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On light surfaces in black hole thermodynamics

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19630%2F22%3AA0000216" target="_blank" >RIV/47813059:19630/22:A0000216 - isvavai.cz</a>

  • Result on the web

    <a href="https://link.springer.com/article/10.1140/epjc/s10052-022-10370-5" target="_blank" >https://link.springer.com/article/10.1140/epjc/s10052-022-10370-5</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1140/epjc/s10052-022-10370-5" target="_blank" >10.1140/epjc/s10052-022-10370-5</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    On light surfaces in black hole thermodynamics

  • Original language description

    We discuss the fundamentals of classical black hole (BH) thermodynamics in a new framework determined by light surfaces and their frequencies. This new approach allows us to study BH transitions inside the Kerr geometry. In the case of BHs, we introduce a new parametrization of the metric in terms of the maximum extractable rotational energy or, correspondingly, the irreducible mass, which is an alternative to the spin parametrization. It turns out that BH spacetimes with spins a/M = root 8/9 and a/M = 1/root 2 show anomalies in the rotational energy extraction and surface gravity whereas the case a/M = root 3/2 is of particular relevance to study the variations of the horizon area. We find the general conditions under which BH transitions can occur and express them in terms of the masses of the initial and final states. This shows that BH transitions in the Kerr geometry are not arbitrary but depend on the relationship between the mass and spin of the initial and final states. From an observational point of view, we argue that near the BH poles it is possible to detect photon orbits with frequencies that characterize the light surfaces analyzed in this work.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2022

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    European Physical Journal C

  • ISSN

    1434-6044

  • e-ISSN

  • Volume of the periodical

    82

  • Issue of the periodical within the volume

    5

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    25

  • Pages from-to

    „456-1“-„456-25“

  • UT code for WoS article

    000797554900001

  • EID of the result in the Scopus database

    2-s2.0-85130278830