Landau's Derivation of Lorentz Transformations: Questions Answered

In summary, the Lorentz transformations can be described using the invariance of the interval between two events. This assumption requires that the origins of the two coordinate systems coincide.
  • #1
Luke Tan
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In his book, Landau derives the Lorentz transformations using the invariance of the interval, and I have some questions about it that I would like to clarify
Screenshot_639.png

1. What is a parallel displacement of a coordinate system?

Does it refer to moving along any axis?

I don't see how any arbitrary translation of the origin will change the interval between any two events

Screenshot_640.png

2. Does this assume that the origins of the two coordinate systems coincide?

The interval between two events is ##s^2=c^2(t_2-t_1)^2-(x_2-x_1)^2##

For this to reduce to ##s = c^2t^2-x^2## this requires that ##x_1## is zero. However, considering that ##x_1## and ##t_1## are the coordinates of the origin, this would imply that in his equations he has assumed that the origin of both systems coincide.

While I understand that this is correct at some instant, would this not become inaccurate as time passes and the origin of one coordinate system moves away?

Any help would be appreciated
Thanks!
 
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  • #2
Luke Tan said:
1. What is a parallel displacement of a coordinate system?
It appears to be any translation - so excludes a translation and scaling (since ticks on some axes wouldn't move in parallel lines).
Luke Tan said:
2. Does this assume that the origins of the two coordinate systems coincide?
I think so, yes. But we may freely translate our coordinate systems so that this is true.
Luke Tan said:
While I understand that this is correct at some instant, would this not become inaccurate as time passes and the origin of one coordinate system moves away?
This is the origin of a coordinate system in spacetime - it's a specified place and time. It doesn't move, any more than "in my back garden at 11am last Tuesday" moves.
 
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  • #3
Luke Tan said:
1. What is a parallel displacement of a coordinate system?

Does it refer to moving along any axis?

I don't see how any arbitrary translation of the origin will change the interval between any two events

It refers to just adding arbitrary constants to each coordinate so, in effect, a translation. His point is exactly that it is trivial that such translations leave the interval invariant so he will not discuss that explicitly.
Luke Tan said:
While I understand that this is correct at some instant, would this not become inaccurate as time passes and the origin of one coordinate system moves away?
To underscore @Ibix point, the coinciding origin refers to the spacetime origin, not the spatial origin (which is a frame dependent world line).
 
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  • #4
Well, the space-time translations may be "trivial" in the sense of the transformation, but as a symmetry it implies the conservation laws for energy and momentum, which is not quite that unimportant, I'd say ;-))).
 
  • #5
vanhees71 said:
Well, the space-time translations may be "trivial" in the sense of the transformation, but as a symmetry it implies the conservation laws for energy and momentum, which is not quite that unimportant, I'd say ;-))).
Of course not, trivial does not mean unimportant or uninteresting.
 
  • #6
In general relativity, the spacetime coordinates xa are not tied to a metric interpretation, i.e. they are dimensionless. Because of this, their meaning is tied to the solutions represented on them. Without the metric tensor gabdxadxb, these coordinates have no meaning. The location of an event is not determined simply by a choice of coordinates, but also a choice of gauge. In special relativity, the coordinates are defined by the properties of a particular solution called Minkowski space, so they are given in meters and seconds.

Consider a sheet of paper on which a map is drawn. The map can be deformed and moved on the page. The points of the sheet of paper have no meaning independent of the map. The map corresponds to the gravitational field, and the sheet of paper corresponds to the coordinates. The freedom to deform and move the map is a gauge freedom. The sheet of paper is an artifact of this gauge freedom, and has no real meaning other than to facilitate the description of the map drawn on it. The smooth deformations of the map are called diffeomorphisms. Because of the fact that these deformations of the map represent the same physical situation, whatever physical laws the gravitational field satisfies must be invariant under these diffeomorphisms. The simplest formulation of laws will be 'generally covariant' in this sense, because the gauge symmetries must be reflected in the physical symmetries, i.e. acceleration is also in some sense a 'linear transformation' in the sense that a frame accelerated with respect to an inertial frame is also an inertial frame due to the equivalence principle.

