'Mass' of an object at different positions in a weak gravitational field

Click For Summary
The discussion centers on the mass of an object in a weak gravitational field, specifically addressing how raising a 10kg block affects its mass. Participants debate whether mass changes due to gravitational potential energy, with some arguing that potential energy is stored in the field rather than the particles. The concept of "relativistic mass" is criticized as outdated, with emphasis placed on energy changes instead. The conversation also touches on the implications of gravitational binding energy and how it affects the total mass of a system. Ultimately, the consensus suggests that while potential energy increases with height, the effective mass of the object is not simply additive and must be considered within the context of the entire system.
  • #31
For a static field, energy varies in exactly the same way as frequency and clock rates in general, and this is described totally by the local time per coordinate time factor in the metric. Energy is very simple, as ratios of frequencies as seen by observers at rest are the same for all observers in any static coordinate system; it's just a matter of counting.

Momentum is more complicated as it involves space and depends much more heavily on the choice of coordinate system. I don't know why you keep trying to work backwards from momentum to mass or energy.

In GR, mass is normally assumed to be directly equivalent to energy, using the standard c as a conversion factor. This works perfectly well in most contexts, but it is not the same as mass expressed consistently within a flat coordinate system being used to map curved space-time.

Mass in coordinate mass units is not very relevant in GR. If you try to describe it in a non-isotropic coordinate system it's different in different directions. It's more convenient to use alternative forms of the force laws in terms of total energy and momentum.

Conservation laws are not relevant here. I don't think raising and lowering indices has any meaningful relevance, but perhaps my brain is getting scrambled by your attempts to work backwards from a complicated result to a simple one.
 
Physics news on Phys.org
  • #32
Jonathan Scott said:
Momentum is more complicated as it involves space and depends much more heavily on the choice of coordinate system. I don't know why you keep trying to work backwards from momentum to mass or energy.

Energy is the time component of the momentum isn't it?

And if you want the quantity which acceleration depends on won't you have to look at the momentum, since forces are expressed in terms of rate of change of momentum?
 
  • #33
TobyC said:
Energy is the time component of the momentum isn't it?

And if you want the quantity which acceleration depends on won't you have to look at the momentum, since forces are expressed in terms of rate of change of momentum?

For any question in which GR plays any part, you need to think about whose point of view you are trying to use.

The original question was about the apparent mass increase due to potential energy, so it is obviously from the point of view of someone near the mass, in terms of their local view. In that case you can just use the Newtonian mgh for the extra energy combined with E = mc2. You can also compare local time rates at different points in the Schwarzschild solution to get exactly the same result for the energy difference and hence the effective mass difference in local coordinates (at least for the weak approximation case).

The previous expression you derived for momentum is not relative to local coordinates but rather to some external coordinates, so it is not exactly the same momentum, because of additional factors affecting space and time. It is therefore not surprising that it does not vary in the same way with potential.
 
  • #34
Jonathan Scott said:
For any question in which GR plays any part, you need to think about whose point of view you are trying to use.

The original question was about the apparent mass increase due to potential energy, so it is obviously from the point of view of someone near the mass, in terms of their local view. In that case you can just use the Newtonian mgh for the extra energy combined with E = mc2. You can also compare local time rates at different points in the Schwarzschild solution to get exactly the same result for the energy difference and hence the effective mass difference in local coordinates (at least for the weak approximation case).

The previous expression you derived for momentum is not relative to local coordinates but rather to some external coordinates, so it is not exactly the same momentum, because of additional factors affecting space and time. It is therefore not surprising that it does not vary in the same way with potential.

I don't see why the expression I derived is not relative to local coordinates? I defined the gravitational potential to be zero at ground level, so at ground level the metric is just the standard minkowski metric, so the expression should be valid from the point of view of a coordinate system which is located and fixed at ground level, which is the perspective that seems to be implied from the question.
 
