L Drago said:
Suppose person A is at rest relative to the surface of Earth and Person B is travelling in 80 percent speed of light relative to a planet in solar system say let's take Earth as Person A is also in restaurant relative to its surface and Person C is also travelling in 90 percent speed of light relative to planet Earth
Let me be sure that I have the setup straight.
We have an inertial reference frame. It is the rest frame of the Earth's surface. The problem will be described in terms of this frame.
We have three people: A, B and C. A is at rest in our frame. B is moving inertially at 0.8c in our frame. C is moving inertially at 0.9 c in our frame.
The intent is to treat these three people as three "observers". That is, we will consider each as defining an inertial frame of reference in which he or she is at rest.
L Drago said:
We have to calculate by using SR time dilation.
What, exactly, are we calculating?
What is the trajectory for which we will be computing a dilated time?
What is the trajectory for which we will be computing a proper time?
Is there one trajectory? Or three? What are the end points? What is the path between the endpoints?
L Drago said:
Dilated time = Actual time / power root of (1-(v²/c²)). These three persons will not agree to dilated time but will agree to proper time.
I agree in principle.
If we had an object traversing an unaccelerated (geodesic) trajectory from a start event to an end event then all three observers could calculate an elapsed coordinate time (aka "dilated time") for the trajectory by dividing the object's elapsed proper time (not "actual time") by ##\sqrt{1-v^2/c^2}##. Here, ##v## is, of course, the object's velocity relative to the observer's rest frame.
Alternately, all three observers could calculate the elapsed proper time for the object by multiplying their measured coordinate time difference for the trajectory by ##\sqrt{1-v^2/c^2}##.
If the object is traversing an accelerated trajectory then it will not have a single constant velocity ##v##. One may have to evaluate an integral.
One can communicate more effectively by using standard terms (e.g. proper time and coordinate time) rather than non-standard terms (e.g. actual time and dilated time).