B Can space be curved in relation to an absolute straight space?

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Space can be curved intrinsically without needing an external reference for comparison, as demonstrated by the geometry of a sphere. When walking on a sphere, the angles of a triangle formed by three points will sum to more than 180 degrees, indicating intrinsic curvature. This intrinsic curvature is significant in general relativity, which does not rely on an absolute straight space for its definitions. The distinction between intrinsic and extrinsic curvature is crucial; extrinsic curvature requires an external reference, while intrinsic curvature can be measured within the space itself. Ultimately, the concept of curvature does not necessitate the existence of an absolute straight space for validation.
  • #31
I would try to correct and improve my scenario.

Let us prepare two sphere of same area putting at center nothing for sphere 1, massive body for sphere 2.
Radius 2 is larger than radius 1 where radius means the physical distance from the center of the sphere.
Let us imagine life form in 4D Cartesian super world where our world is built in. He observe these spheres.
He observes a radius of sphere 1, say OA where A is a point on the sphere, same way as us.
As for sphere 2 he observes also another OA line that is along our warped world so lengthy. He observes on sphere 2 both the straight thus out of our 3D world OA line and the curved OA line lying in our 3D warped world. Referring to post #6, OP would be happy if he were such a 4D life form.

Draw a circle on a paper. Drop some water on the part of paper around the center of the circle. The paper partly inflates so some co-center ripple circles appear. We can see ups and downs line from center to circle on the paper ...wwwwwwwwww... that is longer than the original straight radius before wet that we can still imagine or even draw in the space out of the paper. I think such is a 2d similar case to my 3d scenario.

My scenarion should not be regarded as an exact one ,for example warped world does not remain in the sphere but goes beyond it.
Best.
 
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  • #32
That scenario is supposed to explain something? It seems far more muddled than the subject matter being explained.

Invoking general relativity to explicate the concept of curved space time that goes into an understanding of general relativity seems a bit recursive.
 
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  • #33
Hi. In my scenario post #31 I try to show OP's suspect,

PauloConstantino said:
How can you tell something is curved at all? You need a reference point, that is, something which isn't curved at all. And so there must be an absolute straight space to compare curved space with, and so the real space must be straight.

can be affirmatively accepted. His "real"( though I would rather say hypothetical and convenient for interpretation) absolute straight space corresponds to my 4D Cartesian super space.  My lengthy curved OA line of sphere 2 belongs to his curved " not real" ( I would say real ) space.   Best.
 
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  • #34
sweet springs said:
His "real"( though I would rather say hypothetical and convenient for interpretation) absolute straight space corresponds to my 4D Cartesian super space.

"Hypothetical and convenient for interpretation" is not the same as "logically required". The OP was claiming the latter. That claim is not correct.
 
  • #35
I see. Thanks for your tutoring.

I am interested in physics which deals existing things. I have no idea about relation between logically required and physical existence. For example Some mathematical constants, e.g. ##\pi##,e is logically required but I am almost sure that it does not physically exist. I am not sure all the existing things are required logically. Maybe it is no use to talk about physical existence of such absolute straight space of our interest until we have a physical maneuver to check it or it becomes a marvelous hypothesis to explain a lot of phenomena. Best.
 
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  • #36
sweet springs said:
Maybe it is no use to talk about physical existence of such absolute straight space of our interest until we have a physical maneuver to check it or it becomes a marvelous hypothesis to explain a lot of phenomena.
Yes. This is the point about general relativity. You can define manifolds without reference to an embedding, in terms of set theory. And no physics requires any of the concepts that embedding a manifold in a higher dimensional space provides. So we have a situation where adding a space in which to embed spacetime does nothing except let us embed spacetime.

Occam's razor strongly suggests that you drop the idea, lest it lead you in completely the wrong direction if and when evidence inconsistent with GR turns up.
 
  • #37
PauloConstantino said:
Is this the sense in which space is curved?

Can anyone comment on this please
Briefly, if a circle has circumference ## 2 \pi r ## then the space is flat. Otherwise the space is not flat.
Alternatively, if the angles of a triangle add up to ## \pi ## then the space is flat, otherwise it is not.
[EDIT - circumference not diameter!]
 
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  • #38
sweet springs said:
I am interested in physics which deals existing things.

