Physics:Formulations of special relativity

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The theory of special relativity was initially developed in 1905 by Albert Einstein. Moving beyond the traditional formulation, newer interpretations of special relativity have been developed on the basis of different foundational axioms. While some are mathematically equivalent to Einstein's theory, others aim to revise or extend it.

Einstein's formulation was based on two postulates, as detailed below. Some formulations modify these postulates or attempt to derive the second postulate by deduction. Others differ in their approach to the geometry of spacetime and the linear transformations between frames of reference.

Einstein's two postulates

Main page: Physics:Postulates of special relativity

As formulated by Albert Einstein in 1905, the theory of special relativity was based on two main postulates:

  1. The principle of relativity: The form of a physical law is the same in any inertial frame.
  2. The speed of light is constant: In all inertial frames, the speed of light c is the same whether the light is emitted from a source at rest or in motion. (Note this does not apply in non-inertial frames, indeed between accelerating frames the speed of light cannot be constant.[1] Although it can be applied in non-inertial frames if an observer is confined to making local measurements.[2])

Using these two postulates, Einstein developed the theory of special relativity. This theory made many predictions which have been experimentally verified, including the relativity of simultaneity, length contraction, time dilation, the relativistic velocity addition formula, the relativistic Doppler effect, relativistic mass, a universal speed limit, mass–energy equivalence, the speed of causality and the Thomas precession.[3][4]

Single-postulate approaches

Several physicists have derived a theory of special relativity from only the first postulate (the principle of relativity), ignoring the second postulate that the speed of light is constant.[1][5][6][7] The term "single-postulate" is misleading because these formulations may rely on unsaid assumptions such as the cosmological principle, that is, the isotropy and homogeneity of space.[8][9] However, the term does not refer to the exact number of postulates, but is rather used to distinguish such approaches from the "two-postulate" formulation. Single postulate approaches generally deduce, rather than assume, that the speed of light is constant.

Without first assuming the universal light-speed, the Lorentz transformations can be obtained up to a nonnegative free parameter. Experiments rule out the validity of the Galilean transformations, implying that the parameter in the Lorentz transformations is nonzero, implying that there is a finite maximum speed before anything about light is said. When this is combined with Maxwell's equations, it is demonstrated that light travels at this maximum speed. In these transformations, the numerical value of the parameter is decided by experiment, just as the numerical values of the parameter pair c and the permittivity of free space are determined by experiment even when Einstein's original postulates are used. When the numerical values in both Einstein's and these other ways are found, the two approaches result in the same theory. As a result, the end outcome of the interlocking triad of "theory + Maxwell's equations + experimental data" is the same. In this sense, rather than postulating, universal light speed can be deduced.

For some historical information, see History of special relativity § Spacetime physics and the section "Lorentz transformation without second postulate" for the approaches of Ignatowski and Frank/Rothe. According to Pauli (1921), Resnick (1967), and Miller (1981), those models were insufficient. However, the constancy of the speed of light is contained in Maxwell's equations. That section includes the phrase "Ignatowski was forced to recourse to electrodynamics to include the speed of light". So, the trio of "principle of relativity + Maxwell's equations + experimental data" gives special relativity, and this should be compared with "principle of relativity + second postulate + Maxwell's equations + experimental data". Since Einstein's 1905 paper is all about electrodynamics, he is assuming Maxwell's equations, and the theory is not practically applicable without numerical values. When compared with things alike, from the point of view of asking what is knowable, the second postulate can be deduced. If you restrict your attention to just the standalone theory of relativity, then yes you need the postulate. But given all the available knowledge we don't need to postulate it. In other words, different domains of knowledge is overlapping and thus taken together have more information than necessary.

This can be summarized as follows:

  1. Experimental results rule out the validity of the Galilean transformations.
  2. That just leaves the Lorentz transformations with a finite maximal speed V.
  3. Given a maximal speed V, the only consistent way of combining the principle of relativity with Maxwell's equations is to identify Maxwell's parameter: [math]\displaystyle{ c = \frac{1}{\sqrt{\mu_0 \varepsilon_0}} \ . }[/math] with the aforementioned maximal speed V.
  4. We are now at the same starting point as if we had postulated the constancy of light, so we proceed to develop all the usual results of special relativity.

