On the non-relativistic Casimir effect

We compute the Casimir energy for a massive scalar field constrained between two parallel planes (Dirichlet boundary conditions) in order to investigate its non-relativistic limit. Instead of employing the usual relativistic dispersion relation omega(p) = <img SRC="http:/img/fbpe/bjp/v31n1/08eq01.gif">, we use the non-relativistic one, omega(p) = p²/2m. It turns out that the Casimir energy is zero. We include the relativistic corrections perturbatively and show that at all orders the Casimir energy remains zero, since each term in the power series in 1/c² is proportional to the Riemann zeta function of a negative even integer. This puzzling result shows that, at least for the free massive scalar field, the Casimir effect is non-perturbative in the relativistic sense.

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Main Authors: Cougo-Pinto,M.V., Farina,C., Mendes,J.F.M., Tort,A.C.
Format: Digital revista
Language:English
Published: Sociedade Brasileira de Física 2001
Online Access:http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332001000100008
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spelling oai:scielo:S0103-973320010001000082002-02-18On the non-relativistic Casimir effectCougo-Pinto,M.V.Farina,C.Mendes,J.F.M.Tort,A.C.We compute the Casimir energy for a massive scalar field constrained between two parallel planes (Dirichlet boundary conditions) in order to investigate its non-relativistic limit. Instead of employing the usual relativistic dispersion relation omega(p) = <img SRC="http:/img/fbpe/bjp/v31n1/08eq01.gif">, we use the non-relativistic one, omega(p) = p²/2m. It turns out that the Casimir energy is zero. We include the relativistic corrections perturbatively and show that at all orders the Casimir energy remains zero, since each term in the power series in 1/c² is proportional to the Riemann zeta function of a negative even integer. This puzzling result shows that, at least for the free massive scalar field, the Casimir effect is non-perturbative in the relativistic sense.info:eu-repo/semantics/openAccessSociedade Brasileira de FísicaBrazilian Journal of Physics v.31 n.1 20012001-03-01info:eu-repo/semantics/articletext/htmlhttp://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332001000100008en10.1590/S0103-97332001000100008
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libraryname SciELO
language English
format Digital
author Cougo-Pinto,M.V.
Farina,C.
Mendes,J.F.M.
Tort,A.C.
spellingShingle Cougo-Pinto,M.V.
Farina,C.
Mendes,J.F.M.
Tort,A.C.
On the non-relativistic Casimir effect
author_facet Cougo-Pinto,M.V.
Farina,C.
Mendes,J.F.M.
Tort,A.C.
author_sort Cougo-Pinto,M.V.
title On the non-relativistic Casimir effect
title_short On the non-relativistic Casimir effect
title_full On the non-relativistic Casimir effect
title_fullStr On the non-relativistic Casimir effect
title_full_unstemmed On the non-relativistic Casimir effect
title_sort on the non-relativistic casimir effect
description We compute the Casimir energy for a massive scalar field constrained between two parallel planes (Dirichlet boundary conditions) in order to investigate its non-relativistic limit. Instead of employing the usual relativistic dispersion relation omega(p) = <img SRC="http:/img/fbpe/bjp/v31n1/08eq01.gif">, we use the non-relativistic one, omega(p) = p²/2m. It turns out that the Casimir energy is zero. We include the relativistic corrections perturbatively and show that at all orders the Casimir energy remains zero, since each term in the power series in 1/c² is proportional to the Riemann zeta function of a negative even integer. This puzzling result shows that, at least for the free massive scalar field, the Casimir effect is non-perturbative in the relativistic sense.
publisher Sociedade Brasileira de Física
publishDate 2001
url http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332001000100008
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