The analysis on Computational Blackbody Radiation (with book) shows that a radiating body can be seen as a linear high gain amplifier with a high-frequency cut-off scaling with noise temperature, modeled by a wave equation with small damping, which after Fourier decomposition in space takes the form of a damped linear oscillator for each wave frequency \nu:
- \ddot u_\nu +\nu^2u_\nu - \gamma\dddot u_\nu = f_\nu,
where u_\nu(t) is oscillator amplitude and f_\nu (t) signal amplitude of wave frequency \nu with t time, the dot indicates differentiation with respect to t, and \gamma is a small constant satisfying \gamma\nu^2 << 1 and the frequency is subject to a cut-off of the form \nu < \frac{T_\nu}{h}, where
- T_\nu =\overline{\dot u_\nu^2}\equiv\int_I \dot u_\nu^2(t)\, dt,
is the (noise) temperature of frequency of \nu, I a unit time interval and h is a constant representing a level of finite precision.
The analysis shows under an assumption of near resonance, the following basic relation in stationary state:
- \gamma\overline{\ddot u_\nu^2} \approx \overline{f_\nu^2},
as a consequence of small damping guiding u_\nu (t) so that \dot u_\nu(t) is out of phase with f_\nu(t) and thus "pumps" the system little. The result is that the signal f_\nu (t) is balanced to major part by the oscillator
- \ddot u_\nu +\nu^2u_\nu,
and to minor part by the damping
- - \gamma\dddot u_\nu,
because
- \gamma^2\overline{\dddot u_\nu^2} \approx \gamma\nu^2 \gamma\overline{\ddot u_\nu^2}\approx\gamma\nu^2\overline{f_\nu^2} <<\overline{f_\nu^2}.
This means that the blackbody can be viewed to act as an amplifier radiating the signal f_\nu under the small input -\gamma \dddot u_\nu, thus with a high gain. The high frequency cut-off then gives a requirement on the temperature T_\nu, referred to as noise temperature, to achieve high gain.
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