Plausible Sources of Dark Energy and Associated Vacuum Properties: Implications for Newton’s G, MOND’s a0, Vacuum Invariants, and the Tully–Fisher and Faber–Jackson Galactic Relations
Abstract
1. Introduction
1.1. CDM Cosmological Constant and QFT Vacuum Catastrophe
1.2. Cosmological Tensions, Evolving Vacuum Properties, and Varying-G Gravity
1.3. Outline
2. Dark Energy Density in Varying-G Gravity
3. Dark Energy Density from Vacuum Properties
- When I is eliminated between the two dimensional relations, then F is eliminated too, and the resulting wave speed cannot define a typical acceleration without a supplementary length L or time T.
- When F is retained, the resulting acceleration is given by , where has dimensions of [power] and represents momentum. But there is presently no bridge to connect charge flow to mechanical momentum in empty space, so this relation is also unable to produce an acceleration scale.
- The gravoelectric constant has dimensions , where Q and M represent charge and mass, respectively. Thus, serves as a bridge between charge and mass, applicable to electrostatic settings.
- The gravomagnetic constant has dimensions , where represents magnetic flux. Thus, serves as a bridge between mass and magnetic flux, applicable to EM transport phenomena. However, this vacuum property has profound unforeseen repercussions, as discussed in depth in Section 5.2.
- The first G-M, , is a composite invariant which is also a lower limit in vacuum. It implies that the gravitational coupling constant in the Einstein field equations attains a minimum value; thus, Einstein’s ubiquitous coupling of spacetime curvature to the stress–energy tensor is strictly minimal (and independent of the amount of mass present) [8,9,10]. Furthermore, has dimensions of [velocity]4[power]−1, a kinematic scaling that turns out to play an important role in vacuum elasticity in response to EM radiative stresses (Section 5.2).
- The second G-M, , defaults to an EM vacuum threshold entirely unrelated to . This behavior has previously appeared in direct comparisons between purely EM Planck units, i.e., in the dual relations (voltage–current), (magnetic flux–charge), and (inductance–capacitance).
4. Comparisons with Planck–CDM Results
5. The Barely Elastic Vacuum Manifold: Discussion and Conclusions
5.1. Vacuum Properties
- Magnetic field B.—Letting in Equation (7), we obtain and T for . Thus, if is assumed to be magnetic pressure, the fluctuating B-field starts out with enormous magnitudes at Planck/Stoney scales and drops immensely at late times.
- Electric field E.—Since , it is expected that the evolution of a fluctuating E-field will track closely that of the magnetic field. In this case, we obtain V m−1 for , clearly not a substantial field magnitude.
- Charge .—Using Gauss’s law, we find that , so the evolution of charge in the vacuum follows closely that of the vacuum capacitance . For , the charge only, and it increases to at the Planck scale10. Thus, some enormous charge densities (1085−88 C m−3) appear at these scales by tiny amounts of charge enclosed within much tinier spherical volumes.
- Current .—Using the vacuum’s evolving G-M timescale (Section 3), we define a current scale by , and we obtainwhere and are the Planck resistance and current, respectively. Quite unexpectedly, this enormous vacuum quantity turns out to be a universal invariant and implies an enormous invariant voltage as well: , where V is the Planck voltage [20]11,12.
5.2. Vacuum Strain Under Stress
- ➀
- Matter present, the TF/FJ galactic relations.—Substituting the static mass defect relation , the stress flux vector becomes proportional to the surface mass density [29], viz.and the stress–strain relation (20) takes the TF/FJ formwhere is MOND’s universal constant and is the enclosed mass. The divergence of reveals that the vacuum stress density is directly proportional to the localized volumetric mass density , yielding the localized source relation
- ➁
- Matter absent, a purely EM vacuum stress.—Substituting the radiative power relation , the stress flux becomes EM momentum flux , viz.and the stress–strain relation (20) takes the formwhere and the Poynting vector due to vacuum EM fields and is defined by in SI units [33]—or in the commonly used Gaussian–CGS units [32]. Then, in the absence of matter, the stress density corresponds to the localized temporal variation of the EM energy density , viz.implying that a localized vacuum stress density is generated by the dynamical time-dependent accumulation or depletion of field energy within the vacuum fabric. In the final step, Poynting’s theorem was applied to a pure vacuum devoid of matter, where there are no charge carriers to sustain a conduction current; thus, the localized current density vanishes identically (). Consequently, the Joule heating (or mechanical work) term drops out of the energy conservation equation [32,33], even in the presence of a time-varying electric field .
