
SECTION 10.2. OSCILLATORY PROPERTIES OF A TUNNEL SOURCE 269
Before providing the results of the numerical analysis of these integrals, we briefly
comment on the physical picture.
According to (10.27) to (10.29), the density of electron excitations in thin
superconducting film oscillates with a small amplitude near its steady-state value owing
to the existence of macroscopic phase coherence in a system of single-electron
excitations. The interaction between the external electromagnetic radiation and the
oscillating electron density of states causes the scattering of the electromagnetic
wave with the formation of satellites at frequencies
The collision operator (10.30) allows one to calculate the response of the
nonequilibrium system, for example, to find the relative intensities of the satellites
in the reflected radiation. From the point of view of spectroscopic experiments,
however, it is easier to deal with the absorption coefficient of the system (specifi-
cally, with the imaginary part of the dielectric constant) or, in other words, with
characteristics of the wave that passes through the film.
Consider a test wave passing through one of the films of an equilibrium
superconducting junction. The absorption coefficient (up to a constant factor) is
given by formula (10.34). We assume that the oscillations of the type mentioned
earlier occur in the film. Then the absorption coefficient would also oscillate in
accordance with (10.33). As a result, the amplitude of the transmitting wave would
be modulated (we assume that and the satellites would appear. The
estimate of their relative intensity is as follows:
The presence of a second film in the junction, in which oscillations also occur,
somewhat distorts this simple picture. We will return to this question later.
Consider now the results of the numerical analysis of the junction’s behavior.
The function was calculated for three metals: lead,
niobium, and tantalum with the parameters shown in Table 10.1 (the data for
aluminum will be used later, in further considerations).
The growth of P with a drop in temperature (Fig. 10.5) is due to the reduction
in the number of equilibrium excitations, which makes the film effectively more
transparent [for convenience Fig. 10.5 shows the dependence in the BCS
*The value of was introduced in calculations as a cutoff factor to remove divergence at the integration
over in (10.35).