Title: By:%20Jennifer%20Doran
1Relativity
2What was Known in 1900
- Newtons laws of motion
- Maxwells laws of electromagnetism
3Contradiction Between Laws
- Newtons Laws
- Predicted that the speed of light should depend
on the motion of the observer and the light source
- Maxwells Laws
- Predicted that light in a vacuum should travel
at a constant speed regardless of the motion of
the observer or source
4Two Postulates of Special Relativity
- The laws of physics are the same for all
non-accelerating observers - The speed of light in a vacuum is constant for
all observers, regardless of motion
5Inconsistencies with Classical Mechanics
- Newtons Laws state that vuV
- Einsteins postulate says that the speed of light
is independent of the motion of all observers and
sources.
6Classical Lorentz Transformation
- x x' u t' y y' z z' t t' OR
- x' x u t y y' z z' t t'
- Then v v' u
- And a a'
- BUT this is only good for ultltv.
- To make the transforms relativistic, assume
- x G (x' u t')
- x' G (x u t)
7Finding G
- A light pulse starts at S at t 0 S' at t' 0
- So in S, x ct, and in S, x c t', by
Einsteins second postulate - Then ct G (c t' u t') G (c u) t'
- And ct' G (c - u) t
- Substitute for t', then ct G(c u)G(c -
u)t/c - Then G2 c2 / (c2-u2) 1/(1- u2/c2)
- G 1/v(1- u2/c2)
8Time Dilation
- ?t G?tp
- ?tp is the proper time, the time between events
which happen at the same place. - Since G is always greater than 1, all clocks run
more slowly according to an observer in relative
motion.
9Time Dilation Example
- An astronaut in a spaceship traveling away from
the earth at u 0.6c decides to take a nap. He
tells NASA that he will call them back in 1 hour.
How long does his nap last as measured on earth?
10Time Dilation Example
- ?tp 1 hour
- 1 (u/v)2 1 (0.6)2 0.64
- Therefore, G v(1/0.64) 1.25
- ?t 1.25 hours
11Length Contraction
- L (1/G)Lp
- Lp is the length of the object in the reference
frame in which the object is at rest. - All observers in motion relative to the object
measure a shorter length, but only in the
direction of motion.
12Length Contraction
13Length Contraction Example
- In the reference frame of a muon traveling at u
0.999978c, what is the apparent thickness of
the atmosphere? (To an observer on earth, the
height of the atmosphere is 100 km.)
14Length Contraction Example
- L (1/G)Lp
- Lp 100 km
- L 100 kmv(1-(0.999978)2)
- L 0.66 km 660 m
15Relativistic Velocity Addition
- When objects are moving at relativistic speeds,
classical mechanics cannot be used. - v (v' u) / (1 v'u/c2)
- v velocity addition
- v' velocity of object moving in the reference
frame of u. - u motion of object
16Relativistic Velocity Addition Example
- A spaceship moving away from Earth at a speed of
0.80c fires a missile parallel to its direction
of motion. The missile moves at a speed of 0.60c
relative to the ship. What is the speed of the
missile as measured by an observer on Earth?
17Relativistic Velocity Addition Example
- Cannot use classical mechanics.
- v is the velocity we are looking for.
- u 0.80c the velocity of the spaceship
- v' 0.60c the velocity of the missile in the
reference frame of the spaceship - v (v' u) / (1 v'u/c2)
- v (0.6c 0.8c) / (1 (0.6c)(0.8c)/c2)
- v 1.40c/1.48 0.95c
18Relativistic Velocity Addition Example
- A star cruiser is moving away from the planet
Mars with a speed of 0.58c and fires a rocket
back towards the planet at a speed of 0.69c as
seen from the star cruiser. What is the speed of
the rocket as measured by an observer on the
planet?
19Relativistic Velocity Addition Example
- v is the velocity we are looking for.
- u 0.58c the velocity of the spaceship
- v' -0.69c the velocity of the rocket in the
reference frame of the star cruiser - v (v' u) / (1 v'u/c2)
- v (0.58c - 0.69c) / (1 (0.58c)(-0.69c)/c2)
- v -0.11c/0.5998 -0.18c
- Compared to 0.11c
20Twin Paradox
- A clock in motion runs slower than one at rest,
including biological clocks. - Apparent paradox with one twin staying on earth
and other going on a relativistic journey. - Solution
21(No Transcript)
22Twin Paradox Example
- Twin sisters Betty and Ann decide to test the
relativity theory. Ann stays on earth. On
January 1, 2000, Betty goes off to a nearby dwarf
star that is 8 light years from Earth. Betty
travels there and back at 0.8c.
23Twin Paradox Example
- What is Bettys travel time to the star according
to Ann? - t d/v 8 light years / 0.8c 10 years
- So Bettys total travel time according to Ann is
20 years.
24Twin Paradox Example
- As soon as Betty reaches the star, she sends her
sister an e-mail message saying, Wish you were
here! via radio. When, from Anns perspective,
does Ann receive the e-mail from Betty? - 2010 8 yrs 2018
25Twin Paradox Example
- When Ann receives Bettys e-mail message, what is
the date on it? - Time dilation G 1/v(1- (0.8c)2/c2)
- So G 0.6c
- 10 years 0.6c 6 years have passed
- So the e-mail will have the date of January 2006.
26Twin Paradox Example
- How much younger is Betty than Ann when Betty
returns from the star? - For Betty, her return date is 2012, but for Ann,
she returns in 2020. - Ann is now 8 years older than Betty.
27Twin Paradox Example
28Newtonian Gravity
- Quote from Newton
- Two masses in Newtons theory inertial mass and
gravitational mass - Newton saw no reason why these masses should be
equal - BUT they are!!!
29Einstein on Gravity
- I was sitting in a chair in the patent office at
Bern when all of a sudden a thought occurred to
me if a person falls freely he will not feel
his own weight. This simple thought made a deep
impression on me. It impelled me toward a theory
of gravitation. - -Albert Einstein
30Principle of Equivalence
- There is no local experiment that can be done to
distinguish between the effects of a uniform
gravitational field in a non-accelerating
inertial frame and the effects of a uniformly
accelerating reference frame.
31Principle of Equivalence
- Free space view is the same as the free fall view
32General Relativity
- The presence of matter causes spacetime to warp
or curve. - Gµv 8?G/c4Tµv
33Schwarzschilds Solution
- Found the first exact solution of one of
Einsteins equations - The metric (distance relation) is
- ds2 -c2(1-2MG/c2r)dt2 dr2/(1-2MG/c2r)
r2(dq2sin2qdf2). - Describes space-time geometry around a spherical
object of mass M - Basis of tests of general relativity
34Testing the General Theory of Relativity
- Deflection of Starlight
- First tested during total solar eclipse in 1919
35Slowing Down of Clocks by Gravity
- Clock closer to the mass measures a shorter
elapsed proper time than a clock that is further
out. - Rc2MG/c2, where Rc is the Schwarzschild radius.