Author Contributions
Funding
Data Availability Statement
Acknowledgments
Conflicts of Interest
Abbreviations
| BH | Black Hole |
| CCP | Cosmological Constant Problem |
| CDL | Cosmic Distance Ladder |
| CDM | Cold Dark Matter |
| CMB | Cosmic Microwave Background |
| CODATA | Committee On DATA [22,23] |
| EM | ElectroMagnetic |
| FJ | Faber–Jackson [62] |
| FLRW | Friedman–Lemaître–Robertson–Walker [18] |
| FSC | Fine-Structure Constant |
| G-M | Geometric Mean |
| GR | General Relativity |
| ISCO | Innermost Stable Circular Orbit |
| MOND | MOdified Newtonian Dynamics |
| QFT | Quantum Field Theory |
| RPS | Reformulated Planck System [20] |
| SI | Système International d’unités |
| TF | Tully–Fisher [59] |
| 2D | Two-Dimensional |
| 3D | Three-Dimensional |
| 4D | Four-Dimensional |
| 1 | |
| 2 | In Ref. [21], the composite constant is defined as |
| 3 | Constant in Note 2 is a precise statement of equipartition between thermal energy per degree of freedom ( is temperature) and magnetic energy (I is current) of an inductor with inductance , where is the Stoney length. |
| 4 | |
| 5 | In a broader theoretical context, restrictions on field theories with effective 4D dynamical scales—such as those encountered in swampland conjectures within string theory, or frameworks featuring target-space scale invariance with a dynamical Planck scale—also emphasize the nontrivial cosmological role of evolving fundamental scales (see, e.g., the Planck mass in Ref. [24]). While our approach remains strictly phenomenological and rooted in vacuum elasticity and varying-G gravity rather than string compactifications, both paradigms highlight how evolving fundamental scales substantially alter our standard cosmological expectations. |
| 6 | The force is one of the few Planck units that do not depend on Planck’s constant h, thus the resulting vacuum energy cannot be considered as quantum mechanical in nature, unlike the recent QFT result of zero dark energy from vacuum fluctuations [11,12] that remedies the vacuum catastrophe in the CCP (Section 1.1), but offers no alternative pathway for the resolution of the CCP itself. |
| 7 | This illustrates the enormous scale mismatch that arises when Equation (7) is extrapolated to the Stoney scale. Any calculation that proceeds up to the Planck or Stoney scale does not yield the present-day dark energy content of the universe which is finite but many orders of magnitude smaller in the late-time epochs (see Equations (5) and (11) in the text and the standard Ref. [1]). In Section 5.1, we demonstrate yet another pronounced scale mismatch: a single electron within the Stoney volume implies an enormous charge density of . |
| 8 | Alternatively, we can obtain another estimate of the present-day dark energy density without adopting from CDM as follows: identifying length L with the present-day particle-horizon distance, neglecting the radiation contribution (), and using for the matter sector, the particle horizon integral gives the self-consistency condition |
| 9 | In either case, we believe that exotic dark fields and strange alternative theories accounting for the same observations and comparable results are evidently disfavored by Occam’s razor [40,41,42,43]. By the same token, one could argue that varying-G gravity should be disfavored against FLRW vacuum energy, were it not for additional galaxy observations providing hints for a possible spatial variation of the Newtonian constant G (see Refs. [26,27,28,29,30,31] and references therein). |
| 10 | |
| 11 | The vacuum invariants and are generated by the well-known vacuum constants , and Newton’s . The invariants result from the following sequence of dependencies: (1) The vacuum energy density in Equation (7) introduces Newton’s and c. (2) They define the Planck force as an invariant. (3) Next, and define the invariant voltage scale . (4) Finally, Ohm’s law produces the invariant current scale . |
| 12 | The Planck units that correspond to the new invariants (Note 11) are the only EM units that do not depend on the Planck constant h (or Dirac’s ℏ for that matter, according to the “old school” [19]). Other common EM units (such as Planck charge and magnetic flux) are not vacuum invariants, and they all depend on h [20]. Furthermore, no fundamental mechanical units (such as Planck energy, momentum, pressure, or density) can be constructed from the new invariants, besides of course the power [19,51] and the obscure Planck units noted below Table 2. |
| 13 | Gauss’s law shows that the source of the gravitational field is or [27,52], but does not imply that mass is also the source of the Newtonian gravitational constant. In analogy to Coulomb’s law, the coupling strength between masses could very well be a vacuum property (see also ’Vacuum Gravitational Constant’ in Section 3). |