  • #35
I won't pretend to understand the formulas and equations that have been used in this thread. Conceptually, the OP seems to be asking in the mass of an object that is raised to a higher level in a gravitational field decreases. Since this section deals with Special and General Relativity, I'm guessing that the question boils down to whether the equivalent mass/energy of the object decreases as it is raised in a gravitational field.

I would look at this problem from the perspective of a distant observer viewing a large colud of interstellar dust and ice unperturbed by any outside forces. This cloud certainly contains a set amount of mass in the form of dust grains and ice particles. It also contains a set amount of gravitational potential energy. In layman's terms, the constituent particles are far away from each other, but their natural tendency is to "fall" together.

If one were to observe this cloud over the course of several million years, there would be a contraction - very slowly at first, but gradually becoming faster and faster. The gravitational potential energy of the once aimlessly drifting particles is being converted into the kinetic energy of particles moving towards each other.

Let's say, for the sake of simplicity, that this cloud eventually coalesces into a sub-stellar object of 10 Jupiter masses. The particles making up this object are the same particles that comprised the original cloud. To be sure, a lot of energy has been radiated away by the heat of all this stuff crashing in on itself.

After 10 or 20 billion years most of this heat will radiate away and there will be a ball of stuff all mashed together as closely as the various inter-molecular forces will allow.

The question posed by to OP is whether the mass of a piece of this ball will decrease if it is raised some distance from the surface.

We can consider that there has been a lot of energy lost by the various particles making up this ball from where they originally started to their final resting place. To time-reverse this process (even for a small piece of this ball) will require the input of energy.

Does this inputed energy reside in the particle's mass, or in the particle's position relative to the big ball of stuff?

My take on this is that the answer is a qualified "yes" to both questions. Considering that every particle in the universe has some equivalent mass/energy relative to every other particle in the universe, the mass/energy of the piece of the ball that is raised above the surface will increase relative to the ball.

I apologize for this unsophisticated reply - bereft of equations such as it is. I may be totally wrong about all this. If so, please feel free to correct me.

Chris
 
  • #36
TobyC said:
I don't see why the expression I derived is not relative to local coordinates? I defined the gravitational potential to be zero at ground level, so at ground level the metric is just the standard minkowski metric, so the expression should be valid from the point of view of a coordinate system which is located and fixed at ground level, which is the perspective that seems to be implied from the question.

As far as I can see, what you've calculated is the momentum in a coordinate system which is flat but locally coincides with the local coordinate system. By the time you get to a different potential, it can no longer match the local coordinate system, in that both time and space have changed in scale, so the coordinate speed of light has changed and the momentum defined by that process differs from local momentum.

However, the change in the energy is only affected by the relative time rate, so that can be compared from any static point of view.
 
  • #37
Jonathan Scott said:
As far as I can see, what you've calculated is the momentum in a coordinate system which is flat but locally coincides with the local coordinate system. By the time you get to a different potential, it can no longer match the local coordinate system, in that both time and space have changed in scale, so the coordinate speed of light has changed and the momentum defined by that process differs from local momentum.

However, the change in the energy is only affected by the relative time rate, so that can be compared from any static point of view.

I don't think I've used a locally flat coordinate system, that would be one in free fall, the coordinate system I'm using is at rest relative to the surface of the earth, or at least that's what I've tried to do.
 
  • #38
csmyth3025 said:
I won't pretend to understand the formulas and equations that have been used in this thread. Conceptually, the OP seems to be asking in the mass of an object that is raised to a higher level in a gravitational field decreases. Since this section deals with Special and General Relativity, I'm guessing that the question boils down to whether the equivalent mass/energy of the object decreases as it is raised in a gravitational field.

I would look at this problem from the perspective of a distant observer viewing a large colud of interstellar dust and ice unperturbed by any outside forces. This cloud certainly contains a set amount of mass in the form of dust grains and ice particles. It also contains a set amount of gravitational potential energy. In layman's terms, the constituent particles are far away from each other, but their natural tendency is to "fall" together.

If one were to observe this cloud over the course of several million years, there would be a contraction - very slowly at first, but gradually becoming faster and faster. The gravitational potential energy of the once aimlessly drifting particles is being converted into the kinetic energy of particles moving towards each other.

