Effective theory of quantum black holes

E. Binetti*, M. Del Piano, S. Hohenegger, F. Pezzella, F. Sannino

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    Abstract

    We explore the quantum nature of black holes by introducing an effective framework that takes into account deviations from the classical results. The approach is based on introducing quantum corrections to the classical Schwarzschild geometry in a way that is consistent with the physical scales of the black hole and its classical symmetries. This is achieved by organizing the quantum corrections in inverse powers of a physical distance. By solving the system in a self-consistent way we show that the derived physical quantities, such as event horizons, temperature and entropy can be expressed in a well-defined expansion in the inverse powers of the black hole mass. The approach captures the general form of the quantum corrections to black hole physics without requiring us to commit to a specific model of quantum gravity.

    OriginalsprogEngelsk
    Artikelnummer046006
    TidsskriftPhysical Review D
    Vol/bind106
    Udgave nummer4
    Antal sider15
    ISSN2470-0010
    DOI
    StatusUdgivet - 23. aug. 2022

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    Publisher Copyright:
    © 2022 American Physical Society.

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