Submitted:
06 April 2026
Posted:
07 April 2026
Read the latest preprint version here
Abstract
Keywords:
- Clocks measure proper time . There are two ways to interpret : In special and general relativity (SR/GR) [1,2], can parameterize worldlines in spacetime. In Euclidean relativity (ER), is the time coordinate of spacetime. As in GR, gravity in ER is the curvature of spacetime. Unlike SR/GR, ER postulates a mathematical background reality (4D Euclidean space), which provides information that is not available in SR/GR.
1. Introduction
- Today’s concepts of space and time were coined by Albert Einstein. In SR, the Minkowski metric describes a flat spacetime. The geometric framework is Minkowski spacetime [3]. The muon lifetime [4] is an often-cited example that supports SR. In GR, the metric tensor and the Einstein tensor describe a curved spacetime. The deflection of starlight [5] and the accuracy of GPS [6] are two examples that support GR. Quantum field theory [7] unifies classical field theory, SR, and quantum mechanics (QM), but not GR.
2. Coordinate Time and Its Shortcomings
- In § 1 of SR [1], Einstein considers a reference frame “in which the equations of Newton’s physics apply” (to a first approximation). If an object is at rest in this frame, its position in 3D space is determined using rigid rods and a 3D Euclidean geometry. If we also want to describe an object’s motion, we have to define time. Einstein gives an instruction on how to synchronize clocks at the points P and Q. At a coordinate time , a light signal is sent from P to Q. At , it is reflected at Q. At , it is back at P. The clocks synchronize if
3. The Physics of Euclidean Relativity
- ER is a new way to describe physical realities. Unlike SR/GR, ER postulates a mathematical background reality. Unlike SR/GR, ER uses a natural time coordinate and an absolute parameter time. Here is how we proceed: To determine an object’s position in an observer’s 3D space, we use the same rigid rods and the same 3D geometry (Euclidean geometry) as in SR. However, we will not use coordinate time as the time coordinate, but the natural, proper time measured by clocks. That is, we do not construct time.
4. Relativistic Effects in Euclidean Relativity
- We consider two rockets “r” and “b” that move uniformly through 3D space. R (or B) is in the rear end of “r” (or else “b”). R (or B) experiences (or else ) as his 3D space. R (or B) experiences (or else ) as his proper time. The two rockets start at the same point P and the same . They move relative to each other at the constant speed . The ES diagrams in Fig. 2 must satisfy our three postulates and the two initial conditions (same P, same ). This is achieved by rotating the red and blue frames against each other. In ES diagrams, objects retain proper length. For better readability, a rocket’s width is drawn in (or ) although its actual width is in and (or else and ).

5. Empirical Evidence for Euclidean Relativity
- Here we show that ER predicts 12 empirical facts. In particular, ER passes those three tests that Albert Einstein himself proposes to validate GR (see § 22 of [2]): gravitational redshift, gravitational lensing, and the precession of Mercury’s perihelion.
5.1. Time’s Arrow
5.2. Gravitational Redshift
5.3. Gravitational Lensing
5.4. Precession of Mercury’s Perihelion
5.5. Cosmic Microwave Background (CMB)
5.6. Hubble–Lemaître Law

5.7. Flat Universe
5.8. Large-Scale Structures
5.9. Cosmic Homogeneity (Horizon Problem)
5.10. Hubble Tension ( Tension)
5.11. Cosmological Redshift
5.12. Quantum Entanglement
6. Conclusions
- ER is a new way to describe physical realities: (1) An observer experiences two projections of ES as space and time. Without gravity, his spacetime is Minkowski-like. As in GR, gravity in ER is the curvature of spacetime. (2) In ER, there is absolute space (ES), an absolute evolution parameter (), and a 4D vector “flow of proper time” (). Information hidden in ES, , and is not available in SR/GR. ES is relevant for modeling an observer’s physical reality. is relevant for modeling galactic motion. is relevant for understanding cosmic homogeneity, cosmological redshift, and entanglement. (3) In ER, is replaced by , and man-made by natural . There is a difference regarding the axis of time dilation. In SR and GR, an observed clock is slow with respect to an observer’s clock in the observed clock’s time axis. In ER, it is slow in the observer’s time axis. Ultimately, this difference is irrelevant because experiments do not reveal in which axis a clock is slow.
