Physical model of measurement for affine geometry, dual

In summary, according to the thread, if you want to measure a vector's length in a space where you don't have a metric, you can use a measure of area and a measure of length along a line that are not parallel.
  • #1
bcrowell
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We recently had a long thread https://www.physicsforums.com/showthread.php?t=666861 about cases where raising and lowering indices isn't completely natural, i.e., where a vector "naturally" wants to be upper-index or lower-index.

If you have a metric, then it's pretty clear to me what real-world measurement processes correspond to the use of the metric. In a Riemannian space, they're basically the ones referred to in Euclid: compass and straightedge or, in some weaker sense, a marked straightedge. In a semi-Riemannian space, you need the universe to contain at least one clock. (A ruler will also work.) Geroch has a very nice popular-level book, Relativity from A to B, that systematically works out this interpretation of GR.

What is the right model of measurement for a space where you don't have a metric but you do have parallelism, e.g., the tangent space on a manifold where no metric exists? In affine geometry, you have a measure of area and you have a measure of length along a line and lines parallel to it. You don't have angular measure, a notion of perpendicularity, congruence, or comparability of vectors that are not parallel. You can take products of vectors with dual vectors, giving real numbers. The best metaphor I've been able to come up with is the ghost of a clock. What I mean by this is that you have a clock that cruises like a ghost through space, moving inertially. You can't interact with it, so you can't, e.g., force it to travel along a curved world-line and measure its proper time. It can move at c or at speeds higher than c. Unlike a physically manipulable clock, it doesn't suffice to establish a frame of reference. You can make copies of it moving along parallel world-lines, but you can't synchronize the copies (because synchronization is perpendicularity). Basically if you take the product of a dual vector with a vector, [itex]\omega\cdot v[/itex], you can think of it as comparing the rate of one ghost-clock against the rate of another ghost-clock.

Is this a correct model? Is there a simpler, more accurate, or more natural model, or one stated in terms of more realistic measuring devices?
 
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  • #2
How about the geometry of null geodesics? That's what I usually think of. But there isn't any real notion of "length" , until you specify a frame of reference. So I'm not sure if it's what you are actually looking for.
 
  • #3
pervect said:
How about the geometry of null geodesics?
But how would you check if a geodesic is null or not? Sure if M is a manifold with linear connection [itex]\triangledown [/itex] then we can just define a curve [itex]\gamma :I\rightarrow M[/itex] as being a geodesic if the covariant derivative (with respect to [itex]\triangledown [/itex] of course) [itex]D_{t}\dot{\gamma }(t) = 0[/itex] but then to demand the geodesic be null we usually require that [itex]\forall t\in I, g_{\gamma (t)}(\dot{\gamma }(t), \dot{\gamma }(t)) = 0[/itex]. How would we define a null geodesic without a metric tensor?
 
  • #4
I wouldn't get rid of the metric tensor to define a null geodesic. But if you have an affinely parameterized curve which is a null geodesic, the length of any segment of the curve will be equal to zero. What I should perhaps have said to be more precise, is that the length (found via the metric tensor) is always zero.

If we used this notion of length, the one from the metric tensor, we'd say that all segments of a null curve "had the same length", because zero = zero. Which is trivally true, and more or less useless.

However, some parameterizations of the null geodesic are affine parameterizations and some are not affine. If we have an affinely parameterized geodesic, we can mark off "equal intervals" along the geodesic according to equal spacings of the affine parameter.

I.e. if the affine parameter is [itex]\lambda[/itex], the interval between [itex]\lambda=0[/itex] and [itex]\lambda=1[/itex] is the same as the interval between [itex]\lambda=1[/itex] and [itex]\lambda=2[/itex].

This notion of 'equal length' is more restrictive enough than the trivial notion of having the same length according to the metric tensor, which is always satisfied and not useful because it's trivial.

Thus we can use Schild's ladder, for instance, to do parallel transport along null geodesics, because we have this notion of "equal length".

So my interpretation of the underlying geometry (the geometry we use to good effect in Schild's ladder, for instance) is that there is a frame independent way to compare lengths (by which I mean the purely spatial part of the distance between two points along a null geodesic), but that the value of said lengths are totally dependent on one's choice of frame and uncertain up to a multiplicative factor.
 
  • #5
bcrowell said:
We recently had a long thread https://www.physicsforums.com/showthread.php?t=666861 about cases where raising and lowering indices isn't completely natural, i.e., where a vector "naturally" wants to be upper-index or lower-index.

