Abstract
We show that the approach proposed by Schwinger to compute the Casimir energy at zero temperature in the context of source theory, can be generalized to include temperature effects. We use a regularization prescription based on analytical continuation methods which allows full employment of the Epstein function techniques. This is to be compared with Schwinger's original regularization method by means of the Poisson summation formula.
Similar content being viewed by others
References
Casimir, H. B. G.: Proc. Kon. Nederl. Akad. Wetensch. 51 (1948), 793.
Schwinger, J.: Phys. Rev. 82 (1951), 664.
Schwinger, J.: Lett. Math. Phys. 24 (1992), 59.
Plunien, G., Muller, B., and Greiner, W.: Physica A 145 (1987), 202.
Svaiter, N. F.: Nuovo Cimento A 105 (1992), 959.
Cougo-Pinto, M. V., Farina, C., and Ségui-Santonja, A. J.: Lett. Math. Phys. 30 (1994), 169–171.
Cougo-Pinto, M. V., Farina, C., and Ségui-Santonja, A. J.: Lett. Math. Phys. 31 (1994), 309–313.
Poisson, S. D.: J. École Polytech. 7(19) (1823), 420.
Gradshteijn, I. S. and Ryzhik, I. M.: Tables of Integrals, Series, and Products, Academic Press, New York, London, 1965.
Ambjorn, J. and Wolfram, S.: Ann. of Phys. 147 (1981), 1.
Elizalde, E. and Romeo, A.: Phys. Rev. D 40 (1989), 436.
Kirsten, K.: J. Math. Phys. 35 (1994), 459.
Elizalde, E. and Romeo, A.: Internat. J. Phys. A 7 (1992), 7365.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Cougo-Pinto, M.V., Farina, C. & Tort, A. Schwinger's formula for the Casimir effect at finite temperature. Letters in Mathematical Physics 37, 159–165 (1996). https://doi.org/10.1007/BF00416018
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00416018