There are references which discuss in more detail the principle of relativity.[10][11]

Test theories of special relativity

Main page: Physics:Test theories of special relativity

Test theories of special relativity are flat spacetime theories which are used to test the predictions of special relativity. They differ from the two-postulate special relativity by differentiating between the one-way speed of light and the two-way speed of light. This results in different notions of time simultaneity. There is Robertson's test theory (1949) which predicts different experimental results from Einstein's special relativity, and there is the Mansouri-Sexl theory (1977) which is equivalent to Robertson's theory. There is also Edward's theory (1963) which cannot be called a test theory because it is physically equivalent to special relativity, [12]

Lorentz ether theory

Main page: Physics:Lorentz ether theory

Hendrik Lorentz and Henri Poincaré developed their version of special relativity in a series of papers from about 1900 to 1905. They used Maxwell's equations and the principle of relativity to deduce a theory that is mathematically equivalent to the theory later developed by Einstein.

Minkowski spacetime

Main page: Physics:Minkowski space

Minkowski space (or Minkowski spacetime) is a mathematical setting in which special relativity is conveniently formulated. Minkowski space is named for the German mathematician Hermann Minkowski, who around 1907 realized that the theory of special relativity (previously developed by Poincaré and Einstein) could be elegantly described using a four-dimensional spacetime, which combines the dimension of time with the three dimensions of space.

Mathematically there are a number of ways in which the four-dimensions of Minkowski spacetime are commonly represented: as a four-vector with 4 real coordinates, as a four-vector with 3 real and one complex coordinate, or using tensors.

Spacetime algebra

Main page: Spacetime algebra

Spacetime algebra is a type of geometric algebra, closely related to Minkowski space, and is equivalent to other formalisms of special relativity. It uses mathematical objects such as bivectors to replace tensors in traditional formalisms of Minkowski spacetime, leading to much simpler equations than in matrix mechanics or vector calculus.

de Sitter relativity

According to the works of Cacciatori, Gorini and Kamenshchik, [7] and Bacry and Lévi-Leblond[13] and the references therein, if you take Minkowski's ideas to their logical conclusion then not only are boosts non-commutative but translations are also non-commutative. This means that the symmetry group of space time is a de Sitter group rather than the Poincaré group. This results in spacetime being slightly curved even in the absence of matter or energy. This residual curvature is caused by a cosmological constant to be determined by observation. Due to the small magnitude of the constant, then special relativity with the Poincaré group is more than accurate enough for all practical purposes, although near the Big Bang and inflation de Sitter relativity may be more useful due to the cosmological constant being larger back then. Note this is not the same thing as solving Einstein's field equations for general relativity to get a de Sitter Universe, rather the de Sitter relativity is about getting a de Sitter Group for special relativity which neglects gravity.

Euclidean relativity

Euclidean relativity[14][15][16] [17] [18][19][20] uses a Euclidean (++++) metric in four-dimensional Euclidean space as opposed to the traditional Minkowski (+---) or (-+++) metric in four-dimensional space-time.[lower-alpha 1] The Euclidean metric is derived from the Minkowski metric by rewriting [math]\displaystyle{ (cd\tau)^2=(cdt)^2-dx^2-dy^2-dz^2 }[/math] into the equivalent [math]\displaystyle{ (cdt)^2=dx^2+dy^2+dz^2+(cd\tau)^2 }[/math]. The roles of time t and proper time [math]\displaystyle{ \tau }[/math] have switched so that proper time [math]\displaystyle{ \tau }[/math] takes the role of the coordinate for the 4th spatial dimension. A universal velocity [math]\displaystyle{ c }[/math] for all objects moving through four-dimensional space appears from the regular time derivative [math]\displaystyle{ c^2=(dx/dt)^2+(dy/dt)^2+(dz/dt)^2+(cd\tau /dt)^2 }[/math]. The approach differs from the so-called Wick rotation or complex Euclidean relativity. In Wick rotation, time [math]\displaystyle{ t }[/math] is replaced by [math]\displaystyle{ it }[/math], which also leads to a positive definite metric, but it maintains proper time [math]\displaystyle{ \tau }[/math] as the Lorentz invariant value whereas in Euclidean relativity [math]\displaystyle{ \tau }[/math] becomes a coordinate. Because [math]\displaystyle{ c^2=(dx/dt)^2+(dy/dt)^2+(dz/dt)^2+(cd\tau /dt)^2 }[/math] implies that photons travel at the speed of light in the subspace {x, y, z} and baryonic matter that is at rest in {x, y, z} travels normal to photons along [math]\displaystyle{ {\tau} }[/math], a paradox arises on how photons can be propagated in a space-time. The possible existence of parallel space-times or parallel worlds shifted and co-moving along [math]\displaystyle{ \tau }[/math] is the approach of Giorgio Fontana.[21] Euclidean geometry is consistent with Minkowski's classical theory of relativity. When the geometric projection of 4D properties to 3D space is made, the hyperbolic Minkowski geometry transforms into a rotation in 4D circular geometry.

