yukcream said:
To pervect:
My problem is I don't know how to write a^i as the vector form, like
{gamma, vgamma} for u^i, the 4-velocity vectors!
where gamma= 1/sqrt[1-v^2/c^2]
Let us suppose you have a particle.
You plot the coordinates of the particle as a function of it's proper time, \tau.
You do this by specifying four functions
\left( t(\tau), x(\tau), y(\tau), z(\tau) \right)
Then you can easily compute it's 4-velocity, which is the derivative of the above expression with respect to tau, and it's 4-acceleration, which is the second derivative of the above expression with respect to tau, i.e.
4 velocity u^i = \frac{d x^i}{d \tau}
4 acceleration a^i = \frac{d^2 x^i}{d \tau^2}
Now (this may be your question?) sometimes you have instead only
(x(t), y(t), z(t)), rather than the above 4 functions.
You then have to compute \tau by the relationship
<br />
d\tau^2 = dt^2 - dx^2 - dy^2 - dz^2<br />
(This is assuming a flat metric - if you are doing general relativity, you havea to use the more general expression
d\tau^2 = g_{ab} dx^a dx^b
where you sum over a=0..3 and b=0..3)
It may be worthwile to re-write the above expression to explicitly solve for tau in a Miknowskian space-time, one with a global Lorentz metric:
\tau = \int \sqrt{1 - \left( \frac{dx}{dt} \right)^2 - \left( \frac{dy}{dt} \right)^2 - \left( \frac{dz}{dt} \right)^2 } dt<br />
This gives you \tau(t). You then have to invert this expression to find t(\tau). Then you can compute the other expressions by substitution, which are x(t(\tau)), y(t(\tau), z(t(\tau))
Fortunately, this does not have to be done very often. Usually, one can specify the a^i directly, then find u^i and x^i, and then (if one is interested), convert them into coordinate form via taking x(t) = x(t(\tau)), etc.