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arXiv · 0711.0549

Nonlocal Astroparticles in Einstein's Universe

I. E. Bulyzhenkov
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Abstract

Gravitational probes should maintain spatial flatness for Einsten-Infeld-Hoffmann dynamics of relativistic matter-energy. The continuous elementary source/particle in Einstein's gravitational theory is the r^{-4} radial energy density rather than the delta-operator density in empty-space gravitation. The space energy integral of such an infinite (astro)particle is finite and determines its nonlocal gravitational charge for the energy-to-energy attraction of other nonlocal (astro)particles. The non-empty flat space of the undivided material Universe is charged continuously by the world energy density of the global ensemble of overlapping radial particles. Nonlocal gravitational/inertial energy-charges incorporate Machian relativism quantitatively into Einstein's gravitation for self-contained SR-GR dynamics without references on Newton's mass-to-mass attraction.

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BibTeXRIS

I. E. Bulyzhenkov. 2008-10-10. Nonlocal Astroparticles in Einstein's Universe. https://doi.org/10.1007/s10773-007-9559-z

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