What is the formula for calculating relative velocities in Special Relativity?

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The discussion centers on calculating relative velocities in Special Relativity, specifically addressing the scenario with three objects: O, A, and B. The participants clarify that the formula for relative velocity in Special Relativity differs from the Newtonian approach. The correct formula for the relative velocity of A with respect to B is given by vAB = (vOB - vOA) / (1 - (vOB * vOA) / c2), where c represents the speed of light. The discussion emphasizes the necessity of using Special Relativity principles rather than Galilean ones when calculating these velocities.

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Lets suppose three objects O,A and B are set up in universe and nothing else.Then O seems A is moving 0.3c And B is moving 0.5c .In Special Relativity we have relative velocities formula I want to formule it but result seems absurd can you find me all possible velocities I mean A, O and B observer
Thank you
 
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Quarlep said:
In Special Relativity we have relative velocities formula I want to formule it but result seems absurd
What results did you get? Why do they seem absurd?
 
VCB=VOB-VOC I thought like this But this is not true in special relativity.In special Relativity it like the relative formule for special relativity isn't it ?
 
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Quarlep said:
VCB=VOB-VOC
You'll need to define your terms. (What is C, for example?)

Quarlep said:
I thought like this But this is not true in special relativity.In special Relativity it like the relative formule for special relativity isn't it ?
You'll certainly need to add the velocities using special relativity, not Galilean relativity.
 
C is speed to O
 
Quarlep said:
VCB=VOB-VOC
But you said there were only 3 objects O, A and B, so there is no object C? I'm going to assume by "C" you mean "A", so, in Newtonian theory it would be<br /> v_{AB} = v_{OB} - v_{OA}.<br />Then in special relativity it is<br /> v_{AB} = \frac{ v_{OB} - v_{OA} } { 1 - \frac{ v_{OB} v_{OA} } {c^2} },<br />(provided all velocities are parallel).
 
Thanks
 

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