Special Relativity in a Model Universe Michael S. A. Graziano Draft Aug 2009

Size: px
Start display at page:

Download "Special Relativity in a Model Universe Michael S. A. Graziano Draft Aug 2009"

Transcription

1 Special Relativity in a Model Universe Michael S. A. Graziano Draft Aug 2009 Introduction The present paper describes a model universe called Hubs and Spokes (HS). HS operates on the basis of two rules. From those rules, a full description of HS can be generated. Objects can be constructed out of point particles according to a set of constraints. Below, the basic structure and rules of HS are defined. Then some examples of particle interactions in HS are described. Finally, the emergence of special relativity in HS is described. A peculiarity of HS is that special relativity and Galilean/Newtonian space-time are equivalent. For this reason, special relativity is particularly easy to understand in HS. Structure of HS 1. HS contains a space of three dimensions. These dimensions are parameterized here as x, y, and t. (The use of three dimensions instead of four is solely for the convenience of graphing the figures below. HS can be trivially extended to four dimensions.) These parameters form a reference frame termed R1. Other reference frames will be discussed below. 2. HS contains point particles. A point particle is a particle that is dimensionless in x and y but not in t. These particles are called grains here. Rules of HS 1. When a grain is not interacting with another grain, it moves in a straight line at speed c with respect to reference frame R1. Thus a non-interacting grain follows the equation: [Eq.1] Δx 2 + Δy 2 - c 2 Δt 2 = 0. This rule is expressed in a frame-dependant manner, as if R1 were a preferred coordinate frame. Later it will be shown that Rule 1 is also valid in other reference frames. 2. Grains interact by absorption or emission. An absorption is when two grains combine on contact to produce a single resultant grain. An emission is a time-reversed absorption. 1

2 Some examples Consider two grains, 1 and 2, traveling on paths that converge on a point in space A at time t. No rule requires an absorption to occur. The grains might pass through each other and continue their separate paths. If an absorption does occur, by Rule 2, the absorption requires contact between the two grains and thus can occur only at point A. In this scenario, grains 1 and 2 combine to produce a single resultant grain 3. This interaction is shown in Figure 1, which illustrates the paths traced by the grains in the x and y dimensions. y grain 3 A grain 1 grain 2 x [Figure 1: Grains 1 and 2 converge at point A; an absorption occurs on contact; grain 3 results. Arrows indicate the direction of movement along the paths of the grains.] By Rule 1, grains 1 and 2 approach each other on straight paths at speed c and grain 3 leaves the point of interaction on a straight path at speed c. The rules of HS do not specify the angles between these three paths; any angles are permissible. There is no such thing as momentum in HS, and no conservation laws govern the resultant trajectory in this interaction. Figure 2 shows two alternative ways to conceptualize the same situation. In the first way (Figure 2, left), grain 1 absorbs grain 2 and then continues its trajectory while grain 2 no longer exists. In this conceptualization, grain 1 can change its direction of motion at the point of absorption. This change in direction is allowed because Rule 1, which specifies a straight path, 2

3 applies only to grains while they are not interacting and thus does not apply to point A, the point at which the interaction occurs. [Figure 2: Two different ways to label the events in Figure 1.] In the second way to conceptualize the situation (Figure 2, right), grain 2 absorbs grain 1 and then continues its trajectory while grain 1 no longer exists. These different ways to conceptualize the interaction between grains are equivalent and merely represent different methods of labeling. They are important, however, in that they illustrate a fundamental property of HS: A grain can change its direction of motion only during an absorption or emission event. d > 0 d =0 y grain 5 y grain 4 B grain 5 grain 3 d grain 4 A grain 1 grain 2 grain 1 grain 2 x x [Figure 3: Two more allowable constructions in HS.] 3

4 Figure 3 (left) shows another construction allowable in HS. Grains 1 and 2 converge at point A and absorb on contact to produce grain 3; grain 3 travels from A to B; an emission occurs at B, resulting in grains 4 and 5 leaving point B. Let d = the distance between point A and B. Since d can be any arbitrary length, consider the limit as d approaches zero, illustrated in Figure 3 (right). In this construction, two grains converge and two grains leave the point of convergence. Using similar constructions, it is easily shown that any whole number of grains >2 can be joined together at a single vertex. The only constraint is that the grains travel toward and away from the vertex in straight lines at speed c. In this sense, HS is a tinker-toy universe in which straight line-segments can be jointed together at vertices. Rule 1 supplies the line segments; Rule 2 supplies the connecting hubs. It is this interaction between the two rules that provides the spatial structure of HS, as described in later sections. Consider the construction in Figure 4. Grain 1 undergoes an emission event at point A, resulting in grains 2 and 3. Let θ = the angle between the paths of grains 2 and 3. The rules of HS do not constrain this angle; any value is permissible. y 2! 3 A 1 x [Figure 4: grain 1 travels to point A; an emission occurs; grains 2 and 3 leave point A.] 4

5 In the special case in which θ = 0, grains 2 and 3 follow the same path and thus are in constant contact. In this case, an absorption can occur, resulting in a single grain 4. This case is diagrammed in Figure 5 (left). Here the construction looks as though a grain is changing its direction of motion spontaneously, but note that the changes of direction still occur at absorption or emission events. Now let point A be brought infinitesimally close to point B; and let grain 4 be re-labeled as grain 1. Figure 5 (right) shows this specialized case in which grain 1 can change its direction due to an emission event followed an infinitesimal time later by an absorption event. This example shows that a vertex in HS can be a joining of as few as two lines. The change of direction of grain 1 seems peculiar, violating expectations of what is permissible in the real universe. We are used to a universe in which momentum is conserved. However, momentum is not defined in HS and the change of direction of grain 1, due to an emission event followed an infinitesimal time later by an absorption event, is permissible. y y 2 & 3,! = 0 A B x x [Figure 5: Permissible constructions in HS. Left: grain 1 emits grains 2 and 3 at point A. Grains 2 and 3 follow the same path and absorb each other at point B to produce grain 4. Right: the same construction but with points A and B infinitesimally close to each other and grain 4 relabeled as grain 1.] 5

