On the Magnetosphere of an Accelerated Pulsar
arXiv:1311.0752 · doi:10.1103/PhysRevD.89.103013
Abstract
We report on a remarkable class of exact solutions to force-free electrodynamics that has four-current along the light cones of an arbitrary timelike worldline in flat spacetime. No symmetry is assumed, and the solutions are given in terms of a free function of three variables. The field configuration should describe the outer magnetosphere of a pulsar moving on the worldline. The power radiated is the sum of an acceleration (Larmor-type) term and a pulsar-type term.
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References in corpus (4)
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- Linking electromagnetic and gravitational radiation in coalescing binary neutron stars
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- Conservation laws and evolution schemes in geodesic, hydrodynamic and magnetohydrodynamic flows
- Stability of exact force-free electrodynamic solutions and scattering from spacetime curvature
- Nonaxisymmetric Poynting Jets
- Crystals of gauged solitons, force free plasma and resurgence
- Metric-independence of vacuum and force-free electromagnetic fields
- Plasma Waves and Jets from Moving Conductors