Time dilation


Time dilation is the phenomenon where the duration of a phenomenon increases if it occurs while moving relative to the observer. In other words, time passes slower for things that move (compared to the observer). For instance, if a stationary (with respect to the observer) kettle takes one minute to boil water, a moving kettle will take more than a minute to boil the water. If Δtrest\Delta t_\text{rest} is a duration measured by a clock at rest and Δtmoving\Delta t_\text{moving} is the same duration measured by a moving clock

Δtmoving=γΔtrest\Delta t_\text{moving}=\gamma\Delta t_\text{rest}

where γ\gamma is the relativistic gamma. The moving time is dilated by a factor γ\gamma.

Thought experiment

Imagine a train cart traveling at some constant speed along a smooth, straight track. In the center of the cart, a light bulb is attached to the ceiling, initially off. Imagine someone turns on the bulb. The light takes some time to reach the floor of the cart. What is this time? For someone on the train, everything is at rest, so the time is exactly the amount of time Δtrest\Delta t_{\text{rest}} it takes for the light, traveling at the speed of light cc, to traverse the height hh of the cart,

Δtrest=hc\Delta t_{\text{rest}}=\frac{h}{c}

where "rest" denotes that we are in the frame of reference of the cart and the light is at rest with respect to the observer. On the other hand, for someone on the ground, the space to travel is greater, as it is the diagonal between the location of the bulb when the light is emitted and the location of the floor after the light has traveled.

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The train, which assume moves at speed vv, travels some distance vΔtv\Delta t while the light reaches the ground. Thus, the actual distance covered is given by the Pythagorean theorem, h2+(vΔtmoving)2\sqrt{ h^{2}+(v\Delta t_\text{moving})^{2} }, and so

Δtmoving=h2+(vΔtmoving)2c\Delta t_\text{moving}=\frac{\sqrt{ h^{2}+(v\Delta t_\text{moving})^{2} }}{c}

Extracting Δtmoving\Delta t_\text{moving} yields

Δtmoving=hc11v2/c2\Delta t_\text{moving}=\frac{h}{c} \frac{1}{\sqrt{ 1-v^{2}/c^{2} }}

By defining the parameter

γ11v2/c2\gamma\equiv \frac{1}{\sqrt{ 1-v^{2}/c^{2} }}

and substituting Δtrest\Delta t_\text{rest}, the ground-observed (moving) time is related to train-observed (rest) time by

Δtmoving=γΔtrest\boxed{\Delta t_\text{moving}=\gamma \Delta t_\text{rest}}

Seeing how γ1\gamma\geq 1, we can make we can see that the ground time Δtmoving\Delta t_\text{moving} must be longer than the train time by a factor γ\gamma: we call this time dilation.

From Lorentz transformations

Time dilation can be seen by applying a Lorentz transformation. Say an observer in a frame of reference S\mathcal{S} at time t=0t=0 reads several clocks moving in a different frame of reference S\mathcal{S}'. The observer finds that the clocks all read different times, depending on their location. The Lorentz transformation in time is

t=γvc2xt'=-\gamma \frac{v}{c^{2}}x

Evidently, the clocks at positive xx will be behind, whereas those at negative xx will be ahead. Only the clock at x=0x=0 (and so t=0t'=0) matches the time of the stationary clocks in S\mathcal{S}. Thus, moving clocks becomes desynchronized from each other and only stationary clocks can be trusted to share correctness. You can do the same exact argument in the reverse direction by doing the inversion transformation

t=γvc2xt=\gamma \frac{v}{c^{2}}x'

only now the time discrepancy works in reverse due to the change in sign.

Say now the observer in S\mathcal{S} looks only at a clock that is at rest in S\mathcal{S}' at some position x=ax'=a and watches it over a time interval Δt=tendtstart\Delta t=t_\text{end}-t_\text{start}. Since xx' is fixed (the clock is at rest within its frame, and thus moving at vv in S\mathcal{S}), then the time transformation

t=γ(t+vc2a)t=\gamma\left( t'+ \frac{v}{c^{2}}a \right)

gives

Δt=tendtstart=γ(tendvc2a)γ(tstartvc2a)=γ(tendtstart)=γΔt\Delta t=t_\text{end}-t_\text{start}=\gamma\left( t'_\text{end}- \frac{v}{c^{2}}a \right)- \gamma\left( t'_\text{start}- \frac{v}{c^{2}}a \right)=\gamma(t'_\text{end}-t'_\text{start})=\gamma \Delta t'

or

Δt=Δtγ\Delta t'=\frac{\Delta t}{\gamma}

which is the time dilation formula, where ΔtΔtmoving\Delta t\equiv \Delta t_\text{moving} (since the clock is moving in S\mathcal{S}) and ΔtΔtrest\Delta t'\equiv \Delta t_\text{rest} (since the clock is at rest in S\mathcal{S}').