**Introduction**

The prevailing concept of spacetime is due primarily to Minkowski’s geometrical contribution (1908) to Einstein’s Special Theory of Relativity. Minkowski saw in the relativistic interpretation of the Lorentz transformations the possibility for a two-dimensional representation of the peculiar interrelationships between bodies having large relative velocities. Assuming the validity of the tenets of Relativity, and assuming the correctness of the chosen geometric representation, it was expected that a graphic portrayal would express and corroborate relativity in its mathematical form, that “physical laws might find their most perfect expression” (1908, 76), facilitating further insights and hypotheses concerning the nature of spacetime. It is my intention to show that while the original expectations remain justified, the spacetime diagram as developed by Minkowski is inherently flawed, and its axiomization has fostered significant misunderstandings about the nature of spacetime and light.

**1. The Minkowski Diagram**

The basic concept of the Minkowski Diagram is to use a single dimension to represent the three spatial dimensions so that one remains available for representing time in a realistic two-dimensional projection. Minkowski first presented the diagram as a derivation of a hyperbolic function (*c ^{2}t^{2}-x^{2} = 1*), but this approach was rendered comparatively cumbersome by subsequent variations. Figure 1 is an example of the most popular version today. As is typical of Minkowski diagrams, the

*x*-axis represents space, while its perpendicular, the

*t*-axis, represents time — both according to an observer

**who is considered to be at rest and moving in time along the**

*S**t*-axis.

^{1}The coordinate axes

*x’*and

*t’*represent the reference frame of an observer

**who is in motion relative to**

*S’***;**

*S**t’*is given by

*x-vt = 0*(where

*v*is the velocity of

**relative to**

*S’***), and**

*S**x’*is given by

*x/t = v*. The diagonal vector determined by

*x = t*is considered to represent the world-line of light emanating from the origin

**.**

*O**Figure 1*

Given this basic construction, any event * P* in spacetime will be located by observers in the diagram as a point at the intersection of lines drawn parallel to their spacetime axes. For

**the coordinates in Figure 1 are (**

*S**x,t*), while for

**they are (**

*S’**x’,t’*). The difference between the two measurements may be derived geometrically by means of “calibration hyperbolae” given by

*x*, from which the unit of measure for

^{2}-t^{2}= constant**can be obtained from the measure of**

*S’***, or they can be derived mathematically by the Lorentz Transformations.**

*S*^{2}The geometric depiction of the relationship thus seems to parallel the mathematics, as is a minimum requirement of any diagram intended as a meaningful representation.

Whereas the Minkowski Diagram in the form shown in Figure 1 is especially designed to depict the differing observations of the same event which result from having different frames of reference (relative motion), a variation as shown in Figure 2 is concerned with the different paths in spacetime (the “world-lines”) of the observers or bodies themselves. In this diagram the reference frame and world-line of the primary observer is given by vector ** A**; vectors

**,**

*B***, and**

*C***are bodies in motion relative to**

*D***, with**

*A***being a light-quantum traveling along one of the**

*D**l-vectors*, which represent the travel of light impinging upon and radiating from the origin

**. The paths of the vectors in relative motion are given by the equation for transforming the primary observer’s time-axis as in Figure 1 (**

*O**x-vt = 0*).

*Figure 2*

Still another variation on the Minkowski Diagram is given in Figure 3, where the interval between two events in the reference frame of a primary observer is compared with the corresponding measures between the events according to various other references. The coordinates described by these observations may be obtained from the Lorentz Transformations, or more readily by the equation for the “invariant interval,” where the proper time *s* of a body in its own frame of reference is compared to its relative spatio-temporal motion according to other frames by *s = (x ^{2}-t^{2})^{.5}*. By plotting a set of hypothetical observations, a parabolic pattern is formed, with the proper time of the primary observer at the vertex and the coordinates of the observations from the more extreme reference frames approaching the light-vectors.

*Figure 3*

**2. The Fundamental Concepts**

The various Minkowski Diagrams share two fundamental concepts which (in addition to the seminal insight concerning the geometric nature of the spatio-temporal relationship) comprise the important contributions of the diagrams to the current understanding of spacetime. One concept is of a parabolic geometry of spacetime, which is thought to supersede the classic notion of flat “Euclidean” space. Even aside from the influence of gravitation, the nature of the equations for transforming coordinates has suggested a parabolic relationship between uniform frames of reference, a function that approaches Euclidean flatness only when relative motion is small relative to *c*. This can be seen in the comparison of unit length between frames, as obtained in Figure 1 with the “calibration hyperbolae,” and in the parabolic pattern in Figure 3 formed by the comparison of observed motion with proper time.

The second concept is of the “light-cones,” the consideration of which has had an enormous influence in shaping subsequent thought about the nature of spacetime, especially in cosmology. From the recognition that it would be impossible for an event to be observed if it were to take place beyond the reach of the fastest signal, and from the graphic representation of that limit with the light-vectors in the Minkowski Diagrams, it has been concluded by some that there exists an “elsewhere,” a set of events lying outside the light-cones which is effectively beyond our spacetime world of experience. Attempts have been made by the more speculatively-inclined to understand everything from black holes to anti-matter in terms of this apparent boundary, and if nothing else the light-cones have consumed a considerable amount of theoretical energy.

Both concepts, of a parabolic geometry and of the light-cones, have seemed to follow from the geometric representation of the tenets of Special Relativity and to have gained credence from that distinguished association. But I wish to show that both are in fact based on a fundamental mistake in the geometric translation of Relativity, the correction of which exposes them as being without foundation.

**3. The Discrepancy**

There is certainly no more important precept in relativity theory than the stricture that in describing the motion of a body we must specify the frame of reference from which the observation is being made. When it’s stated, for instance, that a body travels 3 light-seconds (*ls*) in 5 seconds (*sec*), unless we’re to return to the absolutism of classical physics, we must specify according to whose standard of distance, and according to whose measure of time. If it is to be assumed that unless otherwise stipulated the measurements given are those of an observer at rest in the same reference frame as ourselves, the statement actually consists of an observation that a body travels 3 *ls* in space relative to the observer (and ourselves), while we travel 5 *sec* in time. Although this may be useful in so far at it accounts for two aspects of the relationship, it remains inadequate as a description of the relative motion of the body itself. To fully describe the observed motion relativistically would be to report that a body travels 3 *ls* in space relative to our stationary spatial reference, and a number of *sec* in time that is relative to our corresponding temporal reference of 5 *sec*, given by *(x ^{2}-t^{2})^{.5}*, which in this case yields

*(5*. Strictly speaking, therefore, the body will travel 3

^{2}-3^{2})^{.5}= 4*ls*and 4

*sec*(its clock will be observed to tick 4 seconds), and we will measure that travel from a reference of 0

*ls*and 5

*sec*.

