Nonlocal Astroparticles in Einstein's Universe
| dc.creator | Bulyzhenkov, I. E. | |
| dc.date | 2007-11-04 | |
| dc.date | 2008-10-10 | |
| dc.date.accessioned | 2026-07-07T10:08:36Z | |
| dc.date.available | 2026-07-07T10:08:36Z | |
| dc.description | 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. | |
| dc.description | 9 pages, typos and arguments added | |
| dc.identifier | https://arxiv.org/abs/0711.0549 | |
| dc.identifier | http://arxiv.org/abs/0711.0549 | |
| dc.identifier | doi:10.1007/s10773-007-9559-z | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/171054 | |
| dc.subject | General Physics | |
| dc.title | Nonlocal Astroparticles in Einstein's Universe | |
| dc.type | text |