SH1690 The Consequences of Special Relativity As a result of relativistic motion, Einstein has predicted in his postulates that moving at around the speed of light π has consequences. These consequences are, 1. Relative Simultaneity – It means that one (1) frame of reference views two (2) relativistic objects to be simultaneous, while the other does not with respect to the first. Simply put, it means the first observer observing two (2) moving objects to be moving at the same time, while the other observer only sees one (1) moving and the other resting. 2. Time Dilation – This means that time slows down to a halt if an object is moving very fast. In short, if an object is moving at around the speed of light (c), then time ultimately stops for that object. 3. Length Contradiction – It means that moving very fast results in a shortening of the object’s length. These consequences are represented by mathematical formulas and each of them are using the Lorentz Transformation variable (or πΎ). INVERSE TRANSFORMATION EQUATIONS Consider the following variables, π₯ ′ = πΎ(π₯ − π£π‘) π¦′ = π¦ π§′ = π§ π‘ ′ = πΎ (π‘ − πΎ= π£π₯ ) π2 1 2 √1 − π£2 π These variables are equal in value against their respective S frame variables. Only the Transformation variable remains constant. S’ S 1. Relative Simultaneity – Given the diagram at right, where two (2) events are shown to have happened at the same time. This is the instance where simultaneity is to be observed. Using the equations clocked at around the S’, let us determine if t1' x1’ t2' x2’ x o x' o' x1 x2 t 09 Handout 3 *Property of STI Page 1 of 6 SH1690 simultaneity is apparent in the case of relativity. Given are the equations, π₯′ π¦′ π§′ π‘′ = π₯ − π£π‘ =π¦ =π§ =π‘ And the inverse transformation for static time (π‘), π‘ ′ = πΎ (π‘ − π£π₯ ) π2 The value of each event is as follows, π‘ ′ = πΎ (π‘ − π£π₯ ) π2 ππ ′ = πΈ (π − πππ ) ← ππππππππππππ ππππππππ πππ ππ ππ ππ ′ = πΈ (π − πππ ) ← ππππππππππππ ππππππππ πππ ππ ππ The equations look rather similar, but in theory it is not. If in Classical Physics, simultaneity is possible because of time’s invariance, in Special Relativity, simultaneity cannot be true because it is subjective to the observer. Note that everything that is moving to one (1) observer, to the other it remains static. In short, simultaneity really depends on who is observing the events. 2. Time Dilation – Given the diagram at left, with a swinging pendulum as the source of event. The pendulum is swinging at a constant velocity (v), and is being used to determine time (t). While it t1 was moving, the pendulum also rests t2 on the moving frame (S’). Judging by the way it is being measured, time can be laid out mathematically (in the static frame) as, x v → x' S S’ βπ‘ = π‘2 − π‘1 (1) In the moving frame (S’), the time is inversed as, βπ‘′ = π‘′2 − π‘′1 (2) In the case of relativity, time is not absolute. It is subject to change because time is connected with space and, as a result, shows a slight difference between observers. By adding the Lorentz Transformation variable, time is said to be calculated (in the moving frame) as, 09 Handout 3 *Property of STI Page 2 of 6 SH1690 π‘′ = πΎ (π‘ − π£π₯ ) (3) π2 Combining equations (2) and (3), βπ‘′ = π‘′2 − π‘′1 βπ‘′ = [πΎ (π‘′2 − π£π₯ π£π₯ )] − [πΎ (π‘′ − )] 1 π2 π2 βπ‘′ = πΎπ‘2′ − πΎπ£π₯ πΎπ£π₯ − πΎπ‘1′ + 2 2 π π π ππππππππππ π‘βπ π£πππ’ππ , π‘βπ πππ’ππ‘πππ πππππππ , βπ‘′ = πΎπ‘2′ − πΎπ‘1′ − πΎπ£π₯ πΎπ£π₯ + 2 π2 π π΄ππππ¦πππ ππππππππ‘πππ, π‘βπ πππ’ππ‘πππ πππ£ππ , βπ‘ ′ = πΎπ‘2′ − πΎπ‘1′ βπ‘′ = πΎ(π‘2′ − π‘1′ ) πππππ (π‘2′ − π‘1′ ) = βπ‘ ′ , (π‘2′ − π‘1′ ) = (π‘2 − π‘1 ), πππ (π‘2 − π‘1 ) = βπ‘, ∴ βπ′ = πΈβπ ← π»πππ π«πππππππ By assigning new variables to replace βπ‘ and βπ‘′, we make it easier to remember. Let us assign π‘0 for βπ‘, and π‘π’ for βπ‘ ′ . The equation βπ‘ ′ = πΎβπ‘ looks complicated. For us to know what will happen, let us expand the equation, so that we might better understand time dilation. Here is the short equation, βπ‘ ′ = πΎβπ‘ ππ πππ π‘βπ πππ€ π£ππππππππ , π‘π’ = πΎπ‘0 πππππ πΎ = 09 Handout 3 1 2 √1 − π£2 π , π€π πππ‘, *Property of STI Page 3 of 6 SH1690 π‘π’ = π‘0 ∴ ππ = 1 2 √1 − π£2 ( π ) ππ π √π − ππ π ← π»πππ π«πππππππ The value of π‘π’ represents the moving observer’s time as measured by the static observer. In accordance to time dilation, by traveling at speeds close to the speed of light, time is slowing down. Traveling at the speed of light, time stops. And, by not moving at all, time moves as normal. 3. Length Contradiction – Using the same diagram in #1 (Relative Simultaneity), given are two (2) points of events, each are spaced apart in a certain length (π) measured in a given time (π‘). The measurement is being done in the S frame. Plotting this mathematically, βπ = π₯2 − π₯1 (3) The observer in the S’ frame also performed the same measurement of length at the same time. Plotting it mathematically, βπ′ = π₯′2 − π₯′1 (4) In this case, let us use π₯ = πΎ(π₯′ − π£π‘). Combining it with (4), it gives us, βπ = πΎ(π₯2 − π₯1 ) π₯ = πΎ(π₯′ − π£π‘) βπ = πΎ[(π₯2 − π£π‘) − (π₯1 − π£π‘)] βπ = πΎ(π₯2 − π£π‘) − πΎ(π₯1 − π£π‘) βπ = πΎπ₯2 − πΎπ£π‘ − πΎπ₯1 + πΎπ£π‘ π ππππππππππ π‘βπ π£ππππππππ , βπ = πΎπ₯2 − πΎπ₯1 − πΎπ£π‘ + πΎπ£π‘ π΄ππππ¦πππ ππππππππ‘πππ, βπ = πΎπ₯2 − πΎπ₯1 βπ = πΎ(π₯2 − π₯1 ) 09 Handout 3 *Property of STI Page 4 of 6 SH1690 πππππ βπ ππ πππ π πππ’ππ ππ π£πππ’π π‘π ππ‘π πππ£πππ π (βπ ′ ), βπ = πΈβπ′ Same as in Time Dilation, we have to assign new variables to easily understand this concept. For βπ, we shall assign π0 , and ππ’ for βπ′. Expanding the equation above – and using the new assigned variables, π0 = πΎππ’ πππππ πΎ = 1 2 √1 − π£2 π π0 = ππ’ π0 = , π€π πππ‘, 1 2 π£ √ ( 1 − π2 ) ππ’ 2 √1 − π£2 π But, in this case, it is set in the moving observer’s point of view. To truly demonstrate the effect, we have to rearrange this in order to get length contraction, as what the static observer will measure against a moving object. Transposing the Transformation variable, π0 = ππ’ 2 √1 − π£2 π π0 √1 − π£2 = ππ’ π2 π ππππππππππ π‘βπ πππ’ππ‘πππ, ∴ ππ = ππ √π − 09 Handout 3 ππ ← π³πππππ πͺππππππππππ ππ *Property of STI Page 5 of 6 SH1690 Now, in the final equation, it is now evident to the static observer that the moving observer is experiencing length contraction because, in the simplest of sense, if the static observer measures the length of a moving object at a certain point of origin, he will get a different measurement than the moving observer. References: Bauer, W., & Westfall, G. D. (2016). General physics 1 (2nd ed.). Quezon City: ABIVA Publishing House. Boundless (2016). Boundless physics. Retrieved from https://www.boundless.com/physics/textbooks/boundless-physics-textbook/special-relativity27/consequences-of-special-relativity-179/length-contraction-657-6319/ Freedman, R. A., Ford, A. L., & Young, H. D. (2012). Sears and zemansky's university physics (with Modern physics) (13th ed.). Addison-Wesley. HyperPhysics (2016). Lorentz transformation. Retrieved 2017, January 13 from the HyperPhysics Classroom: http://hyperphysics.phy-astr.gsu.edu/hbase/Relativ/ltrans.html 09 Handout 3 *Property of STI Page 6 of 6