Very special relativity

Main page: Physics:Very special relativity

Ignoring gravity, experimental bounds seem to suggest that special relativity with its Lorentz symmetry and Poincaré symmetry describes spacetime. Surprisingly, Cohen and Glashow[22] have demonstrated that a small subgroup of the Lorentz group is sufficient to explain all the current bounds.

The minimal subgroup in question can be described as follows: The stabilizer of a null vector is the special Euclidean group SE(2), which contains T(2) as the subgroup of parabolic transformations. This T(2), when extended to include either parity or time reversal (i.e. subgroups of the orthochronous and time-reversal respectively), is sufficient to give us all the standard predictions. Their new symmetry is called Very Special Relativity (VSR).

Doubly special relativity

Main page: Physics:Doubly special relativity

Doubly special relativity (DSR) is a modified theory of special relativity in which there is not only an observer-independent maximum velocity (the speed of light), but an observer-independent minimum length (the Planck length).

The motivation to these proposals is mainly theoretical, based on the following observation: the Planck length is expected to play a fundamental role in a theory of quantum gravity, setting the scale at which quantum gravity effects cannot be neglected and new phenomena are observed. If special relativity is to hold up exactly to this scale, different observers would observe quantum gravity effects at different scales, due to the Lorentz–FitzGerald contraction, in contradiction to the principle that all inertial observers should be able to describe phenomena by the same physical laws.

A drawback of the usual doubly special relativity models is that they are valid only at the energy scales where ordinary special relativity is supposed to break down, giving rise to a patchwork relativity. On the other hand, de Sitter relativity is found to be invariant under a simultaneous re-scaling of mass, energy and momentum, and is consequently valid at all energy scales.

Curvilinear coordinates and non-inertial frames

There can be misunderstandings over the sense in which SR can be applied to accelerating frames.

The confusion here results from trying to describe three different things with just two labels. The three things are:
  • A description of physics without gravity using just "inertial frames", i.e. non-accelerating Cartesian coordinate systems. These coordinate systems are all related to each other by the linear Lorentz transformations. The physical laws may be described more simply in these frames than in the others. This is "special relativity" as usually understood.
  • A description of physics without gravity using arbitrary curvilinear coordinates. This is non-gravitational physics plus general covariance. Here one sets the Riemann-Christoffel tensor to zero instead of using the Einstein field equations. This is the sense in which "special relativity" can handle accelerated frames.
  • A description of physics including gravity governed by the Einstein field equations, i.e. full general relativity.

Special relativity cannot be used to describe a global frame for non-inertial i.e. accelerating frames. However general relativity implies that special relativity can be applied locally where the observer is confined to making local measurements. For example, an analysis of Bremsstrahlung does not require general relativity, SR is sufficient.[23][24][25]

The key point is that you can use special relativity to describe all kinds of accelerated phenomena, and also to predict the measurements made by an accelerated observer who is confined to making measurements at one specific location only. If you try to build a complete frame for such an observer, one that is meant to cover all of spacetime, you'll run into difficulties (there'll be a horizon, for one).

