
TL;DR
This paper explores the equation of state in cosmological models, showing how the R_h=ct universe constrains the matter density parameter Omega_m to approximately 0.27, explaining its consistency with observations.
Contribution
It demonstrates that the equation of state in the R_h=ct universe explains the specific value of Omega_m in LCDM when fitting observational data.
Findings
The equation of state w=-1/3 in R_h=ct constrains Omega_m to ~0.27.
Forcing LCDM to satisfy a specific equation of state aligns its parameters with R_h=ct predictions.
The measured Hubble radius c/H_0 matches observations only when Omega_m~0.27 under these constraints.
Abstract
The cosmic spacetime is often described in terms of the FRW metric, though the adoption of this elegant and convenient solution to Einstein's equations does not tell us much about the equation of state, p=w rho, in terms of the total energy density rho and pressure p of the cosmic fluid. LCDM and the R_h=ct Universe are both FRW cosmologies that partition rho into (at least) three components, matter rho_m, radiation rho_r, and a poorly understood dark energy rho_de, though the latter goes one step further by also invoking the constraint w=-1/3. This condition is required by the simultaneous application of the Cosmological principle and Weyl's postulate. Model selection tools in one-on-one comparisons favor R_h=ct with a likelihood of ~90% versus only ~10% for LCDM. Nonetheless, the predictions of LCDM often come quite close to those of R_h=ct, suggesting that its parameters are…
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