Vacuum polarization of the quantized massive scalar field in the global monopole spacetime II: the renormalized quantum stress energy tensor

Abstract

This paper is devoted to the construction of the renormalized quantum stress energy tensor ${⟨T_{\mu }^{\nu }⟩}_{ren}$ for a massive scalar field with arbitrary coupling to the gravitational field of a pointlike global monopole, using the Schwinger-DeWitt approximation, up to second order in the inverse mass $\mu$ of the field. The given stress energy tensor is constructed by functional differentiation with respect to the metric tensor of the one-loop effective action of sufficiently massive scalar field, such that the Compton length of the quantum field is much less than the characteristic radius of the curvature of the background geometry. The results are obtained for a general curvature coupling parameter $\xi$, and specified to the more physical cases of minimal and conformal coupling, showing that in this specific cases, the quantum massive scalar field in the global monopole spacetime violates all the pointwise energy conditions.

arXiv comment23 pages, 9 figures. arXiv admin note: substantial text overlap with arXiv:1904.02367

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Cited by in corpus (3)

• Bifurcation of the Maxwell quasinormal spectrum on asymptotically anti-de Sitter black holes
• Stress-energy of the quantized fields in the spacetime of the Damour-Solodukhin wormhole
• Vacuum polarization of the quantized massive scalar field in the global monopole spacetime I: the field fluctuation