Two dimensional Lorentzian vs Euclidean geometry

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Discussion Overview

The discussion explores the differences between two-dimensional Lorentzian geometry and Euclidean geometry as defined by Euclid's axioms. Participants examine how the axioms of Euclidean geometry apply or fail in the context of Lorentzian geometry, considering implications for concepts such as geodesics, angles, and metrics.

Discussion Character

  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants propose that the interpretation of straight lines in Euclidean geometry as geodesics in Lorentzian geometry leads to difficulties, particularly with axioms 3 and 4.
  • Others argue that all axioms assume the existence of a metric, suggesting that the transition from a metric to a pseudo-metric alters the nature of geometric relationships.
  • A participant claims that Minkowski space fails the first axiom, while another counters that geodesics can connect any two points in Minkowski space.
  • There is a discussion about the nature of geodesics, with some noting that space-like geodesics are also valid and can be considered in the context of the axioms.
  • Some participants introduce the idea of categorizing lines into types (timelike, spacelike, null) to better understand angles and geometry in Lorentzian space.
  • Concerns are raised regarding the treatment of the fourth axiom, with suggestions that allowing only timelike geodesics would lead to a lack of right angles.
  • Participants express uncertainty about how to define angles between different types of geodesics, particularly in relation to null geodesics.
  • References to external materials are shared to provide additional context on the fourth postulate and its implications.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the applicability of Euclidean axioms to Lorentzian geometry, with multiple competing views and unresolved questions regarding the treatment of angles and geodesics.

Contextual Notes

Limitations include the dependence on definitions of angles and geodesics, as well as the unresolved nature of how different types of geodesics interact within the framework of the axioms.

pervect
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Reading a somewhat long and argumentative thread here inspired the following unrelated question in my mind:

Where does a 2 dimensional flat Lorentzian geometry depart from Euclidean geometry as axiomatized by Euclid? I.e. Euclid's axioms (in modern language) can be taken to be:

1. A straight line segment can be drawn joining any two points.

2. Any straight line segment can be extended indefinitely in a straight line.

3. Given any straight line segment, a circle can be drawn having the segment as radius and one endpoint as center.

4. All right angles are congruent.

5. If two lines are drawn which intersect a third in such a way that the sum of the inner angles on one side is less than two right angles, then the two lines inevitably must intersect each other on that side if extended far enough.

We can interpret straight lines in Euclidean geometry as "geodesics" in the Lorentzian geometry. I believe the difficulties start to arise in axioms 3 and 4. A meaningful notion of a "circle" becomes difficult, perhaps we'd replace it with a hyperbola? The concept of rapidity between time-like geodesics is promissing, but doesn't seem to be a sufficiently general replacement for "angle".
 
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I would say that all of the axioms inherently has an assumption on the existence of a metric. From 3 on, you start dealing with things which are not really the same as in Euclidean space if you replace the metric by a pseudo metric. As you say, circles become hyperbolas, I guess we can live with that. Number 4 should be downright false in Minkowski space - you can have several types of vector pairs with an inner product of zero. For example, you can take a time-like and a space-like vector or you can take two space-like vectors. These two sets cannot be transformed into each other by an isometry (i.e., Lorentz transformation).
 
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It fails the first axiom.
...but satisfies the fifth axiom (in Playfair's formulation).
In fact, you can write the first in a form that resembles the projective dual of Playfair.
 
robphy said:
It fails the first axiom.
How? It is perfectly possible to have a geodesic connecting any two points in Minkowski space.
 
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Orodruin said:
There is nothing saying that the line has to be time-like. Space-like geodesics are also geodesics.
The idea comes from I.M. Yaglom's "A Simple Non-Euclidean Geometry and its Physical Basis".
There he distinguishes "lines of the first ["ordinary"], second, and third kind" (corresponding to timelike, spacelike, and lightlike).
It is interesting that the first and fifth axioms can be reformulated in a similar way (via the Playfair formulation) [related by duality].
So, when the first axiom is formulated as such (following Yaglom),
Minkowski fails that axiom since there are point-events that cannot be connected by timelike lines.

The whole scheme is part of what is called "Cayley-Klein Geometry" (what I call Spacetime Trigonometry).
 
So how do you treat the 4th axiom? By only allowing time-like geodesics, there will be no lines at right angles.

While it may be interesting to consider other options, I would consider the direct generalisation of straight lines to general (space-like, time-like, or null) geodesics to be the natural one.

Also to add to my first response, I did not consider the two-dimensional restriction. You cannot have space-like vectors which are orthogonal in two dimensions. However, you still have two different types of right angles, those between a time-like and a space-like geodesic and those between a null geodesic and itself. These form two distinct equivalence classes under Poincaré transformations.
 
Orodruin said:
So how do you treat the 4th axiom? By only allowing time-like geodesics, there will be no lines at right angles.

While it may be interesting to consider other options, I would consider the direct generalisation of straight lines to general (space-like, time-like, or null) geodesics to be the natural one.

Also to add to my first response, I did not consider the two-dimensional restriction. You cannot have space-like vectors which are orthogonal in two dimensions. However, you still have two different types of right angles, those between a time-like and a space-like geodesic and those between a null geodesic and itself. These form two distinct equivalence classes under Poincaré transformations.

I don't know how to handle the fourth axiom.
My goal in my poster (and in answering the OP)
was to identify a Euclidean axiom where Minkowski fails... thus, rendering it as non-euclidean.

The rest of the poster is exploring the Cayley-Klein geometry approach to those 9 two-dimensional geometries
and how it can be applied to physics... specifically, trying to formulate physical concepts in Galilean and Minkowskian relativity in a unified way.
Considering the rest of the euclidean axioms may be interesting... but that hasn't been my main focus.

In the Cayley-Klein approach, the emphasis is on projective geometry (not Euclidean geometry).
 
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I hadn't contemplated breaking up lines into three types, but it does seem to make the concept of "angle" a lot more meaningful. Rapidity as the concept of angle between two timelike geodesics makes perfect sense, my concept of angle with null geodesics would be that they're at a right angle to everything (which is distinctly odd from a Euclidean perspective), and I I'm probably still confusing myself over what "angle" might be between space-like geodesics (especially if we restrict ourself to one spatial dimension), but I probably don't really need to figure that out at this point.

And the consequence of breaking up lines into the different types would be that the first axiom doesn't hold anymore.

Thanks for the references, I haven't read all of them at this point yet.
 
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pervect said:
my concept of angle with null geodesics would be that they're at a right angle to everything

Actually they're not. Null vectors are orthogonal to themselves, but not to null vectors in different directions. For example, in two dimensions, the null vector ##(1, 1)## is not orthogonal to the null vector ##(1, -1)##. Nor are null vectors orthogonal to all non-null vectors; for example, ##(1, 1)## is not orthogonal to either the timelike vector ##(1, 0)## or the spacelike vector ##(0, 1)##. (In three dimensions, null vectors in the t-x plane would be orthogonal to spacelike vectors in the y-z plane.)
 

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