Abstract
A pre-relativistic cosmological approach to electromagnetism and gravitation is explored that leads to a cosmic time variation of the fundamental constants. Space itself is supposed to have physical substance, which manifests by its permeability. The scale factors of the permeability tensor induce a time variation of the fundamental constants. Atomic radii, periods, and energy levels scale in cosmic time, which results in dispersionless redshifts without invoking a space expansion. Hubble constant and deceleration parameter are reviewed in this context. The time variation of the gravitational constant at the present epoch can be expressed in terms of these quantities. This provides a completely new way to restrain the deceleration parameter from laboratory bounds on the time variation of the gravitational constant. This variation also affects the redshift dependence of angular diameters and the surface brightness, and we study in some detail the redshift scaling of the linear sizes of radio sources. The effect of the varying constants on source counts is discussed, and an estimate on the curvature radius of the hyperbolic3-space is inferred from the peak in the quasar distribution. The background radiation in this dispersionless, permeable space-time stays perfectly Planckian. Cosmic time is discussed in terms of atomic and gravitational clocks, as well as cosmological age dating, in particular how the age of the Universe relates to the age of the Galaxy in a permeable space-time.
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Bahcall, J.N., Pinsonneault, M.H. and Wasserburg, G.J.: 1995, Solar models with helium and heavy element diffusion, Rev.Mod.Phys. 67, 781.
Barthel, P.D. and Miley, G.K.: 1988, Evolution of radio structure in quasars, Nature 333, 319.
Caso, C., et al.: 1998, Review of particle physics, Eur.Phys.J.C 3, 1.
Chandrasekhar, S.: 1967, An Introduction to the Study of Stellar Structure, Dover Publ., New York.
Cowan, J.J., et al.: 1997, The thorium chronometer in CS 22892–052: Estimates of the age of the Galaxy, Astrophys.J. 480, 246.
Cowan, J.J., et al.: 1999, R-process abundances and chronometers in metal-poor stars, Astrophys.J. 521, 194.
Dabrowski, Y., Lasenby, A. and Saunders, R.: 1995, Testing the angular-size versus redshift relation with compact radio sources, Mon.Not.R.Astron.Soc. 277, 753.
Davies, P.C.W.: 1972, Time variation of the coupling constants, J.Phys.A 5, 1296.
Degl'Innocenti, S., et al.: 1996, Time variation of Newton's constant and the age of globular clusters, Astron.Astrophys. 312, 345.
Dickey, J.O., et al.: 1994, Lunar laser ranging: A continuing legacy of the Apollo program, Science 265, 482.
Dirac, P.A.M.: 1937, The cosmological constants, Nature 139, 323; also in: R.H. Dalitz (ed.), The Collected Works of P.A.M.Dirac, 1924–1948, Cambridge Univ. Press, Cambridge, 1995.
Dirac, P.A.M.: 1974, Cosmological models and the Large Numbers hypothesis, Proc.Roy.Soc.(London) A 338, 439.
Dyson, F.J.: 1972, The fundamental constants and their time variation, in: A. Salam and E.P. Wigner (eds.), Aspects of Quantum Theory, Cambridge Univ. Press, Cambridge.
García-Berro, E., et al.: 1995, The rate of change of the gravitational constant and the cooling of white dwarfs, Mon.Not.R.Astron.Soc. 277, 801.
Guenther, D.B., Krauss, L.M. and Demarque, P.: 1998, Testing the constancy of the gravitational constant using helioseismology, Astrophys.J. 498, 871.
Hartwick, F.D. and Schade, D.: 1990, The space distribution of quasars, Annu.Rev.Astron.Astrophys. 28, 437.
Irvine, J.M.: 1983, Limits on the variability of coupling constants from the Oklo natural reactor, Phil.Trans.Roy.Soc.(London) A 310, 239.
Kaspi, V.M., Taylor, J.H. and Ryba, M.F.: 1994, High-precision timing of millisecond pulsars, Astrophys.J. 428, 713.
Kasting, J.F. and Grinspoon, D.H.: 1991, The faint young sun problem, in: C.P. Sonett et al. (eds.), The Sun in Time, Univ. of Arizona Press, Tucson.
Lindner, M., et al.: 1986, Direct laboratory determination of the 187Re half-life, Nature 320, 246.
Lineweaver, C.H.: 1999, A younger age for the Universe, Science 284, 1503.
Maloney, A. and Petrosian, V.: 1999, The evolution and luminosity function of quasars from complete optical surveys, Astrophys.J. 518, 32.