| 14 | In the linear theory of elasticity, Hooke’s law is written in terms of localized stress (in Pa) and dimensionless geometric strain as , where Y is Young’s modulus (in Pa) [67,68]. To map Equation (22) to Hooke’s law, we define the vacuum stress by and the vacuum strain by , in which case we obtain the effective Young’s modulus . Thus, as the radius of a spherical surface , the localized stiffness of the vacuum against deformation becomes insurmountable (). This formidable localized rigidity provides a mechanical barrier against infinite compression, suggesting the existence of a geometric mechanism that could prevent the formation of GR-type runaway singularities. This can also be seen in a purely geometric description of the scalar curvature (where is the radius of curvature), which implies a vacuum strain of and a Hooke’s law of the form —if , then is finite and thus , preventing the formation of a singularity. |
| 15 | Conversely, at cosmological scales where r∼, the effective modulus drops to ∼50 pPa, failing by many orders of magnitude to match the elastic compliance of even the softest terrestrial bulk solids, such as vulcanized rubber (Y∼1–10 MPa). This dramatic scale-dependent relaxation of the late-time vacuum ensures that its fabric offers virtually no mechanical resistance against the expansion of the global background metric. So, the origin of the extra drag onto the expanding background (needed to resolve the universal tensions in , , and [13,14,15]) must be sought in nonlinear perturbations of the matter content of our -dominated universe [18] or, by those defying Occam’s razor, in heretofore undetected exotic fields [69,70,71,72]. |
| 16 | Extending the discussion of Note 14 to black holes (BHs), on the horizon of a Schwarzschild BH (where spacetime is effectively at the onset of fracture), the stiffness , where is the rest-energy density stored in the BH. (Here, since , and the vacuum is assumed to remain in the linear-elastic regime as .) But is also a measure of the maximum stress exerted by the BH onto the vacuum at the horizon, thus [67], leading to the remarkable conclusion that the dimensionless strain , a universal constant for all BHs in the FLRW universe. This strain is isotropic and the number 3 signifies the dimensionality of space. Thus, the strain per degree of freedom is , implying a maximum kinematic yield of speed on the horizon in any spatial direction. For comparison, and at (ISCO). |
| 17 | In cases 3 and 4 listed in Table 3, the stress field and its source density over volume V in spherical symmetry are as follows:
These equations and those in the main text underscore the general principles of vacuum elasticity (A is area and V is volume):
Although it has remained inconspicuous for many years, this principle has been ingrained in the literature—adopting an elastic material stress with in the framework—since the Faber–Jackson [62,63,64] and Tully–Fisher [59,60,61] relations were first established for elliptical and spiral galaxies, respectively. We note that in this framework, is not a fitted parameter borrowed from galactic dynamics, but an empirical constant whose SI magnitude coincides with the SI magnitude of the vacuum’s [20]. Consequently, setting provides a physical interpretation for this MOND product for the first time in terms of vacuum elasticity theory, answering the fundamental question of what this force scale may represent in real galaxies. On the other hand, this principle has gone unrecognized for electrostatic and EM stresses in GR, with the single exception of the famous Casimir effect [77,78,79,80,81,82,83,84] that so far has been interpreted as the relativistic analogue of the classical van der Waals forces in which retardation effects due to the finite speed of light are taken into account [78,80,83,85]. |
| 18 | In the Casimir effect, the vacuum stress–strain relation acquires the scaled form , where P represents pressure, is the Planck/RPS pressure, and d is the distance between the two flat, parallel, perfectly conducting plates [20]. We then find that the implied geometric curvature along the principal axis running between the plates is , and the kinematic yield v of the vacuum between the plates can be obtained from the proportion . Equivalently, the effective kinematic viscosity of the vacuum between the plates turns out to be , where is the Planck unit of kinematic viscosity in the RPS [20], in which the reformulated Planck length is defined (in terms of Planck’s constant h) by ; thus, we conclude that m2 s−1. Furthermore, the effective curvature radius can be obtained from the equation . For a typical plate separation of m [86,87,88], we find that Mpc, a truly enormous, yet finite curvature radius for a laboratory vacuum, corresponding to a Casimir pressure of mPa (see also Refs. [89,90,91,92] for recent experimental results). |
