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:<math>E=mc^2(x)</math> ...... (1)
 
:<math>E=mc^2(x)</math> ...... (1)
   −
where <math>c^2(x)</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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where <math>c^2(x)</math> is square of speed of light in vacuum adjusted by <math>(d\tau/dt)</math> (ratio of proper time to coordinate time
 +
<ref>
    
This ratio is expressed usually as
 
This ratio is expressed usually as
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:<math>d\tau/dt=\sqrt{g_{oo}}</math>,
 
:<math>d\tau/dt=\sqrt{g_{oo}}</math>,
   −
in sign convention used in physics, where times are considered to be positive and distances negative <math>g_{oo}</math> in both notations is time-time component of metric of spacetime, which means that  
+
in sign convention used in physics, where times are considered to be positive and distances negative.
 +
 
 +
:<math>g_{oo}</math>
 +
 
 +
in both notations is time-time component of metric of spacetime, which means that  
    
:<math>E=mc^2 \sqrt{g_{oo}(x)}</math>  
 
:<math>E=mc^2 \sqrt{g_{oo}(x)}</math>  
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