GPS system and general relativity

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Discussion Overview

The discussion centers around the GPS satellite system and its relationship with general relativity, particularly focusing on the effects of gravitational time dilation and the role of the Earth-Centered Inertial (ECI) coordinate system. Participants explore theoretical aspects, practical implications, and the mathematical underpinnings of these phenomena.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants propose that the GPS system employs the Schwarzschild spacetime model to evaluate time dilation due to differences in gravitational potential between Earth's surface and GPS satellites.
  • There is a suggestion that the motion of GPS satellites introduces additional components to time dilation, with some participants noting the gravitational blue shift observed from Earth's perspective.
  • One participant mentions that without relativity corrections, GPS locations would be inaccurate by over 6 miles per day, with specific time discrepancies attributed to gravitational and special relativistic effects.
  • Clarifications are made regarding the overall GPS satellite clock correction, with participants discussing the contributions from gravitational effects and satellite motion.
  • Some participants express uncertainty about the role of the ECI coordinate system, with discussions on its relevance to navigation and calculations in the context of GPS.
  • There are corrections regarding the units of time discrepancies, with a consensus emerging that the correct value is in microseconds per day rather than milliseconds.
  • One participant questions whether astrophysical phenomena might need to account for these relativistic effects, leading to further discussion on observational accuracy.

Areas of Agreement / Disagreement

Participants generally agree on the significance of relativistic effects in GPS systems, but there are multiple competing views regarding the specifics of time dilation components and the role of the ECI coordinate system. The discussion remains unresolved in terms of fully clarifying these aspects.

Contextual Notes

Some participants express uncertainty about the definitions and transformations between different coordinate systems, such as Schwarzschild and ECI, indicating potential limitations in understanding the mathematical relationships involved.

Who May Find This Useful

This discussion may be of interest to those studying general relativity, GPS technology, and the mathematical modeling of gravitational effects in navigation systems.

  • #91
PeterDonis said:
Your factor here is wrong. Check your math. (Two hints: first, clocks hovering at finite ##r## run slow relative to Schwarzschild coordinate time; second, the time dilation factor is not ##g_{tt}## itself, remember that the line element is a formula for ##ds^2##.)
Yes sorry, the conversion factor is actually ##1/\sqrt{g_{tt}}## hence for the specific case it is $$\frac {1} {\sqrt {(1 - r_s/r)}}$$
From my understanding, in principle, the "construction" in the previous post can be done locally in any spacetime (in other words there is always a spacetime transformation such that locally ##g_{0\alpha} = 0## and using the timelike congruence "at rest/adapted" to such a local chart the above construction can be applied). In a sense it defines 4 spacetime directions at any point/event such that the 3 spacelike directions are orthogonal to the timelike one.

My question is: in the general case does always exist a transformation that brings the metric components locally in the form ##g_{00}=1, g_{0\alpha}=0## leaving "at rest" the "old" timelike coordinate lines in the new local chart being defined (i.e. leaving at rest in the new chart the timelike curves described by ##\{x_\alpha = c_\alpha, \alpha =1,2,3 \}## in the old chart one started with) ?
 
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  • #92
cianfa72 said:
the conversion factor is actually ##1/\sqrt{g_{tt}}## hence for the specific case it is $$\frac {1} {\sqrt {(1 - r_s/r)}}$$
Yes.

cianfa72 said:
From my understanding, in principle, the "construction" in the previous post can be done locally in any spacetime (in other words there is always a spacetime transformation such that locally ##g_{0\alpha} = 0## and using the timelike congruence "at rest/adapted" to such a local chart the above construction can be applied). In a sense it defines 4 spacetime directions at any point/event such that the 3 spacelike directions are orthogonal to the timelike one.
Yes, this is just a version of constructing a local inertial frame centered on a point.

cianfa72 said:
in the general case does always exist a transformation that brings the metric components locally in the form ##g_{00}=1, g_{0\alpha}=0## leaving "at rest" the "old" timelike coordinate lines in the new local chart being defined (i.e. leaving at rest in the new chart the timelike curves described by ##\{x_\alpha = c_\alpha, \alpha =1,2,3 \}## in the old chart one started with) ?
You can always construct Fermi normal coordinates on an open region centered on a chosen timelike worldline. You might have to make some additional adjustments to enforce ##g_{00} =1## and ##g_{0 \alpha} = 0## on the chosen worldline. If you want those conditions to hold in an open region centered on the worldline, the congruence of timelike worldlines you choose must be irrotational.
 
