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Asymptotically flat vacuum solutions in order-reduced semiclassical gravity

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arxiv 2212.09375 v2 pith:MB5BGJHY submitted 2022-12-19 gr-qc hep-th

classification gr-qchep-th
keywords semiclassicalapproximationsolutionsequationsorderrsetfieldorder-reduced
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We investigate the effects of quantum backreaction on the Schwarzschild geometry in the semiclassical approximation. The renormalized stress-energy tensor (RSET) of a scalar field is modelled via an order reduction of the analytical approximation derived by Anderson, Hiscock and Samuel (AHS). As the resulting AHS semiclassical Einstein equations are of fourth-derivative order in the metric, we follow a reduction of order prescription to shrink the space of solutions. Motivated by this prescription, we develop a method that allows to obtain a novel analytic approximation for the RSET that exhibits all the desired properties for a well-posed RSET: conservation, regularity, and correct estimation of vacuum-state contributions. We derive a set of semiclassical equations sourced by the order-reduced AHS-RSET in the Boulware state. We classify the self-consistent solutions to this set of field equations, discuss their main features and address how well they resemble the solutions of the higher-order semiclassical theory. Finally, we establish a comparison with previous results in the literature obtained through the Polyakov approximation for minimally coupled scalar fields.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Macroscopic backreaction of the trace anomaly on classical vacuum backgrounds

    gr-qc 2025-12 conditional novelty 6.0 of 10

    Order-reduced backreaction of the trace-anomaly RSET on Schwarzschild gives a naked singularity without compensatory terms and a wormhole throat with them.

  2. Quantum corrected Einstein-Yang-Mills black holes in semiclassical gravity

    gr-qc 2025-02 conditional novelty 6.0 of 10

    Quantum vacuum backreaction in the Polyakov approximation removes the classical horizon from Einstein-Yang-Mills black holes, replacing it with a wormhole for large horizons and a compact horizonless object for small ones.

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