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nydus/The Theory of Heat RadiationPublic

This text examines the physical distinction between heat conduction and heat radiation, noting that radiation is independent of the medium through which it passes. It establishes that heat rays are physically identical to light rays and applies the principles of experimental optics to the study of thermal radiation.

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149.

The evaluation of these integrals is greatly simplified by the fact that, according to [eqn:(239)] (239), ω0τ and therefore also ωτ are large numbers, at least for all values of ω which have to be considered. Hence it is possible to replace the expression sin2ωτ in the integral J1 by its mean value 12 and thus we obtain: J1=14ω0. It is readily seen that, on account of the last factor, we obtain J2=0 for the second integral.

In order finally to calculate the third integral J3 we shall lay off in the series of values of ω on both sides of ω0 an interval extending from ω1 (<ω0) to ω2 (>ω0) such that ω0ω1ω0andω2ω0ω0are small,\Label[eqn](243)\upshape (243) and simultaneously (ω0ω1)τand(ω2ω0)τare large.\Label[eqn](244)\upshape (244) This can always be done, since ω0τ is large. If we now break up the integral J3 into three parts, as follows: J3=0=0ω1+ω1ω2+ω2, it is seen that in the first and third partial integral the expression sin2ω0ω2τ may, because of the condition [eqn:(244)] (244), be replaced by its mean value 12. Then the two partial integrals become: 0ω1ω0dω2(ω0+ω)(ω0ω)2andω2ω0dω2(ω0+ω)(ω0ω)2.\Label[eqn](245)\upshape (245) These are certainly smaller than the integrals: 0ω1dω2(ω0ω)2andω2dω2(ω0ω)2

which have the values 12ω1ω0(ω0ω1)and12(ω2ω0)\Label[eqn](246)\upshape (246) respectively. We must now consider the middle one of the three partial integrals: ω1ω2dωω0(ω0+ω)(ω0ω)2·sin2ω0ω2τ. Because of condition [eqn:(243)] (243) we may write instead of this: ω1ω2dω·sin2ω0ω2τ2(ω0ω)2 and by introducing the variable of integration x, where x=ωω02τ and taking account of condition [eqn:(244)] (244) for the limits of the integral, we get: τ4+sin2xdxx2=τ4π. This expression is of a higher order of magnitude than the expressions [eqn:(246)] (246) and hence of still higher order than the partial integrals [eqn:(245)] (245) and the integrals J1 and J2 given above. Thus for our calculation only those values of ω will contribute an appreciable part which lie in the interval between ω1 and ω2, and hence we may, because of [eqn:(243)] (243), replace the separate coefficients An2 and Bn2 in the expression for the total absorbed energy by their mean values A02 and B02 in the neighborhood of ω0 and thus, by taking account of [eqn:(242)] (242), we shall finally obtain for the total value of the energy absorbed by the oscillator in the time τ: 1Lτ8(A02+B02)𝖳.\Label[eqn](247)\upshape (247) If we now, as in [eqn:(158)] (158), define 𝖨, the "intensity of the vibration

exciting the oscillator," by spectral resolution of the mean value of the square of the exciting field-strength z: z2\Strut=0𝖨νdν\Label[eqn](248)\upshape (248) we obtain from [eqn:(235)] (235) and [eqn:(242)] (242): z2\Strut=121(An2+Bn2)=120(An2+Bn2)𝖳dν, and by comparison with [eqn:(248)] (248): 𝖨=12(A02+B02)𝖳. Accordingly from [eqn:(247)] (247) the energy absorbed in the time τ becomes: 𝖨4Lτ,

that is, in the time between two successive emissions, the energy U of the oscillator increases uniformly with the time, according to the law dUdt=𝖨4L=a.\Label[eqn](249)\upshape (249) Hence the energy absorbed by all N oscillators in the time dt is: N𝖨4Ldt=Nadt.\Label[eqn](250)\upshape (250)

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