Mass Damping Theory
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Mass Damping Theory (MDT) is a speculative framework in theoretical physics proposing that gravity arises not solely from spacetime curvature but from the damping of spacetime's inherent vibratory nature by mass. It seeks to explain gravitational anomalies traditionally attributed to dark matter and dark energy without invoking unseen particles.
Core Tenets
- Spacetime is a vibratory medium.
- Mass damps the local vibrational modes of spacetime.
- Damped spacetime behaves as if it exerts stronger gravity.
- Mass damping effects emerge predominantly in regions where General Relativity is weak.
Implications
- Explains why low-density galaxies exhibit greater gravitational discrepancies than high-density ones.[1][2][3][4][5]
- Predicts enhanced effective gravity in diffuse systems without requiring dark matter.[6][7]
- Suggests that cosmic acceleration may result from reduced damping as the universe becomes less dense.[8]
- Reinterprets gravitational lensing and galactic rotation curves through vibrational interaction rather than missing mass.
References
- ↑ Bullock, James S.; Boylan-Kolchin, Michael (2017). "Small-Scale Challenges to the ΛCDM Paradigm". Annual Review of Astronomy and Astrophysics. 55 (1): 343–387. arXiv:1707.04256. Bibcode:2017ARA&A..55..343B. doi:10.1146/annurev-astro-091916-055313.
- ↑ Di Cintio, Arianna; Brook, Chris B.; Dutton, Aaron A.; Macciò, Andrea V.; Obreja, Aura; Domínguez-Tenreiro, Rosa (2017). "NIHAO XVIII: The Diversity of Dwarf Galaxy Rotation Curves". Monthly Notices of the Royal Astronomical Society: Letters. 466 (1): L1–L5. arXiv:1608.01327. Bibcode:2017MNRAS.466L...1D. doi:10.1093/mnrasl/slw210.
- ↑ Papastergis, Evangelos; Cattaneo, Andrea; Huang, Shan; Giovanelli, Riccardo; Haynes, Martha P. (2012). "A direct measurement of the baryonic mass function of galaxies and implications for the galactic baryon fraction". The Astrophysical Journal. 759 (2): 138. arXiv:1208.5229. Bibcode:2012ApJ...759..138P. doi:10.1088/0004-637X/759/2/138.
- ↑ McGaugh, Stacy S.; Rubin, Vera C.; de Blok, W. J. G. (2001). "High-Resolution Rotation Curves of Low Surface Brightness Galaxies. II. Mass Models". The Astronomical Journal. 122 (5): 2381–2395. arXiv:astro-ph/0107326. Bibcode:2001AJ....122.2381M. doi:10.1086/323448.
- ↑ Oh, Se-Heon; de Blok, W. J. G.; Brinks, Elias; Walter, Fabian; Kennicutt, Robert C. (2011). "Dark and Luminous Matter in THINGS Dwarf Galaxies". The Astronomical Journal. 141 (6): 193. arXiv:1011.0899. Bibcode:2011AJ....141..193O. doi:10.1088/0004-6256/141/6/193.
- ↑ Milgrom, M. (1983). "A modification of the Newtonian dynamics as a possible alternative to the hidden mass hypothesis". The Astrophysical Journal. 270: 365–370. Bibcode:1983ApJ...270..365M. doi:10.1086/161130.
- ↑ Famaey, Benoit; McGaugh, Stacy (2012). "Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions". Living Reviews in Relativity. 15 (10). arXiv:1112.3960. Bibcode:2012LRR....15...10F. doi:10.12942/lrr-2012-10. PMC 5255531. PMID 28163623. Unknown parameter
|article-number=ignored (help) - ↑ Trippe, Sebastian (2014). "Toward a Resolution of the Dark Matter Problem by Modified Gravity". Journal of Korean Astronomical Society. 47 (1): 15–33. arXiv:1401.1911. Bibcode:2014JKAS...47...15T. doi:10.5303/JKAS.2014.47.1.15.
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