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Mixed scalarization of charged black holes: From spontaneous to nonlinear scalarization

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F24%3A00597877" target="_blank" >RIV/68378271:_____/24:00597877 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1103/PhysRevD.110.044014" target="_blank" >https://doi.org/10.1103/PhysRevD.110.044014</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1103/PhysRevD.110.044014" target="_blank" >10.1103/PhysRevD.110.044014</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Mixed scalarization of charged black holes: From spontaneous to nonlinear scalarization

  • Original language description

    Scalarized black holes (BH) have been shown to form dynamically in extended-scalar-tensor theories, either through spontaneous scalarization-when the BH is unstable against linear perturbations-or through a nonlinear scalarization. In the latter, linearly stable BHs can ignite scalarization when sufficiently perturbed. These phenomena are, however, not incompatible and mixed scalarization is also possible. explore two aspects of the Einstein-Maxwell-scalar model: solutions containing, simultaneously, linear (also known as standard) and nonlinear scalarization and the effects of having one of the coupling constants with an "opposite sign" to the one leading to scalarization. Both points are addressed constructing and examining the mixed scalarization's domain of existence. An overall dominance of spontaneous scalarization over the nonlinear scalarization is observed. Thermodynamically, an entropical preference for mixed over the standard scalarization (spontaneous or nonlinear) exists. In the presence counter scalarization, a quench of the scalarization occurs, mimicking the effect of a scalar particle's mass/ positive self-interaction term.

  • 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

    <a href="/en/project/GM21-16583M" target="_blank" >GM21-16583M: New avenues in the hunt for dark energy</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2024

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Physical Review D

  • ISSN

    2470-0010

  • e-ISSN

    2470-0029

  • Volume of the periodical

    110

  • Issue of the periodical within the volume

    4

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    11

  • Pages from-to

    044014

  • UT code for WoS article

    001292742700015

  • EID of the result in the Scopus database

    2-s2.0-85200499322