Β© ABCC Australia 2015 new-physics.com
Cosmic Adventure 5.11
VELOCITY TRANSFORMATION IN RELATIVITY & VISONICS
Β© ABCC Australia 2015 new-physics.com
VELOCITY IN CLASSICAL PHYSICS
Cosmic Adventure 5.11a
Β© ABCC Australia 2015 new-physics.com
Motion in a Straight Line
When an object moves at a constant speed π£ along a straight line, it will cover a certain distance βπ₯ within a certain period of time βπ‘.
Distance units in cm, m, km, etc.
βπ‘
βπ₯
Β© ABCC Australia 2015 new-physics.com
Definition of Speed
The ratio between βπ₯ and βπ‘ is what we call speed π£ β a scalar quantity.
If this motion is carried out in a certain direction, we call it velocity and it is identified as a vector β a speed with a direction.
However since we are dealing with velocity along a straight axis, both definitions will work without any difference.
π£ =Ξπ₯
Ξπ‘
Space Ratio
Time
Β© ABCC Australia 2015 new-physics.com
Units of Speed
Distance is measured in meters, kilometers, feet, or miles. Time is in seconds, minutes or hours. For example, the unit of velocity can be written as km per second, or miles pet hour, etc.
Β© ABCC Australia 2015 new-physics.com
Geometric Representation of Speed
Since distance (space) and time are two independent quantities, they can be represented by the two perpendicular coordinates of a Cartesian coordinate system: y-axis looks after distance and x-axis looks after time. Velocity become the slanting line or slope across space and time (the so called βspace-timeβ).
Dis
tanc
e (s
pace
) Time
Ξπ₯
Ξπ‘
π£ =Ξπ₯
Ξπ‘
Β© ABCC Australia 2015 new-physics.com
Cosmic Adventure 5.11b
VELOCITY IN RELATIVITY
Β© ABCC Australia 2015 new-physics.com
Moving Frame
To find the velocity in relativistic transformations, we again employ the same reference system which we use to find the position and time.
In this system, one observer at Oβ moves along the common x-axis at a constant velocity v with respect to another observer at O.
π
π₯
π₯β²
0 P 0β
π£
Moving frame
Β© ABCC Australia 2015 new-physics.com
Position and Time
The relativistic position π₯β² and time π‘β² are as what we have found in previous discussions:
π₯β² =π₯ β π£π‘
1 βπ£2
π2
π‘β² =π‘ β π£π₯/π2
1 βπ£2
π2
π
π₯
π₯β²
0
P
0β
π£
Β© ABCC Australia 2015 new-physics.com
Relativistic Velocity
Since only uniform motion is involved, it is valid to consider small distance βπ₯β²and time βπ‘β². Then the equations are slightly changed to:
π₯β² =π₯ β π£π‘
1 βπ£2
π2
βπ₯β²=βπ₯ β π£βπ‘
1 βπ£2
π2
π‘β² =π‘ β π£π₯/π2
1 βπ£2
π2
βπ‘β²=βπ‘ β π£βπ₯/π2
1 βπ£2
π2
Β© ABCC Australia 2015 new-physics.com
The Transformation of Velocity
We then simply divide the small distance βπ₯β with the small duration of time βπ‘β to obtain our velocity π’β²:
π’β² =βπ₯
βπ‘β²
β²
=βπ₯ β π£βπ‘
1 βπ£2
π2
Γ·βπ‘ β π£βπ₯/π2
1 βπ£2
π2
π’β² =βπ₯ β π£βπ‘
βπ‘ β π£βπ₯/π2
=βπ₯/βπ‘ β π£βπ‘/βπ‘
1 β π£βπ₯/βπ‘π2
=π’ β π£
1 βπ£π2 π’
Β© ABCC Australia 2015 new-physics.com
Differential Approach
A more sophisticated way is to take the βdifferentialsβ of the transformed Lorentz coordinates:
ππ₯β² =ππ₯ β π£ππ‘
1 βπ£2
π2
ππ‘β² =ππ‘ β π£ππ₯/π2
1 βπ£2
π2
But the results will the same:
π’β² =π’ β π£
1 βπ£π2 π’
Β© ABCC Australia 2015 new-physics.com
Β© ABCC Australia 2015 new-physics.com
Cosmic Adventure 5.11c
VELOCITY TRANSFORM IN VISONICS
Β© ABCC Australia 2015 new-physics.com
Previous Equations
The position and timing of an object at constant motion has been discussed in the session on moving objects. So the relevant equations are those that have been formulated. Cosmic Adventure 5.4
Β© ABCC Australia 2015 new-physics.com
π£
A
Real clock A Real clock B
Situation 1
At time βt = 0, both clocks are at the starting position A. Clock A is at rest while clock be is moving at velocity π£.
