Abstract
Application of recently developed non-Archimedean algebra to a flat and finite universe of total mass M 0 and radius R 0 is described. In this universe, mass m of a body and distance R between two points are bounded from above, i.e., 0≤m≤M 0, 0≤R≤R 0. The universe is characterized by an event horizon at R 0 (there is nothing beyond it, not even space). The radial distance metric is compressed toward horizon, which is shown to cause the phenomenon of red shift. The corresponding modified Minkowski's metric and Lorentz transforms are obtained. Applications to Newtonian gravity shows a weakening at large scales (R→R 0) and a regular behavior as R→0.
Similar content being viewed by others
REFERENCES
K. Avinash, Specul. Sci. Technol. 9, 291 (1986).
V. L. Rvachev, Sov. Phys. Dokl. 36(2), 130 (1991).
P. K. Rashevskii, Usp. Mat. Nauk. 28, 243 (1973).
V. L. Rvachev and A. V. Dabagyan, Sov. Phys. Dokl. 37(10), 497 (1992).
V. L. Rvachev, Sov. Phys. Dokl. 36(12), 803 (1991).
V. F. Kravchenko, V. L. Rvachev, A. N. Shevchenko, and T. I. Sheiko, Radiotekhn. Elektron. 7, 1076_1094 (1995).
G. Bothun, Modern Cosmological Observations and Problems (Taylor 6 Francis, London, 1998).
W. Rindler, Notices Roy. Astron. Soc. 116, 662 (1956).
V. Sabbata and M. Gasperini, Introduction to Gravitation (World Scientific, Singapore, 1985).
E. Harrison, Cosmology__The Science of the Universe (Cambridge University Press, Cambridge, 1981).
H. C. Arp and T. Van Flandern, Phys. Lett. A 164, 263 (1992).
I. E. Segal, J. F. Nicoll, P. Wu, and Z. Zhou, Ap. J. 411, 465 (1993).
V. S. Troitskii, Astrophys. Space Sci. 201, 203 (1993).
E. Milne, Q. J. Math. 5, 64 (1934).
A. Guth, Phys. Rev. D 23, 347 (1981).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Avinash, K., Rvachev, V.L. Non-Archimedean Algebra: Applications to Cosmology and Gravitation. Foundations of Physics 30, 139–152 (2000). https://doi.org/10.1023/A:1003647210704
Issue Date:
DOI: https://doi.org/10.1023/A:1003647210704