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Abstract
We establish new constraints on f(T) gravity models by using cosmological data. In particular, we investigate the restrictions given by the gas mass fraction measurements of galaxy clusters and transversal BAO data. Both data sets are regarded as weakly dependent on a fiducial cosmology. In addition, we also include a CMB measurement of the temperature power spectrum first peak, along with H(z) values from cosmic chronometers and supernovae data from the Pantheon data set. We also perform a forecast for future constraints on the deviation of f(T) models from the
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1 Universidade Federal do Rio Grande do Norte, Departamento de Física, Natal, Brazil (GRID:grid.411233.6) (ISNI:0000 0000 9687 399X)
2 Universidade Federal de Sergipe, Departamento de Física, Aracaju, Brazil (GRID:grid.411252.1) (ISNI:0000 0001 2285 6801)
3 Universidade Federal do Rio Grande do Norte, Departamento de Física, Natal, Brazil (GRID:grid.411233.6) (ISNI:0000 0000 9687 399X); Universidade do Estado do Rio Grande do Norte, Departamento de Física, Mossoró, Brazil (GRID:grid.440576.4) (ISNI:0000 0001 0449 6953)