- #1
FunkyDwarf
- 489
- 0
Hello,
I have a couple of questions regarding the calculation of circular orbits in the Schwarzschild exterior spacetime and then the extension of these arguments to other (interior) metrics.
First of all, in a few different books/sets of notes there seems to be a bit of 'drift' in the nomenclature which I was hoping to clear up. Specifically, is the condition that r-double-dot (w.r.t tau) = 0 a condition for a circular orbit to exist, or a condition for a stable circular orbit. I suspect the former ( can have max or min, i.e. stable or unstable, part of the potential).
Secondly, the standard way to construct the effective potential in the Schwarzschild case is to identify symmetries and thus constants of the motion, and then to solve for dr/dtau either using some conserved four-momentum or equivalently looking at timelike (for massive particles ofc) curves and setting the spacetime interval to something.
This turns out quite nicely as the schwarzschild metric (ds^2 = -a(r) dt^2 +b(r)dr^2...) has the nice property that a(r)b(r) = 1. In the case of say the Schwarzschild interior metric, or it's neater companion the Florides metric, this is not true.
Thus when you follow the usual procedure it is difficult to separate out a constant 'energy' part and effective potential to then look for circular orbits in.
I was wondering if there is a standard trick to getting around this. I thought of using tortoise coordinates (or more generally, coordinates that put your metric in a conformally flat form) which works well in say the wave equation for a scalar particle, but here I don't see how it would help.
Sorry for the tl;dr, and thanks in advance for help/advice!
-FD
I have a couple of questions regarding the calculation of circular orbits in the Schwarzschild exterior spacetime and then the extension of these arguments to other (interior) metrics.
First of all, in a few different books/sets of notes there seems to be a bit of 'drift' in the nomenclature which I was hoping to clear up. Specifically, is the condition that r-double-dot (w.r.t tau) = 0 a condition for a circular orbit to exist, or a condition for a stable circular orbit. I suspect the former ( can have max or min, i.e. stable or unstable, part of the potential).
Secondly, the standard way to construct the effective potential in the Schwarzschild case is to identify symmetries and thus constants of the motion, and then to solve for dr/dtau either using some conserved four-momentum or equivalently looking at timelike (for massive particles ofc) curves and setting the spacetime interval to something.
This turns out quite nicely as the schwarzschild metric (ds^2 = -a(r) dt^2 +b(r)dr^2...) has the nice property that a(r)b(r) = 1. In the case of say the Schwarzschild interior metric, or it's neater companion the Florides metric, this is not true.
Thus when you follow the usual procedure it is difficult to separate out a constant 'energy' part and effective potential to then look for circular orbits in.
I was wondering if there is a standard trick to getting around this. I thought of using tortoise coordinates (or more generally, coordinates that put your metric in a conformally flat form) which works well in say the wave equation for a scalar particle, but here I don't see how it would help.
Sorry for the tl;dr, and thanks in advance for help/advice!
-FD