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References
- Einstein, A. Zur Elektrodynamik bewegter Körper. Ann. Phys. 1905, 322, 891–921. [Google Scholar] [CrossRef]
- Einstein, A. Die Grundlage der allgemeinen Relativitätstheorie. Ann. Phys. 1905, 354, 769–822. [Google Scholar] [CrossRef]
- Minkowski, H. Die Grundgleichungen für die elektromagnetischen Vorgänge in bewegten Körpern. Math. Ann. 1910, 68, 472–525. [Google Scholar] [CrossRef]
- Rossi, B.; Hall, D.B. Variation of the rate of decay of mesotrons with momentum. Phys. Rev. 1941, 59, 223–228. [Google Scholar] [CrossRef]
- Dyson, F.W.; Eddington, A.S.; Davidson, C. A determination of the deflection of light by the sun’s gravitational field, from observations made at the total eclipse of May 29, 1919. Phil. Trans. R. Soc. A 1920, 220, 291–333. [Google Scholar] [CrossRef]
- Ashby, N. Relativity in the global positioning system. Living Rev. Relativ. 2003, 6, 1–42. [Google Scholar] [CrossRef]
- Ryder, L. Quantum Field Theory; Cambridge University Press: Cambridge, 1985. [Google Scholar]
- Newburgh, R.G.; Phipp, T.E., Jr. Physical Sciences Research Papers no. 401. United States Air Force (1969).
- Montanus, H. Special relativity in an absolute Euclidean space-time. Phys. Essays 1991, 4, 350–356. [Google Scholar] [CrossRef]
- Montanus, J.M.C. Proper-time formulation of relativistic dynamics. Found. Phys. 2001, 31, 1357–1400. [Google Scholar] [CrossRef]
- Montanus, H. Proper Time as Fourth Coordinate; 2023; ISBN 978-90-829889-4-9. Available online: https://greenbluemath.nl/proper-time-as-fourth-coordinate/ (accessed on 06 April 2026).
- Almeida, J.B. An alternative to Minkowski space-time. arXiv 2001, arXiv:gr-qc/0104029. [Google Scholar] [CrossRef]
- Gersten, A. Euclidean special relativity. Found. Phys. 2003, 33, 1237–1251. [Google Scholar] [CrossRef]
- Hudgin, R.H. Coordinate-free relativity. Synthese 1972, 24, 281–297. [Google Scholar] [CrossRef]
- Misner, C.W.; Thorne, K.S.; Wheeler, A. Gravitation; W. H. Freeman and Company: San Francisco, 1973. [Google Scholar]
- Michelson, A.A.; Morley, E.W. On the relative motion of the Earth and the luminiferous ether. Am. J. Sci. 1887, 34, 333–345. [Google Scholar] [CrossRef]
- Dodelson, S.; Schmidt, F. Modern Cosmology; Elsevier: London, 2025. [Google Scholar]
- Church, A.E.; Bartlett, G.M. Elements of Descriptive Geometry. Part I. Orthographic Projections; American Book Company: New York, 1911. [Google Scholar]
- Nowinski, J.L. Applications of Functional Analysis in Engineering; Plenum Press: New York, 1981. [Google Scholar]
- Wald, R.M. General Relativity; The University of Chicago Press: Chicago, 1984. [Google Scholar]
- Wick, G.C. Properties of Bethe-Salpeter wave functions. Phys. Rev. 1954, 96, 1124–1134. [Google Scholar] [CrossRef]
- Matthews, P.C. Vector Calculus; Springer-Verlag: London, 1998. [Google Scholar]
- Hafele, J.C.; Keating, R.E. Around-the-world atomic clocks: predicted relativistic time gains. Science 1972, 177, 166–168. [Google Scholar] [CrossRef]
- Ellis, G.F.R.; Maartens, R.; MacCallum, M. Relativistic Cosmology; Cambridge University Press: Cambridge, 2012. [Google Scholar]
- Oppenheimer, J.R.; Snyder, H. On continued gravitational contraction. Phys. Rev. 1939, 56, 455–459. [Google Scholar] [CrossRef]
- Abbott, B.P.; et al. Observation of gravitational waves from a binary black hole merger. Phys. Rev. Lett. 2016, 116, 061102. [Google Scholar] [CrossRef]