The significance of the distinction being made here is most striking in the description of light: When it’s said in a Newtonian perspective that light travels 1 *ls* in 1 *sec*, we make a relativistic correction and say that it actually travels 1 *ls* relative to our state of rest in space (although our spatial reference is arbitrary in the special case of light) and 0 *sec* relative to our motion in time.

To neglect either of these distinctions is to invite a serious error in the development of one’s understanding of relativistic phenomena. Yet it’s an oversight built right in to the Minkowski diagrams, as I will attempt to demonstrate.

Figure 4 is a composite of the various Minkowski diagrams already discussed, and will serve to illustrate the permeation of a pre-relativistic confusion inherent to all of them. Vector ** A** again represents the primary observer who is at rest in the coordinate system defined by the

*x*and

*t*axes, and who is located initially at events (0,0) and ultimately, after 5 sec, at (0,5). Vector

**represents a body in motion having the coordinate system defined by the**

*B**x’t’*axes;

**is located by**

*B***after 5 seconds at (3,5). Point**

*A**is an event located by*

**P****at (2,3) and by**

*A***, according to the Lorentz Transformations, at (0.25,2.25). Point**

*B***represents the measurements of an observer who locates**

*C***at the completion of the interval represented by the diagram at the coordinates (-4.9,7.0).**

*A**Figure 4*

Let’s examine the various features of Figure 4 in terms of Relativity. First, if ** A** is considered to be at rest and measuring its own time interval as

*t = 5 sec*, we know that its observation of the clock of any other body will be given by

*t’ = t (1-v*. If a body is in motion relative to

^{2})^{.5}**, this will yield a value for**

*A**t’*that is less than

*t*, reflecting the fact that a moving clock, i.e., relative motion in time, slows when there is relative motion in space. Yet the Minkowski Diagram depicts the world-lines of bodies in motion as attaining the same temporal ordinate as the rest frame — note, for instance, vector

**, and the light vectors, in Figure 4. This is not just an oversight, nor is it a misrepresentation of the intent. It’s an error upon which the spacetime diagram in its present form is founded. The notion of the light-cones, which may be taken as characterizing the format of the Minkowski Diagram, is what makes this conclusion unavoidable. The light vectors, representing the limit**

*B**c*, are projected according to relative motion in space, but according to the observer’s own time, treated as an independent, absolute measure. This is a remarkable misrepresentation, given that it’s axiomatic in relativity theory that light would not travel 5

*ls*in 5

*sec*relative to observer

**in the diagram — it would travel 5**

*A**ls*in 0

*sec*, and it should therefore be drawn directly along the

*x*-axis in an accurate projection. To portray light as traveling along the diagonals is not only to produce a distortion of the relative motion of light, but of any world-line in the diagram, because as limits, the placement of the light-vectors requires that all coordinates representing relative motion be delimited accordingly.

The location of event * P* in Figure 4 displays a similar sort of misrepresentation, as the clocks of the observers are superimposed on the event, treated as an instantaneous object of observation. The coordinates of

*in the diagram, whether according to*

**P****or**

*A***, express a spatial relationship between event and observers, appropriately enough, but not so the given temporal ordinates, which represent the distance in time of each observer from her own earlier reference points (where**

*B**t*and

*t’*= 0 according to

**). Relativity theory holds that it’s meaningless to project an observer’s clock at the location of a distant event — there is no time of an isolated event, no duration to express in comparison to the motion in time of various observers; there are, according to Relativity, only times as registered by the observers as an event is detected.**

*A*It is important to keep in mind that a spacetime diagram is a representation of process — it projects the world of an observer as it develops relative to an observer who moves in time — and because a diagram is unavoidably static, the time-vector of the observer can easily be mistaken as somehow leaving space behind, on the *x*-axis. But at any moment represented in the diagram the observer’s time-vector is still actually *in* space, *on* the space-axis, and an isolated event — no matter when it occurs — takes place somewhere *in* the observer’s projection of space. So to portray an event in a spacetime diagram, it’s best understood as taking place on a world-line, at a time corresponding to a clock traveling along the world-line. If it’s an isolated event it could be placed on the space axis, where it is taken as occurring when *t = 0* in the primary observer’s frame of reference, when the time of the event can be considered *null*.^{3}

Before leaving Figure 4, there is one additional consideration, the significance of point ** C**. The anomaly in this case is that while we know that a rest frame represented by the

*x,t*axes will undergo more motion in time than it will observe in any other (in other words, the clock of any other reference frame will appear to be moving more slowly), the coordinates of

**place it at**

*C**t = 7*relative to

*t = 5*for the rest frame of

**. This is because the coordinates at**

*A***(-4.9,7) express the measure of some observer’s own proper time and observed spatial distance attained between**

*C***and**

*O***corresponding to the given measure of**

*A***at 0**

*A**ls*and 5

*sec*. The observations of one reference system have thus been superimposed upon another, without any actual congruence between the observation and the

*x,t*axes. The coordinates of point

**and the form of diagram in which they appear (Figure 3) actually depict relative measurement, not relative motion; the**

*C**x,t*axes are used both as a reference system for the primary observer and as a matrix for the superimposition of other observations. There may be nothing inherently wrong with superimposing reference frames in this manner, except as with the location of events according to an absolute standard of time, it is done in the Minkowski Diagrams in a way that misrepresents the relativistic reality in a pre-relativistic, two-dimensional projection.