Let's say, for the sake of simplicity, that this cloud eventually coalesces into a sub-stellar object of 10 Jupiter masses. The particles making up this object are the same particles that comprised the original cloud. To be sure, a lot of energy has been radiated away by the heat of all this stuff crashing in on itself.

After 10 or 20 billion years most of this heat will radiate away and there will be a ball of stuff all mashed together as closely as the various inter-molecular forces will allow.

The question posed by to OP is whether the mass of a piece of this ball will decrease if it is raised some distance from the surface.

We can consider that there has been a lot of energy lost by the various particles making up this ball from where they originally started to their final resting place. To time-reverse this process (even for a small piece of this ball) will require the input of energy.

Does this inputed energy reside in the particle's mass, or in the particle's position relative to the big ball of stuff?

My take on this is that the answer is a qualified "yes" to both questions. Considering that every particle in the universe has some equivalent mass/energy relative to every other particle in the universe, the mass/energy of the piece of the ball that is raised above the surface will increase relative to the ball.

I apologize for this unsophisticated reply - bereft of equations such as it is. I may be totally wrong about all this. If so, please feel free to correct me.

Chris

I can't really correct you as I obviously don't know the answer to this question (that's why I made the thread). However, I think what you're getting at is the idea that the potential energy of a system should manifest itself in an increased mass of the particles? Although the gravity question is still unclear for me I am pretty confident that in electrostatics for example, the potential energy doesn't work this way. Instead the energy, and the mass that goes with it, is stored at every point in space with a density proportional to the square of the magnitude of the electric field at that point.
 
  • #39
TobyC said:
I don't think I've used a locally flat coordinate system, that would be one in free fall, the coordinate system I'm using is at rest relative to the surface of the earth, or at least that's what I've tried to do.

By "local" coordinates I mean static SR coordinates in the local vicinity of the static observer, who observes that light locally always travels at the standard c. Such a system can however only be approximate in a region where the gravitational potential varies, as local space-time is curved. However, we can instead use a coordinate system which is flat and which locally matches local coordinates, but begins to diverge a bit further away; there is more than one possible scheme for such coordinates.

As an analogy, consider a flat map of a large part of the earth. It can be exactly accurate in scale and shape at some chosen point, but the further away one gets the more the scale or shape has to change.

I think (although I'm not sure) that you've effectively started with an expression that defines momentum relative to the map, with the result that it has an extra scale factor because of the difference between the map and the local value.
 
  • #40
Jonathan Scott said:
By "local" coordinates I mean static SR coordinates in the local vicinity of the static observer, who observes that light locally always travels at the standard c. Such a system can however only be approximate in a region where the gravitational potential varies, as local space-time is curved. However, we can instead use a coordinate system which is flat and which locally matches local coordinates, but begins to diverge a bit further away; there is more than one possible scheme for such coordinates.

As an analogy, consider a flat map of a large part of the earth. It can be exactly accurate in scale and shape at some chosen point, but the further away one gets the more the scale or shape has to change.

I think (although I'm not sure) that you've effectively started with an expression that defines momentum relative to the map, with the result that it has an extra scale factor because of the difference between the map and the local value.

I don't think this is what I've done. The coordinate system I've used should accurately describe everything, not just local things, from the point of view of an observer stationary relative to the ground.
 
  • #41
TobyC said:
I don't think this is what I've done. The coordinate system I've used should accurately describe everything, not just local things, from the point of view of an observer stationary relative to the ground.

Yes, that's what a coordinate system is for, but it is NOT the same as the values a local observer would observe at each of the mapped points. As I've been saying, it is like a map. It can describe everything, but it cannot be the same scale and shape as the local view everywhere, because the local view is curved.
 

Similar threads

  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 8 ·
Replies
8
Views
1K
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 5 ·
Replies
5
Views
1K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 3 ·
Replies
3
Views
1K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 35 ·
2
Replies
35
Views
3K
Replies
16
Views
2K