LECTURE # 4

31
LECTURE # 4 DOPPLER –SPACETIME DIAGRAMS PHYS 420-SPRING 2006 Dennis Papadopoulos

description

PHYS 420-SPRING 2006 Dennis Papadopoulos. LECTURE # 4. DOPPLER –SPACETIME DIAGRAMS. REVIEW. Last week we learned that length and time are not absolute, but instead, depend on the frame of reference of the observer. We derived the relations:. time dilation. length contraction. - PowerPoint PPT Presentation

Transcript of LECTURE # 4

Page 1: LECTURE # 4

LECTURE # 4

DOPPLER –SPACETIME DIAGRAMS

PHYS 420-SPRING 2006

Dennis Papadopoulos

Page 2: LECTURE # 4

Last week we learned that length and time are not absolute, but instead, depend on the frame of reference of the observer.

We derived the relations:

2

21

'

cv

TT

2

21

cv

LL p

Using only geometrical arguments and applying Pythagorean's theorem.

time dilation

length contraction

dcT/2 222 2/2/ cTdvT

2/2 cTd in red frame

in blue frame

REVIEW

Page 3: LECTURE # 4

Time always runs slower when measured by an observer moving with respect to the clock.

The length of an object is always shorter when viewed by an observer who is moving with respect to the object.

To an observer at rest in one frame, the light in the other frame travels further because the other frame is moving with respect to the observer. Since c is constant in all frames, to each observer time appears to be moving more slowly and length appears to be contracted in a reference frame moving with respect to the observer.

Everything is slowed/contracted by afactor of:

in a frame moving with respect to the observer.

2

21

1

cv

Page 4: LECTURE # 4

The Lorentz transformations!S S’

v

x x’

The transformation:

To transform from S’ back to S:

Page 5: LECTURE # 4

Velocity Transformation

)](1[

)](1[

)(1

2

'

2

'

2

'

cvu

uu

cvu

uu

cvuvu

u

x

zz

x

yy

x

xx

To find the u as a function of u’ replace v by -v

What happens for ux=c ?

Page 6: LECTURE # 4

Fig. 1-19, p. 30

Find speed of B wr to A

Take S’ attached to A -> v=.75 c. uB=-.85 c

Speed of B wr A=u’= c

ccccc

9771.)75.)(85.(

1

75.85.

2

Page 7: LECTURE # 4

Fig. 1-20, p. 30

Page 8: LECTURE # 4

Fig. 1-21, p. 31

How fast does B recede as seen by A

Page 9: LECTURE # 4

Fig. 1-22, p. 31

Steps: Go to ref frame S’ and transform velocities from S to S’

''yx uuu

Page 10: LECTURE # 4

CLASSICAL DOPPLER EFFECT

Source moving

sound

source

o

cUf

f1

)/1( soundreceivero cUff

Receiver moving

Page 11: LECTURE # 4

Relativistic Doppler Shift Qualitatively Different from Classical

To observer

Firstsignal

Secondsignal

Time between emission of signals in source frame to

Time between emission of signals in observers frame tg=to

Time between arrival of signals to the observer t=tg (v/c) cos +tg==to[1+(v/c) cos]

v

0/1,/1

cos)/(1

/

tftf

cv

ff

o

o

RELATIVISTIC DOPPLER SHIFT

VR=v cos

cosgtv

VR

Page 12: LECTURE # 4

BLUE AND RED SHIFT

cos

)1(

vVc

Vf

f

R

R

o

/

02/

/1

/1

180

0

o

R

R

Ro

R

R

ff

V

cV

cVff

vV

vV

o

R

Ro

or

cV

cV

cf

/1

/1

Page 13: LECTURE # 4

x

y

Let’s look at coordinate systems: thinking classically…

You rolls a cat toy across the floor towards her cat.

x

y

The same cat, the same cat toy, different (arbitrary) choice of

coordinate systems.

By Pythagorean’s theorem, the toy rolls:

22 yxd

Easier visualization, easier calculation—You are happy

(although her cat probably doesn’t care as long as she gets his toy.)

This is an example of rotating your coordinate axes in space.

Coordinate systems

Page 14: LECTURE # 4

Space-time Diagrams

Page 15: LECTURE # 4
Page 16: LECTURE # 4

Time, the fourth dimension?

“Spacetime”

x

ct

In x,y space the two space dimensions are interchangeable if they have the same units. A similar relationship can be used to express the relationship between space and time in relativity.

x=ct

Light propagating in one dimension in a spacetime coordinate system as viewed from a frame S. The distance traveled is equal to the speed of light times the time elapsed.

ct=x

45°

Page 17: LECTURE # 4

The red and blue spaceships viewed in spacetime coordinates.

