inst 240 revolutions lecture 8 spacetime diagrams

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INST 240 Revoluti ons Lecture 8 Spacetime Diagrams

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Page 1: INST 240 Revolutions Lecture 8 Spacetime Diagrams

INST 240

RevolutionsLecture 8

Spacetime Diagrams

Page 2: INST 240 Revolutions Lecture 8 Spacetime Diagrams

Cause and Effect

• How does relativity ensure that some events appear in the “correct” order, while for others it doesn’t matter?

• We’ll see later that these events are in different categories (space-like and time-like connected)

• It will be easy to figure out which is which with the help of a light-cone diagram

Page 3: INST 240 Revolutions Lecture 8 Spacetime Diagrams

Spacetime &The Light Cone

Page 4: INST 240 Revolutions Lecture 8 Spacetime Diagrams
Page 5: INST 240 Revolutions Lecture 8 Spacetime Diagrams

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Position vs Time GraphsPosition

1 ft

0 ft

2 ft

1 ns0 ns 2 ns Time

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Spacetime graphs (Axes flipped)

Space(Position)

Time

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Spacetime graphs

Space(Position)

Time

A and B have the same place, different times

× A

× B

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Spacetime graphs

Space(Position)

Time

Everybody snap your fingers like this.

× A × B

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Spacetime graphs

Space(Position)

Time

× A

× B

Everybody snap your fingers like thisEverybody snap your fingers like this

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Spacetime graphs

Space

Time

You can use spacetime graphs to tell a simple story.

B

A

Albert started at home at 8:00 AM (A). He immediately started walking east and reached the corner of his block (B).

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Spacetime graphs

Space

Time

B

C

Aa).. he stubbed his toe and

limped the rest of the way.b)..he looked at his watch,

realized he was late and sped up.

c).. nothing happened.Eventually, he reached school at 9:00 AM (C).

Page 12: INST 240 Revolutions Lecture 8 Spacetime Diagrams

Spacetime = Space plus Time

• In relativity space and time are not independent of each other (if one is measured differently by a second observer, so is the other)

• Makes sense to upgrade time to a direction (dimension) rather than viewing it as an (unchanging) parameter

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Worksheet Part 1

• Make up stories using the space-time diagrams

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Moving right to B, then back to the same position as A at a later time

Space

Time

B

A

C

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Two friends parting ways: one going to the right, the other left

Space

Time

B

A

C

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Two friends starting out at different positions, moving at different velocities to meet at C,

then changing velocities to move to D

Space

Time

BA

CD

Page 17: INST 240 Revolutions Lecture 8 Spacetime Diagrams

What is ct?

• Skippyjon Jones The units for 'c' are meters/second.  The units for 't' are seconds.  When these two units are multiplied, we are simply left with meters. (m/s)(s)=m.  'ct' is used to represent distance in time.

• Somebody In this expression, 'ct' would be represented by meters in spacetime.  This 'c' represents the cosmic speed, which can be considered the speed of light, and 't' is time.  Therefore, 'ct' could be used to represent the distance in spacetime.

Page 18: INST 240 Revolutions Lecture 8 Spacetime Diagrams

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What is this (ct) thing?

ct means c times tt is in secondsct is in meters

So c is in meters/second

If t = 1 second,(ct) = 3 x 108 m/s x 1 s = 3 x 108 m

We can say “the time was 300 000 000 meters” instead of “the time was 1 second”

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Example

In lab, we bounced a laser off a mirror 15 feet away.

10 ft 20 ft 30 ft0 ft

10 ft

20 ft

30 ft

Page 20: INST 240 Revolutions Lecture 8 Spacetime Diagrams

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Example

In lab, we bounced a laser off a mirror 15 feet away.

0 ft 10ft 20 ft 30 ft

10 ft

20 ft

30 ft

Light travels at exactly 45 degree lines.

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Light Cone

Light travels at exactly 45 degree lines.

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QuestionA

BC

Which lines represent objects moving at the speed of light?

D

a)Ab)Bc)Dd)A and Be)B and Df)C and D

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QuestionA

BC

D

a)Ab)Cc)A and C

Which lines represent objects moving faster than the speed of light?

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Worksheet II

• Label both axes with the right units

• Draw the spacetime graphs for the stories

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A spaceship starts at earth and travels a distance of 3 light-years at 3/4 the speed of light.

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A spaceship starts at earth and travels a distance of 4 light-years at twice the speed of light.

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The light from two exploding stars reaches earth at the same time. The first star is 20 light-years away;the other is 30 light-years away.

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Cosmic speed limit

So far, scientists have not observed any phenomenon that moves faster than the speed of light.

This includes any form of communication or information transit.

Later we will see WHY we think this to be universally true, but let’s just take it as a fact for

the moment.

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We are here and nowO×

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A× We can walk or send a rocket or a message from O to A, so we can affect it.

