Calculating proper time using schwartzchild metric

demonelite123
Messages
216
Reaction score
0
I am using the schwartzchild metric given as ds^2 = (1 - \frac{2M}{r})dt^2 - (1 - \frac{2M}{r})^{-1} dr^2, where I assume the angular coordinates are constant for simplicity.

So if a beam of light travels from radius r0 to smaller radius r1, hits a mirror, and travels back to r0, I am trying to find how much proper time has passed for an observer fixed at r0. So far, i have that this path can be parametrized by r = r0 and t = x, where x is just my parameter. Therefore, r' = 0 and t' = 1. Using the formula for arc length, i have that the proper time is given by \int \sqrt{1 - \frac{2M}{r_0}} dx.

this is where i am stuck as i am having trouble determining the limits of my integral. can someone give me a hint or two in the right direction? thanks
 
Physics news on Phys.org
Your integrand doesn't have any variable in it. The r_0 shouldn't be inside the integral; it should relate to a limit of integration.

You could try setting ds^2=0 and then separating variables and integrating to get a relation between r and t for the light beam.
 
First of all, you don't really need the extra parameter x; as far as the observer fixed at r0 is concerned, he's just traveling from t0, the time when he emits the light beam, to t1, the time when it returns to him. So you could just write the integral as:

\tau = \int_{t_{0}}^{t_{1}} \sqrt{1 - \frac{2M}{r_{0}}} dt

But the integrand doesn't depend on t, so you can just factor it out, and that makes the integral trivial:

\tau = \sqrt{1 - \frac{2M}{r_{0}}} \left( t_{1} - t_{0} \right)

Which, of course, should make you realize that the real focus of the problem is determining the coordinate time interval t1 - t0. The way to do that is to focus, not on the worldline of the observer fixed at r0, but on the worldline of the light beam. There are two segments to it (the one from r0 inward to r1, and the one from r1 back outward to r0), but they are mirror images, so to speak, so they should take equal coordinate time to traverse. So figuring out the coordinate time for one is sufficient. That's where I would recommend focusing your efforts. The key fact you need, in addition to what you've already posted, is that the light beam's worldline is null; that is, the interval ds^2 along the light beam's worldline is zero.
 
Well, the way I'd approach it is this:

Integrating along the path that the light takes won't give us the right answer - we want to integrate along the path that the clock takes between transmission and reception. Which is a simple path, of constant r = r0.

So we need to draw a space-time diagram with the ingoing light beam, and the outgoing lightbeam. How do we do this?

Given the line element

ds^2 = (1 - \frac{2M}{r})dt^2 - (1 - \frac{2M}{r})^{-1} dr^2p

we know that for a light beam, ds = 0. This immediately gives us the ratio dr/dt for the light beam - which will be a function of r.

So we'll have f(r) dr = dt, where I'm too lazy to write out f(r).

Integrating this we'll get \Delta t=F(r). We'll have the same \Delta t on the ingoing and outgoing null geodesic - so we double it.

This will give us the coordinate time that elapses between emission and reception. To get the proper time, we integrate along the worldline at r=r0 between the emission and reception events. dr=0 for this intergal, so we get a simple time dilation factor

ds = \int \sqrt{1 - \frac{2M}{r}} \, dt = \sqrt{1 - \frac{2M}{r}} \Delta t
 
Last edited:
ok so setting ds^2 = 0, i get (1 - \frac{2M}{r})dt^2 = (1 - \frac{2M}{r})^{-1} dr^2 or dt^2 = (1 - \frac{2M}{r})^{-2} dr^2. then taking the square root of both sides, i get dt = (1 - \frac{2M}{r})^{-1} dr.

now i can integrate both sides and i get t_1 - t_0 = \int_{r_1}^{r_0} \frac{r}{r - 2M}dr = (r_0 - r_1) + 2Mln(r_0 - 2M) - 2Mln(r_1 - 2M).

would this be correct? thanks for you replies.
 
demonelite123 said:
now i can integrate both sides and i get t_1 - t_0 = \int_{r_1}^{r_0} \frac{r}{r - 2M}dr = (r_0 - r_1) + 2Mln(r_0 - 2M) - 2Mln(r_1 - 2M).

would this be correct? thanks for you replies.

As noted before, to get the final answer you need to multiply the result by 2 because the integral you have given gives the "one-way" time, and you need the "round trip" time. The integral itself looks OK to me.
 
Thread 'Can this experiment break Lorentz symmetry?'
1. The Big Idea: According to Einstein’s relativity, all motion is relative. You can’t tell if you’re moving at a constant velocity without looking outside. But what if there is a universal “rest frame” (like the old idea of the “ether”)? This experiment tries to find out by looking for tiny, directional differences in how objects move inside a sealed box. 2. How It Works: The Two-Stage Process Imagine a perfectly isolated spacecraft (our lab) moving through space at some unknown speed V...
Insights auto threads is broken atm, so I'm manually creating these for new Insight articles. The Relativator was sold by (as printed) Atomic Laboratories, Inc. 3086 Claremont Ave, Berkeley 5, California , which seems to be a division of Cenco Instruments (Central Scientific Company)... Source: https://www.physicsforums.com/insights/relativator-circular-slide-rule-simulated-with-desmos/ by @robphy
Does the speed of light change in a gravitational field depending on whether the direction of travel is parallel to the field, or perpendicular to the field? And is it the same in both directions at each orientation? This question could be answered experimentally to some degree of accuracy. Experiment design: Place two identical clocks A and B on the circumference of a wheel at opposite ends of the diameter of length L. The wheel is positioned upright, i.e., perpendicular to the ground...
Back
Top