How do you test, experimentally, whether something "exists" or not?

sweet springs said:
I have no idea about relation between logically required and physical existence.

"Physical existence" is not a precise concept so this is not surprising. But this thread is about what is logically required to define the concept of curvature of a manifold.
 
  • #39
I'm trying to answer the OP's question without using extrinsic curvature at all. We keep coming back to that, which is likely only enhancing his belief that it is required.

You and I are in a spaceship and we both start out 1 million kilometers apart and on parallel paths.
We fly past the sun.
Each of us maintains a course that is straight to several decimal places.

After passing the sun, we discover that we are actually converging, even though neither of us has changed our heading.
When we finally meet, we measure our angle of intersection and draw a diagram of the triangle formed by our two starting points and our intersection.

The angles at our starting points are both 90 degrees (we were alongside each other and moving parallel) but our intersection is much less than 90. In curved space, parallel lines can converge (or diverge). When the angles of a triangle do not add up to 180, we know we are embedded in curved space.

We know, without external reference that we have been moving through curved space. Notice that there was no 3D surface upon which we moved, or made reference to. We simply flew straight on our parallel courses.

Alternately, if we used each other to establish parallelicity, we would find that we would have to make course corrections to our heading in order to remain at the same distance apart. We would have to veer off our straight course away from each other just to keep our 1 million km distance.
 
  • #40
DaveC426913 said:
Each of us maintains a course that is straight to several decimal places.

A key part of this is to define, physically, how this is done. The way it is done is to stay in free fall, as accurately as you can measure. That is important because you can measure whether you are in free fall without any input from outside the spaceship.

DaveC426913 said:
(The only sticky bit is this: how did we know we were moving in straight lines?)

It's not "sticky", just important to make clear. See above.
 
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  • #41
PeterDonis said:
The way it is done is to stay in free fall, as accurately as you can measure. That is important because you can measure whether you are in free fall without any input from outside the spaceship.
Nicely done.
 
  • #42
Paulo Constantino, the purpose of my response is to just encourage you in your pursuit of understanding. Your intuition seems to be driving you to pursue some underlying fundamental aspect of space. I’ve tried thinking through the problem from the viewpoint implied by your questioning. So far I haven’t developed a string of thoughts that I feel would provide you with a satisfactory response. Yet I can’t help but feel that your questions are worthy of discussion here.

It was of course very necessary to first make sure you understand the intrinsic and extrinsic curvature concepts. I think that by now you’ve had ample instruction about that. We who have been through a doctoral program in Relativity had that drummed into our heads early in our grad school courses. Yet, I am still sympathetic with the direction your intuition drives you. Further discussions genuinely trying to respond to your fundamental question, expanding beyond the mathematical definitions of curvature and the “mass tells space how to curve, and space tells mass where to go” would probably soon get out of the intended bounds for discussion on this Forum. If it makes you feel any better, I’m sure there are other members of the forum who share your wonder about the fundamental nature of space.
 
  • #43
PeterDonis said:
A key part of this is to define, physically, how this is done. The way it is done is to stay in free fall, as accurately as you can measure. That is important because you can measure whether you are in free fall without any input from outside the spaceship.
It's not "sticky", just important to make clear. See above.

Even in free fall aren't the craft still subject to their mutual gravitational attraction causing their paths to converge?
Measurements in free fall without any input from outside the ship... include Weyl and Ricci?
 
  • #44
bahamagreen said:
Even in free fall aren't the craft still subject to their mutual gravitational attraction causing their paths to converge?

In GR, gravity is not a force. The craft are in free fall, moving on geodesics of the spacetime they are in. The geometry of that spacetime is affected by the stress-energy of the craft, which makes it curved, so the geodesics the craft are moving on converge.

bahamagreen said:
Measurements in free fall without any input from outside the ship... include Weyl and Ricci?

No; measuring that you are in free fall, by itself, doesn't tell you the curvature (if any) of the spacetime you are in. It just tells you that you are moving on a geodesic of whatever the spacetime geometry is.

If the two ships want to know whether they are converging, diverging, or neither, they can exchange light signals. In the case @DaveC426913 described, the light signal exchange will tell them that they start out neither converging nor diverging (i.e., at rest relative to each other), but then start converging. That tells them that the spacetime they are in must be curved, because in flat spacetime, if they started out at rest relative to each other and were both in free fall, they would stay at rest relative to each other forever.

