A Proposed Model for Capturing Gravitational Spin Anomalies

Details A Proposed Model for Capturing Gravitational Spin Anomalies A Proposed Model for Capturing Gravitational Spin Anomalies

Feb 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..699.1098m&link_type=abstract

SPACE TECHNOLOGY AND APPLICATIONS INTERNAT.FORUM-STAIF 2004: Conf.on Thermophys.in Microgravity; Commercial/Civil Next Gen.Space

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Wave Propagation And Interactions, Black Holes, Other Topics In General Relativity And Gravitation

Scientific paper

During the 2003 STAIF Conference, the author proposed a theory based upon gravitational anomalies, that would use a universal gravitation model with a radial force term coupled with angular momentum. This extended the previous work of Murad and Baker, Dyatlov who explains angular momentum effects as consequences of a `spin' field, and also of Jefimenko. Angular momentum may explain various spin asymmetries allowing the transfer of gravitational radiation directly into angular momentum observed in some anomalous gyroscope experiments; planets orbiting around the sun; moons orbiting larger planetary bodies; and planetary rotation direction. Moreover, a decrease in rotation of a rapidly spinning neutron star may be due to generating gravitational waves as the star loses energy and angular momentum in a tangential direction by changes within its gravitational field. Similarly a coalescing binary black hole ``loses'' up to 12% of its total angular momentum. A High-Frequency Gravitational Wave (HFGW) experiment using a mini-synchrotron could test this proposed theory. Results suggest Jefimenko's cogravity field may represent the elusive `spin' or `torsion' field. The model also indicates gravity strength may increase with the speed of a moving body or spacecraft. Finally, if true, these new effects can have a revolutionary impact upon theoretical physics and Astronautics.

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