Newtonian limit of scalar-tensor theories and galactic dynamics: isolated and interacting galaxies
We use the Newtonian limit of a general scalar-tensor theory around a background field to study astrophysical effects. The gravitationaltheory modifies the standard Newtonian potential by adding a Yukawa term to it, which is quantified by two theoretical parameters: ¸, thelenghtscale of the gravitat...
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| Pubblicato in: | Revista Mexicana de Física |
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| Autori principali: | , , , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Sociedad Mexicana de Física A.C.
2007
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57066405 https://www.redalyc.org/journal/570/57066405/ https://www.redalyc.org/journal/570/57066405/html/ https://www.redalyc.org/journal/570/57066405/57066405.epub https://www.redalyc.org/journal/570/57066405/movil |
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