Translation

On the Electrodynamics of Moving Bodies

Zur Elektrodynamik bewegter Körper

by A. Einstein

I. Kinematical Part.

II. Electrodynamical Part.

§ 8. Transformation of the Energy of Light Rays. Theory of the Radiation Pressure Exerted on Perfect Mirrors.

Since A2/8πA^2/8\pi is equal to the light energy per unit volume, we have to regard A′2/8πA'^2/8\pi, by the principle of relativity, as the light energy in the moving system. Hence A′2/A2A'^2/A^2 would be the ratio of the “measured-in-motion” and the “measured-at-rest” energy of a given light complex, if the volume of a light complex were the same measured in KK and measured in kk. This, however, is not the case. If aa, bb, cc are the direction cosines of the wave normal of the light in the stationary system, then through the surface elements of the spherical surface moving with the velocity of light (x−Vat)2+(y−Vbt)2+(z−Vct)2=R2(x - V a t)^2 + (y - V b t)^2 + (z - V c t)^2 = R^2Position in the stationary systemSpeed of lightDirection cosine (stationary system)Time in the stationary systemPosition in the stationary systemDirection cosine (stationary system)Position in the stationary systemDirection cosine (stationary system)Light-sphere radiusExplain this equation no energy passes; we can therefore say that this surface permanently encloses the same light complex. We ask for the quantity of energy which this surface encloses, regarded in the system kk, that is, for the energy of the light complex relative to the system kk.

The spherical surface is — regarded in the moving system — an ellipsoidal surface, which at the time τ=0\tau = 0 has the equation: (βξ−aβvVξ)2+(η−bβvVξ)2+(ζ−cβvVξ)2=R2.\left( \beta \xi - a \beta \frac{v}{V} \xi \right)^2 + \left( \eta - b \beta \frac{v}{V} \xi \right)^2 + \left( \zeta - c \beta \frac{v}{V} \xi \right)^2 = R^2 .Lorentz factorPosition in the moving systemDirection cosine (stationary system)Speed of the moving systemSpeed of lightPosition in the moving systemDirection cosine (stationary system)Position in the moving systemDirection cosine (stationary system)Light-sphere radiusExplain this equation If SS is called the volume of the sphere and S′S' that of this ellipsoid, then, as a simple calculation shows: S′S=1−(vV)21−vVcos⁡φ.\frac{S'}{S} = \frac{\sqrt{1 - \left( \frac{v}{V} \right)^2}}{1 - \frac{v}{V} \cos \varphi} .Volume of the light packet, moving systemVolume of the light packet, stationary systemSpeed of the moving systemSpeed of lightAngle to the motion, stationary systemExplain this equation If, therefore, we call EE the light energy measured in the stationary system and E′E' the light energy measured in the moving system, enclosed by the surface under consideration, we obtain: E′E=A′28πS′A28πS=1−vVcos⁡φ1−(vV)2,\frac{E'}{E} = \frac{\frac{A'^2}{8\pi} S'}{\frac{A^2}{8\pi} S} = \frac{1 - \frac{v}{V} \cos \varphi}{\sqrt{1 - \left( \frac{v}{V} \right)^2}} ,Energy of the light packet, moving systemEnergy of the light packet, stationary systemLight amplitude (moving system)Volume of the light packet, moving systemLight amplitude (stationary system)Volume of the light packet, stationary systemSpeed of the moving systemSpeed of lightAngle to the motion, stationary systemExplain this equation a formula which for φ=0\varphi = 0 passes over into the simpler one: E′E=1−vV1+vV.\frac{E'}{E} = \sqrt{\frac{1 - \frac{v}{V}}{1 + \frac{v}{V}}} .Energy of the light packet, moving systemEnergy of the light packet, stationary systemSpeed of the moving systemSpeed of lightExplain this equation

It is remarkable that the energy and the frequency of a light complex vary with the observer’s state of motion according to the same law.

Now let the coordinate plane ξ=0\xi = 0 be a perfectly reflecting surface, at which the plane waves considered in the last section are reflected. We ask for the light pressure exerted on the reflecting surface, and for the direction, frequency and intensity of the light after reflection.

