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Constraining gravity theories with the gravitational stability mass
The measurement of the size of gravitationally bounded structures is an important test of gravity theories. For a given radius different theories can in fact predict a different gravitational stability mass (GSM) necessary to ensure the stability of the structure in presence of dark energy. We compu...
Autores principales: | Santa Vélez, Camilo, Enea Romano, Antonio |
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Lenguaje: | eng |
Publicado: |
2019
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2020/06/022 http://cds.cern.ch/record/2725291 |
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