Notes on Relativity and Cosmology - Physics Department, UCSB
Notes on Relativity and Cosmology - Physics Department, UCSB
Notes on Relativity and Cosmology - Physics Department, UCSB
You also want an ePaper? Increase the reach of your titles
YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.
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.’