Abstract
Any attempt at unification of gravity with quantum physics inevitably leads to the Planck length, usually interpreted as defining the distance scale at which quantum corrections to general relativity are expected to become important. Here we arrive at a scalelength of the same magnitude from the cosmological requirement that gravitating vacuum or zero-point energy does not overdominate the dynamics of the Universe. Other cosmological considerations are again seen to imply such a constraining lower scalelength.
Similar content being viewed by others
References
Klein, O.: 1956,Helv. Phys. Acf. Suppl. 4, 93.
Landau, L. D.: 1955, inNiels Bohr and Development of Physics, McGraw-Hill, New York.
Motz, L.: 1962,Nuovo Cimento 26, 1.
Motz, L.: 1972,Nuovo Cimento 12B, 239.
Pauli, W.: 1956,Helv. Phys. Act. Suppl. 4, 136.
Sakharov, A.: 1968,Soviet Phys. Dokl. 12, 1040.
Sivaram, C.: 1974,Nuovo Cimento Letters 10, 227.
Sivaram, C.: 1982a,Astrophys. Space Sci. 88, 507.
Sivaram, C.: 1982b,Am. J. Phys. 50, 279.
Sivaram, C.: 1983,Am. J. Phys. 51, 277.
Sivaram, C.: 1984a, in De Sabbata (ed.),Relativistic Astrophysics and Cosmology, World Scientific, Singapore, pp. 228–247.
Sivaram, C.: 1984b,Astrophys. Space Sci. 100, 467.
Sivaram, C.: 1986a,Int. J. Theor. Phys. 25, 825.
Sivaram, C.: 1986b, to be published.
Weinberg, S.: 1972,Gravitation and Cosmology, Wiley and Sons, New York.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Sivaram, C. The Planck length as a cosmological constraint. Astrophys Space Sci 127, 133–137 (1986). https://doi.org/10.1007/BF00637768
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00637768