Pulsar Geometrodynamics: The Classical and Quantum Structure of the Stars

Details Pulsar Geometrodynamics: The Classical and Quantum Structure of the Stars Pulsar Geometrodynamics: The Classical and Quantum Structure of the Stars

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ap%26ss.272..263d&link_type=abstract

Astrophysics and Space Science, v. 272, Issue 1/3, p. 263-274 (2000).

Astronomy and Astrophysics

Astrophysics

Scientific paper

Franz Kahn's ideas on pulsar magnetospheres are exposed. Charged particle motion close and beyond the speed of light cylinder might explain hard gamma-ray radiation, and creates current density distributions producing radio frequency superluminal beaming, and shaping the structure of the magnetospheric electromagnetic field. A quasi-classical (stochastic) description of motion, related with the incoherent nature of gamma-ray radiation, replaces the classical (deterministic) description. Future studies involve vacuum electrodynamics.

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