Anisotropy of space

Details Anisotropy of space Anisotropy of space

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992jpsj...61.1125m&link_type=abstract

Physical Society of Japan, Journal (ISSN 0031-9015), vol. 61, no. 4, April 1992, p. 1125, 1126.

Statistics

Computation

4

Celestial Mechanics, Milky Way Galaxy, Solar System, Anisotropy, Computational Astrophysics, Metric Space, Relativity

Scientific paper

When a point mass (radiator) is moving with speed v on a circular orbit around another massive point mass (accelerator) at a distance r, the metric seen by an observer far from the accelerator but close by and moving with the radiator, shows space anisotropy. The value of this anisotropy is 10 exp -12 for the sun, accelerated by the center of the Milky Way, and is 4 x 10 exp -16 for earth, accelerated by the sun. Brillet and Hall's experiment, which claims accuracy to 5 x 10 exp -14 for the anisotropy of space, can detect the predicted anisotropy near the sun if the detector is modified properly.

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