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• W2313290147 abstract "The perturbative solution to the semiclassical Einstein field equations with a positive cosmological constant describing a static and spherically symmetric family of charged black holes for which the temperature of the event horizon equals the temperature of the cosmological horizon is constructed. The source term of the equations is the sum of the stress-energy tensor of the electromagnetic field and the renormalized stress-energy tensor of the quantized spinor and vector fields in a large mass limit, constructed within the framework of the Schwinger-DeWitt method. The main characteristics of the quantum-corrected black holes are calculated and expressed in terms of the horizon radii of the unperturbed problem. It is shown that the quantized fields tend to increase the temperature of the lukewarm black hole. The corrections to the event horizon are always negative, whereas the analogous corrections to the cosmological horizon are always positive. This behavior may be contrasted with that of the scalar field, which strongly depends on the coupling parameter. The renormalized stress-energy tensor of the massive spinor and vector field in general static and spherically symmetric geometry is presented. The related problem of charged black holes in quadratic gravity with a cosmological constant is briefly discussed." @default.
• W2313290147 created "2016-06-24" @default.
• W2313290147 creator A5026706319 @default.
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• W2313290147 date "2012-10-18" @default.
• W2313290147 modified "2023-09-26" @default.
• W2313290147 title "Quantized spinor and vector fields in the spacetime of lukewarm black holes" @default.
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• W2313290147 doi "https://doi.org/10.1103/physrevd.86.084040" @default.
• W2313290147 hasPublicationYear "2012" @default.
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