Let the incident light be defined by the quantities AA, cos⁡φ\cos \varphi, ν\nu (referred to the system KK). Regarded from kk, the corresponding quantities are: A′=A1−vVcos⁡φ1−(vV)2,A' = A \frac{1 - \frac{v}{V} \cos \varphi}{\sqrt{1 - \left( \frac{v}{V} \right)^2}} ,Light amplitude (moving system)Light amplitude (stationary system)Speed of the moving systemSpeed of lightAngle to the motion, stationary systemExplain this equation cos⁡φ′=cos⁡φ−vV1−vVcos⁡φ,\cos \varphi' = \frac{\cos \varphi - \frac{v}{V}}{1 - \frac{v}{V} \cos \varphi} ,Angle to the motion, moving systemAngle to the motion, stationary systemSpeed of the moving systemSpeed of lightExplain this equation ν′=ν1−vVcos⁡φ1−(vV)2.\nu' = \nu \frac{1 - \frac{v}{V} \cos \varphi}{\sqrt{1 - \left( \frac{v}{V} \right)^2}} .Frequency, moving systemFrequency, stationary systemSpeed of the moving systemSpeed of lightAngle to the motion, stationary systemExplain this equation For the reflected light we obtain, when we refer the process to the system kk: A′′=A′,cos⁡φ′′=−cos⁡φ′,ν′′=ν′.\begin{aligned} A'' &= A' , \\ \cos \varphi'' &= - \cos \varphi' , \\ \nu'' &= \nu' . \end{aligned}Reflected light amplitude (moving system)Light amplitude (moving system)Reflected propagation angle (moving system)Angle to the motion, moving systemReflected light frequency (moving system)Frequency, moving systemExplain this equation Finally, by transforming back to the stationary system KK, we obtain for the reflected light: A′′′=A′′1+vVcos⁡φ′′1−(vV)2=A1−2vVcos⁡φ+(vV)21−(vV)2,A''' = A'' \frac{1 + \frac{v}{V} \cos \varphi''}{\sqrt{1 - \left( \frac{v}{V} \right)^2}} = A \frac{1 - 2 \frac{v}{V} \cos \varphi + \left( \frac{v}{V} \right)^2}{1 - \left( \frac{v}{V} \right)^2} ,Reflected light amplitude (stationary system)Reflected light amplitude (moving system)Speed of the moving systemSpeed of lightReflected propagation angle (moving system)Light amplitude (stationary system)Angle to the motion, stationary systemExplain this equation cos⁡φ′′′=cos⁡φ′′+vV1+vVcos⁡φ′′=−(1+(vV)2)cos⁡φ−2vV1−2vVcos⁡φ+(vV)2,\cos \varphi''' = \frac{\cos \varphi'' + \frac{v}{V}}{1 + \frac{v}{V} \cos \varphi''} = - \frac{\left( 1 + \left( \frac{v}{V} \right)^2 \right) \cos \varphi - 2 \frac{v}{V}}{1 - 2 \frac{v}{V} \cos \varphi + \left( \frac{v}{V} \right)^2} ,Reflected propagation angle (stationary system)Reflected propagation angle (moving system)Speed of the moving systemSpeed of lightAngle to the motion, stationary systemExplain this equation ν′′′=ν′′1+vVcos⁡φ′′1−(vV)2=ν1−2vVcos⁡φ+(vV)2(1−vV)2.\nu''' = \nu'' \frac{1 + \frac{v}{V} \cos \varphi''}{\sqrt{1 - \left( \frac{v}{V} \right)^2}} = \nu \frac{1 - 2 \frac{v}{V} \cos \varphi + \left( \frac{v}{V} \right)^2}{\left( 1 - \frac{v}{V} \right)^2} .Reflected frequencyReflected light frequency (moving system)Speed of the moving systemSpeed of lightReflected propagation angle (moving system)Frequency, stationary systemAngle to the motion, stationary systemExplain this equation

The energy (measured in the stationary system) incident on unit area of the mirror per unit time is evidently A2/8π(Vcos⁡φ−v)A^2/8\pi (V \cos \varphi - v). The energy leaving unit area of the mirror in unit time is A′′′2/8π(−Vcos⁡φ′′′+v)A'''^2/8\pi (- V \cos \varphi''' + v). By the energy principle, the difference of these two expressions is the work done by the light pressure in unit time. If we set the latter equal to the product P⋅vP \cdot v, where PP is the light pressure, we obtain: P=2A28π(cos⁡φ−vV)21−(vV)2.P = 2 \frac{A^2}{8\pi} \frac{\left( \cos \varphi - \frac{v}{V} \right)^2}{1 - \left( \frac{v}{V} \right)^2} .Radiation pressure on a mirrorLight amplitude (stationary system)Angle to the motion, stationary systemSpeed of the moving systemSpeed of lightExplain this equation To a first approximation we obtain, in agreement with experience and with other theories P=2A28πcos⁡2φ.P = 2 \frac{A^2}{8\pi} \cos^2 \varphi .Radiation pressure on a mirrorLight amplitude (stationary system)Angle to the motion, stationary systemExplain this equation

By the method employed here, all problems of the optics of moving bodies can be solved. The essential point is that the electric and magnetic force of the light which is influenced by a moving body are transformed to a coordinate system at rest relative to the body. In this way every problem of the optics of moving bodies is reduced to a series of problems of the optics of bodies at rest.

In conclusion I remark that in working on the problem treated here my friend and colleague M. Besso stood loyally by my side, and that I owe him several valuable suggestions.

Bern, June 1905.

(Received 30 June 1905.)