Equilibrium solutions of relativistic rotating stars with mixed poloidal and toroidal magnetic fields

Koji Uryu, Eric Gourgoulhon, Charalampos M. Markakis, Kotaro Fujisawa, Antonios Tsokaros, Yoshiharu Eriguchi

    研究成果: Article査読

    16 被引用数 (Scopus)

    抄録

    Stationary and axisymmetric solutions of relativistic rotating stars with strong mixed poloidal and toroidal magnetic fields are obtained numerically. Because of the mixed components of the magnetic field, the underlying stationary and axisymmetric spacetimes are no longer circular. These configurations are computed from the full set of the Einstein-Maxwell equations, Maxwell's equations, and from first integrals and integrability conditions of the magnetohydrodynamic equilibrium equations. After a brief introduction of the formulation of the problem, we present the first results for highly deformed magnetized rotating compact stars.

    本文言語English
    論文番号101501
    ジャーナルPhysical Review D - Particles, Fields, Gravitation and Cosmology
    90
    10
    DOI
    出版ステータスPublished - 2014 11 7

    ASJC Scopus subject areas

    • 核物理学および高エネルギー物理学

    フィンガープリント

    「Equilibrium solutions of relativistic rotating stars with mixed poloidal and toroidal magnetic fields」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。

    引用スタイル