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Hubble Constant, CMBR, Fine Structure Constant & Friedmann Density Parameters

David E. Fuller, Ruud Loeffen

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Abstract

Hubble Constant, CMBR, Fine Structure Constant & Friedmann Density Parameters ((((7.04370151e+4 * (m / s)) / (1 Mpc)) / (160.4589 GHz)) / G) * (6.5248935 * (kg^(-1)) * (m / s)) * (c^2) * (8 s) = 1 7.04370151e+4 / (6.5248935 / (2pi)) = 67827.7459024 https://en.wikipedia.org/wiki/Hubble%27s_law#Observed_values_of_the_Hubble_constant (((7.04370151e+4 * (m / s)) / (1 Mpc)) / (160.4589 GHz)) * (hbar / planck length) * (4 (s / (m^4))) = 3.71295774e-28 kg / m^3 https://en.wikipedia.org/wiki/Friedmann_equations#Density_parameter

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Hubble Constant, CMBR, Fine Structure Constant & Friedmann Density Parameters ((((7.04370151e+4 * (m / s)) / (1 Mpc)) / (160.4589 GHz)) / G) * (6.5248935 * (kg^(-1)) * (m / s)) * (c^2) * (8 s) = 1 7.04370151e+4 / (6.5248935 / (2pi)) = 67827.7459024 https://en.wikipedia.org/wiki/Hubble%27s_law#Observed_values_of_the_Hubble_constant (((7.04370151e+4 * (m / s)) / (1 Mpc)) / (160.4589 GHz)) * (hbar / planck length) * (4 (s / (m^4))) = 3.71295774e-28 kg / m^3 https://en.wikipedia.org/wiki/Friedmann_equations#Density_parameter

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Available abstract

Hubble Constant, CMBR, Fine Structure Constant & Friedmann Density Parameters ((((7.04370151e+4 * (m / s)) / (1 Mpc)) / (160.4589 GHz)) / G) * (6.5248935 * (kg^(-1)) * (m / s)) * (c^2) * (8 s) = 1 7.04370151e+4 / (6.5248935 / (2pi)) = 67827.7459024 https://en.wikipedia.org/wiki/Hubble%27s_law#Observed_values_of_the_Hubble_constant (((7.04370151e+4 * (m / s)) / (1 Mpc)) / (160.4589 GHz)) * (hbar / planck length) * (4 (s / (m^4))) = 3.71295774e-28 kg / m^3 https://en.wikipedia.org/wiki/Friedmann_equations#Density_parameter

Key concepts: Hubble's law, Friedmann equations, Physics, Cosmic microwave background, Planck, Planck time, Constant (computer programming), Mathematical physics

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