6 Stationary objects in HS Thus far we have considered the behavior of grains in HS that travel at speed c in reference frame R1. It is possible to construct objects in HS that are stationary in R1. Figure 6 shows an especially simple example. In the first time period (Figure 6, left), grain 1 travels from point D to point A and grain 2 travels from point B to point A. At A, grain 1 absorbs grain 2 and then an infinitesimal time later emits it. During the second time period (Figure 6, center), grain 1 travels from A to D, while grain 2 travels from A to B. Two other grains, 3 and 4, follow similar motions along opposite sides of the construction. These four grains interact at the four vertices and continually bounce back and forth, forming a construction that is stationary in R1. Note that there is nothing to hold the grains to these trajectories. It is equally permissible in HS that the grains, upon absorption and re-emission, fly off at odd angles and never encounter one another again. The object in Figure 6 is only one arbitrary member of the infinite set of permissible constructions in HS. Because there are no dynamical laws in HS, there is no way to assess the likelihood that the object in Figure 6 will actually occur in HS. All we can do is take the tinker-toy components given to us and explore what objects can and can t be built out of them. The object in Figure 6 can be built, and belongs to the specific subset of stationary objects. [Figure 6: An example of a stationary object permissible in HS. The pattern of motion of this object repeats indefinitely.] Since the size of the object in Figure 6 is arbitrary, consider the case in which the height and width approach zero. The object in this case becomes dimensionless in x and y. It is 6

7 reduced to a point particle. Thus, even though grains are constrained to travel at speed c with respect to R1, it is possible to construct a point particle that is stationary in R1. Indeed, it is possible to construct objects and point particles in HS that move at any speed v c. It is not possible to construct objects in HS that move at speeds greater than c, because the component grains of all objects are fixed at speed c. Moving objects in HS Consider the object in Figure 7. (All features of the object in Figure 7 are designated with an underline.) It is constructed to be similar to the object in Figure 6. It has the same number of grains interacting at the same number of vertices. Segments AB and DC are parallel to the x axis, and segments AD and BC are parallel to the y axis, matching the object in Figure 6. Its height, AD, is equal to the height of the object in Figure 6, AD. However, the object in Figure 7 is moving in the positive x direction at some speed v < c. That is, points A, B, C, and D are all moving to the right at speed v. Because of this motion, the object in Figure 7 must have a different structure from the object in Figure 6. Three main differences are discussed below. [Figure 7: This object is moving to the right at speed v in R1.] Clock rate In the object in Figure 6, grain 1 travels from A to D and back to A. Its pattern of motion repeats after this round trip, thus after a time interval of: [Eq.2] "t 1 = (2AD). c 7

8 In the object in Figure 7, grain 1 travels from A to D and back to A, traversing the height of the object. At the same time, the grain is moving to the right at speed v, in tandem with the object. Since the total speed of the grain is fixed at c, and the horizontal speed is v, the vertical speed of the grain must be (c 2 -v 2 ) 1/2. The pattern of motion of grain 1 therefore repeats after a time interval of: [Eq.3] "t 1 = (2AD) (c 2 # v 2 ) 1/ 2. Since we have set the two objects to the same height: [Eq.4] AD = AD. Combining equations 2-4, we find: [Eq.5] "t 1 = "t 1 (1# v 2 /c 2 ) 1/ 2. Thus, grain 1 repeats its pattern of motion on a slower time scale than grain 1. That is, the rate at which internal events occur for the moving object in Figure 7 is slower than for the stationary object in Figure 6. The greater the speed v, the longer the time interval Δt between these internal events. In the limit as v approaches c, all internal motion in the object will stop. The component grains will be constrained to move in the positive x direction in straight lines at speed c. Length For the object in Figure 6, we know that grain 1 and grain 2 must always reach point A at the same time for the required absorption to occur. Therefore, the round-trip time for grain 1 must equal the round-trip time for grain 2. Thus: 8

9 2AD/c = 2AB/c, or: [Eq.6] AD = AB. That is, the height equals the length. For the object in Figure 7, again, grain 1 and grain 2 must always reach point A at the same time. Therefore the round-trip time for grain 1 must equal the round-trip time for grain 2. Thus: [Eq.7] 2AD AB = (c 2 " v 2 1/ 2 ) (c " v) + AB (c + v). Combining equations 4, 6, and 7: [Eq.8] AB = AB(1" v 2 /c 2 ) 1/ 2. That is, the length of the object in Figure 7 does not equal the length of the object in Figure 6. Instead, the length in Figure 7 is shortened. In the limit as v approaches c, the length of the object approaches zero. Simultaneity of events Consider grains 1 and 2 in the object in Figure 6. The grains leave point A at the same time (Figure 6, center). They travel the same distance at the same speed, thus grain 1 reaches point D at the same time that grain 2 reaches point B. The absorption that occurs at point D, and the absorption that occurs at point B, are therefore simultaneous. For the object in Figure 7, the two corresponding events are not simultaneous. Grains 1 and 2 leave point A at the same time. Grain 1 arrives at point D after a time AD/(c 2 -v 2 ) 1/2. Grain 2, however, arrives at point B after a time AB/(c-v). The time difference between these two events is as follows: 9

10 [Eq.9] t (event at B) - t (event at D) = AB (c " v) " AD (c 2 " v 2 ). 1/ 2 By using equations 4, 6, and 8, we can express the right-hand side of equation 9 in terms of AB: [Eq.10] t (event at B) - t (event at D) = AB(v /c 2 ) (1" v 2 /c 2 ) 1/ 2. That is, events that were simultaneous in the stationary object in Figure 6 are not simultaneous in the moving object in Figure 7. The time difference between the two events in Figure 7 is proportional to the x distance between the corresponding two events in Figure 6. The object in Figure 6 and the object in Figure 7 are therefore clearly different. We can try to construct them in the same way, with the same number of grains interacting at the same number of vertices. We can align their segments in the same way with respect to the x and y axes. We can give them the same height. Beyond these similarities, however, the rules of HS require the objects to be different. The object that is moving in R1 repeats on a slower time scale; its length is shortened along the direction of motion; and events that were simultaneous in the stationary object may not be simultaneous in the moving object. Moving reference frames in HS. Consider a reference frame other than R1. Let R2 be a reference frame moving in the positive x direction at speed v with respect to R1. For sake of ease of explanation, let us accept the somewhat fanciful supposition that HS is inhabited, and the creatures in R1 and R2 are in communication. They attempt to define a set of measurement standards so that they can communicate in a meaningful fashion. R1 chooses a standard object; for example, the square object in Figure 6. The height and length of this object provide standard units of distance in the x and y dimensions. Each vertex of the object is the location of an event, an emission of one grain by another, that repeats in time. The time between these repeating events can serve as a clock. Let us call this object S1 for the standard object in R1. It is like a pocket ruler and 10