None of these measurements require any "embedding" of the spacetime in a higher dimensional space. But the second measurement (exchanging light signals) differs from the first in that neither spaceship can make it on its own; the two need to cooperate, unlike the measurement of being in free fall, which each ship can do on its own, with no outside input.
 
  • #45
PauloConstantino said:
What I want to say is that it seems to me impossible for something to be curved unless it is curved in relation to absolute straightness.
I think PauloConstantino is looking for a more fundamental answer, about against which reference space is curved.
My answer would be: against an mathematical Euclidean space, which is absolute straight, connected to the masses causing the curvature.
Measuring is easy: sit on the mass (earth) under a tree and see an apple fall.
 
  • #46
DParlevliet said:
My answer would be: against an mathematical Euclidean space, which is absolute straight, connected to the masses causing the curvature.
Your answer is not consistent with the mathematics of general relativity.
 
  • #47
DParlevliet said:
I think PauloConstantino is looking for a more fundamental answer, about against which reference space is curved.

And if that is the answer he is looking for, then such an answer does not exist, because the concept of curvature that is used in GR is intrinsic curvature, which, as has already been pointed out a number of times in this thread, is not defined against any reference space. It is an intrinsic property of the manifold and its metric and does not require comparison with anything else.

DParlevliet said:
My answer would be: against an mathematical Euclidean space

And this answer is wrong. See above.

DParlevliet said:
Measuring is easy: sit on the mass (earth) under a tree and see an apple fall

That doesn't tell you that spacetime is curved; if you in a rocket accelerating at 1 g in flat spacetime, and you release an apple, it falls the same way it would if the rocket were sitting at rest on the Earth's surface.

Spacetime curvature is tidal gravity, so you need to measure tidal gravity in order to measure spacetime curvature.
 
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  • #48
DParlevliet said:
I think PauloConstantino is looking for a more fundamental answer, about against which reference space is curved.
We all agree with you that that is what he wants. Unfortunately he's badly confused about how curvature is defined in relativity - there is no such reference. Or at least, we've no evidence of one and we don't need one to describe any known physics. So he's doomed to disappointment.
 
  • #49
Then I am doomed to disappointment too. I will think about it.
 
  • #50
DParlevliet said:
Then I am doomed to disappointment too.
It's all about expectations management. You should not expect all naming conventions in math and science to be intuitive. Here in particular, using the same term "curvature" for the extrinsic and the intrinsic one might not have been ideal.
 
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  • #51
Allright, I understand that because spacetime is an intrinsic curvature it does not need a reference. However basically both extrinsic and intrinsic curvature are curved against what an observer sees, its mathematical Euclidean space. This probably is not useful for GR theory and calculation, but can be used for understanding spacetime curvature by layman (as I am). If GT would be extrinsic curved, like a cylinder, it would also cause gravity (of a very different shape). I suppose (until he answers) that PauloConstantino understands space as what we see, so if space is curved then our reference, our observations are curved too.

Anyway, to rephrase I think that spacetime is also curved against the mathematical Euclidean space of an observer. This is not the reference, but a self chosen reference. This approximation shows easily the effects of curvature and is useful for simple calculations, like the radius of the curvature on the Earth's surface. But indeed this is not useful for GT theory and will fail in details and extreme situations.
 
  • #52
DParlevliet said:
This probably is not useful for GR theory and calculation, but can be used for understanding spacetime curvature...
Or rather misunderstanding it.

DParlevliet said:
If GT would be extrinsic curved, like a cylinder, it would also cause gravity (of a very different shape).
Nope. Any extrinsic curvature of space-time would undetectable within space-time, per definition.
 
  • #53
DParlevliet said:
basically both extrinsic and intrinsic curvature are curved against what an observer sees, its mathematical Euclidean space.

This is not correct. Measuring intrinsic curvature does not require comparison with anything else. This has already been pointed out several times in this thread.

DParlevliet said:
to rephrase I think that spacetime is also curved against the mathematical Euclidean space of an
observer

This is personal speculation and is off topic here. Please review the PF rules.
 
