Nonlocal Astroparticles in Einstein's Universe
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.
Cite
@article{arxiv.0711.0549,
title = {Nonlocal Astroparticles in Einstein's Universe},
author = {I. E. Bulyzhenkov},
journal= {arXiv preprint arXiv:0711.0549},
year = {2008}
}
Comments
9 pages, typos and arguments added