11 stop-watch that R1 can use to measure events. By tiling the space of HS with many copies of S1, the observer R1 can construct a coordinate grid. Now consider an object S2, a similar standard object but at rest in R2. In order to function as a meaningful measurement standard, S2 must be calibrated with respect to S1. But we have already seen that S1 and S2 are required to be different in some respects. Thus observer 1, using S1 to build a coordinate grid, may measure an event to occur at coordinates x, y, and t; whereas observer 2 using S2 to build a coordinate grid will arrive at a different set of measurements, x, y, and t. Suppose the coordinate grid built of S1 and the coordinate grid built of S2 are aligned such that both have the same origin. The point (x=0, y=0, t=0) is the same as the point (x =0, y =0, t =0). Then the equations that relate the primed and unprimed variables can be derived with a small amount of algebra using the equations that relate S1 and S2. They are: [Eq.11] [Eq.12] x'= y'= y x " vt (1" v 2 /c 2 ) 1/ 2 [Eq.13] t'= t " xv /c 2 (1" v 2 /c 2 ) 1/ 2 These equations are the Lorentz transformation equations of special relativity. They were derived using the objects S1 and S2 as measurement standards. However, any object of sufficient complexity that is stationary in R1, and its matching counterpart that is stationary in R2, can be used to arrive at the same transformation equations. (To step through this derivation in the general case of an arbitrary object is somewhat tedious and is not included here for the sake of brevity.) The transformation equations are independent of how the measuring rods and clocks are constructed. They are a consequence of the rules of HS. 11

12 Special Relativity in HS Special relativity was originally derived by Einstein from two postulates: the constancy of the speed of light, and the principle of relativity, or the principle that the laws of physics are the same for any observer in constant motion. Do these two principles hold true in HS? Constancy of the speed of light. Consider a grain moving from one point to another. R1 measures the locations and times and calculates the speed of the grain as c (by definition, according to Rule 1). R2 also measures the same events and calculates the speed of the grain. Equations imply that R2 will also measure a speed of c. That is, the speed of any grain is always measured as c regardless of the reference frame. Thus the first postulate of special relativity, the constancy of the speed of light in all reference frames, holds true in HS. Principle of relativity. Rule 1 of HS states that when grains are not interacting they travel at a fixed speed c in reference frame R1. We now know that this rule also holds true in reference frame R2. Rule 2 states that grains can absorb or emit each other. This rule is independent of any specific reference frame. Thus, both rules of HS are the same in any arbitrary reference frame in uniform motion, satisfying the postulate of relativity. Note that both postulates of special relativity had to be derived in HS. They were not provided at the outset as postulates. In particular, Rule 1 is expressed in a frame dependant fashion, as if reference frame R1 were a preferred reference frame. It is only by examining the properties of HS that we find out that R1 is not a preferred reference frame and that Rule 1 is unchanged in other reference frames. Einstein vs Newton Perhaps the most peculiar property of HS is that we can choose between an Einsteinian view or a Newtonian view. Both views are correct. From a Newtonian perspective, we can arbitrarily declare one reference frame (for example R1) to be at absolute rest. The measurement discrepancies between that rest frame and other, moving reference frames can be understood in terms of the mechanical combining and splitting of particles that move at constant speed through a Newtonian space-time. For example, a clock translating through space at high speed has its inner workings slowed down. The reason 12

13 is that its components are fixed at a set speed. If part of that speed is already taken up in the global, translational motion of the clock, then there is less speed left over for the inner workings of the clock. In the limit as the clock reaches the speed c, its components are already translating at their full speed and cannot move with respect to each other, hence all internal motion in the clock must stop. From an Einsteinian perspective, the rules of HS are the same in all reference frames; no experiment can distinguish one reference frame as an absolute rest frame; and space and time are intermixed. Both descriptions, the Newtonian and the Einsteinian, provide mathematically accurate descriptions of HS. They are equivalent. 13

2.1 The Ether and the Michelson-Morley Experiment

2.1 The Ether and the Michelson-Morley Experiment Chapter. Special Relativity Notes: Some material presented in this chapter is taken The Feynman Lectures on Physics, Vol. I by R. P. Feynman, R. B. Leighton, and M. Sands, Chap. 15 (1963, Addison-Wesley)..1

More information

Simultaneity, Time Dilation, and Length Contraction Using Minkowski Diagrams and Lorentz Transformations

Simultaneity, Time Dilation, and Length Contraction Using Minkowski Diagrams and Lorentz Transformations Simultaneity, Time Dilation, and Length Contraction Using Minkowski Diagrams and Lorentz Transformations Dr. Russell L. Herman January 25, 2008 (modified: January 17, 2018) Abstract In these notes we present

More information

Modern Physics. Third Edition RAYMOND A. SERWAY CLEMENT J. MOSES CURT A. MOYER

Modern Physics. Third Edition RAYMOND A. SERWAY CLEMENT J. MOSES CURT A. MOYER Modern Physics Third Edition RAYMOND A. SERWAY CLEMENT J. MOSES CURT A. MOYER 1 RELATIVITY 1.1 Special Relativity 1.2 The Principle of Relativity, The Speed of Light 1.3 The Michelson Morley Experiment,

More information

Physics 2D Lecture Slides Lecture 3. January 8, 2010

Physics 2D Lecture Slides Lecture 3. January 8, 2010 Physics 2D Lecture Slides Lecture 3 January 8, 2010 Immediate Consequences of Einstein s Postulates: Recap Events that are simultaneous for one Observer are not simultaneous for another Observer in relative

More information

Experimental Values of Lorentz Transformations of Mass and Time

Experimental Values of Lorentz Transformations of Mass and Time Experimental Values of Lorentz Transformations of Mass and Time Lorentz Transformation Thought Experiment GPS Clock Calculations Pound-Rebka Experiment Triplet Paradox Experiment The Lorentz transformation

More information

On the Arbitrary Choice Regarding Which Inertial Reference Frame is "Stationary" and Which is "Moving" in the Special Theory of Relativity