**4. An Alternative Diagram**

The relativity of spacetime imposes the requirement that in any portrayal of the motion between frames of reference we take the perspective of one at a time, and maintain it consistently as we determine the progress of the other(s). Figure 5 is a construction of such a procedure. Vector ** A** represents the motion of an observer whose frame of reference is described by the coordinate axes

*x,t*. A travels 5

*sec*in time in the scope of the diagram while being considered at rest in space. Body

**, which as a matter of convenience is located initially at**

*B***, moves away from the vicinity of**

*O***at a rate, according to**

*A***, which takes it 4**

*A**ls*in 5

*sec*. The coordinates of

**(4,3) can again be derived from the Lorentz transformations, or geometrically by means of the gradations in the diagram. By locating**

*B***at 3 seconds in time, it is indicated that the clock of**

*B***has moved 3**

*B**sec*in the reference frame of

**.**

*A**Figure 5*

Note that the world-line of ** B** in this alternative diagram is especially interesting in its contrast with the world-lines of the Minkowski Diagrams: At a velocity of .8

*c*relative to

**, the vector of**

*A***has already transgressed the 45**

*B*^{o}angle of the “light-cones”; in fact, as can be verified easily enough, a 45

^{o}angle to the coordinate axes in Figure 5 would represent a velocity of only .71

*c*. A consideration of higher relative velocities can provide an appreciation that the vectors representing their motion will approach the

*x*-axis as the limit

*c*, and that a vector representing the motion of light will travel directly along the axis.

**5. A Reevaluation of the Minkowskian Concepts**

The two fundamental contributions of the Minkowski diagrams to our idea of spacetime can now be reevaluated in view of the foregoing discussion. The concept of the parabolic or “Lorentz” geometry of spacetime is a residue of the pre-relativistic nature of the diagram: Given the absolute treatment of the temporal perspective in the Minkowski Diagram, all vectors except the world-line of the primary observer are distorted by a parabolic function simply because their motion in time is confounded with that of that observer. The same sort of function results from the attempt to correlate an instantaneous point with other events located at coordinates given by relative spatial distance but the observer’s absolute temporal orientation; this has been supposed to be a relationship of independent points, but is actually just the relationship of a frame of reference to its own absolutized temporal perspective. It is the misrepresentation of Relativity, not Relativity itself, that is responsible (in terms of non-accelerating frames of reference) for the concept of a non-Euclidean geometry of spacetime.

Secondly, the “light-cones” have been made to disappear by a rigorous relativistic representation of relative motion. In their place, in two-dimensional terms, is a circular boundary as shown in Figure 6, formed by the projection of possible world-lines emanating from and impinging on ** O**. The boundary of the circle isn’t the horizon of an exotic “elsewhere,” but simply the limit imposed by the temporal scope chosen for the particular diagram.

*Figure 6*

**6. Exploration of the Alternative**

The most outstanding feature of the alternative diagram is the Euclidean triangle formed by the relationship between an observer and a body in motion, as shown in Figure 7. Vector A describes the time it takes according to observer A for body B to reach its x-ordinate at the termination of the diagram; these measures are given in Figure 7 as t sec and x ls, respectively. The temporal ordinate t’ of vector B is, once again, given by the Lorentz transformation, or by the equation for the invariant interval. Vector A thus relates to x and t’ as a hypotenuse to a Euclidean triangle; and since vector B constitutes the actual hypotenuse of that triangle, it follows that regardless of the relative velocity between the two bodies, their world-lines will be the same length. This suggests that uniform motion in spacetime may be relative, but uniform motion itself is absolutely equivalent across reference frames.

*Figure 7*

Another interesting feature of the relationship between bodies according to the alternative concerns the “invariant interval.” In the Minkowski Diagrams, and in Relativity theory in general, the Interval is conceived as no more than the “separation,” an apparently fortuitous constant without physical significance, generally termed as the square root of the difference between the spatial distance between events according to the observer (squared) and the time according to the observer (squared) — i.e., *s = (x ^{2}-t^{2})^{.5}*. This formula has seemed to require the introduction of the imaginary number

*i*, the square root of a negative. In terms of the alternative, it’s just a misrepresentation of the actual relationship given by

*t = (x*, or

^{2}+t’^{2})^{.5}*t’ = (t*. In these latter expressions, and in the graphic representation, the interval is comprehensible as an actual physical measure, the proper time of the body being observed.

^{2}-x^{2})^{.5}It is arguable that the two-dimensional depiction of the relationship between observer and a body in motion in the alternative diagram expresses the actual relativistic relationship, at least in terms of the gravity-free spacetime motion between bodies according to one frame of reference. If we are to consider the alternative to have heuristic value it is reasonable to expect that it can somehow render the reversal of frames geometrically comprehensible, and Figure 8 demonstrates the manner by which such a transformation can be effected, expanding on the relationship depicted in Figure 5.

*Figure 8*

First, based on the principle that vector ** B**, while skewed relative to

**, is at rest in its own frame with**

*A***considered to be in motion, the**

*A**x’*-axis is drawn perpendicular to

**in order to represent its spacetime orientation relative to**

*B***. Now since it is desired to view**

*A***as it appears to**

*A***concurrent with**

*B***observing**

*A***at the coordinates (4,3), the temporal ordinate of**

*B***must be determined relative to the proper time of**

*B***, which is 5**

*A**sec*.

^{4}To find this mathematically it is reasoned that if

**measures the temporal motion of**

*B***as 5**

*A**sec*, and if by the reversal of frames

**is now taken to be traveling at .8**

*A**c*, then by the Lorentz transformations (

*t’ = t / (1-v*), the clock of

^{2})^{.5}**in its own frame is 8.33**

*B**sec*; the ultimate distance between

**and**

*A***according to**

*B***is given by**

*B**x’ = x / (1-v*, which yields 6.67

^{2})^{.5}*ls*.

