If Φ = 0, this reduces to the simple form

$$ A'^2 = A^2 \frac {1 - \frac {v}{c}} {1 + \frac {v}{c}} $$

From these equations, it appears that for an observer, which moves with

the velocity c towards the source of light, the source should appear

infinitely intense.

§ 8. Transformation of the Energy of the Rays of Light. Theory of the

Radiation-pressure on a perfect mirror.

Since A²/8π is equal to the energy of light per unit volume, we have to

regard A²/8π as the energy of light in the moving system. A′²/A² would

therefore denote the ratio between the energies of a definite

light-complex “measured when moving” and “measured when stationary,” the

volumes of the light-complex measured in K and _k_ being equal. Yet this

is not the case. If _l_, _m_, _n_ are the direction-cosines of the

wave-normal of light in the stationary system, then no energy passes

through the surface elements of the spherical surface

(_x_ - _clt_)² + (_y_ - _cmt_)² + (_z_ - _cnt_)² = R²,

which expands with the velocity of light. We can therefore say, that

this surface always encloses the same light-complex. Let us now consider

the quantity of energy, which this surface encloses, when regarded from

the system _k_, _i.e._, the energy of the light-complex relative to the

system _k_.

Regarded from the moving system, the spherical surface becomes an

ellipsoidal surface, having, at the time τ = 0, the equation:—

$$ (\beta \xi - l \beta \frac {v}{c} \xi)^2 + (\eta - m \beta \frac

{v}{c} \xi)^2 + (\zeta - n \beta \frac {v}{c} \xi)^2 = R^2 $$

If S = volume of the sphere, S′ = volume of this ellipsoid, then a

simple calculation shows that:

$$ \frac {S'}{S} = \frac {\beta}{\sqrt{1 - \frac {v}{c} \cos \Phi}} $$

If E denotes the quantity of light energy measured in the stationary

system, E′ the quantity measured in the moving system, which are

enclosed by the surfaces mentioned above, then

$$ \frac {E'}{E} = \frac {\frac {A'^2}{8\pi} S'}{\frac {A^2}{8\pi}S} =

\frac {1 - \frac {v}{c} \cos \Phi}{\sqrt{1 - \frac {v^2}{c^2}}} $$

The Principle of Relativity · 第 30 / 203 题