Abstract
The vacuum energy density is calculated for all topologically nonequivalent configurations of massive scalar and spinor fields in space-times with topology (S1)2 × R2 and planar metric.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
Literature cited
A. A. Grib, S. G. Mamaev, and V. M. Mostepanenko, Quantum Effects in Intense External Fields [in Russian], Atomizdat, Moscow (1980).
C. J. Isham, Proc. R. Soc. Lond.,A362, 383 (1978).
C. J. Isham, Proc. R. Soc. Lond.,A364, 591 (1978).
B. S. DeWitt, C. F. Hart, and C. J. Isham, Physica,96A, 197 (1979).
G. Kennedy, Phys. Rev.,D23, 2884 (1981).
G. F. R. Ellis, Gen. Rel. Grav.,2, 7 (1971).
S. J. Avis and G. J. Isham, Proc. R. Soc. Lond.,A363, 581 (1978).
L. H. Ford, Phys. Rev.,D21, 933 (1980).
E. M. Stein and G. Weiss, Introduction to Fourier Analysis on Euclidean Spaces, Princeton University Press (1971).
Author information
Authors and Affiliations
Additional information
Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 9, pp. 27–30, September, 1982.
In conclusion the author is grateful to A. B. Venkov and L. A. Takhtadzhyan for discussing summation equations.
Rights and permissions
About this article
Cite this article
Goncharov, Y.P. Casimir effect in multiply connected space-time. Massive fields. Soviet Physics Journal 25, 791–794 (1982). https://doi.org/10.1007/BF00892390
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00892390