Vacuum polarization induced by a cylindrical boundary in the cosmic string spacetime

E. R. Bezerra de Mello, V. B. Bezerra, A. A. Saharian, and A. S. Tarloyan
Phys. Rev. D 74, 025017 – Published 24 July 2006

Abstract

In this paper we investigate the Wightman function, the renormalized vacuum expectation values of the field square, and the energy-momentum tensor for a massive scalar field with general curvature coupling inside and outside of a cylindrical shell in the generalized spacetime of straight cosmic string. For the general case of Robin boundary condition, by using the generalized Abel-Plana formula, the vacuum expectation values are presented in the form of the sum of boundary-free and boundary-induced parts. The asymptotic behavior of the vacuum expectation values of the field square, energy density, and stresses are investigated in various limiting cases. The generalization of the results to the exterior region is given for a general cylindrically symmetric static model of the string core with finite support.

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  • Received 29 May 2006

DOI:https://doi.org/10.1103/PhysRevD.74.025017

©2006 American Physical Society

Authors & Affiliations

E. R. Bezerra de Mello1,*, V. B. Bezerra1,†, A. A. Saharian1,2,‡, and A. S. Tarloyan2

  • 1Departamento de Física, Universidade Federal da Paraíba, 58.059-970, Caixa Postal 5.008, João Pessoa, PB, Brazil
  • 2Department of Physics, Yerevan State University, 375025 Yerevan, Armenia

  • *Electronic address: emello@fisica.ufpb.br
  • Electronic address: valdir@fisica.ufpb.br
  • Electronic address: saharyan@server.physdep.r.am

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Issue

Vol. 74, Iss. 2 — 15 July 2006

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