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

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

Oct 14, 2014

7 pages

Published in:

Phys.Rev.D 90 (2014) 10, 101501

Published: Nov 7, 2014

e-Print:

1410.3913 [astro-ph.HE]

DOI:

10.1103/PhysRevD.90.101501

Report number:

DPUR-TH-42

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Abstract: (APS)

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.

Note:

7 pages, to appear in PRD rapid communication

04.40.Dg
04.20.-q
04.25.D-
04.40.Nr

References(61)

Figures(3)

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