A tentative derivation of the main cosmological parameters
A. Dinculescu

TL;DR
This paper attempts an independent derivation of key cosmological parameters using simplified assumptions, achieving results consistent with recent observational data.
Contribution
It presents a novel, approximate method to derive main cosmological parameters independently from observational data.
Findings
Derived values closely match recent observational data.
Method provides a simplified approach to estimate cosmological parameters.
Results support the validity of the assumptions used.
Abstract
Based on the assumption that some apparent properties of the observable universe are accurate at a reasonable level of approximation, a tentative is made to independently derive the values of the baryon density parameter, the Hubble constant, the cosmic microwave background temperature and the helium mass fraction. The obtained values are in excellent agreement with those given by the most recent observational data.
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