ph 301 dr. cecilia vogel lecture 5. review outline velocity transformation not simple addition ...
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Review
Outline Velocity transformation
NOT simple addition Spacetime
intervals, diagrams
Lorentz transformations order of events twin paradox
Velocity u = dx/dt u’ = dx’/dt’
( ' ')x x vt
'dx dx dtv
dt dt dt
'
'
dx dx dtv
dt dt dt
' /'
dtu u v
dt
Velocity Transformation
Note: Speed will never be bigger than c If u’ and v are <c, then u<c If |u’| or |v| =c, then u=c
speed of light the same
Pay attention to the sign of velocities Pay attention to order of frames
2
'
1
u vu
u vc
Using Velocity Transformation Step 1: Let u = answer you seek.
Step 2: u = velocity of A rel to B, so A and B are determined.
Step 3: Identify frame C -- what’s left? Step 4: Determine u’
u’= velocity of A rel to C If you have C rel to A, use opposite sign
Step 5: Determine v v = velocity of C rel to B If you have B rel to C, use opposite sign
Step 6: Plug in the numbers to compute u. Step 7: Check that your answer makes sense!
EXAMPLE A spaceship is approaching the
planet Zorgon at a speed of 0.85c. A diplomatic shuttle is sent ahead to arrive at the planet earlier. With what velocity should the shuttle be launched relative to the ship, in order to approach the planet at a rate of 0.95c? u = velocity of shuttle relative to the ship
so… A is ________ and B is _____
Then C is _________
EXAMPLE A spaceship is approaching the
planet Zorgon at a speed of 0.85c. A diplomatic shuttle is sent ahead to arrive at the planet earlier. With what velocity should the shuttle be launched relative to the ship, in order to approach the planet at a rate of 0.95c? u’ = velocity of A relative to C
so… u’ is velocity of ________ relative to _____ u’ = +0.95 c
EXAMPLE A spaceship is approaching the
planet Zorgon at a speed of 0.85c. A diplomatic shuttle is sent ahead to arrive at the planet earlier. With what velocity should the shuttle be launched relative to the ship, in order to approach the planet at a rate of 0.95c? v = velocity of C relative to B, so… v is
velocity of _______________ relative to _____
v =Ship relative to Zorgon is +0.85 c, so
EXAMPLEWith what velocity should the shuttle be
launched relative to the ship, in order to approach the planet at a rate of 0.95c?
u’ = +0.95 c, v = -0.85 c
2 2
' 0.95 0.85(0.95 )( 0.85 )
1 1
0.10.52
1 (0.95)(0.85)
u v c cu
u v c cc cc
c
EXAMPLE A proton is traveling at a speed of
0.75c relative to the lab. A neutron is to collide with it at a relative speed of 0.90c. With what velocity should the neutron go relative to the lab?
u = velocity of neutron relative to the labso… A is ________ and B is _____
Then C is _________
EXAMPLE A proton is traveling at a speed of
0.75c relative to the lab. A neutron is to collide with it at a relative speed of 0.90c. With what velocity should the neutron go relative to the lab?
u’ = velocity of A relative to Cso… u’ is velocity of ________ relative to _____
neutronu’ =proton
EXAMPLE A proton is traveling at a speed of
0.75c relative to the lab. A neutron is to collide with it at a relative speed of 0.90c. With what velocity should the neutron go relative to the lab?
v = velocity of C relative to B, so… v is velocity of _______________ relative to _____
lab
v =
proton
EXAMPLEWith what velocity should the
neutron go relative to the lab?
2 2
' 0.9 0.75( 0.9 )(0.75 )
1 1
0.150.46
1 (0.9)(0.75)
u v c cu
u v c cc cc
c
Space-time Considers time as a fourth
dimension. An event is given by a 4-
component vector: 3 space, 1 time
I can’t draw in 4 dimensions Let’s consider 1 space & 1 time
Space-time Diagrams An event is a
point on the diagram.
x
ct
A world-line is the path of an object on the diagram. The steeper the slope, the slower it’s going.
Wor
ld-li
ne o
f
light
Slope = 1, means speed c.
Classical Invariant
( )x x vt
In classical relativity, everyone measures the same distance between two events in space:
If
2 2 2x y z d Then
2 2 2x y z d
Invariant in Space-time In space-time, we let the 4-component
vector be (x, y, z, ict) So that the space-time interval,
2 2 2 2 2( )s x y z c t is invariant.
2 2 2 2 2( )s x y z c t
Spacetimerecall
special relativity (ch 2)An event is something that occurs at a particular place and time – at a particular point in spacetime
Spacetime graph Graphs an event as a point in 4-D spacetime
(x, y, z, t)We will consider 1-D space, 1-D time
2-D graphs are easier to draw!
Worldline Worldline of an object
Is the set of all spacetime points occupied by the objectAlthough t is ordinate, and x is abscissa, do not think of t(x)
Slope of worldlined(ct)/dx = c/(dx/dt)v/c = 1/slope
steeper slowervertical stopped|slope| = 1 |v|=c, worldline of lightgenerally, worldline |slope|>1
Transform WorldlinesA Spacetime graph is drawn from a particular reference frameIn the spacetime graph drawn from a different reference frame
the slope of the worldline of a massive object is different
according to the velocity transformation equation
the slope of the worldline of light is not different
slope is still +1
Spacetime FutureGiven a particular event at xo, yo, zo, to,
the points on a spacetime graph are divided into 3 regions: its future, its past, and its elsewhere
Spacetime Future of the eventthe set of all spacetime points such that
t> to, ANDd<ct
d = spatial distance between x, y, z and xo, yo, zo
t= t- to
Spacetime PastSpacetime Past of the event
the set of all spacetime points such that
t< to, ANDd<c|t|
NOTE:The event can be reached by a signal from its past
this event can be affected by events in the past
A signal from the event can reach points in the future
this event can affect events in its future
LightconeAn event’s lightcone
is the set of spacetime points such that
d=c|t|It is the boundary of the future and of the past
A signal from this event can only reach events in the lightcone
by traveling at the speed of light
This event can only be reached by a signal from an event in the lightcone
if the signal travels at speed of light
Elsewhere The Elsewhere Elsewhere of the event
consists of all the other spacetime points (other than lightcone, past, future)
d>c|t|The event cannot be reached by, nor can anything from the event reach, an event in its elsewhere
this event cannot affect nor be affected by events in its elsewhere
Elsewhere is not…This does NOT mean
that an event that is currently in our elsewhere can never affect us
that event may be in the past of future points on our worldline
It also does NOT meanthat an event that is currently in our elsewhere can never have been affected by us
that event may have been in the future of past points on our worldline
Elsewhere ExampleFor example
if the sun had disappeared 4 minutes ago
that event is in our elsewhere right nowd= 8c-min, c|t| = 4 c-min, d>c|t|
BUT, four minutes from now, that event will be in our past, and we will be gravely affected!
ourworldline
sundisappearing
worldlineof sunlight
- 4 min
+ 4 min