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:Substituting <math>E_d(r)=E_o-E(r)</math> where <math>E(r)</math> is energy of photons at distance <math>r</math> from their source and <math>1/R_E^2=4\pi G\rho/c^2</math>, number called in cosmology "curvature of space of Einstein's universe" (or <math>R_E=</math>"Einstein's radius of universe"), we get  
 
:Substituting <math>E_d(r)=E_o-E(r)</math> where <math>E(r)</math> is energy of photons at distance <math>r</math> from their source and <math>1/R_E^2=4\pi G\rho/c^2</math>, number called in cosmology "curvature of space of Einstein's universe" (or <math>R_E=</math>"Einstein's radius of universe"), we get  
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:<math>d^2E(r)/dr^2=E(r)/R_E^2</math>
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::<math>d^2E(r)/dr^2=E(r)/R_E^2</math>
    
==== Step 6: Solving the above equation ====
 
==== Step 6: Solving the above equation ====
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