On the Arbitrary Choice Regarding Which Inertial Reference Frame is Stationary and Which is Moving in the Special Theory of Relativity Regarding Which Inertial Reference Frame is "Stationary" and Which is "Moving" in the Special Theory of Relativity Douglas M. Snyder Los Angeles, CA The relativity of simultaneity is central to the special

More information

On Einstein s Time Dilation and Length Contraction

On Einstein s Time Dilation and Length Contraction On Einstein s Time Dilation and Length Contraction Stephen J. Crothers Tasmania, Australia thenarmis@yahoo.com 17 February, 2017 ABSTRACT Einstein s time dilation and length contraction in his Special

More information

Rigid body motion Limits on Acceleration

Rigid body motion Limits on Acceleration Rigid body motion Limits on Acceleration John Freidenfelds, PhD December 23, 2016 Abstract It is well-known that, according to special relativity, there is an absolute speed limit on objects traveling

More information

16. Einstein and General Relativistic Spacetimes

16. Einstein and General Relativistic Spacetimes 16. Einstein and General Relativistic Spacetimes Problem: Special relativity does not account for the gravitational force. To include gravity... Geometricize it! Make it a feature of spacetime geometry.

More information

Special Theory of Relativity (I) Newtonian (Classical) Relativity. Newtonian Principle of Relativity. Inertial Reference Frame.

Special Theory of Relativity (I) Newtonian (Classical) Relativity. Newtonian Principle of Relativity. Inertial Reference Frame. Special Theory of Relativity (I) Newtonian (Classical) Relativity Einstein s Postulates The Lorentz Transformation Time Dilation and Length Contraction Addition of Velocities Assumption It is assumed that

More information

SPECIAL RELATIVITY: PART TWO Bertrand Wong, Eurotech, S pore,

SPECIAL RELATIVITY: PART TWO Bertrand Wong, Eurotech, S pore, SPECIAL RELATIVITY: PART TWO Bertrand Wong, Eurotech, S pore, Email: bwong8@singnet.com.sg Abstract According to Einstein s Special Theory of Relativity, the speed of light always remains constant at 186,000

More information

Chapter 37. Relativity. PowerPoint Lectures for University Physics, 14th Edition Hugh D. Young and Roger A. Freedman Lectures by Jason Harlow

Chapter 37. Relativity. PowerPoint Lectures for University Physics, 14th Edition Hugh D. Young and Roger A. Freedman Lectures by Jason Harlow Chapter 37 Relativity PowerPoint Lectures for University Physics, 14th Edition Hugh D. Young and Roger A. Freedman Lectures by Jason Harlow Learning Goals for Chapter 37 Looking forward at why different

More information

Kinematics of special relativity

Kinematics of special relativity Chapter 2 Kinematics of special relativity 2.1 Special Relativity 2.1.1 Principles of Relativity Einstein postulated that there was still Galilean invariance, i. e. all uniformly moving observers had the

More information

MINKOWSKIAN SPACE, GRAPHS, EVENTS, WORLD LINES and MEASURING TIME

MINKOWSKIAN SPACE, GRAPHS, EVENTS, WORLD LINES and MEASURING TIME MINKOWSKIAN SPACE, GRAPHS, EVENTS, WORLD LINES and MEASURING TIME One second after we started our stop watch, little Johnny pukes in the corner of his room. Relative to the corner, the happening occurs

More information

Introduction to Kinematics. Motion, Forces and Energy

Introduction to Kinematics. Motion, Forces and Energy Introduction to Kinematics Motion, Forces and Energy Mechanics: The study of motion Kinematics The description of how things move 1-D and 2-D motion Dynamics The study of the forces that cause motion Newton

More information

Special Theory of Relativity. The Newtonian Electron. Newton vs. Einstein. So if Newtonian Physics is wrong. It is all Relative.

Special Theory of Relativity. The Newtonian Electron. Newton vs. Einstein. So if Newtonian Physics is wrong. It is all Relative. Special Theory of Relativity Chapter 26 The Newtonian Electron Newtonian Theory (everything we have done so far in class) can be tested at high speeds by accelerating electrons or other charged particles

More information

Lorentz Transformations and the Twin Paradox By James Carter

Lorentz Transformations and the Twin Paradox By James Carter Lorentz Transformations and the Twin Paradox By James Carter The Lorentz transformation m = M/ 1-v 2 /c 2 is a principle of measurement that can be classed as one of the laws of physics. (A moving body

More information

Derivation of Special Theory of Relativity from Absolute Inertial Reference Frame

Derivation of Special Theory of Relativity from Absolute Inertial Reference Frame Derivation of Special Theory of Relativity from Absolute Inertial Reference Frame: Michelson-Morley Experiment, Lorentz Contraction, Transverse Doppler Red-Shift, Time Dilation Justin Lee October 8 th,

More information

The Pound-Rebka Experiment as Disproof of Einstein s General Relativity Gravity Theory.

The Pound-Rebka Experiment as Disproof of Einstein s General Relativity Gravity Theory. The Pound-Rebka Experiment as Disproof of Einstein s General Relativity Gravity Theory. By James Carter When Einstein first used his equations to predict the transverse gravitational red shift of photons

More information

PHYSICS - CLUTCH CH 34: SPECIAL RELATIVITY.

PHYSICS - CLUTCH CH 34: SPECIAL RELATIVITY. !! www.clutchprep.com CONCEPT: INERTIAL REFERENCE FRAMES A reference frame is a coordinate system that you make measurements in, and there are two types: - Inertial reference frames, which move at velocity

More information

2.3 The Lorentz Transformation Eq.

2.3 The Lorentz Transformation Eq. Announcement Course webpage http://highenergy.phys.ttu.edu/~slee/2402/ Textbook PHYS-2402 Lecture 3 HW1 (due 9/13) Chapter 2 20, 26, 36, 41, 45, 50, 51, 55, 58 Sep. 6, 2016 2.3 The Lorentz Transformation

More information

The Foundations of Special Relativity

The Foundations of Special Relativity The Foundations of Special Relativity 1 Einstein's postulates of SR: 1. The laws of physics are identical in all inertial reference frames (IFs). 2. The speed of light in vacuum, c, is the same in all

More information

The spacetime of special relativity

The spacetime of special relativity 1 The spacetime of special relativity We begin our discussion of the relativistic theory of gravity by reviewing some basic notions underlying the Newtonian and special-relativistic viewpoints of space

