the4thamigo_uk
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I was thinking again about the enclosed black body thought experiment. It seems for a 'steady state' when the outer body is maintained at constant temperature, we can equate the net energy flow for the inner body and make the following equation :
total power emitted from outer body = total radiative power lost by inner body.
However, if neither body is maintained at a constant temperature we could argue that we could still make this identity. Niaevely we will get the same result, that the temperatures of the two bodies in thermal equilibrium are different. Which is a contradiction in terms.
It would seem that the crucial difference is that there is a finite distance between the inner surface of the outer body and the outer surface of the inner body. Hence the radiation must travel a distance (R-r) and therefore take a finite time (R-r)/c.
So we have a subtle set of differential equations :
\frac{dQ_{i}(t)}{dt} = k_{i}\frac{dT_{i}(t)}{dt} = 4\pi R_{o}^{2} \sigma T_{o}^{4} (t - \Delta t) - 4\pi R_{i}^{2} \sigma T_{i}^{4} (t)
\frac{dQ_{o}(t)}{dt} = k_{o}\frac{dT_{o}(t)}{dt} = 4\pi R_{i}^{2} \sigma T_{i}^{4} (t - \Delta t) - 4\pi R_{o}^{2} \sigma T_{o}^{4} (t)
\Delta t = \frac{R_{o} - R_{i}}{c}
Q - net heat flow into body
T - temperature of body
t- time (brackets denote function arguments)
k - specific heat of body
R - radius of body
subscripts denote _{i}nner and _{o}uter black body
It seems to me that this must be the crucial difference between the two systems. Problem is I have no idea how to go about solving this set of equations? What techniques are required when there is a shift \Delta T to the variables? I wonder if there is potential for a harmonic type damped oscillation to thermal equilibrum or would it be a nice smooth decline?
total power emitted from outer body = total radiative power lost by inner body.
However, if neither body is maintained at a constant temperature we could argue that we could still make this identity. Niaevely we will get the same result, that the temperatures of the two bodies in thermal equilibrium are different. Which is a contradiction in terms.
It would seem that the crucial difference is that there is a finite distance between the inner surface of the outer body and the outer surface of the inner body. Hence the radiation must travel a distance (R-r) and therefore take a finite time (R-r)/c.
So we have a subtle set of differential equations :
\frac{dQ_{i}(t)}{dt} = k_{i}\frac{dT_{i}(t)}{dt} = 4\pi R_{o}^{2} \sigma T_{o}^{4} (t - \Delta t) - 4\pi R_{i}^{2} \sigma T_{i}^{4} (t)
\frac{dQ_{o}(t)}{dt} = k_{o}\frac{dT_{o}(t)}{dt} = 4\pi R_{i}^{2} \sigma T_{i}^{4} (t - \Delta t) - 4\pi R_{o}^{2} \sigma T_{o}^{4} (t)
\Delta t = \frac{R_{o} - R_{i}}{c}
Q - net heat flow into body
T - temperature of body
t- time (brackets denote function arguments)
k - specific heat of body
R - radius of body
subscripts denote _{i}nner and _{o}uter black body
It seems to me that this must be the crucial difference between the two systems. Problem is I have no idea how to go about solving this set of equations? What techniques are required when there is a shift \Delta T to the variables? I wonder if there is potential for a harmonic type damped oscillation to thermal equilibrum or would it be a nice smooth decline?
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