To achieve the same result geometrically, it can be derived by extending the vector of ** B** in Figure 8 to the point

**where it would intersect a line drawn from**

*B’***parallel with the**

*A**x*-axis, as this forms a Euclidean triangle in which vector

**and the distance along**

*A**x*between

**and**

*A***relate to**

*B’***as a hypotenuse. And since the angle**

*B’***(read “?” as the Greek letter Theta as represented in Figure 9) between vectors is the same in either spacetime orientation,**

*?***relates to**

*B’***as the measure of proper time as**

*A***had related to the proper time of**

*A***. This is proven by the following:**

*B* ** B’** =

*A***csc**

*?*= 5 * 5/3

= 8.33

while

*x’*is given by

*x’*=

*A***cot**

*?*= 5 * 4/3

= 6.67

This result from the perspective of ** B** is given in Figure 9. Vector

**is extended to**

*A***at a length that will equal that of**

*A”***in accordance with the earlier postulate of the equivalence of world-lines; at this point the spatial distance of body**

*B’***from the origin according to**

*A***is exactly what we would expect mathematically, as is its proper time.**

*B**Figure 9*

Two bodies having different frames of reference are thus simultaneously represented both as they appear to themselves and to each other, and a diagrammatic symmetry corresponding to that of the four-dimensional relationship is achieved. This result should not be surprising, because once the misconception that the relationship between two bodies in uniform motion is non-Euclidean has been corrected, it is to be expected that the spacetime structure (abstracting from gravitation) can be accurately represented in a two-dimensional Euclidean projection. The Lorentz Transformations presume, after all, a simple perpendicular relationship between space and time; and although the relationship between particular temporalities given by *t’ = (t ^{2}-x^{2})^{.5}* is indeed parabolic, the fact that a hypotenuse relates to its sides by a parabolic function presupposes the right-angle of a Euclidean triangle. The parabolic relationship between different reference frames should therefore be understood as derivative and incidental to the essential Euclidean relationship between world-lines.

Several significant corollaries can be derived from the consideration of the two-dimensional depiction of spacetime. The representation of motion in spacetime as a relative variation from the perpendicular structure suggests that the distortion of time between frames is just the product of the perspective from which one views a motion which is — no matter what its spatial or temporal components — entirely homologous: Motion in space can be regarded as motion in time slightly skewed, while motion in time, although it seems to be something quite distinct, is simply the same sort of motion but in a perpendicular “direction.” This idea, if not new, is nonetheless translated into a coherent picture in the alternative, with a potential for the greater clarification of our concept of time.

Another significant entailment of the alternative illuminates the otherwise perplexing contradiction wherein two bodies can each be at rest and yet also in relative motion. In the coordinate system of ** A** in Figure 9 the vectors

**and**

*A***each have an equal extension in time, while in the coordinate system of**

*B’***, vectors**

*B***and**

*B***have an equal temporal extension. Thus from either frame of reference there is a suggestion of an underlying simultaneity between the temporal position of a body at rest and that of a body in motion when the one in motion is observing the one at rest; the instant of observation according to one frame takes place at another instant according to the second, but that latter instant coincides with precisely the same distance in time according to the first. Despite their differing individual orientations in spacetime — despite the relativity of motion — each body in uniform motion is moving orthographically in spacetime, and at a rate identical to all others in uniform motion. The paradox can be attributed to a dichotomy between finite references and a non-finite spacetime structure. But the exploration of this and other entailments of relative motion according to the alternative can best be undertaken in another context.**

*A”***7. On the Nature of Light**

A further consideration worth making here is of the nature of light as it is suggested by the alternative diagram. We know that the proper time of light is zero when measured from any other reference frame. This peculiarity is given by the mathematics of Special Relativity, although it’s not made strikingly evident by that more abstract form of representation, and although the Minkowski Diagram has tended to obfuscate the fact. In the geometric translation of the alternative diagram this zeroing of temporal motion is quite graphically revealed as suggesting that light literally does not move in time – and not just relatively so, because all coordinate systems agree on the motionless clock.

It may be arguable that is makes just as much sense to say that from the frame of reference of a photon, only light moves in time, but that issue is secondary here – either way, there is an explanation available for what has otherwise been accepted as inexplicable.

There are two characteristics of light that are distinctive and comprehensible in terms of the diagram if light doesn’t move in time, at least from the frame of reference of non-luminous bodies: As is well-known, the velocity of light is both invariant and ultimate. If uniform temporal motion is, by the equivalence of world-lines (as demonstrated in the alternative diagram), taken to be identical in magnitude to motion along the space-axis, it follows that each un-accelerated observer will measure light in its three-dimensional motion as traveling the same distance in space as time elapses in that observer’s reference frame. While the measure of the distance traveled by a beam of light will vary between frames, the rate will always be agreed upon.

The ultimate, or limiting characteristic of the velocity of light is explained with the recognition of the space-axis as the limit of relative motion. If the world-lines of all bodies are, again, taken as having the same extension, but as having varying spatial and temporal components to their relative trajectories, the limiting spatial velocity will be the magnitude of a world-line along the space axis measured in terms of the same magnitude along the time axis. Hence one second in time is the same distance (but in a perpendicular direction) as 300,000 km.

**8. Conclusion**

The Minkowski Diagrams have been shown to be based on a non-relativistic perspective, a view of developments taken from an absolute projection of the observer’s clock. The result has been a confusion of frames of reference and a parabolic distortion of relativistic relationships which, in the limited realm of Special Relativity, actually remain Euclidean. The use of the Minkowski Diagram has led to significant misconceptions, as with theories involving the light-cones and the geometry of spacetime in the absence of gravitational influences, and to obfuscations, as of the distinctive nature of light.

An alternative diagram has been offered, one that maintains a relativistic frame of reference, and is able as a result to consistently represent other bodies in their relationships to that frame. It has been shown that the alternative diagram is capable, at least in those respects considered, of maintaining an independent conformity with the predicted relationships of relativity, and that it provides a means of comprehending some of the otherwise inexplicable properties of light.

**Notes**

1. As a matter of convenience *t* is generally multiplied by *c* so that space and time can be expressed in distances of the same scale. I prefer instead to calibrate them by giving time in seconds (*sec*) and space in light-seconds (*ls*).

2. The Lorentz Transformations are *t’ = (t-v)/(1-v ^{2})^{.5}* and

*x’ = (x-vt)/(1-v*, with

^{2})^{.5}*v*as velocity proportional to

*c*.

3. If it is considered important to represent the occurrence of an isolated event after the diagram “begins,” or if it’s desired to portray a series of isolated events on the diagram, some of them occurring when the time of the observer is not at

*t = 0*, each event could be placed on a cut-away space-axis above or below the

*x*-axis, labeled

*t = 2*for example, but at a point given by coordinates like (null,3). A broken line, a diagonal, might be used to show the connection between the occurrence of the event at

*t = 2*and the observation of the event (at, say,

*t = 5*), without suggesting that the connection is in any way related to a world-line.

