Pulsar electrodynamics

Details Pulsar electrodynamics Pulsar electrodynamics

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...251..674a&link_type=abstract

Astrophysical Journal, Part 1, vol. 251, Dec. 15, 1981, p. 674-686.

Astronomy and Astrophysics

Astrophysics

9

Electrodynamics, Electromagnetic Fields, Magnetohydrodynamics, Pulsars, Stellar Models, Green'S Functions, Maxwell Equation, Quasi-Steady States, Wave Equations

Scientific paper

It is shown that with the quasi-static constraint ∂/∂t - ω∂/∂φ ≠ 0, there exist no retarded solutions to the inhomogeneous Maxwell's equations for which the electromagnetic fields are nonsingular at the light cylinder r = c/ω, unless at all points of this surface the densities of both electric charge and electric current are zero (ω is a constant angular frequency, c is the speed of light, t is time, and r and φ are the radius and the azimuthal angle in cylindrical coordinates).

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