References
- Aghanim, N.; Akrami, Y.; Ashdown, M.; Aumont, J.; Baccigalupi, C.; Ballardini, M.; Banday, A.J.; Barreiro, R.B.; Bartolo, N.; Planck Collaboration; et al. Planck 2018 results. VI. Cosmological parameters. Astron. Astrophys. 2020, 641, A6. [Google Scholar]
- Alam, S.; Aubert, M.; Avila, S.; Balland, C.; Bautista, J.E.; Bershady, M.A.; Bizyaev, D.; Blanton, M.R.; Bolton, A.S.; eBOSS Collaboration; et al. Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory. Phys. Rev. D 2021, 103, 083533. [Google Scholar] [CrossRef] [Scilit]
- Einstein, A. Kosmologische Betrachtungen zur allgemeinen Relativitätstheorie. Sitzungsber. Königlich Preuss. Akad. Wiss. 1917, 6, 142–152. [Google Scholar]
- Riess, A.G.; Filippenko, A.V.; Challis, P.; Clocchiatti, A.; Diercks, A.; Garnavich, P.M.; Gilliland, R.L.; Hogan, C.J.; Jha, S.; Kirshner, R.P.; et al. Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant. Astron. J. 1998, 116, 1009. [Google Scholar] [CrossRef] [Scilit]
- Perlmutter, S.; Aldering, G.; Goldhaber, G.; Knop, R.A.; Nugent, P.; Castro, P.G.; Deustua, S.; Fabbro, S.; Goobar, A.; Groom, D.E.; et al. Measurements of Ω and Λ from 42 High-Redshift Supernovae. Astrophys. J. 1999, 517, 565. [Google Scholar] [CrossRef] [Scilit]
- Shajib, A.J.; Frieman, J.A. Scalar-field dark energy models: Current and forecast constraints. Phys. Rev. D 2025, 112, 063508. [Google Scholar] [CrossRef] [Scilit]
- Carroll, S.M. The Cosmological Constant. Living Rev. Relativ. 2001, 3, 1. [Google Scholar] [CrossRef] [Scilit] [PubMed]
- Martin, J. Everything you always wanted to know about the cosmological constant problem (but were afraid to ask). C. R. Phys. 2012, 13, 566. [Google Scholar] [CrossRef] [Scilit]
- Weinberg, S. The Cosmological Constant Problem. Rev. Mod. Phys. 1989, 61, 1. [Google Scholar] [CrossRef] [Scilit]
- Peebles, P.J.E.; Ratra, B. The Cosmological Constant and Dark Energy. Rev. Mod. Phys. 2003, 75, 559. [Google Scholar] [CrossRef] [Scilit]
- Ryskin, G. Vanishing vacuum energy. Astropart. Phys. 2020, 115, 102387. [Google Scholar] [CrossRef] [Scilit]
- Ryskin, G. The emergence of cosmic repulsion. Astropart. Phys. 2015, 62, 258. [Google Scholar] [CrossRef] [Scilit]
- Verde, L.; Treu, T.; Riess, A.G. Tensions between the early and late Universe. Nat. Astron. 2019, 3, 891. [Google Scholar] [CrossRef] [Scilit]
- Di Valentino, E.; Mena, O.; Pan, S.; Visinelli, L.; Yang, W.; Melchiorri, A.; Mota, D.F.; Riess, A.G.; Silk, J. In the realm of the Hubble tension—A review of solutions. Class. Quantum Grav. 2021, 38, 153001. [Google Scholar] [CrossRef] [Scilit]
- Perivolaropoulos, L.; Skara, F. Challenges for ΛCDM: An update. New Astron. Rev. 2022, 95, 101659. [Google Scholar]
- Riess, A.G.; Yuan, W.; Macri, L.M.; Scolnic, D.; Brout, D.; Casertano, S.; Jones, D.O.; Murakami, Y.; Anand, G.S.; Breuval, L.; et al. A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team. Astrophys. J. Lett. 2022, 934, L7. [Google Scholar] [CrossRef] [Scilit]
- Freedman, W.L. Measurements of the Hubble Constant: Tensions in Perspective. Astrophys. J. 2021, 919, 16. [Google Scholar] [CrossRef] [Scilit]
- Christodoulou, D.M.; Kazanas, D.; Laycock, S.G.T. A common origin of the H0 and S8 cosmological tensions and a resolution within a modified ΛCDM framework. Galaxies 2026, 14, 16, Correction in Galaxies 2026, 14, 25. [Google Scholar] [CrossRef] [Scilit]
- Christodoulou, D.M.; Kazanas, D. The Upgraded Planck System of Units That Reaches from the Known Planck Scale All the Way Down to Subatomic Scales. Astronomy 2023, 2, 235–268. [Google Scholar] [CrossRef] [Scilit]
- Christodoulou, D.M.; Kazanas, D.; Laycock, S.G.T. Natural Constants Determined to High Precision from Boltzmann’s Constant and Avogadro’s Number—A Challenge to Experiments and Astrophysical Observations to Match the Precision of the Results. Galaxies 2025, 13, 119. [Google Scholar] [CrossRef] [Scilit]
- Christodoulou, D.M.; Kazanas, D.; Laycock, S.G.T. Composite universal constants combining 2–5 known constants reveal latent connections between disparate physical regimes and the role of dimensionless constants in systems of units. Galaxies 2026, 14, 74. [Google Scholar] [CrossRef] [Scilit]
- Tiesinga, E.; Mohr, P.J.; Newell, D.B.; Taylor, B.N. CODATA recommended values of the fundamental physical constants: 2018. Rev. Mod. Phys. 2021, 93, 025010. [Google Scholar] [CrossRef] [Scilit] [PubMed]
- Mohr, P.J.; Newell, D.B.; Taylor, B.N.; Tiesinga, E. CODATA recommended values of the fundamental physical constants: 2022. Rev. Mod. Phys. 2025, 97, 025002. [Google Scholar] [CrossRef] [Scilit]