  • #93
PeterDonis said:
Yes, this is just a version of constructing a local inertial frame centered on a point.
Sorry, to get a local inertial frame centered on a point, the metric components in that local chart should be exactly ##(1,-1,-1,-1)## with vanish derivatives on that point.

PeterDonis said:
You can always construct Fermi normal coordinates on an open region centered on a chosen timelike worldline. You might have to make some additional adjustments to enforce ##g_{00} =1## and ##g_{0 \alpha} = 0## on the chosen worldline. If you want those conditions to hold in an open region centered on the worldline, the congruence of timelike worldlines you choose must be irrotational.
You mean that locally (i.e. in an open neighborhood of any point) in any spacetime there is always an irrotational timelike congruence.
 
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  • #94
cianfa72 said:
to get a local inertial frame centered on a point, the metric components in that local chart should be exactly ##(1,-1,-1,-1)## with vanish derivatives on that point.
Yes.

cianfa72 said:
Your mean that locally (i.e. in an open neighborhood of any point) in any spacetime there is always an irrotational timelike congruence.
That's not what I said. Go read what I said again, carefully.
 
  • #95
PeterDonis said:
That's not what I said. Go read what I said again, carefully.
From Synchronous frame in any spacetime in any open neighborhood there is a (synchronous) coordinate chart such that ##g_{00}=1, g_{0\alpha}=0##. I believe the timelike curves (actually geodesics) at rest in it form an irrotational congruence.
 
  • #96
  • #97
PeterDonis said:
Sure, I remember that thread. The take-home message was that in a finite open patch of any spacetime one can always build a synchronous reference frame/chart (such a chart may not extend globally since sooner or later the timelike geodesics starting orthogonal to the initially chosen spacelike hypersurface will intersect).
 
  • #98
cianfa72 said:
Sure, I remember that thread. The take-home message was that in a finite open patch of any spacetime one can always build a synchronous reference frame/chart (such a chart may not extend globally since sooner or later the timelike geodesics starting orthogonal to the initially chosen spacelike hypersurface will intersect).
Yes, and what I said in post #55 did not contradict any of that. But it did not just repeat it either.
 
  • #99
Ok, so the fact that in any open patch of spacetime one can always build a synchronous coordinate chart implies that any spacetime admits a locally proper time synchronizable congruence/frame using the terminology of Sachs and Wu section 2.3 (i.e. ##d\omega = 0## and by Poincaré lemma ##\omega = dt## for some smooth function ##t## in that open region).
 
  • #100
cianfa72 said:
in any open patch of spacetime one can always build a synchronous coordinate chart
Actually, as you state this, it's too strong. The correct statement is that, given a spacelike hypersurface, one can always find some open neighborhood of that hypersurface in which Gaussian normal coordinates, i.e., a "synchronous coordinate chart", can be constructed. But one cannot guarantee that such coordinates will be valid for any open neighborhood, of any size whatever.

cianfa72 said:
any spacetime admits a locally proper time synchronizable congruence/frame using the terminology of Sachs and Wu section 2.3 (i.e. ##d\omega = 0## and by Poincaré lemma ##\omega = dt## for some smooth function ##t## in that open region).
With the qualifications given above, yes.
 
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  • #101
PeterDonis said:
Actually, as you state this, it's too strong. The correct statement is that, given a spacelike hypersurface, one can always find some open neighborhood of that hypersurface in which Gaussian normal coordinates, i.e., a "synchronous coordinate chart", can be constructed. But one cannot guarantee that such coordinates will be valid for any open neighborhood, of any size whatever.
Ok, let me say the point is that, given an open patch in spacetime, it might be so much larger that timelike geodesics starting orthogonal from a spacelike hypersurface within it will intersect inside that region, though.
 
  • #102
cianfa72 said:
the point is that, given an open patch in spacetime, it might be so much larger that timelike geodesics starting orthogonal from a spacelike hypersurface within it will intersect inside that region, though.
It doesn't have to be "so much" larger, just large enough for geodesics to intersect.

This is getting pretty far off the original topic of this thread, btw. The frames used in GPS are not examples of synchronous coordinates.
 
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  • #103
cianfa72 said:
Hi, we had a thread some time ago about GPS satellite system.
One starts considering the ECI coordinate system in which the Earth's center is at rest with axes pointing towards fixed stars. One may assume it is an inertial frame in which the Earth's surface undergoes circular motion.
Do you mean this ? I would thank you for your contribution.
 
  • #104
binis said:
Do you mean this ? I would thank you for your contribution.
No, the thread I was referring to is this.
 

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