Full-disk Newtonian integration with parametrized surface density reproduces galactic rotation curves with masses scaled by a factor of ~0.67 relative to conventional dynamical estimates.
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This review summarizes the theory, detection methods, and cosmological applications of gravitationally lensed gravitational waves from astrophysical sources such as compact binary mergers.
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Galactic Rotation Curves from Full-Disk Newtonian Modeling: The Lost and Found Framework
Full-disk Newtonian integration with parametrized surface density reproduces galactic rotation curves with masses scaled by a factor of ~0.67 relative to conventional dynamical estimates.
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Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
This review summarizes the theory, detection methods, and cosmological applications of gravitationally lensed gravitational waves from astrophysical sources such as compact binary mergers.
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