Observation of distances w.r.t. metric

In summary: Yes, the answer to the question is yes, in such conditions one can get a picture how distorted an observer being outside the sphere will see the line.
  • #1
VladZH
56
1
Hello. I don't know exactly if my question can be treated physically but so...
Let us have a 3D space with non-constant metric. We are in the first region with a euclidian metric.
[itex]ds^2=dx^2+dy^2+dz^2[/itex]
So the distance between two points is got through pythagorean theorem
Then near us we have the second region that has another metric such as
[itex]ds^2=a^2dx^2+b^2dy^2+c^2dz^2[/itex]
where [itex]a,b,c[/itex] - some coefficients
In our region we have line with [itex]A(x_1,y_1,z_1)[/itex] and [itex]B(x_2,y_2,z_2)[/itex] at the ends. So the length of the line is [itex]L_1=\sqrt{(x_1-x_2)^2+(y_1-y_2)^2+(z_1-z_2)^2}[/itex]
Then we take our line and put in the second region, so the line ends have coordiantes [itex]C(x_3,y_3,z_3)[/itex] and [itex]D(x_4,y_4,z_4)[/itex]. Its length is
[itex]L_2=\sqrt{a^2(x_3-x_4)^2+b^2(y_3-y_4)^2+c^2(z_3-z_4)^2}[/itex]
The question is:
Will we really observe the line smaller or bigger after putting it into the second region?
 
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  • #2
VladZH said:
Then we take our line and put in the second region
What do you mean by this? The two are different lines, they are not the same lines at different locations.
 
  • #3
Orodruin said:
What do you mean by this? The two are different lines, they are not the same lines at different locations.
By that I mean continuous translation
 
  • #4
VladZH said:
By that I mean continuous translation
Without to know how you define continuity at the border between the two different metric spaces or even the presumably common border itself, and what you mean by "observe", because to live in one metric means to me you only have this metric for comparison, the closest picture I can come up with is someone standing in front of a convex or concave mirror as they can be found in, e.g. amusement parks.
 
  • #5
This still is not well defined. You need to specify what this continuous translation is and how it affects the points on the lines. These things are not unique on curved manifolds. In particular, the way I suspect you will want to define it is going to be coordinate dependent.
 
  • #6
fresh_42 said:
Without to know how you define continuity at the border between the two different metric spaces or even the presumably common border itself
Orodruin said:
You need to specify what this continuous translation is and how it affects the points on the lines.
For example, that region has a border as a circle. But the circle has some width. So the metric is changing smoothly passing through border

fresh_42 said:
someone standing in front of a convex or concave mirror as they can be found in, e.g. amusement parks.
So how can one derive the accurate picture that the observer sees?
 
  • #7
VladZH said:
For example, that region has a border as a circle. But the circle has some width. So the metric is changing smoothly passing through borderSo how can one derive the accurate picture that the observer sees?

This answers nothing about the issues that were raised, or what you mean by an "observer". There is no such thing as "translation" of an extended object in a general manifold. You can define continuous transforms based on parallel transport, but this has issues to. What you are asking is simply not well defined.
 
  • #8
Orodruin said:
This answers nothing about the issues that were raised, or what you mean by an "observer". There is no such thing as "translation" of an extended object in a general manifold. You can define continuous transforms based on parallel transport, but this has issues to. What you are asking is simply not well defined.

Let it be 3D differential manifold. Let we have metrics [itex]g[/itex] that is euclidian and [itex]\eta[/itex] that is
[itex]\eta = \begin{pmatrix}
a & 0 & 0 \\
0 & b & 0 \\
0 & 0 & c
\end{pmatrix}[/itex]
The circle in image represents sphere as a border of region with metric [itex]\eta[/itex](omitted here z coordinate)
Untitled-1.png

Let metric moving in arrow direction changes in a way that when you moving closer to the circle interior it looks like
[itex]\mu = \begin{pmatrix}
\alpha & 0 & 0 \\
0 & \beta & 0 \\
0 & 0 & \gamma
\end{pmatrix}[/itex]
where [itex]\alpha \rightarrow a, \beta \rightarrow b, \gamma \rightarrow c[/itex]
And vice versa, if you moving in opposite direction of the arrow the metric is the same but
[itex]\alpha \rightarrow 1, \beta \rightarrow 1, \gamma \rightarrow 1[/itex]

So do the question in the first post have answer in such conditions?
And again in such conditions can one get a picture how distorted an observer being outside the sphere will see the line?

When I say "observer" I mean the one who just stays there if such manifold was a part of our physical space.
 
  • #9
Your statements are still not mathematically sound, you are just repeating the same thing you have already said.
 
  • #10
Orodruin said:
Your statements are still not mathematically sound, you are just repeating the same thing you have already said.
Could you explain what things I need to define mathematically or maybe guide me that?
Thanks.
 
