Gravitational Influence: Limits & GR Effects

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Discussion Overview

The discussion revolves around the limits of gravitational influence in both Newtonian gravity and General Relativity (GR), particularly in the context of dark energy and its effects on gravitational fields. Participants explore theoretical implications and the nature of gravitational propagation over vast distances.

Discussion Character

  • Exploratory
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • Some participants assert that under Newtonian gravity, the gravitational influence has no limits except for the speed of causality and the age of the object, suggesting that the Sun's influence could extend to 4.6 billion light-years.
  • Others clarify that in Newtonian mechanics, gravitational fields propagate instantaneously, while in GR, changes propagate at the speed of light.
  • A participant questions whether the gravitational field in GR is also infinite, leading to a discussion about the necessity of infinite time for propagation.
  • Some propose that dark energy might act as an anti-gravity effect, potentially limiting the propagation of gravitational fields at longer distances.
  • Another participant argues that any effect of dark energy would manifest as a change in spacetime curvature, which is inherently linked to the gravitational field in GR.
  • There is a suggestion that dark energy does not flatten the universe but produces a different type of spacetime curvature that does not cancel out the effects of gravitational fields.
  • One participant expresses uncertainty about the understanding of dark energy, noting that some scientists believe it could be an unknown force while others think it indicates incompleteness in gravitational theory.
  • The discussion includes a rephrasing of the original question regarding whether gravity may be attenuated differently at large distances compared to smaller scales, with a focus on the interaction between two distant stars in both Newtonian and GR frameworks.
  • Another participant emphasizes that stars must be formed from existing matter, suggesting that gravitational interactions at large distances are influenced by the historical distribution of matter.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the nature of gravitational influence, the role of dark energy, and the propagation of gravitational fields in GR. The discussion remains unresolved with no consensus on these complex topics.

Contextual Notes

Participants acknowledge limitations in understanding dark energy and its implications for gravitational fields, as well as the dependence on historical matter distribution for gravitational interactions at large distances.

Leonardo Muzzi
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As I understand, under Newtonian Gravity, there are no limits for the length of the gravitational influence of an object, except the speed of causality and the age of that object. So, considering the Sun as an example, which is roughly 4.6 billion years old, its gravitational influence would expand for 4.6 billion light-years.

Of course, that scenario considers the Sun just appeared out of nowhere. Considering the matter that originated the Sun was there before it became a star, the Sun gravitational influence would possibly expands to the whole Universe.

How that works under General Relativity? Considering the existence of Dark Energy, and any other stuff of GR meaningful to the question, would the limits of the gravitational influence of objects be different?
 
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Under Newtonian gravity, the range of the gravitational field is infinity and the gravitational field propagates instantaneously. There is no "speed of causality" in Newtonian mechanics. In GR, gravitational changes propagate through space at the speed of light.
 
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NFuller said:
Under Newtonian gravity, the range of the gravitational field is infinity and the gravitational field propagates instantaneously. There is no "speed of causality" in Newtonian mechanics. In GR, gravitational changes propagate through space at the speed of light.

But in GR is the gravitational field also infinite?
 
Only if it has infinite time to propagate, so generally speaking no.
 
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NFuller said:
Only if it has infinite time to propagate, so generally speaking no.

Right! So besides the speed of light + time limit, there is nothing that limits a gravitational field?

I am thinking about some kind of anti-gravity, dark energy effect, that would prevent a gravitational field from propagating infinitely.

After all, if dark energy flattens the Universe, doesn't that mean it cancels out the effects of gravitational fields at longer distances, otherwise the Universe would be curved?
 
Leonardo Muzzi said:
I am thinking about some kind of anti-gravity, dark energy effect, that would prevent a gravitational field from propagating infinitely.

Any such effect would not "prevent" a gravitational field from propagating, because any such effect would show up as an effect on spacetime curvature, and spacetime curvature is the "gravitational field", at least in the sense in which anything can be said to "propagate" in GR.
 
Leonardo Muzzi said:
I am thinking about some kind of anti-gravity, dark energy effect, that would prevent a gravitational field from propagating infinitely.

After all, if dark energy flattens the Universe, doesn't that mean it cancels out the effects of gravitational fields at longer distances, otherwise the Universe would be curved?
I don't think anyone knows the answer to that. Dark energy is not understood in any sense, we don't even know if it exists. Some scientists subscribe to the idea that there is some unknown force or energy that is accelerating the expansion of the universe while others assume that our theory of gravity is incomplete and that this is the cause of the discrepancy. I personally lean towards the latter here.
 
Leonardo Muzzi said:
if dark energy flattens the Universe, doesn't that mean it cancels out the effects of gravitational fields at longer distances, otherwise the Universe would be curved?

Dark energy does not "flatten" the universe. It produces spacetime curvature that is different from the kind produced by ordinary matter and energy, but they don't "cancel each other out" to produce flat spacetime.

You will see cosmologists talking about the universe being "flat", but they mean spatially flat, not flat spacetime. The universe is observed to be spatially flat as best we can tell with our current instruments, and that requires the total energy density (counting dark energy, dark matter, and ordinary matter and radiation) to have a particular value; but that doesn't mean dark energy flattens the universe.
 
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PeterDonis said:
Dark energy does not "flatten" the universe. It produces spacetime curvature that is different from the kind produced by ordinary matter and energy, but they don't "cancel each other out" to produce flat spacetime.
I think the OP is trying to ask if gravity may be attenuated differently at very large distance scales than it is at smaller scales. Maybe some clarification would help?
 
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NFuller said:
I think the OP is trying to ask if gravity may be attenuated differently at very large distance scales than it is at smaller scales. Maybe some clarification would help?

Yes fair enough!

So to rephrase it: In Newtonian physics, if I take an empty Universe and put two Suns perfectly still to each other, 13 Billion light-years away, the gravitational fields of each will affect and attract the other.

Is that still true in GR?
 
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Leonardo Muzzi said:
Is that still true in GR?

Yes.
 
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  • #12
You can't just make Suns appear out of nothing. They have to be constructed from stuff from nearby locations. The gravity between two stars separated by large distance is due to the gravity of the stuff which existed near the stars location in the past.
 

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