More information

Gravitational Effects on Light Propagation. Copyright 2009 Joseph A. Rybczyk

Gravitational Effects on Light Propagation. Copyright 2009 Joseph A. Rybczyk Gravitational Effects on Light Propagation Copyright 2009 Joseph A. Rybczyk Abstract An examination of the theoretical relationship between gravity and light propagation is presented that focuses on the

More information

Unit 2 - Linear Motion and Graphical Analysis

Unit 2 - Linear Motion and Graphical Analysis Unit 2 - Linear Motion and Graphical Analysis Motion in one dimension is particularly easy to deal with because all the information about it can be encapsulated in two variables: x, the position of the

More information

Special Relativity-General Discussion

Special Relativity-General Discussion Chapter 1 Special Relativity-General Discussion Let us consider a space-time event. By this we mean a physical occurence at some point in space at a given time. In order to characterize this event we introduce

More information

Announcement. Einstein s Postulates of Relativity: PHYS-3301 Lecture 3. Chapter 2. Sep. 5, Special Relativity

Announcement. Einstein s Postulates of Relativity: PHYS-3301 Lecture 3. Chapter 2. Sep. 5, Special Relativity Announcement PHYS-3301 Lecture 3 Sep. 5, 2017 2 Einstein s Postulates of Relativity: Chapter 2 Special Relativity 1. Basic Ideas 6. Velocity Transformation 2. Consequences of Einstein s Postulates 7. Momentum

More information

Before we work on deriving the Lorentz transformations, let's first look at the classical Galilean transformation.

Before we work on deriving the Lorentz transformations, let's first look at the classical Galilean transformation. Background The curious "failure" of the Michelson-Morley experiment in 1887 to determine the motion of the earth through the aether prompted a lot of physicists to try and figure out why. The first attempt

More information

Black Holes -Chapter 21

Black Holes -Chapter 21 Black Holes -Chapter 21 The most massive stellar cores If the core is massive enough (~3 M ; total initial mass of star > 25 M or so), even neutron degeneracy pressure can be overwhelmed by gravity. A

More information

A. B. Lahanas University of Athens, Physics Department, Nuclear and Particle Physics Section, Athens , Greece

A. B. Lahanas University of Athens, Physics Department, Nuclear and Particle Physics Section, Athens , Greece SPECIAL RELATIVITY A. B. Lahanas University of Athens, Physics Department, Nuclear and Particle Physics Section, Athens 157 71, Greece Abstract We give an introduction to Einstein s Special Theory of Relativity.

More information

Physics 2D Lecture Slides Lecture 4. April 3, 2009

Physics 2D Lecture Slides Lecture 4. April 3, 2009 Physics 2D Lecture Slides Lecture 4 April 3, 2009 Synchronizing Clocks Sam v Sally After coincidence of their origins at t=0, t = 0 Sam and Sally agree to send light signals to each other after time t

More information

CHAPTER 2 Special Theory of Relativity-part 1

CHAPTER 2 Special Theory of Relativity-part 1 CHAPTER 2 Special Theory of Relativity-part 1 2.1 The Apparent Need for Ether 2.2 The Michelson-Morley Experiment 2.3 Einstein s Postulates 2.4 The Lorentz Transformation 2.5 Time Dilation and Length Contraction

More information

LIGHT SPEED CANNOT BE A UNIVERSAL CONSTANT

LIGHT SPEED CANNOT BE A UNIVERSAL CONSTANT LIGHT SPEED CANNOT BE A UNIVERSAL CONSTANT CHAN RASJID KAH CHEW 4 March 2017 ABSTRACT. That motion is relative is an accepted physical principle as everything is in motion relative to some other thing

More information

Mathematical review trigonometry vectors Motion in one dimension

Mathematical review trigonometry vectors Motion in one dimension Mathematical review trigonometry vectors Motion in one dimension Used to describe the position of a point in space Coordinate system (frame) consists of a fixed reference point called the origin specific

More information

Physics. Special Relativity

Physics. Special Relativity Physics Special Relativity 1 Albert Einstein, the high school dropout and patent office clerk published his ideas on Special Relativity in 1905. 2 Special vs. General Relativity Special Relativity deals

More information

Rethinking the Principles of Relativity. Copyright 2010 Joseph A. Rybczyk

Rethinking the Principles of Relativity. Copyright 2010 Joseph A. Rybczyk Rethinking the Principles of Relativity Copyright 2010 Joseph A. Rybczyk Abstract An analysis of all of the principles involved in light propagation lead to the discovery that the relativistic principle

More information

Lecture 4 - Lorentz contraction and the Lorentz transformations

Lecture 4 - Lorentz contraction and the Lorentz transformations Lecture 4 - Lorentz contraction and the Lorentz transformations E. Daw April 4, 2011 1 The inadequacy of the Galilean transformations In Lecture 1 we learned that two inertial (non-accelerating) observers,

More information

Chapter 11. Special Relativity

Chapter 11. Special Relativity Chapter 11 Special Relativity Note: Please also consult the fifth) problem list associated with this chapter In this chapter, Latin indices are used for space coordinates only eg, i = 1,2,3, etc), while

More information

Advantages of Three-Dimensional Space-Time Frames

Advantages of Three-Dimensional Space-Time Frames Frontiers in Science 01, (3): 18-3 DOI: 10.593/j.fs.01003.01 Advantages of Three-Dimensional Space-Time Frames Tower Chen 1,*, Zeon Chen 1 Unit of Mathematical Sciences, College of Natural and Applied

More information

The Other Meaning of Special Relativity

The Other Meaning of Special Relativity The Other Meaning of Special Relativity Robert A. Close* ABSTRACT Einstein s special theory of relativity postulates that the speed of light is a constant for all inertial observers. This postulate can

More information

Chapter 5. Past and Proposed Experiments Detecting Absolute Motion

Chapter 5. Past and Proposed Experiments Detecting Absolute Motion Chapter 5 Past and Proposed Experiments Detecting Absolute Motion In this Chapter I gave different interpretations for the results of some famous past experiments. My interpretations are based on the following

More information

College Physics B - PHY2054C. Special Relativity 11/10/2014. My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building.

