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Descripción de materia oscura por soluciones exactas de relatividad general

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 2012 Argentina Spanish; Castilian Publisher:Asociación Física Argentina
Authors: Gallo, Emanuel; Geser, Federico Alejandro; Moreschi, Osvaldo Mario;

handle: 11336/26103 , 20.500.12110/afa_v24_n02_p136

Descripción de materia oscura por soluciones exactas de relatividad general

Abstract

We present a solution of the Einstein equations with spherical symmetry which represents the mass dynamically estimated of dark matter and fit several associated observational data of dark matter phenomena

Presentamos una solución a las ecuaciones de Einstein con simetría esférica que representa la masa estimada dinámicamente y ajusta los datos observacionales de los fenómenos de la materia oscura.

Fil: Geser, Federico Alejandro. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física (UNC-FaMAF). Córdoba. Argentina

Fil: Moreschi, Osvaldo Mario. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física (UNC-FaMAF). Córdoba. Argentina

Fil: Gallo, Emanuel. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física (UNC-FaMAF). Córdoba. Argentina

Country
Argentina
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Keywords

MATERIA OSCURA, SOLUCIONES EXACTAS, RELATIVIDAD GENERAL, DARK MATTER, https://purl.org/becyt/ford/1.3, LENTES GRAVITACIONALES, https://purl.org/becyt/ford/1, 530, GENERAL RELATIVITY

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
Green