Fundamentals of Time and Relativity

Light Cone

  • There is a fundamental distinction between what is measured in relativity and what is visually observed.
  • What an observer sees at a particular instant of time, is light received from events on his past light cone.

In the literature one finds many thought experiments that try to explain time dilatation and Lorentz contraction by visualizing these effects for certain situations. However, there is a fundamental difference between physical measurement with respect to a grid of spacetime coordinates, on the one hand, and visual appearance on the other.

To understand what an inertial observer O actually sees at a particular event E on his worldline, one must consider the photon worldlines that pass through E . These worldlines are the generators of the past light cone of E . For an event P to be on the past light cone of E , the displacement four-vector Δx=(Δt,Δx) from P to E must be null and future-pointing.

Light emitted from a source S at P arrives at the observer from the direction of the unit vector n:=Δx/Δt , where Δx is the three-distance from the source to O . The unit sphere around the observer traced out by the the set of directions {n} is called the ‘sky’. All that the observer sees at any instant of time can be mapped onto this sphere; see Fig. 6.1.

Ruimtetijddiagram
Fig 6.1 The 'sky' and its map onto the tangent plane (the ‘screen’) by stereo-graphic projection from the point θ=π . The angle subtended by an arc of a circle at the circumference is half of the angle subtended at the center.

Let us assume that the emitted light consists of photons having frequency four-vector k=(κ,k) , with κ=| k |=2πν and k=κn . For an observer stationary with respect to the source, the observed light-frequency is equal to the emitted frequency κ . However, for a moving observer the frequency of light, i.e., the color, is different (Doppler shift) as is the observed direction (light aberration).   

  • The visual appearance of an object is affected by the varying lengths of time that light takes to travel from different points on the object to one's eye.
  • Relativity theory, in particular the element of time dilation, is required to correctly account for the observed effects of Doppler shift and aberration.