LIGO GW150914 and GW151226 Gravitational Wave Detection and Generalized Gravitation Theory (MOG)
arXiv:1603.05225 · doi:10.1016/j.physletb.2016.10.082
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 and the spin parameter . 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, .
12 pages. No figures. New text and references added. Added text and typo corrected. Version that replicates the published version in Physics Letters B
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- Constraints on Modified Gravity Models from White Dwarfs
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- Polarized image of a rotating black hole in Scalar-Tensor-Vector-Gravity theory
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- Weak cosmic censorship conjecture in Kerr black holes of modified gravity
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- Quasinormal-modes of the Kerr-Newman black hole: GW150914 and fundamental physics implications
- Scalar-tensor black holes in an expanding universe
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- Misaligned Spin Merging Black Holes in Modified Gravity (MOG)
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- Regular Rotating MOG Dark Compact Object
- Terrestrial Sagnac delay in scalar-tensor-vector-gravity
- Dynamics of Dwarf Galaxies in Scalar-Tensor-Vector-Gravity
- The Weak Lensing Mass of Cosmic Web Filaments and Modified Gravity (MOG)
- Relativistic Thermal Emission from Accretion Disks in Kerr-MOG Spacetimes
- The Yilmaz-Rosen and Janis-Newman-Winicour metric solutions in the scalar-Einstein-Gauss-Bonnet gravitational model