COSMOLOGICAL BOUNDS ON OPEN FLRW SOLUTIONS OF MASSIVE GRAVITY

被引：0

作者：

Pereira, S. H. ^{[1
,4
]}

Mendonca, E. L. ^{[1
,4
]}

Pinho, A. S. S. ^{[1
,4
]}

Jesus, J. F. ^{[2
,3
]}

机构：

[1] UNESP, Fac Engn Guaratingueta, Guaratingueta, Brazil

[2] UNESP, Campus Expt Itapeva, Itapeva, Brazil

[3] UNESP Univ Estadual Paulista Julio de Mesquita Fi, Campus Expt Itapeva,R Geraldo Alckmin, BR-18409010 Itapeva, SP, Brazil

[4] UNESP Univ Estadual Paulista Julio de Mesquita Fi, Fac Engn Guaratingueta, Dept Fis & Quim, Av Dr Ariberto Pereira da Cunha 333, BR-12516410 Guaratingueta, SP, Brazil

来源：

REVISTA MEXICANA DE ASTRONOMIA Y ASTROFISICA | 2016年 / 52卷 / 01期

关键词：

cosmology: theory; dark energy; dark matter; CONSTRAINTS; SUPERNOVAE;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this work we analysed some cosmological bounds concerning an open FLRW solution of massive gravity. The constraints from recent observational H(z) data are found and the best fit values for the cosmological parameters are in agreement with the Lambda CDM model, and also point to a nearly open spatial curvature, as expected from the model. The graviton mass dependence with the constant parameters alpha(3) and alpha(4), related to the additional lagrangians terms of the model, are also analysed, and we obtain a strong dependence on such parameters, although the condition m(g) similar or equal to H-0(-1) seems dominant for a large range of the parameters alpha(3) and alpha(4).

引用

页码：125 / 131

页数：7

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