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where <math>c^2</math> is square of speed of light in vacuum adjusted by <math>(d\tau/dt)</math> (ratio of proper time to coordinate time<ref>
 
where <math>c^2</math> is square of speed of light in vacuum adjusted by <math>(d\tau/dt)</math> (ratio of proper time to coordinate time<ref>
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This ratio is expressed sometimes as  
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This ratio is expressed usually as  
 
:<math>d\tau/dt=\sqrt{-g_{oo}}</math>,  
 
:<math>d\tau/dt=\sqrt{-g_{oo}}</math>,  
 
where <math>(-g_{oo})</math> is time-time component of metric of spacetime, which means that <math>mc^2 \sqrt{-g_{oo}}</math> is not a constant but a function of time and we may take its non vanishing derivative with respect to time to calculate gravitational force.
 
where <math>(-g_{oo})</math> is time-time component of metric of spacetime, which means that <math>mc^2 \sqrt{-g_{oo}}</math> is not a constant but a function of time and we may take its non vanishing derivative with respect to time to calculate gravitational force.
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