special relativity

The equation explained

t′=φ(−v)β(−v){τ+vV2ξ}=φ(v)φ(−v)t,x′=φ(−v)β(−v){ξ+vτ}=φ(v)φ(−v)x,y′=φ(−v)η=φ(v)φ(−v)y,z′=φ(−v)ζ=φ(v)φ(−v)z.\begin{aligned} t' &= \varphi(-v) \beta(-v) \left\{ \tau + \frac{v}{V^2} \xi \right\} &&= \varphi(v) \varphi(-v) t , \\ x' &= \varphi(-v) \beta(-v) \{ \xi + v \tau \} &&= \varphi(v) \varphi(-v) x , \\ y' &= \varphi(-v) \eta &&= \varphi(v) \varphi(-v) y , \\ z' &= \varphi(-v) \zeta &&= \varphi(v) \varphi(-v) z . \end{aligned}
In wordsThe time of the third system and its coordinates, reached by transforming twice: first into the moving system's time and its coordinates, then back with the speed reversed, through the unknown function at each speed, the factor and the velocity of light. What comes out is the stationary system's own time and coordinates, each multiplied by the two unknown functions.OverviewThe transformation applied twice: into a system moving with the speed, then into one moving back with the same speed. Everything returns to the stationary system's letters, multiplied by the two unknown factors.Full explanationThis is the device that determines the unknown function. A third system is introduced, moving relative to the moving system with the velocity −v-v along its first axis, so that it is at rest relative to the stationary system. The transformation of p. 900 is applied twice, the second time with −v-v in place of vv. Each pair of terms that the reversal of sign produces cancels, and what is left in each line is the stationary system's own quantity multiplied by φ(v)φ(−v)\varphi(v) \varphi(-v). The factor β\beta does not survive: it appears once in each application and the two cancel, because β\beta is the same for vv and for −v-v.Every stepβ(−v)=β(v)\beta(-v) = \beta(v)The factor is built from (vV)2\left( \frac{v}{V} \right)^2, so reversing the sign of the velocity leaves it unchanged. The paper still writes β(−v)\beta(-v) in the display, to show where it came from.τ+vV2ξ=φ(v)β[(t−vV2x)+vV2(x−vt)]=φ(v)β t(1−v2V2)=φ(v)tβ\tau + \frac{v}{V^2} \xi = \varphi(v) \beta \left[ \left( t - \frac{v}{V^2} x \right) + \frac{v}{V^2} (x - v t) \right] = \varphi(v) \beta \, t \left( 1 - \frac{v^2}{V^2} \right) = \varphi(v) \frac{t}{\beta}The bracket in the first line, with the first transformation put in. The two terms in xx cancel exactly, and β(1−v2V2)\beta \left( 1 - \frac{v^2}{V^2} \right) is 1β\frac{1}{\beta}.φ(−v)β⋅φ(v)tβ=φ(v)φ(−v) t\varphi(-v) \beta \cdot \varphi(v) \frac{t}{\beta} = \varphi(v) \varphi(-v) \, tMultiply by what stands in front of the bracket. The two factors cancel, and the time of the third system is the stationary system's time multiplied by the two unknown functions.ξ+vτ=φ(v)β[(x−vt)+v(t−vV2x)]=φ(v)β x(1−v2V2)=φ(v)xβ\xi + v \tau = \varphi(v) \beta \left[ (x - v t) + v \left( t - \frac{v}{V^2} x \right) \right] = \varphi(v) \beta \, x \left( 1 - \frac{v^2}{V^2} \right) = \varphi(v) \frac{x}{\beta}The same for the first coordinate. Here it is the two terms in tt that cancel, and the same bracket appears.φ(−v)η=φ(−v)φ(v) y\varphi(-v) \eta = \varphi(-v) \varphi(v) \, yAcross the motion there is no bracket at all: each application multiplies by its own unknown function, and the two stand side by side.Historian's marginThe third system is at rest relative to the stationary one, and the paper says why in the next sentence: the relations between the two sets of coordinates do not contain the time. That is the whole of the argument, and it is worth noticing how little it assumes. It does not assume that the transformation is its own inverse, nor that reversing the velocity reverses the transformation; it assumes only that going out with vv and back with −v-v must leave a system at rest relative to where it started.Also

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