- Guendelman, E.I. Dynamical string tension theories with target space scale invariance SSB and restoration. Eur. Phys. J. C 2025, 85, 276. [Google Scholar] [CrossRef] [Scilit]
- Sheykin, A.; Manida, S. Universal Constants and Natural Systems of Units in a Spacetime of Arbitrary Dimension. Universe 2020, 6, 166. [Google Scholar] [CrossRef] [Scilit]
- Christodoulou, D.M.; Kazanas, D. Interposing a varying gravitational constant between modified Newtonian dynamics and weak Weyl gravity. Mon. Not. R. Astron. Soc. 2018, 479, L143. [Google Scholar] [CrossRef] [Scilit] [PubMed]
- Christodoulou, D.M.; Kazanas, D. Gauss’s law and the source for Poisson’s equation in modified gravity with Varying G. Mon. Not. R. Astron. Soc. 2019, 484, 1421. [Google Scholar] [CrossRef] [Scilit]
- Christodoulou, D.M.; Kazanas, D. Universal expansion with spatially varying G. Mon. Not. R. Astron. Soc. 2019, 487, L53. [Google Scholar] [CrossRef] [Scilit]
- Christodoulou, D.M.; Kazanas, D. Varying-G gravity: Physical properties, asymptotic regimes, and Green’s functions, an event horizon, the vacuum energy density, and the external pressure that modifies Jeans instability. Mon. Not. R. Astron. Soc. 2023, 519, 1277. [Google Scholar] [CrossRef] [Scilit]
- Milgrom, M. MOND laws of galactic dynamics. Mon. Not. R. Astron. Soc. 2014, 437, 2531. [Google Scholar] [CrossRef] [Scilit]
- Milgrom, M. MOND theory. Can. J. Phys. 2015, 93, 107. [Google Scholar] [CrossRef] [Scilit]
- Jackson, J.D. Classical Electrodynamics; Wiley: New York, NY, USA, 1962; pp. 611–621, Section 6.8. [Google Scholar]
- Griffiths, D.J. Introduction to Electrodynamics, 4th ed.; Pearson: Boston, MA, USA, 2013. [Google Scholar]
- Rindler, W. Visual Horizons in World Models. Mon. Not. R. Astron. Soc. 1956, 116, 662. [Google Scholar] [CrossRef] [Scilit]
- Peebles, P.J.E. Principles of Physical Cosmology; Princeton University Press: Princeton, NJ, USA, 1993; pp. 98–99, 287–290. [Google Scholar]
- Dodelson, S. Modern Cosmology; Academic Press: San Diego, CA, USA, 2003. [Google Scholar]
- Ade, P.A.R.; Aghanim, N.; Arnaud, M.; Ashdown, M.; Aumont, J.; Baccigalupi, C.; Banday, A.J.; Barreiro, R.B.; Bartlett, J.G.; Planck Collaboration; et al. Planck 2015 results. XIII. Cosmological parameters. Astron. Astrophys. 2016, 594, A13. [Google Scholar]
- Aghanim, N.; Akrami, Y.; Arroja, F.; Ashdown, M.; Aumont, J.; Baccigalupi, C.; Ballardini, M.; Banday, A.J.; Barreiro, R.B.; Planck Collaboration; et al. Planck 2018 results. I. Overview and the cosmological legacy of Planck. Astron. Astrophys. 2020, 641, A1. [Google Scholar]
- Cosmological Constant—Wikipedia. Available online: https://en.wikipedia.org/wiki/Cosmological_constant (accessed on 17 July 2026).
- Newton, I. Philosophiæ Naturalis Principia Mathematica; J. Societatis Regiæ: London, UK, 1687. [Google Scholar]
- Einstein, A. On the Method of Theoretical Physics. Philos. Sci. 1934, 1, 163. [Google Scholar] [CrossRef] [Scilit] [PubMed]
- Jeffreys, H. Theory of Probability; Oxford University Press: Oxford, UK, 1939. [Google Scholar]
- Baker, A. Occam’s Razor in science: A case study from biogeography. Biol. Philos. 2007, 22, 193. [Google Scholar] [CrossRef] [Scilit]
- Padmanabhan, T. Cosmological constant—The weight of the vacuum. Phys. Rep. 2003, 380, 235. [Google Scholar] [CrossRef] [Scilit]
- Narimani, A.; Afshordi, N.; Scott, D. How does pressure gravitate? Cosmological constant problem confronts observational cosmology. JCAP 2014, 08, 049. [Google Scholar] [CrossRef] [Scilit]
- Bengochea, G.R.; León, G.; Okon, E.; Sudarsky, D. Can the quantum vacuum fluctuations really solve the cosmological constant problem? Eur. Phys. J. C 2020, 80, 18. [Google Scholar] [CrossRef] [Scilit]
- Fukugita, M.; Hogan, C.J.; Peebles, P.J.E. The Cosmic Baryon Budget. Astrophys. J. 1998, 503, 518. [Google Scholar] [CrossRef] [Scilit] [PubMed]
- Fukugita, M.; Peebles, P.J.E. The Cosmic Energy Inventory. Astrophys. J. 2004, 616, 643. [Google Scholar] [CrossRef] [Scilit]
- Nicastro, F.; Kaastra, J.; Krongold, Y.; Borgani, S.; Branchini, E.; Cen, R.; Dadina, M.; Danforth, C.W.; Elvis, M.; Fiore, F.; et al. Observations of the missing baryons in the warm–hot intergalactic medium. Nature 2018, 558, 406. [Google Scholar] [CrossRef] [Scilit] [PubMed]
- Macquart, J.-P.; Prochaska, J.X.; McQuinn, M.; Bannister, K.W.; Bhandari, S.; Day, C.K.; Deller, A.T.; Ekers, R.D.; James, C.W.; Marnoch, L.; et al. A census of baryons in the Universe from localized fast radio bursts. Nature 2020, 581, 391. [Google Scholar] [CrossRef] [Scilit] [PubMed]
- Elert, G. The Physics Hypertextbook. 2022. Available online: https://physics.info/planck/ (accessed on 17 July 2026).