College Physics B - PHY2054C. Special Relativity 11/10/2014. My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building. College - PHY2054C 11/10/2014 My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building Outline 1 2 3 1 The speed of light is the maximum possible speed, and it is always measured to have the same value

More information

4-Vector Notation. Chris Clark September 5, 2006

4-Vector Notation. Chris Clark September 5, 2006 4-Vector Notation Chris Clark September 5, 2006 1 Lorentz Transformations We will assume that the reader is familiar with the Lorentz Transformations for a boost in the x direction x = γ(x vt) ȳ = y x

More information

Rotational motion of a rigid body spinning around a rotational axis ˆn;

Rotational motion of a rigid body spinning around a rotational axis ˆn; Physics 106a, Caltech 15 November, 2018 Lecture 14: Rotations The motion of solid bodies So far, we have been studying the motion of point particles, which are essentially just translational. Bodies with

More information

Answers to examination-style questions. Answers Marks Examiner s tips

Answers to examination-style questions. Answers Marks Examiner s tips Chapter (a) There is a much greater gap between the mean values of x B for the 0.00 and 0.200 kg masses than there is between the 0.200 and 0.300 kg masses. Measurements for two more values of m between

More information

Chapter 11 Reference Frames

Chapter 11 Reference Frames Chapter 11 Reference Frames Chapter 11 Reference Frames... 2 11.1 Introduction... 2 11.2 Galilean Coordinate Transformations... 2 11.2.1 Relatively Inertial Reference Frames and the Principle of Relativity...

More information

Relativity. Physics April 2002 Lecture 8. Einstein at 112 Mercer St. 11 Apr 02 Physics 102 Lecture 8 1

Relativity. Physics April 2002 Lecture 8. Einstein at 112 Mercer St. 11 Apr 02 Physics 102 Lecture 8 1 Relativity Physics 102 11 April 2002 Lecture 8 Einstein at 112 Mercer St. 11 Apr 02 Physics 102 Lecture 8 1 Physics around 1900 Newtonian Mechanics Kinetic theory and thermodynamics Maxwell s equations

More information

Special Relativity-General Discussion

Special Relativity-General Discussion Chapter 1 Special Relativity-General Discussion Let us consider a spacetime event. By this we mean a physical occurence at some point in space at a given time. in order to characterize this event we introduce

More information

04. Kinematical Effects 1. Time Dilation

04. Kinematical Effects 1. Time Dilation 04. Kinematical Effects 1. Time Dilation B D y' S' P x' Consider a "light clock" that defines a reference frame S'. One "tick" of this clock = time for light to travel PBP = t = 2D c. y y' S' x' S-clock

More information

Gravitation and Cosmology

Gravitation and Cosmology Lecture : Reading: Ohanian, Ch. ---- all!, Ch 2., 2.2 The principle of relativity The principle of relativity was discovered by Galileo. It states that the laws of nature do not permit experimental measurement

More information

Relativistic Constant Acceleration Distance Factor. Copyright 2010 Joseph A. Rybczyk

Relativistic Constant Acceleration Distance Factor. Copyright 2010 Joseph A. Rybczyk Relativistic Constant Acceleration Distance Factor Copyright 2010 Joseph A. Rybczyk Abstract A formalized treatment of a previously discovered principle involving relativistic constant acceleration distances

More information

Basics of Special Relativity

Basics of Special Relativity Basics of Special Relativity You must understand special relativity in order to really understand general relativity. Here s a brief summary of the basic ideas and terminology of special relativity (there

More information

Lorentz Transformation Equations in Galilean Form

Lorentz Transformation Equations in Galilean Form Lorentz Transformation Equations in Galilean Form Sadanand D. Agashe Department of Electrical Engineering Indian Institute of Technology Bombay, Powai, Mumbai-76 India - 400076 email: eesdaia@ee.iitb.ac.in

More information

EPGY Special and General Relativity. Lecture 4B

EPGY Special and General Relativity. Lecture 4B Lecture 4B In the previous lecture we found that the proper description of the universe is one consisting of a four-dimensional manifold (space) endowed with a Lorentzian metric, (of course we are restricting

More information

The True Nature of the Special Relativity Light Clock. Copyright 2012 Joseph A. Rybczyk

The True Nature of the Special Relativity Light Clock. Copyright 2012 Joseph A. Rybczyk The True Nature of the Special Relativity Light Clock Copyright 2012 Joseph A. Rybczyk Abstract It is generally believed that the light clock typically associated with special relativity correlates the

More information

Special Theory of Relativity. A Brief introduction

Special Theory of Relativity. A Brief introduction Special Theory of Relativity A Brief introduction Classical Physics At the end of the 19th century it looked as if Physics was pretty well wrapped up. Newtonian mechanics and the law of Gravitation had

More information

FORCE AND MOTION Study Notes

FORCE AND MOTION Study Notes FORCE AND MOTION Study Notes FORCE: a push or pull acting on an object. examples of forces are gravity, friction, magnetism, and applied forces. Forces cause an object to change its speed, direction, or

More information

dt = p m, (2.1.1) dt = p

dt = p m, (2.1.1) dt = p Chapter 2 Special relativity 2.1 Galilean relativity We start our discussion of symmetries by considering an important example of an invariance, i.e. an invariance of the equations of motion under a change

More information

Lecture 12 Notes, Electromagnetic Theory II Dr. Christopher S. Baird, faculty.uml.edu/cbaird University of Massachusetts Lowell

Lecture 12 Notes, Electromagnetic Theory II Dr. Christopher S. Baird, faculty.uml.edu/cbaird University of Massachusetts Lowell Lecture 12 Notes, Electromagnetic Theory II Dr. Christopher S. Baird, faculty.uml.edu/cbaird University of Massachusetts Lowell 1. Velocities in Special Relativity - As was done in Galilean relativity,

More information

Spacetime diagrams and Bondi s k-calculus

Spacetime diagrams and Bondi s k-calculus Spacetime diagrams and Bondi s k-calculus Two important consequences of Einstein s 1905 paper on SR: 1. It was immediately apparent that physicists had been taking the assignment and measurement of coordinates

More information

Chapter 36 The Special Theory of Relativity. Copyright 2009 Pearson Education, Inc.

