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Slowly rotating anisotropic relativistic stars

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19630%2F24%3AA0000375" target="_blank" >RIV/47813059:19630/24:A0000375 - isvavai.cz</a>

  • Result on the web

    <a href="https://journals.aps.org/prd/abstract/10.1103/PhysRevD.110.024052" target="_blank" >https://journals.aps.org/prd/abstract/10.1103/PhysRevD.110.024052</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1103/PhysRevD.110.024052" target="_blank" >10.1103/PhysRevD.110.024052</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Slowly rotating anisotropic relativistic stars

  • Original language description

    The present paper is devoted to a study of the equilibrium configurations of slowly rotating anisotropic stars in the framework of general relativity. For that purpose, we provide the equations of structure where the rotation is treated to second order in the angular velocity. These equations extend those first derived by Hartle for slowly rotating isotropic stars. As an application of the new formalism, we study the rotational properties of Bowers-Liang fluid spheres. A result of particular interest is that the ellipticity and mass quadrupole moment are negative for certain highly anisotropic configurations; thus, such systems are prolate rather than oblate. Furthermore, for configurations with high anisotropy and compactness close to their critical value, quantities like the moment of inertia, change of mass, and mass quadrupole moment approach to the corresponding Kerr black hole values, similar to other ultracompact systems like subBuchdahl Schwarzschild stars and analytic rotating gravastars.

  • 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

    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

  • Volume of the periodical

    110

  • Issue of the periodical within the volume

    2

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    27

  • Pages from-to

    „024052-1“-„024052-27“

  • UT code for WoS article

    001277678500021

  • EID of the result in the Scopus database

    2-s2.0-85199539708