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RELATIVITY E van Zyl Part III This is the transformation which is needed to convert a reading x'
in the K' system of coordinates to an x value in the K system, if K' moves
with a speed of v relative to the K system. According to classical Galileian / Newtonian
mechanics: x' = x - vt. A light signal along the positive x axis ( to the right )
of frame K is transformed according to the Relative to K' the transformation is x' - ct' = 0 (2) Space-time points ( called events ) which satisfy (1) must also satisfy (2). i.e. where l is a constant (3) In the negative direction where m is a constant (4) Add (4) to (3)
i.e. (5 i)
Equation (3) Equation (4) Subtract (4) from (3) So that i.e. ..So that (5 ii) The problem now is to find the values of a and b.
For the origin of K', x' = 0 (6) and or , and . v is the relative velocity of the two systems of co-ordinates. The Principle of Relativity states: Relative to K the length of a unit measuring rod at rest to K', must be exactly the same as the length of the rod relative to K' of a unit measuring rod at rest to K. Insert a particular value of t ( time of K ), e.g. t = 0, Then (5 i) becomes x' = ax - bc(0), So that x' = ax If x' increases by 1 unit ( infinitesimally small ) ax = 1 so that (7) Relative to K' where t' = 0 , eliminating t from equations (5 i) and (5 ii) we get: bct = ax - x' and act = ct' + bx . Thus and so that . so that .. . But and from (6)
ie so that . Thus points on the x-axis separated by distance 1 relative to K will be represented by the distance x' = a ( 1 - v2 / c2 )1 and this must be equal to ( from (7) ) . Therefore (8) Equations (6) and (8)
determine the values of a and b . Insert these values of
The time t' can be derived from: It equals the classical transformation divided by |
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