Spacetime Torque as a Universal Parameter for Cosmogenesis: Difference between revisions
Imported from text file |
Fill in keywords from the wiki's abstract records |
||
| (One intermediate revision by the same user not shown) | |||
| Line 2: | Line 2: | ||
| title = Spacetime Torque as a Universal Parameter for Cosmogenesis | | title = Spacetime Torque as a Universal Parameter for Cosmogenesis | ||
| author = [[Nassim Haramein]], [[Elizabeth A Rauscher]] | | author = [[Nassim Haramein]], [[Elizabeth A Rauscher]] | ||
| keywords = angular momentum, dark matter, Dark Energy, black hole | |||
| published = 2008 | | published = 2008 | ||
}} | }} | ||
Latest revision as of 07:29, 21 July 2026
| Scientific Paper | |
|---|---|
| Title | Spacetime Torque as a Universal Parameter for Cosmogenesis |
| Author(s) | Nassim Haramein, Elizabeth A Rauscher |
| Keywords | angular momentum, dark matter, Dark Energy, black hole |
| Published | 2008 |
Abstract
We present a first order approximation scaling law for all organized matter in which spacetime torque is computed and plotted against the radius of the system utilizing the Haramein-Rauscher metric approach. The scaling law approximates the torque necessary to produce the angular momentum of a system from atomic structure to astrophysical objects such as stars, galaxies and the universe. Further we demonstrate that the 1.3 Fermi proton data point can be treated as the horizon of a mini black hole giving a semi-classical solution correctly predicting the measured value of the nucleonic emission. Dark matter and dark energy are discussed in the context of these findings as well as the source of the anomalous magnetic and angular moment.