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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
An 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
(cΔt´)2
=
v
 Imagine a spaceship travelling at speed v between two stars a
distance Δx 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/v
 The observer in the spaceship also sees Δt´ = Δx´/v where v is the
same for both frames
 We know from time dilation that Δt´=
 Thus the measured lengths must be different as well! The
observer on the spaceship sees a contracted length Δx´ = 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=3xm/s t
ct ct’
 If an object, ct’, is moving and
another object, ct is at rest, relative
to ct’, it looks like ct is moving
Tilted Axis
ct’
x’
θ
 Spacetime distance
between 2 points:
s2
x2
+ y2
+ z2
- (ct)2
 The speed of light is the
same for all axis
x=ct
1. 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

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Special Relativity theory of Einstein...

  • 2.  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
  • 3.  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
  • 4. c 2d d v mirror An observer inside a moving train views a ray of light as follows:
  • 5. An observer outside a moving train, on the ground, at rest views a ray of light as follows: d (cΔt´)2 = v
  • 6.  Imagine a spaceship travelling at speed v between two stars a distance Δx 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/v  The observer in the spaceship also sees Δt´ = Δx´/v where v is the same for both frames  We know from time dilation that Δt´=  Thus the measured lengths must be different as well! The observer on the spaceship sees a contracted length Δx´ = 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
  • 7.  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
  • 8.  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
  • 9. ct x  An object sitting at rest, whose position (x) stays the same x ct  An object with some velocity, v
  • 10.  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
  • 12. 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=3xm/s t
  • 13. ct ct’  If an object, ct’, is moving and another object, ct is at rest, relative to ct’, it looks like ct is moving Tilted Axis ct’ x’ θ  Spacetime distance between 2 points: s2 x2 + y2 + z2 - (ct)2  The speed of light is the same for all axis x=ct
  • 14. 1. 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
  • 15. 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.
  • 16. 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.
  • 17. 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
  • 18. Momentum & Energy: Adding Velocities: Special Relativity: Time Dilation: Length Contraction: Equations to Know