# PlanetPhysics/Time Dilation

Time dilation is the difference in time intervals between inertial frames of reference moving with respect to each other. This is usually studied in Physics, but here is the mathematics behind it.\linebreak Consider a train moving with speed $u$ and an observer standing still. Let the station (where observer is standing) be inertial frame of reference $S$, and train be inertial frame of reference $S'$. A light source and a mirror are placed vertically above each other in the train as shown. \begin{figure}
   \includegraphics{draw2.eps} \caption{Path of light according to a person in the train}
\end{figure} Let $\Delta t_{0}$ denote the time taken for light to travel from the source back to the source according to a person on the train. In other words, in frame of reference $S'$ the time taken for light to travel is given by: Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "http://localhost:6011/en.wikiversity.org/v1/":): {\displaystyle \Delta t_0 = \frac{2d}} where $c$ is the speed of light. The round-trip time measured by the observer in frame $S$ is a different interval $\Delta t$. This is what he would observe: \begin{figure}
   \includegraphics{draw3.eps} \caption{Path of light according to observer}
\end{figure} To the observer, the events of light leaving the source and coming back occur at different points in space. The distance travelled by light in this case is $2l$, and by the Pythagorean theorem: $l={\sqrt {d^{2}+\left({\frac {u\Delta t}{2}}\right)^{2}}}$ Now the time for light to travel, according to observer, is: $\Delta t={\frac {2l}{=}}{\frac {2}{\sqrt {d^{2}+\left({\frac {u\Delta t}{2}}\right)^{2}}}}$ But we know from the equation above that $\Delta t_{0}=2d/c$, and by rearranging, $d=c\Delta t_{0}/2$. Now we substitute to get: $\Delta t={\frac {2}{\sqrt {\left({\frac {c\Delta t_{0}}{2}}\right)^{2}+\left({\frac {u\Delta t}{2}}\right)^{2}}}}$ Now lets rearrange and solve for $\Delta t$: $c^{2}\Delta t^{2}=c^{2}\Delta t_{0}^{2}+u^{2}\Delta t^{2}$ $(c^{2}-u^{2})\Delta t^{2}=c^{2}\Delta t_{0}^{2}$ $\Delta t^{2}={\frac {c^{2}\Delta t_{0}^{2}}{c^{2}-u^{2}}}$ Dividing the numerator and denominator by $c^{2}$ and taking the square root yields: $\Delta t={\frac {\Delta t_{0}}{\sqrt {1-u^{2}/c^{2}}}}$ Since the expression $1/{\sqrt {1-u^{2}/c^{2}}}$ occurs quite frequently in relativity, sometimes it is preferable to use the letter $\gamma$ to represent it. Therefore: $\gamma ={\frac {1}{\sqrt {1-u^{2}/c^{2}}}}$ The equation for time dilation can then be written this way: $\Delta t=\gamma \Delta t_{0}$ \paragraph{History and Uses} This is a very famous result in relativity, and in fact it was the basis for the evolvement of relativistic mechanics, in which Albert Einstein defiantly challenged Newton's equations for objects with very high speeds. From this, mechanics was classified into two branches: Newtonian mechanics and Relativistic mechanics. It was also the basis of Einstein's theory of relativity $E=mc^{2}$, and many other equations in relativity. The time dilation equation can be used to calculate the difference in time intervals between two inertial frames moving with respect to each other.