A Non-Standard Relativistic Approach for Simulating Disk Galaxies: Quasi-Particles with Reduced Relativistic Properties v < v(max) < c Fit Rotation Curves of Disk Galaxies
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Medimops DE
A Non-Standard Relativistic Approach for Simulating Disk Galaxies: Quasi-Particles with Reduced Relativistic Properties v < v(max) < c Fit Rotation Curves of Disk Galaxies
Medimops DE
24-08-2026 09:57:58
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