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Hawking radiation by effective two-dimensional theories

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arxiv hep-th/9807123 v1 pith:XTDNSAZH submitted 1998-07-17 hep-th gr-qc

R. Balbinot , A. Fabbri This is my paper · ORCID
classification hep-thgr-qc
keywords effectivehawkingradiationactionsallowsanomalyblackcorrectly
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Recently proposed 2D anomaly induced effective actions for the matter-gravity system are critically reviewed. Their failure to correctly reproduce Hawking's black hole radiation or the stability of Minkowski space-time led us to a modification of the relevant ``quantum'' matter stress energy tensor that allows physically meaningful results to be extracted.

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  1. The fate of Schwarzschild--de Sitter black holes: nonequilibrium evaporation

    hep-th 2025-11 conditional novelty 5.0 of 10

    In the Unruh–de Sitter state the anomaly flux J=(N/48π)(κ_b²−κ_c²) is positive throughout the static patch, so every neutral SdS black hole evaporates monotonically and only the Nariai limit has zero flux.

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