(Nostradamus sending a letter to start the Great Fire of London)

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O× A×From O, we can’t affect something at A:light doesn’t have time to get there

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From O, we can’t affect something at A:light doesn’t have time to get there

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Things we can affect in the futureO×

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A was a butterfly 100 years agoO is me now

A could be part of my history

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O×A×

A happened in the pastO is me now

But I can’t possibly know A has happened... light from A hasn’t reached me yet.

e.g. a star 100 light years away exploded 50 years ago.

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Things that could have affected us from the past

Things we can affect in the future

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Events that can’t have anything to do with here-and-now...they’re too far away!

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Definitions

O×O×

Events in this region aretime-like separatedfrom O.

Events in this region arespace-like separatedfrom O.

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Definitions

O×O×

O×Things on the blue lines areon the light cone.

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Why “Light Cone”?

Here’s the picture with 2 space dimensions(i.e. N/S, E/W) and time.

Page 41: INST 240 Revolutions Lecture 8 Spacetime Diagrams

Invariants: totally constant

• are65adfg5h4634 An invariant quantity is a value which is unchanged when applied to a different coordinate system. An example of an invariant quantity would be the distance between two points on a line.

• Mikey Cigars Laws of nature will not change no matter what your viewing point is.  For example, a TV will work in the family room of your house just the same as if it were in the kitchen.  Two different places does not change the result.

Page 42: INST 240 Revolutions Lecture 8 Spacetime Diagrams

Invariants

• Observers can disagree on many things (distances, time intervals)

• Can they agree on something?– Speed of light– Physics– Invariants!

Page 43: INST 240 Revolutions Lecture 8 Spacetime Diagrams

How do we construct an invariant?

• Pragmatic way: see what stuff (physics) we have to agree on, then express them in terms of the quantities we do not have agree on (coordinates)

• Often, invariants are connected to symmetries

Page 44: INST 240 Revolutions Lecture 8 Spacetime Diagrams

Example: Rotational symmetry

• Consider a circle: it looks round, no matter how you describe it.

Rotated Observer

Page 45: INST 240 Revolutions Lecture 8 Spacetime Diagrams

Was the circle rotated? Can you tell?

• The coordinates of a point on the circle are different for two observers. How can you tell whether they talk about the same circle?

Rotated Observer

x x

Page 46: INST 240 Revolutions Lecture 8 Spacetime Diagrams

Calculate the radius!

Rotated Observer

x x

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Every observer has to agree on the radius; it’s what makes this

circle this circle!

• The radius of the circle is an invariant– It stems from rotational symmetry

Page 48: INST 240 Revolutions Lecture 8 Spacetime Diagrams

Pythagoras doesn’t work in Relativity!

• See textbook: the “geometry” of spacetime is not as simple as the geometry of a flat sheet of paper (euclidean geometry, aka the geometry where Pythagoras works, the sum of the angles of a triangle is 180 degrees, etc.)

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Example

View from Earth

A×A spaceship starts at earth and travels a distance of 3 light-years at 3/5 the speed of light.

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Example

View from Earth

O - they whizz past earthA - they arrive at their destination

3 light-years

5 light-years

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Gamma etc.

View from Rocket

if v/c = 3/5c then

γ = 5/4=1.25

cT’ = proper time= “c time” seen from rocket= 4 light-years

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View from Rocket

L’ = proper distance= distance seen from earth= 3 light-years

L = contracted distance= L’/γ = 3 light-years/1.25= 12/5 ly = 2.4 light-years

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From Earth

RocketO×

From Rocket

Can we come up with a number that we both agree on for the distance/time between O and A?

earthRoc

ketearth

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Spacetime interval

The rationale is in Cox and Forshaw

s is the spacetime intervalt = time between two events

x = distance between two events(we used L so far)

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O-A measured by earth:t = 5 years so,ct = 5 light-yearsx = 3 light-years

s2 = (ct)2 - x2

s2 = (5)2 - (3)2

s2 = 25 - 9 = 16s = 4 light-years

O-A measured by rocket:t = 4 years so,ct = 4 light-yearsx = 0 light-years (rocket doesn’t move)

s2 = (ct)2 - x2

s2 = (4)2 - (0)2

s2 = 16 - 0 = 16s = 4 light-years

That is... s is just another name for the proper time!

Page 56: INST 240 Revolutions Lecture 8 Spacetime Diagrams

The invariant!

Every observer will calculate the same number:s = 4 light-yearsbetween the rocket leaving and the rocket arriving.

Page 57: INST 240 Revolutions Lecture 8 Spacetime Diagrams

All points (events) on the red curve, are a “space-time distance” s away from the origin

Page 58: INST 240 Revolutions Lecture 8 Spacetime Diagrams

All points (events) on the red curve, are a “space-time distance” s away from the origin