Monday, November 25, 2024

The Second Radiation Constant is my Gamma unit scaling.


h = α³β/c
G = α³/β
k = α³β/γ
ε₀ = δ²/(α³β)
And the values for each parameter:
α ≈ 1.53844×10⁻⁶ m (length scaling)
β ≈ 5.45551×10⁻⁸ kg (mass scaling)
γ ≈ 1.438776877504×10⁻² K⁻¹ (temperature scaling)
δ ≈ 1.32621132205611221308×10⁻¹⁸ C (charge scaling)

I converted the second radiation constant over to my frame work and the formula simplified completely away.  I end up just setting the scaling factor for 

I started with the standard formula I got from the wiki page on physical constants. 

c_2 = (h c) / k_b

as you can see above we can substitute in the formula for h as α³β/c which cancels out the c and just leaves α³β, and  k_b =  α³β / γ, so the α³β cancels out of the equation and the γ goes to the top, leaving just c_2 = γ. This means the gamma I isolated out from the kg and meter scaling for Boltzmann is the second radiation constant that was a ratio in the Bolzmann constant all along.


    #c_2_calc = (h_calc * constants.c) / (boltzmann_calc)

    #c_2_calc = ((decimal_pow(constants.alpha, Decimal(3)) * constants.beta) )

             # / (decimal_pow(constants.alpha, Decimal(3)) * constants.beta / constants.gamma)

    c_2_calc =  constants.gamma


    #inprogress

    #cosmo_calc = decimal_pow(constants.alpha, Decimal(9) ) / Decimal(9) * pi**3








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