Acceleration of pulsars by asymmetric radiation. II - Theoretical generalizations and discussions

Details Acceleration of pulsars by asymmetric radiation. II - Theoretical generalizations and discussions Acceleration of pulsars by asymmetric radiation. II - Theoretical generalizations and discussions

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...209..245t&link_type=abstract

Astrophysical Journal, vol. 209, Oct. 1, 1976, pt. 1, p. 245-251

Astronomy and Astrophysics

Astrophysics

4

Dipole Moments, Pulsars, Radiation Distribution, Relativistic Effects, Stellar Rotation, Angular Distribution, Astrodynamics, Asymmetry, Electric Dipoles, Light Speed, Magnetic Dipoles, Stellar Radiation

Scientific paper

This paper derives the asymmetric emission of low-frequency electromagnetic radiation from pulsars with asymmetrical magnetization and polarization. In particular, rotating stars with asymmetrically displaced magnetic and/or electric dipole moments are found to radiate asymmetrically and therefore experience a reaction force. The nature of asymmetric radiation is investigated further and is shown to be a direct result of the Einstein definition of simultaneity (owing to the finite speed of light).

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