- Carroll, S.M. Lecture notes on general relativity. arXiv 1997, arXiv:gr-qc/9712019. [Google Scholar] [CrossRef]
- Lee, V.S.H.; Zurek, K.M. Proper time observables of general perturbations in laser interferometry-based gravitational wave detectors. Phys. Rev. D. 2025, 111, 124037. [Google Scholar] [CrossRef]
- Holstein, B.R. Graviton physics. Am. J. Phys. 2006, 74, 1002–1011. [Google Scholar] [CrossRef]
- Ellis, G. The standard cosmological model: achievements and issues. Found. Phys. 2018, 48, 1226–1245. [Google Scholar] [CrossRef]
- Abdalla, E.; et al. Cosmology intertwined: a review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies. J. High. En. Astrophys. 2022, 34, 49–211. [Google Scholar]
- Penzias, A.A.; Wilson, R.W. A measurement of excess antenna temperature at 4080 Mc/s. Astrophys. J. 1965, 142, 419–421. [Google Scholar] [CrossRef]
- Hubble, E. A relation between distance and radial velocity among extra-galactic nebulae. Proc. Natl. Acad. Sci. U.S.A 1965, 15, 168–173. [Google Scholar] [CrossRef] [PubMed]
- Lemaître, G. Un univers homogène de masse constante et de rayon croissant, rendant compte de la vitesse radiale des nébuleuses extra-galactiques. Ann. Soc. Sci. Brux. A 1927, 47, 49–59. [Google Scholar]
- Linde, A. Inflation and Quantum Cosmology; Academic Press: Boston, 1990. [Google Scholar]
- Guth, A. The Inflationary Universe; Perseus Books: New York, 1997. [Google Scholar]
- Aghanim, N.; et al. Planck 2018 results. VI. Cosmological parameters. Astron. Astrophys. 2020, 641, A6. [Google Scholar]
- Riess, A.G.; et al. A comprehensive measurement of the local value of the Hubble constant with 1 km s−1 Mpc−1 uncertainty from the Hubble Space Telescope and the SH0ES team. Astrophys. J. Lett. 2022, 934, L7. [Google Scholar] [CrossRef]
- Perlmutter, S.; et al. Measurements of Ω and Λ from 42 high-redshift supernovae. Astrophys. J. 1999, 517, 565–586. [Google Scholar] [CrossRef]
- Riess, A.G.; et al. Observational evidence from supernovae for an accelerating universe and a cosmological constant. Astron. J. 1998, 116, 1009–1038. [Google Scholar] [CrossRef]
- Turner, M. Dark matter and dark energy in the universe. arXiv 1998, arXiv:astro-ph/9811454. [Google Scholar] [CrossRef]
- Schrödinger, E. Die gegenwärtige Situation in der Quantenmechanik. Naturwissenschaften 1935, 23, 807–812. [Google Scholar] [CrossRef]
- Einstein, A.; Podolsky, B.; Rosen, N. Can quantum-mechanical description of physical reality be considered complete? Phys. Rev. 1935, 47, 777–780. [Google Scholar] [CrossRef]
- Bell, J.S. On the Einstein Podolsky Rosen paradox. Physics 1964, 1, 195–200. [Google Scholar] [CrossRef]
- Freedman, S.J.; Clauser, J.F. Experimental test of local hidden-variable theories. Phys. Rev. Lett. 1972, 28, 938–941. [Google Scholar] [CrossRef]
- Aspect, A.; Dalibard, J.; Roger, G. Experimental test of Bell’s inequalities using time-varying analyzers. Phys. Rev. Lett. 1982, 49, 1804–1807. [Google Scholar] [CrossRef]
- Bouwmeester, D.; et al. Experimental quantum teleportation. Nature 1997, 390, 575–579. [Google Scholar] [CrossRef]
- Hensen, B.; et al. Loophole-free Bell inequality violation using electron spins separated by 1.3 kilometres. Nature 2015, 526, 682–686. [Google Scholar] [CrossRef] [PubMed]
- Einstein, A. Über einen die Erzeugung und Verwandlung des Lichtes betreffenden heuristischen Gesichtspunkt. Ann. Phys. 1905, 322, 132–148. [Google Scholar] [CrossRef]
- Plato: Politeia, 514a.





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