Hostname: page-component-78c5997874-xbtfd Total loading time: 0 Render date: 2024-11-12T00:23:46.504Z Has data issue: false hasContentIssue false
  • English
  • Français

Dark energy and dark matter as due to zero point energy

Published online by Cambridge University Press:  26 November 2012

BO LEHNERT
BO LEHNERT*
Affiliation:
Alfvén Laboratory, Royal Institute of Technology, 10044 Stockholm, Sweden (Bo.Lehnert@ee.kth.se)
Get access Rights & Permissions [Opens in a new window]

Abstract

An attempt is made to explain dark energy and dark matter of the expanding universe in terms of the zero point vacuum energy. This analysis is mainly limited to later stages of an observable nearly flat universe. It is based on a revised formulation of the spectral distribution of the zero point energy, for an ensemble in a defined statistical equilibrium having finite total energy density. The steady and dynamic states are studied for a spherical cloud of zero point energy photons. The ‘antigravitational’ force due to its pressure gradient then represents dark energy, and its gravitational force due to the energy density represents dark matter. Four fundamental results come out of the theory. First, the lack of emitted radiation becomes reconcilable with the concepts of dark energy and dark matter. Second, the crucial coincidence problem of equal orders of magnitude of mass density and vacuum energy density cannot be explained by the cosmological constant, but is resolved by the present variable concepts, which originate from the same photon gas balance. Third, the present approach becomes reconcilable with cosmical dimensions and with the radius of the observable universe. Fourth, the deduced acceleration of the expansion agrees with the observed one. In addition, mass polarity of a generalized gravitation law for matter and antimatter is proposed as a source of dark flow.

Type
Papers
Information
Journal of Plasma Physics , Volume 79 , Issue 3 , June 2013 , pp. 327 - 334
Copyright
Copyright © Cambridge University Press 2012 

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Casimir, H. B. G. 1948 On the attraction between two perfectly conducting plates. Proc. Kon. Nederland. Akad. Wetensch. B 51, 793–795.Google Scholar
Crease, R. P. 2007 Critical point dark energy. Phys. World December, 19–22.Google Scholar
Einstein, A. 1950 The Meaning of Relativity. London: Methuen and Co., pp. 86 and 102.Google Scholar
Heitler, W. 1954 The Quantum Theory of Radiation, Oxford: Clarendon Press, pp. 57 and 326.Google Scholar
Hogan, C. J., Kirshner, R. P. and Suntzeff, N. B. 1999 Surveying space-time with supernovae. Sci. Am. January, 28–33.Google Scholar
Kashlinsky, A., Atrio-Barandela, F. and Eberling, H. 2011 Measuring the dark flow with public X-ray cluster data. Astrophys. J. 732, 1–7.CrossRefGoogle Scholar
Kennard, E. H. 1938 Kinetic Theory of Gases, 1st edn. New York, London: McGraw-Hill, Sec. 226.Google Scholar
Lamoreaux, S. K. 1997 Demonstration of the Casimir force in the 0.6 to 6 μ m range. Phys. Rev. Lett. 78, 5–8.CrossRefGoogle Scholar
Lehnert, B. 2009a On dark energy and matter of the expanding universe. Prog. Phys. 2, 77–82.Google Scholar
Lehnert, B. 2009b A possible interpretation of dark energy and matter of the expanding universe. In: AIP Conference Proceedings on New Developments in Nonlinear Plasma Physics (eds. Eliasson, B. and Shukla, P. K.). Melville, New York: American Institute of Physics, pp. 345–355.Google Scholar
Lehnert, B. 2009c, A zero point energy distribution of finite density. Int. Rev. Phys. 3 (6), 304–308.Google Scholar
Lehnert, B. 2010, Problems of the zero point energy distribution. Int. Rev. Phys. 4 (5), 237–242.Google Scholar
Lehnert, B. 2011 The point mass concept. Prog. Phys. 2, 15–19.Google Scholar
Linde, A. 1994 The self-reproducing inflationary universe. Sci. Am. November, 32–39.Google Scholar
Linder, E. and Perlmutter, S. 2007 Dark energy: the decade ahead. Phys. World December, 24–30.Google Scholar
Loudon, R. 2000 The Quantum Theory of Light, 3rd edn. Oxford, UK: Oxford University Press, ch. 1, Sec. 6.12.CrossRefGoogle Scholar
Luminet, J.-P., Starkman, G. D. and Wecks, J. R. 1999 Is space finite? Sci. Am. April, 68–75.Google Scholar
Milonni, P. W. 1994 The Quantum Vacuum. New York: Academic Press Inc.CrossRefGoogle Scholar
Perlmutter, S. 2003 Supernovae, dark energy, and the accelerating universe. Phys. Today April, 53–60.Google Scholar
Riess, A. G. and Turner, M. S. 2004 From slowdown to speedup. Sci. Am. February, 50–55.Google Scholar
Schiff, L. I. 1949 Quantum Mechanics. New York: McGraw-Hill, ch. IV, Sec. 13.Google Scholar
Schmidt, B. 2005 In supernovae as cosmological lighthouses. APS Conf. Series 342, 443.Google Scholar
Terletskii, Ya. P. 1971 Statistical Physics. Amsterdam, London: North-Holland, ch. VI.Google Scholar
Turner, M. S. 2003 Dark energy: just what theorists ordered. Phys. Today April, 10–11.Google Scholar