Universes, Black Holes and Elementary Particles: Difference between revisions
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The divergence in the energy density of zero-point radiation can be removed by addition of self-gravitational potential energy density, provided that the resulting finite energy density closes the universe at radius R. Gravitational renormalization removes also the divergence of the self-energy of the electron. The black hole condition is satisfied at r = R, for both internal and external motion. Extended Newtonian cosmology in flat space-time is valid only with coordinate-dependent units. The equivalent Einstein cosmology (with constant units) is that of de Sitter space-time. Being a black hole, the universe is perfectly isolated from the rest of the cosmos, and is one of an infinity of universes. A universe is to be regarded as an isolated system surrounding any test mass m whose boundary surface adjusts so as to produce at m in the rest frame of m a constant gravitational potential irrespective of the distribution of surrounding matter. | The divergence in the energy density of zero-point radiation can be removed by addition of self-gravitational potential energy density, provided that the resulting finite energy density closes the universe at radius R. Gravitational renormalization removes also the divergence of the self-energy of the electron. The black hole condition is satisfied at r = R, for both internal and external motion. Extended Newtonian cosmology in flat space-time is valid only with coordinate-dependent units. The equivalent Einstein cosmology (with constant units) is that of de Sitter space-time. Being a black hole, the universe is perfectly isolated from the rest of the cosmos, and is one of an infinity of universes. A universe is to be regarded as an isolated system surrounding any test mass m whose boundary surface adjusts so as to produce at m in the rest frame of m a constant gravitational potential irrespective of the distribution of surrounding matter. | ||
[[Category:Scientific Paper]] | [[Category:Scientific Paper|universes black holes elementary particles]] | ||
[[Category:Cosmology]] | [[Category:Cosmology]] | ||
Revision as of 13:36, 1 January 2017
| Scientific Paper | |
|---|---|
| Title | Universes, Black Holes and Elementary Particles |
| Read in full | Link to paper |
| Author(s) | Peter F Browne |
| Keywords | zero-point radiation, cosmology, de Sitter space-time |
| Published | 1994 |
| Journal | Apeiron |
| Volume | 1 |
| No. of pages | 7 |
| Pages | 6-13 |
Read the full paper here
Abstract
The divergence in the energy density of zero-point radiation can be removed by addition of self-gravitational potential energy density, provided that the resulting finite energy density closes the universe at radius R. Gravitational renormalization removes also the divergence of the self-energy of the electron. The black hole condition is satisfied at r = R, for both internal and external motion. Extended Newtonian cosmology in flat space-time is valid only with coordinate-dependent units. The equivalent Einstein cosmology (with constant units) is that of de Sitter space-time. Being a black hole, the universe is perfectly isolated from the rest of the cosmos, and is one of an infinity of universes. A universe is to be regarded as an isolated system surrounding any test mass m whose boundary surface adjusts so as to produce at m in the rest frame of m a constant gravitational potential irrespective of the distribution of surrounding matter.