Imagine a bucket of water which rotates. The edges of the water surface will rise. This, according to Newton, must be ascribed to the rotation with respect to 'absolute space'. Newtonian mechanics involves the idea of an acceleration d2x/dt2 with respect to this absolute space. In relativity, this so-called 'absolute space' is nothing but the particular spacetime solution we happen to live in. The idea of acceleration with respect to 'abosolute space' is replaced by the idea of an acceleration with respect to the gravitational field.
 
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  • #7
PrashantGokaraju said:
In general relativity, the spacetime coordinates xa are not tied to a metric interpretation, i.e. they are dimensionless.
This is wrong. While you certainly can have dimensionless coordinates in GR, many of the coordinates will not be dimensionless. Consider the r and t coordinates of the Schwarzschild metric as an example. The metric tensor is important in terms of physical interpretation, but this in no way stops coordinates from having physical dimension. (That x = 2 m has absolutely no meaning without knowing the metric is a separate issue.)
PrashantGokaraju said:
In special relativity, the coordinates are defined by the properties of a particular solution called Minkowski space, so they are given in meters and seconds.
Absolutely nothing stops me from imposing dimensionless coordinates on Minkowski space. I can use ##\xi = x/R## and ##\tau = t/T## for some constants R and T. Those coordinates will be dimensionless. (Of course R and T will show up in the metric in those coordinates, but I did not change the fact that I am still in Minkowski space.)
 
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  • #8
The coordinates in general relativity do not have any significance independent of the gravitational field. If you have two world lines which coincide at a point, the location of that point is not a gauge invariant concept in general relativity. Because of the gauge invariance of general relativity, the equations of motion for the gravitational field cannot have any dynamical meaning. The solutions are 'off-shell'
 
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  • #9
Orodruin said:
It refers to just adding arbitrary constants to each coordinate so, in effect, a translation. His point is exactly that it is trivial that such translations leave the interval invariant so he will not discuss that explicitly.
To underscore @Ibix point, the coinciding origin refers to the spacetime origin, not the spatial origin (which is a frame dependent world line).
Yes, but in a galilean transformation we consider that the origin is translating spatially, so why should we consider the origin to always coincide in a lorentz transformation?

Galilean transformations preserve spatial distances, but that doesn't mean that galilean transformations are spatial rotations.

By analogy, why are spacetime transformations different?
 
  • #10
Luke Tan said:
Yes, but in a galilean transformation we consider that the origin is translating spatially, so why should we consider the origin to always coincide in a lorentz transformation?
Because the full group that include space snd time translations is called Poincaré transformations. Normally only Lorentz transformations are considered because translations do not add any conceptual difficulty. It is trivial that they also conserve the spacetime interval.
 

FAQ: Landau's Derivation of Lorentz Transformations: Questions Answered

1. What are the Lorentz transformations and why are they important?

The Lorentz transformations are mathematical equations that describe how measurements of space and time change when viewed from different frames of reference. They are important because they are a fundamental part of Einstein's theory of special relativity, which revolutionized our understanding of space and time.

2. Who is Landau and what is his contribution to the derivation of Lorentz transformations?

Lev Landau was a Soviet physicist who made significant contributions to the fields of theoretical physics and astrophysics. In 1937, he published a paper that provided a clear and concise derivation of the Lorentz transformations, which had previously been derived by Henri Poincaré and Albert Einstein using more complex methods.

3. What is the significance of Landau's derivation?

Landau's derivation of the Lorentz transformations is significant because it provides a more intuitive and elegant approach to understanding these equations. It also highlights the fundamental principles of special relativity, such as the constancy of the speed of light and the relativity of simultaneity.

4. How does Landau's derivation differ from previous derivations?

Previous derivations of the Lorentz transformations involved using mathematical equations and concepts from electromagnetism and geometry. Landau's derivation, on the other hand, is based on the principle of relativity and the concept of time dilation. This makes it more accessible to those without a strong background in mathematics.

5. Can Landau's derivation be applied to other physical phenomena?

Yes, Landau's derivation of the Lorentz transformations is a general and fundamental principle that can be applied to various physical phenomena. It has been used in fields such as particle physics, astrophysics, and cosmology to understand the behavior of particles and objects at high speeds and in different frames of reference.

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