4. We could, of course, just as well reverse the frames according to the given proper time of

**, and observe**

*B***as it appears to**

*A***when**

*B***is at 3**

*B**sec*.

**References**

Minkowski, H., “Space and Time”, 1908, in *The Principle of Relativity*, H.A. Lorentz, A. Einstein, H. Minkowski, and H. Weyl, trans: W. Perrett and G.B. Jeffery, 1923.

ivaedocvunf@gmail.com

ivaedocvunf@gmail.com

ivaedocvunf@gmail.com

I have identified an alternate form of Loedel diagram that I think is worth considering. In this alternate form, the x and x’ labels on the axes of the standard Loedel diagram are switched, as the the labels on the ct and (ct’) axes. One then determines the coordinates of a point in space-time by dropping normals to the axes, rather than drawing lines parallel to the axes. The transformation between x’-ct and x-ct’ is orthogonal, involving a pure rotation through the angle alpha, where sin(alpha) = v/c. Check it out, and see what you think. Is it easier to use?

Chet Miller

Wilmington DE USA

DI Herculis Eclipsing Binary Stars Solution: The problem that Einstein’s 100,000 PHD space-time Physicists could not solve

This is the solution to DI Her “Quarter of a century” Smithsonian-NASA Posted motion puzzle that Einstein and the 100,000 space-time physicists including 109 years of Nobel prize winner physics and physicists and 400 years of astronomy and Astrophysicists could not solve and solved here and dedicated to Drs Edward Guinan and Frank Maloney

Of Villanova University Pennsylvania who posted this motion puzzle and started the search collections of stars with motion that can not be explained by any published physics

For 350 years Physicists Astrophysicists and Mathematicians and all others including Newton and Kepler themselves missed the time-dependent Newton’s equation and time dependent Kepler’s equation that accounts for Quantum – relativistic effects and it explains these effects as visual effects. Here it is

Universal- Mechanics

All there is in the Universe is objects of mass m moving in space (x, y, z) at a location

r = r (x, y, z). The state of any object in the Universe can be expressed as the product

S = m r; State = mass x location

P = d S/d t = m (d r/dt) + (dm/dt) r = Total moment

= change of location + change of mass

= m v + m’ r; v = velocity = d r/d t; m’ = mass change rate

F = d P/d t = dÂ²S/dtÂ² = Force = m (dÂ²r/dtÂ²) +2(dm/d t) (d r/d t) + (dÂ²m/dtÂ²) r

= m ? + 2m’v +m”r; ? = acceleration; m” = mass acceleration rate

In polar coordinates system

r = r r(1) ;v = r’ r(1) + r ?’ ?(1) ; ? = (r” – r?’Â²)r(1) + (2r’?’ + r?”)?(1)

F = m[(r”-r?’Â²)r(1) + (2r’?’ + r?”)?(1)] + 2m'[r’r(1) + r?’?(1)] + (m”r) r(1)

F = [dÂ²(m r)/dtÂ² – (m r)?’Â²]r(1) + (1/mr)[d(mÂ²rÂ²?’)/d t]?(1) = [-GmM/rÂ²]r(1)

dÂ² (m r)/dtÂ² – (m r) ?’Â² = -GmM/rÂ²; d (mÂ²rÂ²?’)/d t = 0

Let m =constant: M=constant

dÂ²r/dtÂ² – r ?’Â²=-GM/rÂ² —— I

d(rÂ²?’)/d t = 0 —————–II

rÂ²?’=h = constant ————– II

r = 1/u; r’ = -u’/uÂ² = – rÂ²u’ = – rÂ²?'(d u/d ?) = -h (d u/d ?)

d (rÂ²?’)/d t = 2rr’?’ + rÂ²?” = 0 r” = – h d/d t (du/d ?) = – h ?'(dÂ²u/d ?Â²) = – (hÂ²/rÂ²)(dÂ²u/d?Â²)

[- (hÂ²/rÂ²) (dÂ²u/d?Â²)] – r [(h/rÂ²)Â²] = -GM/rÂ²

2(r’/r) = – (?”/?’) = 2[? + ? ? (t)] – hÂ²uÂ² (dÂ²u/d?Â²) – hÂ²uÂ³ = -GMuÂ²

dÂ²u/d?Â² + u = GM/hÂ²

r(?, t) = r (?, 0) Exp [? + ? ? (t)] u(?,0) = GM/hÂ² + Acos?; r (?, 0) = 1/(GM/hÂ² + Acos?)

r ( ?, 0) = hÂ²/GM/[1 + (AhÂ²/Gm)cos?]

r(?,0) = a(1-?Â²)/(1+?cos?) ; hÂ²/GM = a(1-?Â²); ? = AhÂ²/GM

r(0,t)= Exp[?(r) + ? ? (r)]t; Exp = Exponential

r = r(? , t)=r(?,0)r(0,t)=[a(1-?Â²)/(1+?cos?)]{Exp[?(r) + Ã¬ ?(r)]t} Nahhas’ Solution

If ?(r) ? 0; then:

r (?, t) = [(1-?Â²)/(1+?cos?)]{Exp[? ?(r)t]

?'(r, t) = ?'[r(?,0), 0] Exp{-2?[?(r)t]}

h = 2? a b/T; b=a? (1-?Â²); a = mean distance value; ? = eccentricity

h = 2?aÂ²? (1-?Â²); r (0, 0) = a (1-?)

?’ (0,0) = h/rÂ²(0,0) = 2?[?(1-?Â²)]/T(1-?)Â²

?’ (0,t) = ?'(0,0)Exp(-2?wt)={2?[?(1-?Â²)]/T(1-?)Â²} Exp (-2iwt)

?'(0,t) = ?'(0,0) [cosine 2(wt) – ? sine 2(wt)] = ?'(0,0) [1- 2sineÂ² (wt) – ? sin 2(wt)]

?'(0,t) = ?'(0,t)(x) + ?'(0,t)(y); ?'(0,t)(x) = ?'(0,0)[ 1- 2sineÂ² (wt)]

?'(0,t)(x) â€“ ?'(0,0) = – 2?'(0,0)sineÂ²(wt) = – 2?'(0,0)(v/c)Â² v/c=sine wt; c=light speed

? ?’ = [?'(0, t) – ?'(0, 0)] = -4? {[? (1-?) Â²]/T (1-?) Â²} (v/c) Â²} radians/second

{(180/?=degrees) x (36526=century)

? ?’ = [-720×36526/ T (days)] {[? (1-?) Â²]/ (1-?) Â²}(v/c) = 1.04Â°/century

This is the T-Rex equation that is going to demolished Einstein’s space-jail of time

The circumference of an ellipse: 2?a (1 – ?Â²/4 + 3/16(?Â²)Â²—) ? 2?a (1-?Â²/4); R =a (1-?Â²/4)

v (m) = ? [GMÂ²/ (m + M) a (1-?Â²/4)] ? ? [GM/a (1-?Â²/4)]; m<<M; Solar system

v = v (center of mass); v is the sum of orbital/rotational velocities = v(cm) for DI Her

Let m = mass of primary; M = mass of secondary

v (m) = primary speed; v(M) = secondary speed = ?[GmÂ²/(m+M)a(1-?Â²/4)]

v (cm) = [m v(m) + M v(M)]/(m + M) All rights reserved. joenahhas1958@yahoo.com

I just realized – you’re right. I took the subtraction of velocities according to A.

Still, the extension of B to when and where he observes E expresses the invariance, the proper time of E from both frames, A and B.

Burt,

You wrote, regarding his modification and commentary on my diagram, â€œI’ve treated E simply as an event, an instant of time somewhere in space, not as the end of a world-line. By definition, events are not bodies with clocks and speed – they just happen somewhere and that’s that.â€¦ The 0.84 that I mentioned is not time; it is ds^2 = dt^2-dx^2, the square of the spacetime interval.â€

If youâ€™re treating

Esimply as an event, then nothing I wrote about a world-line related toEapplies. According toA, it happens at 1 second, 0.4lsdistant. There is no meaningful spacetime interval betweenOandEâ€“ as you said, an event doesnâ€™t travel in space, which means there are no relativistic effects for the observer. Similarly,Bwill record the event in time at a point parallel to the xâ€™ axis betweenEandBâ€™s world-line, and in space at a point parallel to the tâ€™ axis betweenEand the x-axis.Burt continues: â€œLet’s stick to two coordinate systems and two events (O and E) and then you show me how your diagram treats the invariance of the spacetime interval between O and E for observers A and B (obviously with spacetime interval defined as per standard relativity theory).â€

I did treat just two coordinate systems â€“ the reference frame of world-line

OEwasnâ€™t considered, I merely connected the events to give substance to your spacetime interval.If

OandEare unconnected events, there is no world-line, there is no meaningful spacetime interval between them, there is only the observerâ€™s measure of space and the observerâ€™s measure of time, all within his coordinate system. If an observer records a flash of light in the distance, it might be the explosion of an object that was stationary relative to the observer, or the object might have been traveling at .5c. As an isolated event it has no history.Iâ€™ve shown that the spacetime interval is not a mysterious constant, but actually a bodyâ€™s proper time when projected on the alternative diagram, and constant for that reason, and meaningful for that reason. If youâ€™re going to critique the alternative diagram, you canâ€™t do it in terms of the Minkowski diagram. If however we consider a world-line between

OandE, there is an invariance, and itâ€™s the proper time of the body moving along the world-line, as Iâ€™ll show below.Burt rejects my claim that the alternative diagram works exactly as it should, with

BobservingEâ€™s interval, or proper time, as 0.92 seconds at a distance of about 0.68 ls: â€œWrong result and exactly the problem with your diagram! In a correct relativistic treatment, your B will observe event E to happen 1.2 seconds after event O and at a distance of ~0.775 ls ‘behind’ B (as per my Fig. 2, modified from your figure 8).â€If my math is wrong itâ€™s no reflection on the diagram, the projection is essentially the same. But Iâ€™ll take it step by step. Whether you posit a â€œspacetime intervalâ€ with relativistic effects or a world-line between

OandE, the observations ofEbyAandBwill be the same in terms of the proper time or the â€œspacetime intervalâ€ ofOEbetween events. In your example, considerOEto be a world-line, the spatial distance betweenOandEaccording toAis 0.4 ls after 1 second according toAâ€™s clock,Bmoves 0.8 ls in the same time according toA:Eâ€™s velocity relative toBis given by the relativistic subtraction of velocities (with velocities expressed proportional toc):v = (v1-v2) / (1 – (v1)(v2))

= (.8-.4)/(1-.8*.4)

= .4/.68

= .59

lsWith a relative velocity of .59

ls, the proper time ofErelative toBat 1 second according toBis given by:tâ€™ = (1-.592).5

= (1-.3481).5

= .6519.5

= .807 seconds

Multiply 1 second by .92/.807 to get

Bâ€™s time when observingEâ€™s proper time at .92 seconds, which yields 1.14 seconds, and multiply .59lsby .92/.807 to get .67ls, the distanceEtravels in 1.14 seconds according toB.The point of all this is that the alternative diagram accurately represents both frames of reference,

AandB, and it does so in a perfectly Euclidean manner. The Minkowski diagram distorts the relationship by first projecting all the world-lines according to the time of the primary observer, then compensating by translating the relationships between axes. If a graphic representation doesnâ€™t illustrate relationships accurately, itâ€™s no improvement on the serial listing of numeric expressions, and itâ€™s problematic in that it leads to invalid or meaningless concepts, as in the light-cones and the invariant interval.Hi Jim.

I’ll respond only to your last one, because on the M-diagram I’ve decided I’ll agree to differ from you and leave it there…

In your second reply you wrote: “In your modification and commentary on my diagram youâ€™ve treated E as both an isolated event 0.4 ls distant from A and as the terminus of a world-line emanating from O.

