https://doi.org/10.1140/epjc/s10052-020-08441-6
Regular Article - Theoretical Physics
Constraints on and degeneracies from linear Nash-Greene perturbations in subhorizon scale
Federal University of Latin-American Integration, 85867-970, Foz do Iguaçu, PR, Brazil
Received:
18
June
2020
Accepted:
5
September
2020
Published online:
28
September
2020
Using a joint statistical analysis, we test a four-dimensional FLRW model embedded in a five-dimensional bulk based on the Nash-Greene embedding theorem. Performing a Markov Chain Monte Carlo (MCMC) modelling, we combine observational data sets as those of the recent growth data, the best-fit Planck2018/CDM parameters on the Cosmic Microwave Background (CMB), the Baryon Acoustic Oscillations (BAO) measurements, the Pantheon Supernovae type Ia and the Hubble parameter data. From linear Nash-Greene fluctuations of the metric, we show the related perturbed equations in longitudinal Newtonian gauge to obtain the evolution of growth matter. A mild alleviation may be obtained from the degeneracies on the model parameter analyzing the tension between the growth amplitude factor and the matter content in the plane - on the observations from CMB and Large Scale Structure (LSS) probes. The Akaike Information Criterion (AIC) is also applied and we find a relative statistical consistence of the present model with both CDM and wCDM models lower than 1 of percentage difference at early times on the evolution of the Hubble function H(z). We also apply the Om(z) diagnosis to distinguish the present model from CDM and wCDM models.
© The Author(s) 2020
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