McElhinny, M.W., Taylor, S.R. and Stevenson, D.J.: 1978, Limits on the expansion of Earth, Moon, Mars & Mercury and to changes in the gravitational constant, Nature 271, 316.
Moles, M., et al.: 1998, On the use of scaling relations for the Tolman test, Astrophys.J.Lett. 495, L31.
Mould, J., Freedman, W. and Kennicutt, R.: 2000, Calibration of the extragalactic distance scale, Rep.Prog.Phys., to appear.
Neeser, M.J., et al.: 1995, The linear-size evolution of classical double radio sources, Astrophys.J. 451, 76.
Newman, M.J. and Rood, R.T.: 1977, Implications of solar evolution for the Earth's early atmosphere, Science 198, 1035.
Perlmutter, S., et al.: 1999, Measurements of Ω and Λ from 42 high-redshift supernovae, Astrophys.J. 517, 565.
Petrosian, V.: 1998, New & old tests of cosmological models and the evolution of galaxies, Astrophys.J. 507, 1.
Prestage, J.D., Tjoelker, R.L. and Maleki, L.: 1995, Atomic clocks and variations of the fine structure constant, Phys.Rev.Lett. 74, 3511.
Riess, A.G., et al.: 1998, Observational evidence from supernovae for an accelerating universe, Astron.J. 116, 1009.
Robertson, H.P. and Noonan, T.W.: 1968, Relativity and Cosmology, Saunders, Philadelphia.
Sagan, C. and Chyba, C.: 1997, The early faint sun paradox, Science 276, 1217.
Sandage, A.: 1988, Observational tests of world models, Annu.Rev.Astron.Astrophys. 26, 561.
Sandage, A. and Perelmuter, J.-M.: 1991, The surface brightness test for the expansion of the universe, Astrophys.J. 370, 455.
Schmidt, M., Schneider, D.P. and Gunn, J.E.: 1995, Spectroscopic CCD surveys for quasars at large redshift, Astron.J. 110, 68.
Shapiro, I.I.: 1990, Solar system tests of GR, in: N. Ashby et al. (eds.), General Relativity and Gravitation, Cambridge Univ. Press, Cambridge.
Shlyakhter, A.J.: 1976, Direct test of the constancy of fundamental nuclear constants, Nature 264, 340.
Steigman, G.: 1978, A crucial test of the Dirac cosmologies, Astrophys.J. 221, 407.
Teller, E.: 1948, On the change of physical constants, Phys.Rev. 73, 801.
Thorsett, S.E.: 1996, The gravitational constant, the Chandrasekhar limit, and neutron star masses, Phys.Rev.Lett. 77, 1432.
Tomaschitz, R.: 1997, Chaos and topological evolution in cosmology, Int.J.Bifurcation & Chaos 7, 1847.
Tomaschitz, R.: 1998a, Cosmic ether, Int.J.Theor.Phys. 37, 1121.
Tomaschitz, R.: 1998b, Nonlinear, non-relativistic gravity, Chaos, Solitons & Fractals 9, 1199.
Tomaschitz, R.: 1998c, Ether, luminosity and galactic source counts, Astrophys.Space Sci. 259, 255.
Tomaschitz, R.: 1999a, Cosmic tachyon background radiation, Int.J.Mod.Phys.A 14, 4275.
Tomaschitz, R.: 1999b, Tachyons in the Milne universe, Class.Quant.Grav. 16, 3349.
Tomaschitz, R.: 1999c, Interaction of tachyons with matter, Int.J.Mod.Phys.A 14, 5137.
VandenBerg, D.A., Bolte, M. and Stetson, P.B.: 1996, The age of the galactic globular cluster system, Annu.Rev.Astron.Astrophys. 34, 461.
Varshalovich, D.A. and Potekhin, A.Y.: 1995, Cosmological variability of fundamental physical constants, Space Sci.Rev. 74, 259.
Weinberg, S.: 1972, Gravitation and Cosmology, Wiley, New York.
Whittaker, E.: 1951, A History of the Theories of Aether and Electricity, Vol. 1, Thomas Nelson & Sons, London.
Williams, J.G., Newhall, X.X. and Dickey, J.O.: 1996, Relativity parameters determined from lunar laser ranging, Phys.Rev.D 53, 6730.
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Tomaschitz, R. Cosmic Time Variation of the Gravitational Constant. Astrophysics and Space Science 271, 181–203 (2000). https://doi.org/10.1023/A:1002495020703
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DOI: https://doi.org/10.1023/A:1002495020703