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• W3100138417 abstract "A gravitational field model based on two symmetric tensors, $g_{mu nu}$ and $tilde{g}_{mu nu}$, is studied, using a Markov Chain Monte Carlo (MCMC) analysis with the most updated catalog of SN-Ia. In this model, new matter fields are added to the original matter fields, motivated by an additional symmetry ($tilde{delta}$~symmetry). We call them $tilde{delta}$ matter fields. This theory predicts an accelerating Universe without the need to introduce a cosmological constant $Lambda$ by hand in the equations. We obtained a very good fit to the SN-Ia Data, and with this, we found the two free parameters of the theory called $C$ and $L_2$. With these values, we have fixed all the degrees of freedom in the model. The last $H_0$ local value measurement is in tension with the CMB Data from Planck. Based on an absolute magnitude $M_V = -19.23$ for the SN, Delta Gravity finds $H_0$ to be $74.47pm 1.63$ km/(s Mpc). This value is in concordance with the last measurement of the $H_0$ local value, $73.83pm 1.48$ km/(s Mpc)." @default.
• W3100138417 created "2020-11-23" @default.
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• W3100138417 date "2019-02-01" @default.
• W3100138417 modified "2023-09-26" @default.
• W3100138417 title "An Accelerating Universe without Lambda: Delta Gravity Using Monte Carlo" @default.
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• W3100138417 doi "https://doi.org/10.3390/universe5020051" @default.
• W3100138417 hasPublicationYear "2019" @default.
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