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CASIMIR ENERGY IN A CURVED BACKGROUND WITH A SPHERICAL BOUNDARY - AN EXACTLY SOLVABLE CASE
Date
1993-09-15
Author
BAYIN, SS
OZCAN, M
Metadata
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We reconsider the Casimir effect for the massless conformal scalar field in a ''half Einstein universe.'' This case is interesting in that it could be solved analytically by several different methods. Thus, it allows us to compare and understand effects of different approaches. We first calculate the renormalized vacuum energy by using the mode sum method and study the effects of different cutoff functions. Next, we calculate the renormalized vacuum energy-momentum tensor by using the covariant point-splitting method. We construct the Green's functions by using the eigenfunctions, which are obtained by solving the wave equation with the appropriate boundary conditions (Dirichlet and Neumann). We discuss further properties of this case as well as its relation to previous calculations.
Subject Keywords
Zero-point energy
,
Stress
URI
https://hdl.handle.net/11511/64507
Journal
PHYSICAL REVIEW D
DOI
https://doi.org/10.1103/physrevd.48.2806
Collections
Department of Physics, Article
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CASIMIR EFFECT IN A HALF EINSTEIN UNIVERSE - AN EXACTLY SOLVABLE CASE IN CURVED BACKGROUND AND WITH A SPHERICAL BOUNDARY
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S. BAYIN and M. OZCAN, “CASIMIR ENERGY IN A CURVED BACKGROUND WITH A SPHERICAL BOUNDARY - AN EXACTLY SOLVABLE CASE,”
PHYSICAL REVIEW D
, pp. 2806–2812, 1993, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/64507.