A Covariant Viscoelastic Spacetime Origin of the Galactic Acceleration Relation
Fuente:
Zenodo
Salvato in:
| Autore principale: | |
|---|---|
| Natura: | Recurso digital |
| Lingua: | inglese |
| Pubblicazione: |
Zenodo
2026
|
| Soggetti: | |
| Accesso online: | |
| Tags: |
Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!
|
| _version_ | 1866901527525851136 |
|---|---|
| author | Kim, Chang-sik |
| author_facet | Kim, Chang-sik |
| contents | <p>This record is a duplicate created during a versioning error.<br>For the latest and official version of this research (v30 and beyond),<br>please refer to the following permanent<br>link: <strong><a href="https://www.google.com/search?q=https://doi.org/10.5281/zenodo.18911689" target="_blank" rel="noopener">https://doi.org/10.5281/zenodo.18911689</a></strong><br><br><br>This work proposes a covariant viscoelastic spacetime framework<br>in which spacetime possesses a finite relaxation time determined<br>by cosmological expansion.</p> <p>The theory predicts a characteristic acceleration scale</p> <p>a_mem = κ c H0 / (2π)</p> <p>which naturally explains the radial acceleration relation (RAR),<br>flat galaxy rotation curves, and the baryonic Tully–Fisher relation.</p> <p>The model is tested using the SPARC galaxy database.</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_18959153 |
| institution | Zenodo |
| language | eng |
| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | A Covariant Viscoelastic Spacetime Origin of the Galactic Acceleration Relation Kim, Chang-sik modified gravity viscoelastic spacetime gravitational memory radial acceleration relation galaxy rotation curves baryonic Tully–Fisher relation cosmology covariant field theory <p>This record is a duplicate created during a versioning error.<br>For the latest and official version of this research (v30 and beyond),<br>please refer to the following permanent<br>link: <strong><a href="https://www.google.com/search?q=https://doi.org/10.5281/zenodo.18911689" target="_blank" rel="noopener">https://doi.org/10.5281/zenodo.18911689</a></strong><br><br><br>This work proposes a covariant viscoelastic spacetime framework<br>in which spacetime possesses a finite relaxation time determined<br>by cosmological expansion.</p> <p>The theory predicts a characteristic acceleration scale</p> <p>a_mem = κ c H0 / (2π)</p> <p>which naturally explains the radial acceleration relation (RAR),<br>flat galaxy rotation curves, and the baryonic Tully–Fisher relation.</p> <p>The model is tested using the SPARC galaxy database.</p> |
| title | A Covariant Viscoelastic Spacetime Origin of the Galactic Acceleration Relation |
| topic | modified gravity viscoelastic spacetime gravitational memory radial acceleration relation galaxy rotation curves baryonic Tully–Fisher relation cosmology covariant field theory |
| url | https://doi.org/10.5281/zenodo.18959153 |