1. No, I’ve treated E simply as an event, an instant of time somewhere in space, not as the end of a world-line. By definition, events are not bodies with clocks and speed – they just happen somewhere and that’s that. So “the clock of body E would record 0.92 seconds ( tâ€™ = (12-.42).5)” as you wrote is incorrect. It is your observer B (which is not present at event E), that observes 0.92 seconds for the time interval between events O and E (according to your diagram, that is). The 0.84 that I mentioned is not time; it is ds^2 = dt^2-dx^2, the square of the spacetime interval.

You wrote: “As for the coordinate rotation, where you treat E as a world-line, or spacetime interval, the diagram is allegedly â€œflawedâ€ because A doesnâ€™t directly observe Bâ€™s observation of E.”

2. As said in 1, I’m not treating E as a world-line. It is a point on a coordinate system which can be transformed to a point on a rotated coordinate system by simple trig.

3. Your last paragraph is confusing because you treat event E as belonging to a third coordinate system. Let’s stick to two coordinate systems and two events (O and E) and then you show me how your diagram treats the invariance of the spacetime interval between O and E for observers A and B (obviously with spacetime interval defined as per standard relativity theory).

Finally, you wrote: “… the diagram works exactly as it should, with B observing Eâ€™s interval, or proper time, as 0.92 seconds at a distance of about 0.68 ls.”

4. Wrong result and exactly the problem with your diagram! In a correct relativistic treatment, your B will observe event E to happen 1.2 seconds after event O and at a distance of ~0.775 ls ‘behind’ B (as per my Fig. 2, modified from your figure 8).

Regards, Burt

Burt,

In your modification and commentary on my diagram youâ€™ve treated

Eas both an isolated event 0.4lsdistant fromAand as the terminus of a world-line emanating fromO. As an event occurring 0.4lsfromA, the time of the event according toAâ€™s clock is 1 second, whichAwill observe at 1.4 seconds as having occurred 0.4 seconds earlier. As a world-line representing a body moving 0.4lsrelative toA, whenAâ€™s clock has recorded 1 second, the clock of bodyEwould record 0.92 seconds (tâ€™ = (12-.42).5). (Not, incidentally, 0.84 seconds â€“ you neglected to take the square root.)As for the coordinate rotation, where you treat

Eas a world-line, or spacetime interval, the diagram is allegedly â€œflawedâ€ becauseAdoesnâ€™t directly observeBâ€™s observation ofE.The velocity of

Erelative toAis less than the velocity ofErelative toB(.59c), so the difference between the clock ofBand the clock ofEwill be greater than between the clocks ofAandE. Consequently,Bwill observe the event at the terminus ofEâ€™s interval at a later time thanAdoes. If you extendBâ€™s world-line to the time whenBwill observeE(about 1.14 seconds), the diagram works exactly as it should, withBobservingEâ€™s interval, or proper time, as 0.92 seconds at a distance of about 0.67ls.Burt, Iâ€™ll respond to your two comments in separate comments.

First, your subject-line seems to suggest that you think I’ve asserted that the M-diagram is Euclidean. I hope you realize that my point is that it’s a flaw in the diagram that it isn’t Euclidean.

Responding to your points:

1. Burt wrote that the illustration of the relationship between world-lines as they move in spacetime â€œwas a secondary purpose: the main purpose was to show how the speed of light and the spacetime interval ds^2 = |dx^2 – dt^2| remain constant under change of inertial frame of reference. That’s what special relativity is about.â€

Burt, youâ€™re saying that the â€œmain purposeâ€ of special relativity is about two constants? Itâ€™s primarily aboutâ€¦ non-relativity? That would be odd. I have to think Iâ€™m a little closer to the primary purpose when I say itâ€™s about explaining and (for Minkowski in particular) illustrating the relativity of the relationship between world-lines in spacetime (light being exceptional), inspired by the need to explain the constancy of

c.Iâ€™ve shown in the alternative diagram that the â€œspacetime intervalâ€ is the measure of a bodyâ€™s proper time between two events. It is a constant, agreed upon by any inertial frame of reference, but when derived from the Minkowski diagram it has no physical significance – it just

is. And proper time is most clearly expressed in the perfectly Euclidean relationship exampled with a body moving 4 ls according to an observer in 5 seconds of an observerâ€™s time. The â€œspacetime intervalâ€ = the moving bodyâ€™s proper time = 3 seconds, i.e.,tâ€™ = (t2-x2).5. The illustration of this is is one of my primary purposes with the alternative diagram.2. Burt wrote â€œThere are always two inertial frames involved on a Minkowski spacetime diagram â€“ one can call one the reference frame and the other the moving frame, but there are two frames, as per my 1 above.â€

Yes, but I said â€œ

based onone frame of reference.â€ The orthogonal frame xt represents the observer who measures other bodies in relative motion. And itâ€™s the coordinate system of xt that is translated into not necessarily two, but actually any number of other frames.3. Burt wrote â€œThe Minkowski diagram actually portrays both frames’ perspective, more specifically, it gives those â€˜physical laws [that] might find their most perfect expressionâ€™, i.e., the invariance of the speed of light and the spacetime interval in both frames.â€

Iâ€™ll take this up in response to your #6. For the moment Iâ€™ll just refer you back to my point in response to #1.

4. Burt wrote that the Minkowski diagram â€œshows the (two)-dimensional relationship between bodies moving in spacetime pretty accurately if you read the diagram as designed. It is possible that you have a â€˜distorted viewâ€™ of that relationship, maybe because you are sticking to Euclid’s geometry. I have sympathy with this, because I started out more or less the same as you – a very similar diagram of my own that eventually proved to be fatally flawedâ€¦â€

Well, of course, reducing someoneâ€™s difference of opinion to a less-evolved station on the path to wisdom is usually better left unsaid.

If I were to be pedantic I would be satisfied to point out that there is no â€œ(two)-dimensional relationship between bodies in spacetimeâ€, itâ€™s four-dimensional, but that level of nit-picking isnâ€™t productive except as an argument against further mutual nit-picking. More to the point, Iâ€™ve shown in #1 above that the relationship given by

tâ€™ = (t2-x2).5is perfectly Euclidean.5. In response to my point that nothing actually happens on the world-line of the observer in the â€˜staticâ€™ frame (call it A) at 1.833 seconds, Burt agreed (rather triumphantly, it seems): â€œthanks! Yea, I agree: nothing actually happens on the world line of the observer in the â€˜staticâ€™ frame (call it A) at 1.833 seconds. Except that A can perhaps (somehow) read the clock of B at that moment, but that’s not the issue here.â€

Iâ€™ll respond to this point and #6 together.

