Up: Astronomy 9 Lecture Notes
ASTRONOMY 9: HISTORY OF COSMOLOGY
Handout #19
J. E. Baker
UC Berkeley, Spring 2000
Special Relativity (1905)
- Albert Einstein (1879-1955)
- Like Aristotle and Newton, created new conceptual foundation
for physics
- Worked on wide variety of problems (mechanics, gravitation,
quantum and statistical physics)
- Born Ulm, Germany; emigrated to U.S. in 1933; died Princeton,
NJ
- Detached childhood, strong distrust of all authority, but not
an untalented student
- ``Person of the Century'' (Time), socially engaged
- Used his great celebrity to speak out on pacifism, democracy,
Zionism; offered presidency of Israel
- Science as path to self-transcendence; deep belief in Nature
as a mystical riddle
- Motivation for Special Relativity
- At age 16, Einstein thinks about ``riding on a light beam''
- If you catch up, light should appear to stop moving
- But Maxwell's theory says light always moves: no
stationary EM waves allowed!
- Ideas of length contraction and time dilation previously
suggested by Lorentz and Fitzgerald to explain Michelson-Morley
result, but did not understand why
- Postulates of Special Relativity
- 1.
- Laws of physics are the same for all observers
moving with constant velocities
- This is the old idea of (Galilean/Newtonian) relativity
- Motion at constant velocity is relative
- No experiment inside a train with closed windows can
determine if it is moving at constant velocity
- 2.
- The speed of light in empty space is always measured
to be the same, regardless of motion of the source or
observer!
- Very counter-intuitive: simple addition of velocities
doesn't work!
- Maxwell is right, Newton wrong!
- c is absolute (not everything is relative!)
- From these simple postulates, all bizarre implications of
relativity follow (thought experiments)
- Effects are only noticeable when speeds approach c=300,000 km/s, far removed from our everyday world
- Fun Implications of Special Relativity
- 1.
- Simultaneity is relative!
- If two observers are moving relative to each other, two
events that look simultaneous to one will not look
simultaneous to the other!
- Example: passenger stands in middle of moving train car and
shines light forwards and backwards
- Both passenger and station observer measure c
- To passenger, hits front and back simultaneously
- To station observer, hits back of car first!
- 2.
- Time is relative: time dilation!
- Moving observers will not agree that clocks tick at
the same rate
- Demolishes Newtonian idea of absolute time
- Example: ``light clock'' in a moving train
- Tick/tock is light bouncing vertically off mirrors
separated by height H
- For observer moving with clock, tick/tock time is H/c
- For station observer, the light has to go farther, so time
is >H/c!
- Moving clocks run slower! Factor is
(``boost factor'')
- Note reciprocity: observer on train will see that
station observer's clock runs slow
- The fastest-running clock (``proper time'') is
always the one that is moving with the observer
- Note: you always perceive your own time ``flowing''
at the same ``rate''
- 3.
- Space is relative: length contraction!
- Moving rulers become shorter along the direction of their
motion!
- As with time dilation, factor is
- Demolishes Newtonian idea of absolute space
- Example: decaying subatomic particles at speed close to c
- Typical half-life time
for particle at rest
- Particles can live much longer when moving due to
time dilation (observed all the time using cosmic rays)
- This means they can travel much farther than you
would expect before decaying
- But imagine you are Superman, flying along with the
particle
- Since particle is at rest in your frame, it decays in its
usual short time
- But it did manage to cover the longer
distance--how?
- Must be that space contracted along the direction of
motion!
- 4.
- Velocities do not simply add
- Throw a ball forward with speed u from a train moving with
speed v
- Newton and Galileo: observer on ground sees speed u+v
- Einstein: observer on ground sees speed
- Note this is always <c, even if u and v are very close
to c!
- Doppler shift is also more complicated:
- 5.
- Speed of light is the ultimate speed limit!
- In a second 1905 paper, E=mc2
- Mass is a form of energy! Can convert from one to the
other, for example:
- Nuclear fission (first uranium atomic bombs)
- Nuclear fusion (hydrogen bomb, powers the Sun)
- Even chemical reactions that give off energy result in a
(tiny) change in mass
- Even when matter is at rest, still has some energy
- Speed something up, it has more energy, and therefore more
mass:
- v=c would lead to infinite mass, requiring infinite
energy, so cannot be reached
- Any particle traveling at c must have zero ``rest mass''
- Note: this is not simply a problem of engineering (like
sound speed), but a fundamental physical principle!
- Twin ``Paradox''
- Send one twin off to
Centauri and back
- Earth-bound will see the twin's clock run slower, so when she
gets back she will have aged less!
- But the traveler will see Earth's clock run slower, so she
will expect the Earth-bound traveler will have aged less
- Who is right?
- In fact the traveling twin ages less. Why?
- Only Earth-bound twin was in an inertial frame; in order to
come back, traveler had to decelerate, turn around, and
accelerate
- But Earth-bound will always see traveler's clock run
slow, so it is true that traveler ages less upon return
- Have to be careful to account for the acceleration when
talking about what traveler will see
- Absolute Newtonian space and time are replaced by
four-dimensional spacetime
- Space and time not just a background arena, but active
physical entities
- Plot ct (time) vs. x (one dimension of 3-d space)
- Particles at rest in this frame follow vertical lines
- Particles in inertial (uniform velocity) frames follow
straight lines
- Light follows
diagonals
- Spacetime interval:
- Note - sign makes this very different from Euclidean
geometry!
- This interval is invariant: all observers will
measure the same value for
(though different
and
)
- Events outside the 45
light cone are
``elsewhere'' and cannot be in causal contact
- Remaining problem: how does gravity fit in with all this?
- Need for a General Theory!
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Up: Astronomy 9 Lecture Notes
jonathan baker
2000-03-21