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...

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Veröffentlicht in:	Journal of cosmology and astroparticle physics 2020-06, Vol.2020 (6), p.22-22
Hauptverfasser:	Vélez, Camilo Santa, Romano, Antonio Enea
Format:	Artikel
Sprache:	eng
Schlagworte:	Dark energy Galactic clusters Galaxies Gravitation theory Gravity Lower bounds Relativity Structural stability Tensors Theory of relativity
Online-Zugang:	Volltext
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