Chapter 36 The Special Theory of Relativity. Copyright 2009 Pearson Education, Inc. Chapter 36 The Special Theory of Relativity Units of Chapter 36 Galilean Newtonian Relativity The Michelson Morley Experiment Postulates of the Special Theory of Relativity Simultaneity Time Dilation and

More information

Introduction to Kinematics. Motion, Forces and Energy

Introduction to Kinematics. Motion, Forces and Energy Introduction to Kinematics Motion, Forces and Energy Mechanics: The study of motion Kinematics The description of how things move 1-D and 2-D motion Dynamics The study of the forces that cause motion Newton

More information

Chapter 26. Relativity

Chapter 26. Relativity Chapter 26 Relativity Time Dilation The vehicle is moving to the right with speed v A mirror is fixed to the ceiling of the vehicle An observer, O, at rest in this system holds a laser a distance d below

More information

Correct Resolution of the Twin Paradox

Correct Resolution of the Twin Paradox Correct Resolution of the Twin Paradox Michael Huemer In the following, I explain the Twin Paradox, which is supposed to be a paradoxical consequence of the Special Theory of Relativity (STR). I give the

More information

PHYSICS Kinematics in One Dimension

PHYSICS Kinematics in One Dimension PHYSICS Kinematics in One Dimension August 13, 2012 www.njctl.org 1 Motion in One Dimension Return to Table of Contents 2 Distance We all know what the distance between two objects is... So what is it?

More information

Special Theory of Relativity. PH101 Lec-3

Special Theory of Relativity. PH101 Lec-3 Special Theory of Relativity PH101 Lec-3 Clock Synchronization In order to measure the time at which an event occurred at a point in space, we assumed that all of space are filled with clocks, one for

More information

Kinematics in Two Dimensions; 2D- Vectors

Kinematics in Two Dimensions; 2D- Vectors Kinematics in Two Dimensions; 2D- Vectors Addition of Vectors Graphical Methods Below are two example vector additions of 1-D displacement vectors. For vectors in one dimension, simple addition and subtraction

More information

Chapter 10 Momentum, System of Particles, and Conservation of Momentum

Chapter 10 Momentum, System of Particles, and Conservation of Momentum Chapter 10 Momentum, System of Particles, and Conservation of Momentum 10.1 Introduction... 1 10. Momentum (Quantity of Motion) and Impulse... 1 10..1 Average Force, Momentum, and Impulse... 10.. Non-Constant

More information

Kinematic Solutions to the Twin Paradox in Special Relativity

Kinematic Solutions to the Twin Paradox in Special Relativity Vadim N.Matvejev 1, Oleg V. Matvejev 10-Jun-015 This paper deals with the twin paradox within special relativity. The paper reveals the cause of paradoxical time dilation for an inertial stay-at-home twin,

More information

Noncollision Singularities in the n-body Problem

Noncollision Singularities in the n-body Problem Noncollision Singularities in the n-body Problem Danni Tu Department of Mathematics, Princeton University January 14, 2013 The n-body Problem Introduction Suppose we have n points in R 3 interacting through

More information

Modern Physics Part 2: Special Relativity

Modern Physics Part 2: Special Relativity Modern Physics Part 2: Special Relativity Last modified: 23/08/2018 Links Relative Velocity Fluffy and the Tennis Ball Fluffy and the Car Headlights Special Relativity Relative Velocity Example 1 Example

More information

Chapter 3: Vectors and Projectile Motion

Chapter 3: Vectors and Projectile Motion Chapter 3: Vectors and Projectile Motion Vectors and Scalars You might remember from math class the term vector. We define a vector as something with both magnitude and direction. For example, 15 meters/second

More information

Position-Time Graphs

Position-Time Graphs Position-Time Graphs Suppose that a man is jogging at a constant velocity of 5.0 m / s. A data table representing the man s motion is shown below: If we plot this data on a graph, we get: 0 0 1.0 5.0 2.0

More information

Astronomy 421. Lecture 24: Black Holes

Astronomy 421. Lecture 24: Black Holes Astronomy 421 Lecture 24: Black Holes 1 Outline General Relativity Equivalence Principle and its Consequences The Schwarzschild Metric The Kerr Metric for rotating black holes Black holes Black hole candidates

More information

College Physics B - PHY2054C. Special & General Relativity 11/12/2014. My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building.

College Physics B - PHY2054C. Special & General Relativity 11/12/2014. My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building. Special College - PHY2054C Special & 11/12/2014 My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building Outline Special 1 Special 2 3 4 Special Galilean and Light Galilean and electromagnetism do predict

More information

Light and Projectiles

Light and Projectiles Light and Projectiles Roger J Anderton R.J.Anderton@btinternet.com There has been unfortunately a mistake made with how projectiles have been mathematically modelled; it is a subtle problem and has carried

More information

Einstein for Everyone Lecture 3: Special Relativity

Einstein for Everyone Lecture 3: Special Relativity Einstein for Everyone Lecture 3: Special Relativity Dr. Erik Curiel Munich Center For Mathematical Philosophy Ludwig-Maximilians-Universität 1 Summary of Historical Background 2 Emission Theories Introduction

More information

Physics 209 Fall 2002 Notes 5 Thomas Precession

Physics 209 Fall 2002 Notes 5 Thomas Precession Physics 209 Fall 2002 Notes 5 Thomas Precession Jackson s discussion of Thomas precession is based on Thomas s original treatment, and on the later paper by Bargmann, Michel, and Telegdi. The alternative

More information

Video Analysis of a Ball on a Rotating Merry-go-round

Video Analysis of a Ball on a Rotating Merry-go-round Video Analysis of a Ball on a Rotating Merry-go-round Apparatus Tracker software (free; download from http://www.cabrillo.edu/ dbrown/tracker/) video: coriolis-merry-go-round-ball.mov from http://physics.highpoint.edu/

More information

2.4 The Lorentz Transformation

2.4 The Lorentz Transformation Announcement Course webpage http://highenergy.phys.ttu.edu/~slee/2402/ Textbook PHYS-2402 Lecture 4 Jan. 27, 2015 Lecture Notes, HW Assignments, Physics Colloquium, etc.. 2.4 The Lorentz Transformation

More information

Lecture Notes on Special Relativity prepared by

Lecture Notes on Special Relativity prepared by Lecture Notes on Special Relativity prepared by J D Cresser Department of Physics Macquarie University 8 th August2005 Contents 1 Introduction: What is Relativity? 3 2 Frames of Reference 7 2.1 Constructing

More information

We saw last time how the development of accurate clocks in the 18 th and 19 th centuries transformed human cultures over the world.