The issue is that it is impossible to infer from the special relativity postulates that an acceleration will not have a non-trivial effect. For instance, in the situation of the twin paradox, we are aware that the proper solution for the age difference between the twins can be computed by simply integrating the time dilation formula along the path taken by the traveling twin. This implies that one thinks that an inertial observer moving at the same speed as the twin might, at any time, replace the twin on its trajectory. As long as we are computing effects that are local to the traveling twin, this provides the correct response. General relativity predicts that the acceleration that separates the twin's local inertial rest frame from its true frame has no further effects; this has, of course, been experimentally validated.

In 1943, Christian Møller obtained a transform between an inertial frame and a frame moving with constant acceleration, based on Einstein's vacuum field equations and a certain postulated time-independent metric tensor, although this transform is of limited applicability as it does not reduce to the Lorentz transform when a=0.[citation needed][26]

Throughout the 20th century efforts were made in order to generalize the Lorentz transformations to a set of transformations linking inertial frames to non-inertial frames with uniform acceleration. So far, these efforts failed to produce satisfactory results that are both consistent with 4-dimensional symmetry and to reduce in the limit a=0 to the Lorentz transformations.[citation needed]

Hsu and Hsu,[1] who theorised Taiji relativity, argue that they have finally come up with suitable transformations for constant linear acceleration (uniform acceleration). They call these transformations: Generalized Møller-Wu-Lee Transformations. They also say: "But such a generalization turns out not to be unique from a theoretical viewpoint and there are infinitely many generalizations. So far, no established theoretical principle leads to a simple and unique generalization."

Taiji relativity

Taiji relativity is a disputed[27][28] formulation of special relativity developed by Jong-Ping Hsu and Leonardo Hsu.[1][29][30][31] The name of the theory, Taiji, is a Chinese word which refers to ultimate principles which predate the existence of the world.

In SI units, time is measured in seconds, but in Taiji relativity, time is measured in meters - the same units used to measure space. Expressing time in meters has previously been done by other authors: Taylor and Wheeler in Spacetime Physics[32] and Moore in Six Ideas that Shaped Physics.[33]

Hsu and Hsu claimed that this choice allowed them to develop a theory of relativity which is experimentally indistinguishable from special relativity, but without using the second postulate in their derivation.

The transformations that they derive involve the factor [math]\displaystyle{ \frac{1}{\sqrt{1 - \beta^2}} }[/math] where β is the velocity measured in meters per meter (a dimensionless quantity). This looks the same as (but should NOT be conceptually confused with) the velocity as a fraction of light v/c that appears in some expressions for the Lorentz transformations.

The transformations are derived using just the principle of relativity and have a maximal speed of 1, which is quite unlike "single postulate" derivations of the Lorentz transformations in which you end up with a parameter that may be zero. So, this is not the same as other "single postulate" derivations. However, the relationship of Taiji time "w" to standard time "t" must still be found; otherwise, it would not be clear how an observer would measure Taiji time. The Taiji transformations are then combined with Maxwell's equations to show that the speed of light is independent of the observer and has the value 1 in Taiji speed (i.e. ,it has the maximal speed). This can be thought of as saying: a time of 1 metre is the time it takes for light to travel 1 metre. Since we can measure the speed of light by experiment in m/s to get the value c, we can use this as a conversion factor. i.e. we have now found an operational definition of Taiji time: w=ct.

So, we have: w meters = (c m/s) * t seconds

Let r = distance. Then Taiji speed = r meters / w meters = r/w dimensionless.

But it is not just due to the choice of units that there is a maximum speed. It is the principle of relativity, that Hsu & Hsu say, when applied to 4d spacetime, implies the invariance of the 4d-spacetime interval [math]\displaystyle{ s^2=w^2-r^2 }[/math] and this leads to the coordinate transformations involving the factor [math]\displaystyle{ 1\over\sqrt{(1-\beta^2)} }[/math] where beta is the magnitude of the velocity between two inertial frames. The difference between this and the spacetime interval [math]\displaystyle{ s^2=c^2t^2-r^2 }[/math] in Minkowski space is that [math]\displaystyle{ s^2=w^2-r^2 }[/math] is invariant purely by the principle of relativity whereas [math]\displaystyle{ s^2=c^2t^2-r^2 }[/math] requires both postulates. The "principle of relativity" in spacetime is taken to mean invariance of laws under 4-dimensional transformations.

Hsu & Hsu then explore other relationships between w and t such as w=bt where b is a function. They show that there are versions of relativity which are consistent with experiment but have a definition of time where the "speed" of light is not constant. They develop one such version called common relativity which is more convenient for performing calculations for "relativistic many body problems" than using special relativity.


See also

Notes

  1. ↑ The Minkowski metric describes four-dimensional space-time: the coordinates are time and three spatial dimensions. The Euclidean metric describes four-dimensional Euclidean space: it has four spatial coordinates.

References

  1. ↑ 1.0 1.1 1.2 1.3 Hsu, J.-P.; Hsu, L. (2006). A Broader View of Relativity. World Scientific. ISBN 981-256-651-1. 
  2. ↑ Petkov, Vesselin (2006). Relativity and the Nature of Spacetime (illustrated ed.). Springer Science & Business Media. p. 193. ISBN 978-3-540-27700-2. https://books.google.com/books?id=Gj0C8AkEz6sC.  Extract of page 193
  3. ↑ Griffiths, David J. (2013). "Electrodynamics and Relativity". Introduction to Electrodynamics (4th ed.). Pearson. Chapter 12. ISBN 978-0-321-85656-2. 
  4. ↑ Jackson, John D. (1999). "Special Theory of Relativity". Classical Electrodynamics (3rd ed.). John Wiley & Sons, Inc.. Chapter 11. ISBN 0-471-30932-X. 
  5. ↑ von Ignatowsky, W. (1911). "Das Relativitätsprinzip" (in de). Archiv der Mathematik und Physik 17: 1. https://de.wikisource.org/wiki/Das_Relativit%C3%A4tsprinzip_%28Ignatowski%29. 
  6. ↑ Feigenbaum, M. J. (2008). "The Theory of Relativity - Galileo's Child". arXiv:0806.1234 [physics.class-ph].
  7. ↑ 7.0 7.1 Cacciatori, S.; Gorini, V.; Kamenshchik, A. (2008). "Special relativity in the 21st century". Annalen der Physik 520 (9–10): 728–768. doi:10.1002/andp.200810321. Bibcode: 2008AnP...520..728C. 
  8. ↑ C., E. (November 1924). "The Mathematical Theory of Relativity" (in en). Nature 114 (2874): 782–783. doi:10.1038/114782a0. ISSN 1476-4687. Bibcode: 1924Natur.114..782C. https://www.nature.com/articles/114782a0. 
  9. ↑ Einstein, A. (1921), Morgan document 
  10. ↑ Morin, D. (2008). Introduction to Classical Mechanics. Cambridge University Press. Section 11-10. ISBN 978-0-521-87622-3. https://archive.org/details/introductiontocl00mori/page/. 
  11. ↑ Giulini, D. (2006). "Algebraic and Geometric Structures in Special Relativity". Special Relativity. Lecture Notes in Physics. 702. pp. 45–111. doi:10.1007/3-540-34523-X_4. ISBN 978-3-540-34522-0. Bibcode: 2006math.ph...2018G. 
  12. ↑ Zhang, Y.-Z. (1997). Special Relativity and Its Experimental Foundations. World Scientific. ISBN 978-981-02-2749-4. https://archive.org/details/specialrelativit0000chan. 
  13. ↑ Bacry, H.; Lévy-Leblond, J.-M. (1968). "Possible Kinematics". Journal of Mathematical Physics 9 (10): 1605–1614. doi:10.1063/1.1664490. Bibcode: 1968JMP.....9.1605B. 
  14. ↑ Yamashita, Takuya (May 2023). "Theoretical Evidence for Principles of Special Relativity Based on Isotropic and Uniform Four-Dimensional Space". Preprints. doi:10.20944/preprints202305.1785.v1. 
  15. ↑ Hans, H. (2001). "Proper time formulation of relativistic dynamics". Foundations of Physics 31 (9): 1357–1400. doi:10.1023/A:1012274211780. 
  16. ↑ Gersten, A. (2003). "Euclidean special relativity". Foundations of Physics 33 (8): 1237–1251. doi:10.1023/A:1025631125442. Bibcode: 2003FoPh...33.1237G. 
