On Recent Claims Concerning the R_h=ct Universe
Fulvio Melia

TL;DR
The paper defends the R_h=ct cosmological model against recent criticisms, demonstrating its consistency with observations and addressing misconceptions about its theoretical foundations.
Contribution
It provides a detailed rebuttal to critiques of R_h=ct, affirming its observational support and clarifying misunderstandings about its theoretical basis.
Findings
R_h=ct outperforms LCDM in multiple cosmological tests
Likelihood of R_h=ct being correct is 90-95% based on data
Criticisms of R_h=ct are based on incorrect assumptions
Abstract
The R_h=ct Universe is a Friedmann-Robertson-Walker (FRW) cosmology which, like LCDM, assumes the presence of dark energy in addition to (baryonic and non-luminous) matter and radiation. Unlike LCDM, however, it is also constrained by the equation of state (EOS) p=-rho/3, in terms of the total pressure p and energy density rho. One-on-one comparative tests between R_h=ct and LCDM have been carried out using over 14 different cosmological measurements and observations. In every case, the data have favoured R_h=ct over the standard model, with model selection tools yielding a likelihood ~90-95% that the former is correct, versus only ~5-10% for the latter. In other words, the standard model without the EOS p=-rho/3 does not appear to be the optimal description of nature. Yet in spite of these successes---or perhaps because of them---several concerns have been published recently regarding…
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