6. Burt wrote: â€œIn this vaguely stated scenario: B is moving at 0.4c relative to A, one cannot really talk about ‘proper time’, because B can just as well be taken as stationary and then A’s ‘proper time’ must be less than B’s.â€

Iâ€™m sorry, this seems to be making a virtue of conundrum. One cannot really talk about proper time? Of course, if B is considered stationary, then one could talk about Aâ€™s proper time relative to B. But thatâ€™s not the scenario, it is precisely stated that itâ€™s B that is considered to be in motion.

Burt continued: â€œProper time is only relevant when you consider specific events in spacetime, but more about that later. The M-diagram actually does a remarkable job in that it shows that A and B are perfectly equivalent. It’s just that if you choose to plot A on orthogonal axes, then B’s axes must be skewed and visa versa.â€

Thatâ€™s exactly what weâ€™re considering here â€“ two events one at

, the other at two seconds. The â€œperfect equivalenceâ€ where each would observe the same dilation in the otherâ€™s time obscures the fact that once Aâ€™s event (the observation of B) is fixed at 2 seconds, Bâ€™s corresponding observation of A takes place beyond 2 seconds on Bâ€™s clock, at 2.18 seconds. Unless thatâ€™s done you havenâ€™t shown the mutual relationship, youâ€™ve shown independent observations.O7. Burt wrote that I â€œseem to have some problem with the term â€˜projection of a relationship between world-lines.â€™ Your statement makes little sense, so I’m afraid I’ll skip this one, except for what I said in 6.â€

A spacetime diagram is a two-dimensional projection of events occurring in four dimensions. I have no problem with that; I canâ€™t imagine what anyone elseâ€™s problem would be.

8. Burt quoted me: “â€¦the world-line of B isnâ€™t further along in the temporal component of spacetime according to Aâ€™s coordinate system when A is at 2 seconds – B is at 1.833 seconds in Aâ€™s coordinate system when A is at 2 seconds.”

Then Burt wrote: â€œI think this is where your biggest misconception lurks. In my M-diagram the x,t and x’,ct’ axes (call it A and B if you like) are not Euclidean related. Euclidean spacetime would have demanded that dx^2 + dt^2 = constant under a change of inertial coordinates. The relativistic M-diagram demands that |dx^2 – dt^2| = constant under a change of inertial coordinates. This makes a big difference, since this is what relativity is all about. I can show that your ‘alternative diagram’ actually violates this principle, but it will have to wait until this “M-gap” is closed to some extent, otherwise it may prove pointlessâ€¦â€

I agree that in Minkowski the axes are not Euclidean. But thatâ€™s the point of my criticism. Iâ€™ll move on to your second comment a little laterâ€¦.

Burt,

Thank you for your comments. I’ll have no time to respond to them until Monday.

Jim

Hi Jim.

Since it does not look like we’ll get anywhere with the Minkowski diagram soon, and since I agree that the Minkowski is not very user-friendly, maybe it’s time to take a look at your diagram and a possible way forward. I took the liberty of annotating Figure 8 of your OP somewhat.

Since special relativity is all about spacetime intervals, let’s consider two events, O at the origin and E at x=0.4, t=1.0 in A’s frame. Now find the coordinates of event E in B’s frame (by simple coordinate rotation): x=-0.56, t=0.92 (rounded to two decimals). To test the relativistic validity of E’s coordinates in B’s frame, we calculate the spacetime interval between O and E in A’s frame as: ds^2 = |dt^2-dx^2| = 1 – .4^2 = 0.84. In B’s frame it works out to be: ds’^2 = 0.92^2 â€“ (-0.56)^2 = 0.53. This is the main flaw in your diagram: a special relativity spacetime diagram must render the spacetime interval invariant under a change of inertial coordinate system. Your diagram clearly does not.

All is not lost, however. There is a ‘magic trick’ that can render your diagram fully relativistic. Simply re-label the two x-axes by swapping their labels, as I’ve shown below in Figure 2. Because of the skew axes, the event is plotted slightly differently, as shown – in blue for A and in red for B. You can easily verify that the spacetime interval between O and E is now the same for A and B. Hence, you now have a fully relativistic spacetime diagram. Loedel first described it in the 1940s and I think it is a great improvement of the 1920s Minkowski diagram in terms of user-friendliness. Sadly, it has not caught on very muchâ€¦

The modern way of drawing the Loedel diagram is like in Figure 3 below, generalized so that it shows the standard orientation of the light cone. (The original is here: http://www.engineersperspective.com/images/LoedelSpacetimeDiagram1.jpg)

The light cone serves as an “anchor” for the diagram and the two time axes are separated by an angle that depends on their relative speed. When the relative velocity is zero, both time axes will be vertical and when the relative velocity approaches the speed of light, the angle will approach 90 degrees and the time axes will tend towards the light cone.

The scale of all axes is the same and hence it’s very user-friendly. Another benefit of drawing it like this is that only the light cone takes on a ‘privileged’ orientation; the two inertial frames are treated equally and democratically, as it should be. Lastly, Jim, it should please you to know that one can now ‘legitimately’ view progress along the two time axes as spacetime movement. Note that this is not the purpose of the diagram, however: it serves to keep the spacetime intervals between multiple events invariant under a coordinate transformation.

It sounds too good to be true, so where is the catch? As far as I know, the only drawback of the Loedel diagram is that one can only treat two inertial frames at any one time. When you add a third inertial frame, it screws up the symmetry and with it the scale of the third frame so that it is no longer compatible with the rest, i.e., its scale gets ‘funny’, just like the Minkowski diagram’s second inertial frame. This may perhaps explain why Minkowski still rules the relativistic world â€“ since it has one funny scale anyway, one can add as many reference frame with funny scales as you please!

I noticed that http://en.wikipedia.org/wiki/Minkowski_diagram does not make much distinction between the Minkowski and the Loedel diagram anymore. It looks like that article uses whichever suits the situation best and simply call it “Minkowski”, which is probably not strictly correct.

Regards, Burt