To me, the simplest example of a model in which there is a natural notion of parallelism of lines, and distance along a given line, but no metric, is ordinary Euclidean geometry in which different units are used to measure one spatial dimension than the others. For example, on the ocean, in the old days, horizontal distances were measured using nautical miles, while vertical distances were measured using fathoms. Let's use coordinates x and y to measure locations in the horizontal plane, and coordinate z to measure distances in the vertical direction. Imagine a weird law of physics in which objects can rotate freely in the horizontal (x-y) plane, but can't be rotated in the x-z plane or the y-z plane. In the ocean world that I'm talking about, that's approximately the case. The ship itself can easily be spun around in the horizontal plane, but it requires a massive disaster to rotate it in the x-z plane or y-z plane. On the other hand, a chain connected to an anchor can easily be raised and lowered in the z-direction, but it can't easily be laid out in the horizontal direction.

So if objects are constrained to only rotate in the horizontal direction, then there is no good way to compare distances in the vertical direction with distances in the horizontal direction. The most natural geometry for this situation would have separate metrics for the horizontal and vertical directions, and there would be no nondegenerate 3D metric.
 
  • #6
Let me expand on my original answer in a way that I hope is a bit clearer.

bcrowell said:
We recently had a long thread https://www.physicsforums.com/showthread.php?t=666861 about cases where raising and lowering indices isn't completely natural, i.e., where a vector "naturally" wants to be upper-index or lower-index.

If you have a metric, then it's pretty clear to me what real-world measurement processes correspond to the use of the metric. In a Riemannian space, they're basically the ones referred to in Euclid: compass and straightedge or, in some weaker sense, a marked straightedge. In a semi-Riemannian space, you need the universe to contain at least one clock. (A ruler will also work.) Geroch has a very nice popular-level book, Relativity from A to B, that systematically works out this interpretation of GR.

What is the right model of measurement for a space where you don't have a metric but you do have parallelism, e.g., the tangent space on a manifold where no metric exists? In affine geometry, you have a measure of area and you have a measure of length along a line and lines parallel to it. You don't have angular measure, a notion of perpendicularity, congruence, or comparability of vectors that are not parallel. You can take products of vectors with dual vectors, giving real numbers.

My proosal for such a space is null geodesics in flat space-time. You do have parallelism. You also have "similar triangles" in this space, this is used in constructions like Schild's ladder, which can be applied to null geodesics.

(I hope Schild's ladde is familiar? One can find a reference to it in MTW if it's not. It's not really a terribly popular construct, but I personally like it a lot. I have a forum post on it - somewhere or other.)

You have a metric - but it's trivial. The length of any null vector is zero, the dot product of any two null vectors is zero.

You don't have a Lorentz invariant definition of angle. You can somewhat sensibly talk about the "angle" between two light beams (You basically project the null vectors into non-null vectors in some particular frame to get the angle) but the result depends on what frame you use. Or in other words if you construct "orthogonal" light beams in one frame (by making their spatial projectios orthogonal in that frame) they won't be orthogonal in some moving frame. So there isn't any true notion of angle in this space.

Now to repeat, the question was:

What is the right model of measurement for a space where you don't have a metric but you do have parallelism,
And the proposed answer is, in this space, the non-trivial notion of distance is given, up to a scale factor, not by the metric, but by the affine parameterization.

This is all an "intuitive leap" sort of observation, its not something that I've made rigorous.

We can physically interpret this affine parameteriztion.

If you have an EM plane wave, you can mark regular intervals along it in some given frame by taking locations where the E-field is zero in that frame. All frames will agree that the points are "evenly spaced" (I'm not sure they'll all agree that the E-field is zero, but that isn't the claim, the only claim is that they'll agree the points are evenly spaced). And this is the basis of marking out "equal distances" in our affine geometry, rather than using the metric (which always gives zero).

The EM wave is just to provide some physical insight by providing a physical example. Mathematically, all you need is the affine parameterization.
 
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  • #7

What is a physical model of measurement?

A physical model of measurement is a mathematical representation of physical space that allows for accurate measurements and calculations. It is used in affine geometry to study the properties of points, lines, and planes.

How does a physical model of measurement differ from other models?

Unlike other models, a physical model of measurement takes into account the physical properties and constraints of the real world. This means that it can accurately represent distances, angles, and other measurements in physical space.

What is affine geometry?

Affine geometry is a branch of mathematics that deals with the properties and transformations of points, lines, and planes. It is used to study the relationships between these objects in physical space.

What is the dual of a physical model of measurement?

The dual of a physical model of measurement is a mathematical representation of the reciprocal relationships between points, lines, and planes. It allows for the study of projective geometry, which is an extension of affine geometry.

How is a physical model of measurement used in scientific research?

A physical model of measurement is used in scientific research to accurately measure and describe physical phenomena. It can be applied to a variety of fields, including physics, engineering, and architecture, to make precise calculations and predictions.

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