  17. ↑ van Linden, R. F. J. (2006). "Minkowski versus Euclidean 4-vectors". http://www.euclideanrelativity.com/pdf/4vectors-rfjvl.pdf. 
  18. ↑ Crabbe, A. (2004). "Alternative conventions and geometry for Special Relativity". Annales de la Fondation Louis de Broglie 29 (4): 589–608. http://aflb.ensmp.fr/AFLB-294/aflb294m097.pdf. 
  19. ↑ Almeida, J. (2001). "An alternative to Minkowski space-time". arXiv:gr-qc/0104029.
  20. ↑ "Euclidean relativity portal". 28 September 2012. http://www.euclideanrelativity.com. 
  21. ↑ Fontana, G. (2005). "The Four Space‐times Model of Reality". AIP Conference Proceedings 746: 1403–1410. doi:10.1063/1.1867271. Bibcode: 2005AIPC..746.1403F. 
  22. ↑ Cohen, Andrew G.; Glashow, Sheldon L. (2006). "Very special relativity". Physical Review Letters 97 (2): 1601. doi:10.1103/PhysRevLett.97.021601. PMID 16907430. Bibcode: 2006PhRvL..97b1601C. 
  23. ↑ Gibbs, P. (1996). "Can Special Relativity handle accelerations?". The Original Usenet Physics FAQ. http://math.ucr.edu/home/baez/physics/Relativity/SR/acceleration.html. 
  24. ↑ Minguzzi, E. (2005). "Differential aging from acceleration, an explicit formula". American Journal of Physics 73 (9): 876–880. doi:10.1119/1.1924490. Bibcode: 2005AmJPh..73..876M. 
  25. ↑ Van de moortel, D. (6 May 2013). "SR treatment of arbitrarily accelerated motion". http://users.telenet.be/vdmoortel/dirk/Physics/Acceleration.html. 
  26. ↑ [chrome-extension://efaidnbmnnnibpcajpcglclefindmkaj/https://math.mit.edu/~dunkel/Diplom/diss.pdf Relativistic Brownian Motionand Diffusion Processes]. J¨orn Dunkel. 2008. chrome-extension://efaidnbmnnnibpcajpcglclefindmkaj/https://math.mit.edu/~dunkel/Diplom/diss.pdf. 
  27. ↑ Behera, H. (2003). "A comment on the Invariance of the Speed of Light". Bulletin of Orissa Physical Society 10: 4087. Bibcode: 2003physics...4087B. 
  28. ↑ Ai, X.-B (1996). "On the Basis of Taiji Relativity". Chinese Physics Letters 13 (5): 321–324. doi:10.1088/0256-307X/13/5/001. Bibcode: 1996ChPhL..13..321A. 
  29. ↑ Hsu, J.-P.; Hsu, L. (1994). "A physical theory based solely on the first postulate of relativity". Physics Letters A 196 (1–2): 1–6. doi:10.1016/0375-9601(94)91033-2. Bibcode: 1994PhLA..196....1H. 
    Erratum Hsu, Jong-Ping; Hsu, Leonardo (1996). "A physical theory based solely on the first postulate of relativity (Physics Letters a 196 (1994)1)". Physics Letters A 217 (6): 359. doi:10.1016/0375-9601(96)00329-5. Bibcode: 1996PhLA..217..359H. 
  30. ↑ Hsu, J.-P.; Hsu, L. (2008). "Experimental tests of a new Lorentz-invariant dynamics based solely on the first postulate of relativity". Il Nuovo Cimento B 111 (11): 1283–1297. doi:10.1007/BF02742506. Bibcode: 1996NCimB.111.1283H. 
  31. ↑ Hsu, J.-P.; Hsu, L. (2008). "Four-dimensional symmetry of taiji relativity and coordinate transformations based on a weaker postulate for the speed of light". Il Nuovo Cimento B 111 (11): 1299–1313. doi:10.1007/BF02742507. Bibcode: 1996NCimB.111.1299H. 
  32. ↑ Taylor, E. F.; Wheeler, J. A. (1992). Spacetime Physics. W. H. Freeman and Co. ISBN 0-7167-2327-1. https://archive.org/details/spacetimephysics00edwi_0. 
  33. ↑ Moore, T. (2002). Six Ideas that Shaped Physics. McGraw-Hill. ISBN 0-07-043049-7. 



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