  • #11
VladZH said:
Could you explain what things I need to define mathematically or maybe guide me that?
Thanks.
You have defined the manifold and the metric, that has never been in question. Your problem is that you have not defined what you mean by "observer" or what the process of this "observation" is supposed to be. You have also not defined what you think it means to perform a "continuous translation". If by this you mean to just make a coordinate translation ##x^\mu \to x^\mu + a^\mu## where ##a^\mu## is a set of constants, what you are trying to do is coordinate dependent and not something which is inherent in the manifold. Any geometrical property you wish to define should not depend on the coordinates you use on the manifold.

From what I understand from your attempts, what you are trying to ask is simply undefined.
 
  • #12
Orodruin said:
Your problem is that you have not defined what you mean by "observer" or what the process of this "observation" is supposed to be.
I see "observating the line" as perceiving light rays that were reflected from the line.
Orodruin said:
You have also not defined what you think it means to perform a "continuous translation". If by this you mean to just make a coordinate translation xμ→xμ+aμxμ→xμ+aμx^\mu \to x^\mu + a^\mu where aμaμa^\mu is a set of constants, what you are trying to do is coordinate dependent and not something which is inherent in the manifold.
So let's regard continuous translation as translation along geodesic curve. AFAIK we can derive a geodesic from the connection and the connection from the metric.
What else do I need?
 
  • #13
VladZH said:
I see "observating the line" as perceiving light rays that were reflected from the line.

The way you have defined it, you are using a fully Riemannian manifold. What do you mean by light ray? Light rays are things in space-times that are 4-dimensional and have a pseudo metric.

It is also not clear whether or not you are "observing" from the outside, i.e., whether or not you assume some sort of embedding or similar which is not really a property of the manifold itself.

VladZH said:
So let's regard continuous translation as translation along geodesic curve. AFAIK we can derive a geodesic from the connection and the connection from the metric.
What else do I need?
This is not enough. The line is an extended object so you will need one geodesic per point on the line and so you will have to properly define this. Once done, whether the line length is changed or not is going to depend on the metric.
 
  • #14
Orodruin said:
The way you have defined it, you are using a fully Riemannian manifold. What do you mean by light ray? Light rays are things in space-times that are 4-dimensional and have a pseudo metric.
Ok, let it be 4d pseudo riemannian manifold and for [itex]\eta[/itex] I'll add the time coordinate that is invatiant for tensor, so
[itex]\eta = \begin{pmatrix}
-1 & 0 & 0 & 0 \\
0 & a & 0 & 0 \\
0 & 0 & b & 0\\
0 & 0 & 0 & c
\end{pmatrix} [/itex]

Orodruin said:
This is not enough. The line is an extended object so you will need one geodesic per point on the line and so you will have to properly define this. Once done, whether the line length is changed or not is going to depend on the metric.
Why isn't it enough if connection is defined everywhere so do geodesics?
 
  • #15
VladZH said:
Why isn't it enough if connection is defined everywhere so do geodesics?
Because of the exact reason I just mentioned.
 
  • #16
Orodruin said:
Because of the exact reason I just mentioned.
So did you mean I just needed to find more than one geodesic?
 
  • #17
VladZH said:
So did you mean I just needed to find more than one geodesic?
You need to assign a method of assigning a geodesic to each point in the line, i.e., you need to define the 4-velocity of each point.

You also need to note that if you have an actual physical object, it is going to be held together by forces such as EM forces. This will mean the object's parts are not moving along geodesics.
 

Related to Observation of distances w.r.t. metric

1. What is the metric used for measuring distances in observation?

The metric used for measuring distances in observation is typically the Euclidean metric, which is based on the Pythagorean theorem and measures the shortest distance between two points in a flat, 2-dimensional space.

2. How is distance measured in astronomy?

In astronomy, distance is often measured using the astronomical unit (AU) or the light-year (ly). The AU is equal to the average distance between the Earth and the Sun, while the light-year is the distance that light travels in one year.

3. How do scientists measure large distances, such as between galaxies?

Scientists use different methods to measure large distances, such as parallax, redshift, and standard candles. Parallax involves measuring the apparent shift in the position of an object from two different vantage points. Redshift is a measure of how much an object's light has been stretched due to the expansion of the universe. Standard candles are objects with known luminosity that can be used to estimate distances based on their apparent brightness.

4. How does the metric affect our understanding of the universe's expansion?

The metric plays a crucial role in our understanding of the universe's expansion. By measuring the distances between galaxies using various methods, scientists have been able to determine that the universe is expanding at an accelerating rate. This has led to the development of the concept of dark energy, which is thought to be responsible for this expansion.

5. Can the metric be used to measure distances in curved space?

Yes, the metric can be used to measure distances in curved space. In fact, the metric used in general relativity is based on the concept of curved space-time. This allows for the measurement of distances in the presence of massive objects, such as planets and stars, that curve the fabric of space-time around them.

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