arXiv (All)
open access
The modified Newtonian dynamics with an extra anti-dissipation term can yield the MOND model
In this work, we introduced a positive viscosity coefficient into Newtonian dynamics to explore the rotational properties of disk galaxies. Our results show that the rotational behaviors of disk galaxies predicted by this modified Newtonian dynamics share notable similarities with those from the wel
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Bower Reservoir Relation: Newtonian Disk Structure Predicts the Residual Speed Gas Fraction Trend in Disk Galaxies#478478
- Fractal structures and the large scale distribution of galaxies#639463
- Is MOND an Emergent Effective Law of a Complex Dark Matter Sector?#1077423
- Fractional-Dimension Gravity and the Milky Way Galaxy#1155249
- Galaxy-SMBH co-evolution in 2,435 DESI disk galaxies and merger-free BH growth in bulgeless disks#1037117
Record · ID 984420
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive