TY - JOUR
T1 - Equilibrium solutions of relativistic rotating stars with mixed poloidal and toroidal magnetic fields
AU - Uryu, Koji
AU - Gourgoulhon, Eric
AU - Markakis, Charalampos M.
AU - Fujisawa, Kotaro
AU - Tsokaros, Antonios
AU - Eriguchi, Yoshiharu
PY - 2014/11/7
Y1 - 2014/11/7
N2 - 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.
AB - 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.
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U2 - 10.1103/PhysRevD.90.101501
DO - 10.1103/PhysRevD.90.101501
M3 - Article
AN - SCOPUS:84911940209
SN - 1550-7998
VL - 90
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 10
M1 - 101501
ER -