Authors: Jaroslav Hynecek
The detail analysis of Gravitational Waves waveforms detected by LIGO observatory shows that the waves could not have been generated by colliding Black Holes. Most likely they were generated by colliding collapsed stars (“gravistars’ or “collapstars”, G-stars for short), which do not have Event Horizons. This is shown by using a simple model of a Sun mass G-star orbiting a G-star with a mass of 100 Suns. The evaluation is based on the comparison of two different metrics, the Schwarzschild metric, and the new metric derived by the author earlier, which provide the orbital frequencies as functions of a distance from the main G-star center.
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[v1] 2016-06-19 18:38:28
[v2] 2016-06-21 14:31:02
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