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==== Step 4. Integrating both sides of above equation ====
 
==== Step 4. Integrating both sides of above equation ====
−
:<math>-d E_d(r)/dr =(4 \pi G \rho/c^2)\int[E_o-E_d(r)]dr</math>.
+
::<math>-d E_d(r)/dr =(4 \pi G \rho/c^2)\int[E_o-E_d(r)]dr</math>.
 
:... over all spherical shells between "point zero" and <math>r</math> to get total energy of "dust" absorbed from photons, and then '''differentiating both sides with respect to''' <math>r</math> '''to get rid of integral on the right side''' of this equation, we get finally the starting <math>E_d(r)</math> where subscript <math>d</math> now, as before,  means ''"volume of universe of radius <math>r</math> around point zero"''
 
:... over all spherical shells between "point zero" and <math>r</math> to get total energy of "dust" absorbed from photons, and then '''differentiating both sides with respect to''' <math>r</math> '''to get rid of integral on the right side''' of this equation, we get finally the starting <math>E_d(r)</math> where subscript <math>d</math> now, as before,  means ''"volume of universe of radius <math>r</math> around point zero"''
   −
:<math>-d^2 E_d(r)/dr^2 =(4 \pi G \rho/c^2)[E_o-E_d(r)]</math>.
+
::<math>-d^2 E_d(r)/dr^2 =(4 \pi G \rho/c^2)[E_o-E_d(r)]</math>.
    
==== Step 5: Setting differential equation controlling the redshift ====
 
==== Step 5: Setting differential equation controlling the redshift ====
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