Dark matter, MOND or non-local gravity?

2009/07/17 by F. Darabi, Darabi, F.
Biochemistry, Genetics and Molecular Biology · Earth and Planetary Sciences · Physics and Astronomy · #Astrophysics of Galaxies (astro-ph.GA) #Cosmology and Gravitation Theories #FOS: Physical sciences #Geomagnetism and Paleomagnetism Studies #Geophysics and Gravity Measurements

paper · pdf · doi:10.48550/arxiv.0907.3028

openalex publication_date 2009/07/17 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We propose a Machian model of gravitational interaction at galactic scales to explain the rotation curves of these large structures without the need for dark matter or MOND.

Related

• Cosmological Difficulties with Modified Newtonian Dynamics (or: La Fin du MOND?)
• Theory MOND in a Friedmann-Robertson-Walker Cosmology as alternative to the Nonbaryonic Dark Matter paradigm
• The Acceleration Scale, Modified Newtonian Dynamics, and Sterile Neutrinos
• A Suggested Alternative to Dark Matter in Galaxies: I. Theoretical Considerations
• A Nonlocal Realization of MOND that Interpolates from Cosmology to Gravitationally Bound Systems