Einstein’s Relativity Part 2

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Presentation transcript:

Einstein’s Relativity Part 2

Simultaneity is relative, not absolute Observer riding in spaceship at constant velocity sees a flash of light situated in the center of the ship’s chamber hit both ends at the same time But to a stationary observer (or any observer in relative motion), the condition that light travels each way at the same speed in their own frame means that the events will not be simultaneous. In the case pictured, the stationary observer sees the flash hit the back of the ship before the front

One person’s space is another’s time If simultaneity is broken, no one can agree on a universal time that suits all the relative state of motion is important Because the speed of light is constant (and finite) for all observers, space and time are unavoidably mixed we’ve seen an aspect of this in that looking into the distance is the same as looking back in time Space and time mixing promotes unified view of spacetime “events” are described by three spatial coordinates plus a time

The Lorentz Transformation These Equations Relate the Time and Positions of two Different Frames of Reference

The gamma factor Gamma (γ) is a measure of how relativistic you are: When v = 0, γ = 1.0 and things are normal At v = 0.6c, γ = 1.25 a little strange At v = 0.8c, γ = 1.67 Very strange As v→c, γ→∞

What does γ do? Time dilation: clocks on a moving platform appear to tick slower by the factor γ standing on platform, you see the clocks on a fast-moving train tick slowly: people age more slowly, though to them, all is normal Length contraction: moving objects appear to be “compressed” along the direction of travel by the factor γ standing on a platform, you see a shorter train slip past, though the occupants see their train as normal length

Time Dilation T= γT0 T0 = proper time. It’s measured by the observer who is at rest with respect to the clock T = time measured by the observer that sees the clock moving Note: only look at one clock in each problem.

Time Dilation Example A rocket ship moves by you at .866c. The astronaut measures his heart rate at 1beat / second. What do you measure his heart rate to be? To= 1.00s γ = 1/ (1-.8662)1/2 = 2.00 T = γT0 = 2.00s One beat every 2 seconds – he’ll live twice as long as you, all things being equal….

Time Dilation Example A muon has a lifetime 2 microseconds when it is at rest. What does an observer measure the lifetime to be, when the muons are moving at 99%c? To= 2μs γ = 1/ (1-.992)1/2 = 7.10 T = γT0 = 14.2 μs This has been confirmed experimentally. Muons produced in the upper atmosphere should not get to the Earth’s surface – but they do.