Exploration of a possible cumulative action of the zero-point field on intergalactic particles and implications for cosmic rays and a X-ray background from the intergalactic medium.

Details Exploration of a possible cumulative action of the zero-point field on intergalactic particles and implications for cosmic rays and a X-ray background from the intergalactic medium. Exploration of a possible cumulative action of the zero-point field on intergalactic particles and implications for cosmic rays and a X-ray background from the intergalactic medium.

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ncimc...6..523r&link_type=abstract

Nuovo Cimento C, Serie 1, vol. 6C, Sept.-Oct. 1983, p. 523-549. Research supported by the Fondo Colombiano de Investigaciones Ci

Astronomy and Astrophysics

Astronomy

5

Cosmic Rays, Intergalactic Media, Particle Acceleration, Quantum Electrodynamics, X Ray Astronomy, Zero Point Energy, Background Radiation, Big Bang Cosmology, Electromagnetic Fields, Energy Dissipation, Field Theory (Physics), Gamma Rays, Random Walk

Scientific paper

It is argued that electrons either are not accelerated or are accelerated very little by the ZPF (zero-point field) because of zitterbewegung. Protons and nuclei are accelerated but the acceleration is reduced by the uncoupling between effects of the ZPF E and H fields, respectively, associated with the nearly relativistic forced oscillation of their internal components under the ZPF effect. In the very high vacuum of intergalactic space (IGS), cosmic expansion is by far the main dissipation mechanism, determining the shape of the spectrum of ZPF-accelerated particles in th IGS outside superclusters. In addition, it is argued that ZPF acceleration, if it exists, should energize the intergalactic medium (IGM); an X-ray and gamma-ray emitting IGM is expected, though there is no observational evidence for this.

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