- Christodoulou, D.M.; Kazanas, D. Introducing the Effective Gravitational Constant 4πε0G. Preprints 2024, 2024110749. [Google Scholar] [CrossRef] [Scilit]
- Sakharov, A.D. Vacuum quantum fluctuations in curved space and the theory of gravitation. Dokl. Akad. Nauk SSSR 1967, 177, 70. [Google Scholar]
- Sorkin, R.D. Forks in the road, on the way to quantum gravity. Int. J. Theor. Phys. 1997, 36, 2759. [Google Scholar] [CrossRef] [Scilit]
- Padmanabhan, T. Why do we observe a small but nonzero cosmological constant? Class. Quantum Grav. 2002, 19, L167. [Google Scholar] [CrossRef] [Scilit]
- Volonik, G.E. The Universe in a Helium Droplet; Clarendon Press: Oxford, UK, 2003; Chapter 29. [Google Scholar]
- Padmanabhan, T. Gravity as elasticity of spacetime: A paradigm to understand horizon thermodynamics and cosmological constant. Int. J. Mod. Phys. D 2004, 13, 2293. [Google Scholar] [CrossRef] [Scilit]
- Christodoulou, D.M.; Kazanas, D.; Laycock, S.G.T. The Conservative Field of Coupled Newton–Coulomb Sources: Component Coupling Constants, Mass ⇌Charge Cross-Forces, and Radiation from Reissner–Nordström Black Hole Mergers. Axioms 2025, 14, 845. [Google Scholar] [CrossRef] [Scilit]
- Tully, R.B.; Fisher, J.R. A new method of determining distances to galaxies. Astron. Astrophys. 1977, 54, 661. [Google Scholar]
- McGaugh, S.S.; Schombert, J.M.; Bothun, G.D.; de Blok, W.J.G. The baryonic Tully–Fisher relation. Astrophys. J. 2000, 533, L99. [Google Scholar] [CrossRef] [Scilit] [PubMed]
- McGaugh, S.S. The baryonic Tully–Fisher relation of gas-rich galaxies as a test of ΛCDM and MOND. Astron. J. 2012, 143, 40. [Google Scholar] [CrossRef] [Scilit]
- Faber, S.M.; Jackson, R.E. Velocity dispersions and mass-to-light ratios for elliptical galaxies. Astrophys. J. 1976, 204, 668. [Google Scholar] [CrossRef] [Scilit] [PubMed]
- Sanders, R.H. Modified Newtonian Dynamics: A falsification of cold dark matter. Adv. Astron. 2009, 2009, 752439. [Google Scholar] [CrossRef] [Scilit]
- den Heijer, M.; Oosterloo, T.A.; Serra, P.; Józsa, G.I.G.; Kerp, J.; Morganti, R.; Cappellari, M.; Davis, T.A.; Duc, P.-A.; Emsellem, E.; et al. The HI Tully–Fisher relation of early-type galaxies. Astron. Astrophys. 2015, 581, A98. [Google Scholar] [CrossRef] [Scilit]
- Ehlers, J.; Rindler, W. Local and Global Light Bending in Einstein’s and Other Gravitational Theories. Gen. Relativ. Gravit. 1997, 29, 519. [Google Scholar] [CrossRef] [Scilit]
- Sauer, T. Soldner, Einstein, gravitational light deflection and factors of two. Ann. Phys. 2021, 533, 2100203. [Google Scholar] [CrossRef] [Scilit]
- Landau, L.D.; Lifshitz, E.M. Theory of Elasticity, 2nd ed.; Pergamon Press: Oxford, UK, 1970; Volume 7, Sections 1–7. [Google Scholar]
- Barber, J.R. Elasticity, 3rd ed.; Springer: Dordrecht, The Netherlands, 2010; Section 1.3. [Google Scholar]
- Copeland, E.J.; Sami, M.; Tsujikawa, S. Dynamics of dark energy. Int. J. Mod. Phys. D 2006, 15, 1753. [Google Scholar] [CrossRef] [Scilit]
- Clifton, T.; Ferreira, P.G.; Padilla, A.; Skordis, C. Modified gravity and cosmology. Phys. Rep. 2012, 513, 1. [Google Scholar] [CrossRef] [Scilit]
- Gubitosi, G.; Piazza, F.; Vernizzi, F. The effective field theory of dark energy. JCAP 2013, 02, 032. [Google Scholar] [CrossRef] [Scilit]
- Tsujikawa, S. Quintessence: A review. Class. Quantum Grav. 2013, 30, 214003. [Google Scholar] [CrossRef] [Scilit]