  • #54
A.T. said:
Any extrinsic curvature of space-time would undetectable within space-time, per definition.
Indeed then my understanding of spacetime curvature was wrong. So I suppose that if a space is curved extrinsic, an observers Euclidean space is curved in the same way, so he does see this curvature. Or perhaps better: the observers Euclidean space does not have (does not see) the dimension in which it is extrinsic curved. An intrinsic curvature is visible inside the observers Euclidean space.

Still we see the effect of spacetime curvature as a curvature in our "straight" Euclidean space, isn't it? When on Earth I am looking to a photon passing Earth I see a curvature in his path, which I can measure. I suppose that is curved space as it shows to me. Or is my Euclidean space curved?

Please don't be irritated about my statements. It is just a way to figure out how it works and I appreciate your answers. Everybody is using models and I am searching for an easy one which perhaps does not follow exact GT calculation, bus is also not really wrong.
 
  • #55
DParlevliet said:
So I suppose that if a space is curved extrinsic, an observers Euclidean space is curved in the same way

No. Forget about extrinsic curvature of spacetime; the concept is not used at all in GR and has no physical meaning.

DParlevliet said:
Or perhaps better: the observers Euclidean space does not have (does not see) the dimension in which it is extrinsic curved

No. There is no "observer's Euclidean space".

DParlevliet said:
An intrinsic curvature is visible inside the observers Euclidean space.

No. There is no "observer's Euclidean space".

DParlevliet said:
Still we see the effect of spacetime curvature as a curvature in our "straight" Euclidean space, isn't it?

No. There is no "straight Euclidean space" in the sense you are using the term. Spacetime curvature is tidal gravity. We observe tidal gravity without having or needing any "straight Euclidean space" to compare with.

DParlevliet said:
When on Earth I am looking to a photon passing Earth I see a curvature in his path, which I can measure.

No. The photon is traveling on a geodesic of spacetime, i.e., a straight line in a curved geometry. The apparent "curvature" of its path in space is an artifact of using a particular coordinate chart, i.e., a particular splitting of spacetime into "space" and "time". Different splittings give different apparent "curvatures", but none of them are what we are talking about when we talk about spacetime curvature.

The way to see spacetime curvature with photons is to compare the paths of different nearby photons--for example, take two photons which both make close approaches to the Sun, but at slightly different altitudes. The photons will converge as they approach the Sun and then diverge as they fly back out away from the Sun. That is due to tidal gravity, i.e., spacetime curvature. But you need the comparison of both photons' paths to see it.

DParlevliet said:
I am searching for an easy one

The simplest model that will give you reliable answers is the one I stated above: spacetime curvature is tidal gravity.
 
  • #56
DParlevliet said:
...the observers Euclidean space ... our "straight" Euclidean space...
What is this "observer's Euclidean space" of which you speak? There is no Euclidean space outside of geometry textbooks describing a mathematical abstraction that does not exist in the real world - the universe we live in is not Euclidean.
 
  • #57
Nugatory said:
...a mathematical abstraction..
Indeed I suppose that this is what I mean. I notice a curvature of (existing) space against what "I see"', which is probably a mathematical (non existing) straight XYZ "space". Perhaps this is not the curvature of GT calculations, but still results in a curvature in what I see.
 
  • #58
DParlevliet said:
Indeed I suppose that this is what I mean. I notice a curvature of (existing) space against what "I see"', which is probably a mathematical (non existing) straight XYZ "space".
This seems to me to be a statement that spacetime is curved because it's not flat. Which is true, but not very helpful.

What we do is determine the components of the Riemann tensor. If they're all zero then we call the space flat. Otherwise we call it curved.
 
  • #59
DParlevliet said:
I notice a curvature of (existing) space against what "I see"'

This makes no sense. What you "see" is the curved spacetime. You don't "see" anything else.
 
  • #60
DParlevliet said:
Indeed I suppose that this is what I mean. I notice a curvature of (existing) space against what "I see"', which is probably a mathematical (non existing) straight XYZ "space". Perhaps this is not the curvature of GT calculations, but still results in a curvature in what I see.
One thing that you need to understand about extrinsic curvature is that it always occurs in a higher dimensional flat space. If I recall correctly, even a simple spacetime like the Schwarzschild metric would require a 6D flat space for embedding.

So it wouldn't be a "straight XYZ space", but a straight UVWXYZ space. Do you "see" that?
 

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