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Wave Propagation in Linear Media | re-examined

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Part I<br />

<strong>Wave</strong> propagation phenomena<br />

Soon after the formulation of E<strong>in</strong>ste<strong>in</strong>'s theory of <strong>re</strong>lativity, a discussion arose whether or not<br />

certa<strong>in</strong> types of waves can propagate faster than light. These a<strong>re</strong> evanescent electromagnetic<br />

waves and tunnell<strong>in</strong>g quantum particles that a<strong>re</strong> formally equivalent to some electromagnetic<br />

cases. In <strong>re</strong>cent years, the fairly old debate g<strong>re</strong>w <strong>in</strong> <strong>in</strong>tensity when experimental <strong>re</strong>sults<br />

seemed to support `superlum<strong>in</strong>al' theories. The rst part of this work is the<strong>re</strong>fo<strong>re</strong> dedicated<br />

to the many facets of the discussion.<br />

To provide an <strong>in</strong>sight<strong>in</strong>to the subject, the rst chapters give a brief overview on the de nitions<br />

of wave propagation velocities <strong>in</strong> general and on the faster-than-light issue <strong>in</strong> particular. The<br />

variety of op<strong>in</strong>ions and theories is rather unsatisfactory from a practical po<strong>in</strong>t of view, and so<br />

the subsequent chapters p<strong>re</strong>sent anumber of one-dimensional case studies to explo<strong>re</strong> the problems<br />

further. The rst among these a<strong>re</strong> concerned with the propagation of electromagnetic<br />

waves with a special focus on evanescent modes. We shall beg<strong>in</strong> with simple monochromatic<br />

examples whe<strong>re</strong> closed exp<strong>re</strong>ssions for a propagation velocity can still be found. We then<br />

extend the monochromatic <strong>in</strong>vestigation to dispersive media and nally solve the wave equation<br />

for broad-band signals <strong>in</strong> a lossless plasma as well as <strong>in</strong> a <strong>re</strong>ctangular wave guide. These<br />

last examples will demonstrate that sudden signal changes travel at a wave front velocity no<br />

faster than the speed of light.<br />

The second portion of these case studies is dedicated to the classical quantum mechanical<br />

tunnel e ect. Like <strong>in</strong> the sections befo<strong>re</strong>, we start with formulat<strong>in</strong>g the problem for a plane<br />

wave, but immediately extend the <strong>re</strong>sults to the general case of signals with arbitrary bandwidth.<br />

We shall then explo<strong>re</strong> the scatter<strong>in</strong>g of a particle o a potential step. Subsequently,<br />

after hav<strong>in</strong>g looked <strong>in</strong>to quantum mechanical tunnell<strong>in</strong>g time de nitions for plane waves, we<br />

deal with a particle tunnell<strong>in</strong>g through a <strong>re</strong>ctangular barrier. In all these cases, we must<br />

employ numerical techniques to solve the Fourier <strong>in</strong>tegrals that constitute the solutions of the<br />

wave equations. The examples will show that for very small-band pulses, the <strong>re</strong>sults could<br />

be <strong>in</strong>terp<strong>re</strong>ted as superlum<strong>in</strong>al propagation of a wave packet. However, as the bandwidth is<br />

<strong>in</strong>c<strong>re</strong>ased, the tunnell<strong>in</strong>g time becomes even negative, which is quite an absurd <strong>re</strong>sult. So we<br />

eventually arrive at the still open question whether a signal pulse is adequately described by<br />

its peak or cent<strong>re</strong> of mass, or what actually forms the <strong>in</strong>formation be<strong>in</strong>g transmitted.<br />

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