- Padmanabhan, T. Emergent perspective of gravity and dark energy. Res. Astron. Astrophys. 2012, 12, 891. [Google Scholar] [CrossRef] [Scilit]
- Tenev, T.G.; Horstemeyer, M.F. Mechanics of spacetime—A Solid Mechanics perspective on the theory of General Relativity. Int. J. Mod. Phys. D 2018, 27, 1850083. [Google Scholar] [CrossRef] [Scilit]
- Cartas, V.L. The Elasticity of Quantum Spacetime Fabric. Geom. Integr. Quantization 2018, 19, 105. [Google Scholar] [CrossRef] [Scilit]
- David, I. Analogy of spacetime as an elastic medium—Can we establish a thermal expansion coefficient of space from the cosmological constant Λ? Int. J. Mod. Phys. D 2023, 32, 2350091. [Google Scholar] [CrossRef] [Scilit]
- Casimir, H.B.G.; Polder, D. The influence of retardation on the London-van der Waals forces. Phys. Rev. 1948, 73, 360. [Google Scholar] [CrossRef] [Scilit]
- Dzyaloshinskii, I.E.; Lifshitz, E.M.; Pitaevskii, L.P. General theory of van der Waals forces. Sov. Phys. Usp. 1961, 4, 153. [Google Scholar] [CrossRef] [Scilit]
- Schwinger, J. Casimir effect in source theory II. Lett. Math. Phys. 1992, 24, 59. [Google Scholar] [CrossRef] [Scilit]
- Dzyaloshinskii, I.E.; Kats, E.I. Casimir forces in modulated systems. J. Phys. Condens. Matter 2004, 16, 5659. [Google Scholar] [CrossRef] [Scilit]
- Jaffe, R.L. The Casimir effect and the quantum vacuum. Phys. Rev. D 2005, 72, 021301. [Google Scholar] [CrossRef] [Scilit]
- Rodriguez, A.W.; Capasso, F.; Johnson, S.G. The Casimir effect in microstructured geometries. Nat. Photonics 2011, 5, 211. [Google Scholar] [CrossRef] [Scilit]
- Nikolić, H. Proof that Casimir force does not originate from vacuum energy. Phys. Lett. B 2016, 761, 197. [Google Scholar] [CrossRef] [Scilit]
- Nikolić, H. Is zero-point energy physical? A toy model for Casimir-like effect. Ann. Phys. 2017, 383, 181. [Google Scholar] [CrossRef] [Scilit]
- Parsegian, V.A. Van der Waals Forces; Cambridge University Press: Cambridge, UK, 2006. [Google Scholar]
- Mohideen, U.; Roy, A. Precision Measurement of the Casimir Force from 0.1 to 0.9 μm. Phys. Rev. Lett. 1998, 81, 4549. [Google Scholar] [CrossRef] [Scilit]
- Bressi, G.; Carugno, G.; Onofrio, R.; Ruoso, G. Measurement of the Casimir Force between Parallel Metallic Surfaces. Phys. Rev. Lett. 2002, 88, 041804. [Google Scholar] [CrossRef] [Scilit] [PubMed]
- Decca, R.S.; López, D.; Fischbach, E.; Klimchitskaya, G.L.; Krause, D.E.; Mostepanenko, V.M. Tests of new physics from precise measurements of the Casimir pressure between two gold-coated plates. Phys. Rev. D 2007, 75, 077101. [Google Scholar] [CrossRef] [Scilit]
- Postnikov, A.V.; Uvarov, I.V.; Svetovoy, V.B. Experimental setup for measuring the dispersion forces by the adhered cantilever method. Rev. Sci. Instrum. 2023, 94, 043907. [Google Scholar] [CrossRef] [Scilit] [PubMed]
- Elsaka, B.; Yang, X.; Kästner, P.; Dingel, K.; Sick, B.; Lehmann, P.; Buhmann, S.Y.; Hillmer, H. Casimir Effect in MEMS: Materials, Geometries, and Metrologies—A Review. Materials 2024, 17, 3393. [Google Scholar] [CrossRef] [Scilit] [PubMed]
- Klimchitskaya, G.L.; Mostepanenko, V.M. Advances and Prospects in Casimir Physics. Physics 2024, 6, 1072–1082. [Google Scholar] [CrossRef] [Scilit]
- Postnikov, A.V.; Uvarov, I.V.; Morozov, O.V.; Svetovoy, V.B. Casimir–Lifshitz adhesion between Si and Ru measured by the method of adhered cantilever. Int. J. Mod. Phys. A 2025, 40, 2543008. [Google Scholar] [CrossRef] [Scilit]
