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Modified Newtonian Gravity as an Alternative to the Dark Matter Hypothesis

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Modified Newtonian Gravity as an Alternative to the Dark Matter Hypothesis

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dc.contributor.author Acedo Rodríguez, Luis es_ES
dc.date.accessioned 2018-05-13T04:25:27Z
dc.date.available 2018-05-13T04:25:27Z
dc.date.issued 2017 es_ES
dc.identifier.uri http://hdl.handle.net/10251/101850
dc.description.abstract [EN] The applications of Newtonian dynamics in galactic scales have shown that the inverse square law is incompatible with the amount of visible mass in the form of stars and molecular clouds. This manifests as the rotational curves of galaxies being asymptotically flat instead of decaying with the distance to the center of the galaxy. In the context of Newtonian gravity, the standard explanation requires a huge amount of dark mass in the form of hypothetical particles that still remain undetected. A different theory was provided as a modification of Newtonian dynamics (MOND) at low accelerations. This MOND theory still has many supporters and it can easily explain some features of the rotation curves, such as the Tully-Fisher (TF) phenomenological relation between luminosity and velocity. In this paper, we revisit the third approach of a non-Newtonian force, that has resurfaced from time to time, in order to reconcile it with a finite apparent dark mass and the TF relation. es_ES
dc.language Inglés es_ES
dc.publisher MDPI AG es_ES
dc.relation.ispartof Galaxies es_ES
dc.rights Reconocimiento (by) es_ES
dc.subject Dark matter es_ES
dc.subject Galactic rotation curves es_ES
dc.subject Modified theories of gravity es_ES
dc.subject Tully-Fisher relation es_ES
dc.title Modified Newtonian Gravity as an Alternative to the Dark Matter Hypothesis es_ES
dc.type Artículo es_ES
dc.identifier.doi 10.3390/galaxies5040074 es_ES
dc.rights.accessRights Abierto es_ES
dc.description.bibliographicCitation Acedo Rodríguez, L. (2017). Modified Newtonian Gravity as an Alternative to the Dark Matter Hypothesis. Galaxies. 5(4):1-16. doi:10.3390/galaxies5040074 es_ES
dc.description.accrualMethod S es_ES
dc.relation.publisherversion https://doi.org/10.3390/galaxies5040074 es_ES
dc.description.upvformatpinicio 1 es_ES
dc.description.upvformatpfin 16 es_ES
dc.type.version info:eu-repo/semantics/publishedVersion es_ES
dc.description.volume 5 es_ES
dc.description.issue 4 es_ES
dc.identifier.eissn 2075-4434 es_ES
dc.relation.pasarela S\354926 es_ES


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