br />

material, where the presence of the charge (say, in water) distorts the equilibrium between<br />

the positive <strong>and</strong> negative charges that are already present in the water molecules. This is<br />

a fascinating topic (leading to levitating frogs <strong>and</strong> such) but is too much of a digressi<strong>on</strong> to<br />

discuss in detail here. See PHY212 or the advanced E & M course. The subscript 0 <strong>on</strong> ǫ 0 <strong>and</strong><br />

µ 0 indicates that they are the vacuum values or, as physicists of the time put it, the values<br />

for ‘free space.’

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