We saw last time how the development of accurate clocks in the 18 th and 19 th centuries transformed human cultures over the world. We saw last time how the development of accurate clocks in the 18 th and 19 th centuries transformed human cultures over the world. They also allowed for the precise physical measurements of time needed

More information

2.1 Einstein s postulates of Special Relativity. (i) There is no ether (there is no absolute system of reference).

2.1 Einstein s postulates of Special Relativity. (i) There is no ether (there is no absolute system of reference). Chapter 2 Special Relativity The contradiction brought about by the development of Electromagnetism gave rise to a crisis in the 19th century that Special Relativity resolved. 2.1 Einstein s postulates

More information

Space, Time and Simultaneity

Space, Time and Simultaneity PHYS419 Lecture 11: Space, Time & Simultaneity 1 Space, Time and Simultaneity Recall that (a) in Newtonian mechanics ( Galilean space-time ): time is universal and is agreed upon by all observers; spatial

More information

Announcements. l Register your iclicker on LON-CAPA. l First exam: Feb 6 in Life Sciences A133

Announcements. l Register your iclicker on LON-CAPA. l First exam: Feb 6 in Life Sciences A133 Announcements l LON-CAPA #1 and Mastering Physics 1+2 due next Tuesday help room hours (Strosacker Help Room, 1248 BPS): M: 5-8 PM W: 5-8 PM F: 2-6 PM l Guest lecturer next Tuesday l Register for Mastering

More information

The Nature of Space-Time

The Nature of Space-Time Chapter 9 The Nature of Space-Time 9.1 The Problem of Coordinates The basic problem of physics is to track in space and time the development of elements of a system. This requires that we have some method

More information

Special Relativity - Math Circle

Special Relativity - Math Circle Special Relativity - Math Circle Jared Claypoole Julio Parra Andrew Yuan January 24, 2016 Introduction: The Axioms of Special Relativity The principle of relativity existed long before Einstein. It states:

More information

Galilean Spacetime (Neo-Newtonian Spacetime) P t = 2

Galilean Spacetime (Neo-Newtonian Spacetime) P t = 2 (Neo-Newtonian Spacetime) Figure V t t t = t* vt x P t = 2 t = 1 t = 0 O x x vt x I used figure V above to show you how to change the coordinates of point P in the coordinate system S to coordinates in

More information

Motion along a straight line. Physics 11a. 4 Basic Quantities in Kinematics. Motion

Motion along a straight line. Physics 11a. 4 Basic Quantities in Kinematics. Motion Physics 11a Motion along a straight line Motion Position and Average velocity and average speed Instantaneous velocity and speed Acceleration Constant acceleration: A special case Free fall acceleration

More information

Physics 2D Lecture Slides Lecture 2. Jan. 5, 2010

Physics 2D Lecture Slides Lecture 2. Jan. 5, 2010 Physics 2D Lecture Slides Lecture 2 Jan. 5, 2010 Lecture 1: Relativity Describing a Physical Phenomenon Event (s) Observer (s) Frame(s) of reference (the point of View! ) Inertial Frame of Reference Accelerated

More information

Notes - Special Relativity

Notes - Special Relativity Notes - Special Relativity 1.) The problem that needs to be solved. - Special relativity is an interesting branch of physics. It often deals with looking at how the laws of physics pan out with regards

More information

Chapter 10 Momentum, System of Particles, and Conservation of Momentum

Chapter 10 Momentum, System of Particles, and Conservation of Momentum Chapter 10 Momentum, System of Particles, and Conservation of Momentum 10.1 Introduction... 1 10.2 Momentum (Quantity of Motion) and Average Impulse... 1 Example 10.1 Impulse for a Non-Constant Force...

More information

The Lorentz Transformation from Light-Speed Invariance Alone

The Lorentz Transformation from Light-Speed Invariance Alone The Lorentz Transformation from Light-Speed Invariance Alone Steven Kenneth Kauffmann Abstract The derivation of the Lorentz transformation normally rests on two a priori demands namely that reversing

More information

Covariant Formulation of Electrodynamics

Covariant Formulation of Electrodynamics Chapter 7. Covariant Formulation of Electrodynamics Notes: Most of the material presented in this chapter is taken from Jackson, Chap. 11, and Rybicki and Lightman, Chap. 4. Starting with this chapter,

More information

Experimental Values of Lorentz Transformations of Mass and Time

Experimental Values of Lorentz Transformations of Mass and Time Experimental Values of Lorentz Transformations of Mass and Time Measuring the Fitzgerald Contraction Lorentz Transformation Thought Experiment GPS Clock Calculations Pound-Rebka Experiment Triplet Paradox

More information

Do Accelerating Charged Particles Really Radiate?

Do Accelerating Charged Particles Really Radiate? Do Accelerating Charged Particles Really Radiate? Author: Singer, Michael Date: 1st May 2017 email: singer43212@gmail.com Page 1 Abstract In a particle accelerator charged particles radiate when they pass

More information

Chapter 9 Uniform Circular Motion

Chapter 9 Uniform Circular Motion 9.1 Introduction Chapter 9 Uniform Circular Motion Special cases often dominate our study of physics, and circular motion is certainly no exception. We see circular motion in many instances in the world;

More information

Clock synchronization, a universal light speed, and the terrestrial redshift experiment

Clock synchronization, a universal light speed, and the terrestrial redshift experiment Clock synchronization, a universal light speed, and the terrestrial redshift experiment Alan Macdonald Department of Mathematics Luther College, Decorah, IA 52101, U.S.A. macdonal@luther.edu Am. J. Phys.

More information

Generators for Continuous Coordinate Transformations

Generators for Continuous Coordinate Transformations Page 636 Lecture 37: Coordinate Transformations: Continuous Passive Coordinate Transformations Active Coordinate Transformations Date Revised: 2009/01/28 Date Given: 2009/01/26 Generators for Continuous

More information

Lorentz Transformations and Special Relativity

Lorentz Transformations and Special Relativity Lorentz Transformations and Special Relativity Required reading: Zwiebach 2.,2,6 Suggested reading: Units: French 3.7-0, 4.-5, 5. (a little less technical) Schwarz & Schwarz.2-6, 3.-4 (more mathematical)

More information