| Model | References | |||
|---|---|---|---|---|
| 1. Planck-2018 (⋆⋆) | [1,38] | |||
| 2. Planck-2015 (⋆⋆) | [37,39] | |||
| 3. Varying-G Gravity and MOND | [29,30,31] and this work | |||
| 4. Vacuum Properties + CDM’s | [1,19,20,21] and this work | |||
| 5. Vacuum Properties + Fixed Point + CDM’s | [1] and Note 8 in this work | |||
| 1. Fundamental Set | |||
| : Permittivity : Permeability | Lower limits | ||
| Derived G-M Constants | |||
| Speed of Light: | Upper limit | ||
| Impedance of Free Space: | Matching threshold | ||
| Planck Resistance: | Matching threshold | ||
| MOND Critical Acceleration: | Threshold, SI values only | ||
| 2. Constant Set | |||
| : Permittivity : Permeability : Newton’s Constant | Lower limits | ||
| Derived Invariants (⋆⋆) | |||
| Planck Force: | Upper limit | ||
| Planck Voltage: | Upper limit | ||
| Planck Current: | Upper limit | ||
| Planck Power: | Upper limit | ||
| 3. Evolving Set | |||
| : Permittivity : Permeability L: Length Scale | Lower limits () | ||
| Derived Quantities | |||
| Capacitance: | Increasing | ||
| Inductance: | Increasing | ||
| Light-Crossing Time: | Increasing | ||
| Electric Charge: | Increasing | ||
| Acceleration: | Decreasing | ||
| Electric Field: | Decreasing | ||
| Magnetic Field: | Decreasing | ||
| Magnetic Flux: | Increasing | ||
| Stress | Exerted | Kinematic | Stress–Strain | Composite | Intrinsic (⋆⋆) |
|---|---|---|---|---|---|
| Source | Force | Yield (⋆) | Relation | Coupling | Dimensions |
| 1. Mass M | : | ||||
| 2. EM Power | : | ||||
| 3. Electrostatic Potential | : | ||||
| 4. Isotropic Pressure P (GR) | : |
Disclaimer/Publisher’s Note: The statements, opinions and data contained in all publications are solely those of the individual author(s) and contributor(s) and not of MDPI and/or the editor(s). MDPI and/or the editor(s) disclaim responsibility for any injury to people or property resulting from any ideas, methods, instructions or products referred to in the content. |
© 2026 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license.
Share and Cite
Christodoulou, D.M.; Kazanas, D.; Laycock, S.G.T. Plausible Sources of Dark Energy and Associated Vacuum Properties: Implications for Newton’s G, MOND’s a0, Vacuum Invariants, and the Tully–Fisher and Faber–Jackson Galactic Relations. Galaxies 2026, 14, 90. https://doi.org/10.3390/galaxies14050090
Christodoulou DM, Kazanas D, Laycock SGT. Plausible Sources of Dark Energy and Associated Vacuum Properties: Implications for Newton’s G, MOND’s a0, Vacuum Invariants, and the Tully–Fisher and Faber–Jackson Galactic Relations. Galaxies. 2026; 14(5):90. https://doi.org/10.3390/galaxies14050090
Chicago/Turabian StyleChristodoulou, Dimitris M., Demosthenes Kazanas, and Silas G. T. Laycock. 2026. "Plausible Sources of Dark Energy and Associated Vacuum Properties: Implications for Newton’s G, MOND’s a0, Vacuum Invariants, and the Tully–Fisher and Faber–Jackson Galactic Relations" Galaxies 14, no. 5: 90. https://doi.org/10.3390/galaxies14050090
APA StyleChristodoulou, D. M., Kazanas, D., & Laycock, S. G. T. (2026). Plausible Sources of Dark Energy and Associated Vacuum Properties: Implications for Newton’s G, MOND’s a0, Vacuum Invariants, and the Tully–Fisher and Faber–Jackson Galactic Relations. Galaxies, 14(5), 90. https://doi.org/10.3390/galaxies14050090

