Electromagnetically-Induced Frame-Dragging around Astrophysical Objects
arXiv:1504.01763 · doi:10.1103/PhysRevD.91.124047
Abstract
Frame dragging (Lense-Thirring effect) is generally associated with rotating astrophysical objects. However, it can also be generated by electromagnetic fields if electric and magnetic fields are simultaneously present. In most models of astrophysical objects, macroscopic charge neutrality is assumed and the entire electromagnetic field is characterized in terms of a magnetic dipole component. Hence, the purely electromagnetic contribution to the frame dragging vanishes. However, strange stars may posses independent electric dipole and neutron stars independent electric quadrupole moments that may lead to the presence of purely electromagnetic contributions to the frame dragging. Moreover, recent observations have shown that in stars with strong electromagnetic fields, the magnetic quadrupole may have a significant contribution to the dynamics of stellar processes. As an attempt to characterized and quantify the effect of electromagnetic frame-dragging in this kind of astrophysical objects, an analytic solution to the Einstein-Maxwell equations is constructed here on the basis that the electromagnetic field is generated by the combination of arbitrary magnetic and electric dipoles plus arbitrary magnetic and electric quadrupole moments. The effect of each multipole contribution on the vorticity scalar and the Poynting vector is described in detail. Corrections on important quantities such the innermost stable circular orbit (ISCO) and the epyciclic frequencies are also considered.
12 pages, 7 figures
References in corpus (11)
- Gravity Probe B: Final Results of a Space Experiment to Test General Relativity
- The strongest cosmic magnets: Soft Gamma-ray Repeaters and Anomalous X-ray Pulsars
- The surprising magnetic topology of tauSco: fossil remnant or dynamo output?
- A Metric for Rapidly Spinning Black Holes Suitable for Strong-Field Tests of the No-Hair Theorem
- Magnetic fields and accretion flows on the classical T Tauri star V2129 Oph
- The fraction of DA white dwarfs with kilo-Gauss magnetic fields
- Realistic Exact Solution for the Exterior Field of a Rotating Neutron Star
- A stationary q-metric
- Equatorial symmetry/antisymmetry of stationary axisymmetric electrovac spacetimes
- Oblique magnetic fields and the role of frame dragging near rotating black hole
- Poynting vector in stationary axisymmetric electrovacuum spacetimes reexamined
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