Special Relativity The laws of mechanics must be the same in all inertial reference frames - PowerPoint Presentation

Special Relativity

The laws of mechanics must be the same in all inertial reference frames Time is the same across all reference frames Simple addition of velocities between frames Galileo’s Principle of Relativity

The laws of physics must be the same in all inertial reference frames The speed of light in vacuum has the same value in all inertial frames, regardless of the velocity of the observer or the velocity of the source emitting the light Einstein’s Principle of Relativity

c 2d   d v mirror A n observer inside a moving train views a ray of light as follows:

An observer outside a moving train, on the ground, at rest views a ray of light as follows: d (c Δ t´) 2   =   v

Imagine a spaceship travelling at speed v between two stars a distance Δ x apart (as measured in the rest frame of the stars)An observer at rest relative to the stars sees the trip take a time Δt=Δx/vThe observer in the spaceship also sees Δ t´ = Δ x´/v where v is the same for both framesWe know from time dilation that Δt´= Thus the measured lengths must be different as well! The observer on the spaceship sees a contracted length Δ x´ = Δx √(1-v2/c2) The factor is so useful in relativity it’s given it’s own symbol γ For time dilation Δt´ = γΔt and for length contraction Δx´ = Δx/γ  Length contraction

Changing your frame of reference will create an observable change in momentum and energy, but they are both still conserved. Invariant mass energy Not affected by reference frame Energy and momentum are not conserved separately, but as a combination This implies that for a particle at rest: !!!!   Momentum & Energy

There is energy in mass Consider a person weighing 100 kg: A few kilograms of fuel of a nuclear source is worth a few tons of fuel of a chemical source A useful relationship for relativistic momentum and energy:   Momentum & Energy

ct x An object sitting at rest, whose position (x) stays the same x ct An object with some velocity, v

Θ = 45º when the object is moving at the speed of light A real object with mass cannot travel at the speed of light Light has no mass So, a real object cannot go beyond 45º from the y axis, in either direction   θ

Elsewhere FUTURE PAST E L S E W H E R E E L S E W H E R E

Strict Causality X 100 ly Planet X is 100 ly away. t= If a signal were sent from earth, at the speed of light, it would take Planet X 100 years to be able to recognize the signal   C=3x m/s   t

ct c t ’ If an object, ct ’, is moving and another object, ct is at rest, relative to ct’, it looks like ct is moving Tilted Axis c t’ x’ θ Spacetime distance between 2 points: s 2 x 2 + y 2 + z 2 - (ct) 2 The speed of light is the same for all axis x=ct

The pole in the barn effect The pole and barn both see each other as being less than 100 m by the gamma factor. At some instance the doors of the barn could be closed and opened, trapping the pole in the barn.The pole sees the doors of the barn close one at a time, and open one at a time Consequences v 100 m 100 m

2. Twin Paradox A B Twin B Leaves on a rocket to mars. Twin A sees twin B as moving close to the speed of light; he sees twin B as 21 and himself as 25. When the rocket turns around, twin 2 sees himself as 25 and twin A as 21. 20 years old 20 years old Once things accelerate, they are no longer in the inertial reference frame. General Relativity deals with accelerated reference frames.

General Relativity a=9.8m/   g=9.8m/   A person in an elevator ascending at 9.8m/ would feel no different than a person in an elevator at rest. They could not determine whether the force they were feeling was from the acceleration of the elevator or the force due to gravity.  

A person standing on an island wants to know how fast a canon ball is coming toward them. Classical version: v1 + v2 = v’ Relativistic version: If the canon were a ‘photon torpedo’ from the starship enterprise moving at the speed of light:   Adding Velocities v1 v2

Momentum & Energy: Adding Velocities:   Special Relativity: Time Dilation: Length Contraction:   Equations to Know