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LIGO GW150914 and GW151226 Gravitational Wave Detection and Generalized Gravitation Theory (MOG)
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abstract
The nature of gravitational waves in a generalized gravitation theory is investigated. The linearized field equations and the metric tensor quadrupole moment power and the decrease in radius of an inspiralling binary system of two compact objects are derived. The generalized Kerr metric describing a spinning black hole is determined by its mass $M$ and the spin parameter $a=cS/GM^2$. The LIGO-Virgo collaboration data is fitted with smaller binary black hole masses in agreement with the current electromagnetic, observed X-ray binary upper bound for a black hole mass, $M\lesssim 10M_\odot$.
Forward citations
Cited by 2 Pith papers
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Breathing Black Hole Shadows in Modified Gravity (MOG)
In MOG gravity, gravitational waves would make a black hole's shadow breathe in area and then wobble translationally after a time delay, signatures absent in general relativity.
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Regular Rotating Black Hole: Probing the boundaries of the Radiative Signatures and Jet Power
MOG regular rotating black holes are compatible with most X-ray binary data only for beta below about 0.38 to 0.4, and are excluded for the near-extremal source GRS 1915+105.
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