This analysis estimates the age of the universe using wavelength stretching of photons, suggesting insights into early cosmic conditions.
This study presents an order-of-magnitude estimate of the age of the universe based on the wavelength stretching of photons from the early universe to the present cosmic microwave background (CMB). Unlike standard cosmological models, the approach does not rely on a detailed cosmic expansion history or specific predictions for the initial photon energy EinitEᵢₙᵢₜEinit, which remains unknown. Instead, the current Hubble constant H0H_0H0 is used to evaluate the timescale of the universe, yielding an approximate age of 14 Gyr. The study defines a proportionality factor k=Eobs/Einitk = Eobs/Eᵢₙᵢₜk=Eobs/Einit to conceptually represent the wavelength stretching, without requiring numeric values for EinitEᵢₙᵢₜEinit. This framework allows future research to potentially reverse-calculate EinitEᵢₙᵢₜEinit using the estimated universe age and CMB observations, which may provide insights into the state of photons in the early universe and the initial cosmic environment. The work is positioned as a simple, yet conceptually informative, evaluation within the light universe theory.
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Akihito Sugawara (2026) studied this question.
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