The red and blue spaceships are at x=0, t=0 when oneemits a pulse of light.

At that instant one of the spaceships starts to move away from the other with velocity v.

The lightcone- the distance light has traveled since x=0, t=0 as a function of time.

Who perceives him/herself to be at the center of the lightcone? A passenger on the red spaceship or a

passenger on the blue spaceship?

Page 18: LECTURE # 4

The red spaceship’s reality. The blue spaceship’s reality.

They are both at the center of the light cone!

This can be achieved by rotating their coordinate axes as you did when playing with the cat, except one thing…notice that one set of axes is not orthogonal! You need to add a Lorentz boost.

Page 19: LECTURE # 4

The velocity of a particle in spacetime coordinates is:

slope

c

tc

xc

t

xvelocityparticle

The speed of light is absolute, therefore the axes must be drawn to preserve the speed of light!

x

ct

a light pulse is sent out

x=ct

ctx tcx

in frame S

in frame S’

x’

ct’ and x’ axes must be symmetrically placed with respect to the light pulse!

ct’

A spaceship is traveling in a reference frame with v<c w/r to S

ct ct’

xx’ Vtx

Newtonianly:

Vtxx

tt

Page 20: LECTURE # 4

x

ctx=ctct’

x’

The axes aren’t perpendicular but are scaled by some factor. They must be symmetric w/r to the light pulse. What is this factor?

(ct,vt)

tan=Vt/ct=V/c

Page 21: LECTURE # 4

x

ctx=ctct’

x’

ctc

Vxx x

c

Vcttc

The axes aren’t perpendicular but are scaled by some factor. They must be symmetric w/r to the light pulse. What is this factor?

Page 22: LECTURE # 4

Fig. 1-23, p. 32

Page 23: LECTURE # 4

Fig. 1-24, p. 33

Page 24: LECTURE # 4

ct ct’x=ct

x

x’

Spacetime is invariant!

True, observers will differ on the length of objects or the time events occurred, however, they will always agree on how far apart two events are in spacetime.

E1

E2

To find the space and time coordinates of an event in a specific frame, draw lines from the event parallel to the axis of that frame.

212

212

222 xxttcxtcs

212

212

222 xxttcxtcs

22 ss !

`

TO PROVE USE LORENTZ TRANFORMATION FROM THE PRIMED TO THE UNPRIMED FRAME AND DO A LITTLE ALGEBRA

Page 25: LECTURE # 4

ct

x

x=ctx=-ctA B

C

O

Could an event at O cause A?

Yes, because a “messenger” at O would not have to travel at a speed greater than the speed of light to get there.

Could an event at O cause B?

A light signal sent from O could reach B.

Could an event at O cause C?

No, the spacetime distance between O and C is greater than could be covered by light. It would require time travel.

xtc

xtc

xtc

here,now

where light that is here now may have been in the past

where light that is here now may go in the future

Page 26: LECTURE # 4

Fig. 1-25, p. 34

Page 27: LECTURE # 4

DIFFERENT ROUTES IN SPACETIME RESULT IN

DIFFERENT AGES.THE LONGEST TIME TO

GO FROM a TO b IS ALONG THE STRAIGHT

SEGMENT AND THE TIME GETS SHORTER

AS THE SEGMENTabd

APPROACHES THE LIGHTCONE

Page 28: LECTURE # 4

The time measured by a heartbeat or the wristwatch of a person equqls its wordline from a to b. Curved wordlines are shorter than straight wordlines. Thus a person arriving via a bent world line has fewer heartbeats than a person following a straight-line (i.e. moving only through space) Photons never age in free space.

Page 29: LECTURE # 4

TWINS A AND B FOLLOW DIFFERENT LIFES ON STAYING HOME THE OTHER TRAVELING A LOT. EVERY TIME THEY MEET AT THE SAME SPACETIME POSITION Bs WORDLINE IS SLIGTLY SHORTER SINCE SHE HAS MOVED A LOT THROUGH SPACE, WHILE HER BROTHER MOVED ONLY THROUGH SPACE. HER WORDLINE AT THEIR 70TH BIRTHDAY IS SLIGHTLY SMALLER AND HER PHYSICAL AGE SLIGHTLY SHORTER (BY MAY BE A MICROSECOND)

Page 30: LECTURE # 4
Page 31: LECTURE # 4

tB=tA/

OUTWARD JOURNEY

222 )21()2

1()21( BAA tctVtc

xA

EXACTLY THE SAME FOR RETURN JOURNEY

tB=tA/

GAMMA 50, V=.9998c

IF A IS 50 YEARS OLDER

B IS ONLY ONE YEAR OLDER