Distance π₯ = 0 Time βt = 0
Β© ABCC Australia 2015 new-physics.com
π£
A B
Real clock A Real clock B
Situation 2
After time = βπ‘1, clock B has travelled to B, covering a distance π₯1 = π£βπ‘1. Both clocks now register the same time, that is, βπ‘1.
π₯1 = π£βπ‘1
Β© ABCC Australia 2015 new-physics.com
π£
A B
Real clock A Real clock B Image
π
Time of image B Reading βπ‘1
Situation 3 Image Emission
At this moment of time = βπ‘1, clock B sends an image (registering time βπ‘1) towards clock A, while keeps on traveling away from B.
Clock B goes on
Β© ABCC Australia 2015 new-physics.com
π£
A B C
Real clock A Real clock B Image
π
Situation 4
This image takes time βπ‘2 to reach A at speed c. At the same time clock B has reached C with BC= βπ₯1= π£βπ‘2. The time is then βπ‘3 = βπ‘1 + βπ‘2
π₯1 = π£βπ‘1 = πβπ‘2 βπ₯1= π£βπ‘2
Β© ABCC Australia 2015 new-physics.com
π£
A B π₯1 = π£βπ‘1 = πβπ‘2
Image
C
π
Real clock A Real clock B
Actual time βπ‘3= βπ‘1 + βπ‘2
Apparent time = βπ‘1
Situation 5
Actual time βπ‘3= βπ‘1 + βπ‘2
βπ₯ = π£βπ‘2 = π£βπ‘1 Γ π£/π
Β© ABCC Australia 2015 new-physics.com
π£
A B Apparent position π₯1 = π£βπ‘1 = πβπ‘2
Image
C
π
Real clock A Real clock B
Actual time βπ‘3= βπ‘1 + βπ‘2
Apparent time = βπ‘1
Final Situation 6
Actual time βπ‘3= βπ‘1 + βπ‘2
βπ₯ = π£βπ‘2 = π£βπ‘1 Γ π£/π
Actual position π₯3 = π£βπ‘1 + π£βπ‘2
Β© ABCC Australia 2015 new-physics.com
Observation 1 β Positions & Time
The apparent position of clock B is:
π₯1 = π£βπ‘1 = πβπ‘2
The clock reading of image B is βπ‘1. So the apparent time is:
βπ‘1
The actual position of clock B is :
π₯3 = π₯1 + βπ₯ = π£βπ‘1 + π£βπ‘1π£/π
= 1 +π£
ππ£βπ‘1 = 1 +
π£
ππ₯1
The actual time of B is (same as A):
βπ‘3 = βπ‘1 + βπ‘2 = 1 +π£
πβπ‘1
Β© ABCC Australia 2015 new-physics.com
Observation 2 - Velocities
The apparent velocity is:
π’1 =π₯1
βπ‘1= π£
The actual velocity is:
π’2 =π₯3
βπ‘3=
1 +π£π π₯1
1 +π£π βπ‘1
=π₯1
βπ‘1
= π£
π’1 = π’2 = π£
That is, the observed velocity is
the same as the actual velocity!
Β© ABCC Australia 2015 new-physics.com
Β© ABCC Australia 2015 new-physics.com
ACCELERATION
To be continued in Cosmic Adventure 5.12