- #36
- 27,983
- 19,481
You can only push this sort of flaky mathematics so far before you end up with a contradiction.robphy said:is analogous to describing a plane as a sphere of infinite radius
You can only push this sort of flaky mathematics so far before you end up with a contradiction.robphy said:is analogous to describing a plane as a sphere of infinite radius
PeroK said:You can only push this sort of flaky mathematics so far before you end up with a contradiction.
The sphere and the plane are topologically distinct. The sphere is locally homeomorphic to the plane. Which is a better description than saying the plane is an infinite sphere- which I suggest is mathematically meaningless.robphy said:Descriptions are for intuition.
Equations are needed to support the intuition… and provide the context behind the description.
Descriptions alone (without equations) can lead to all sorts of misconceptions.
Like I said, descriptions need context.PeroK said:The sphere and the plane are topologically distinct. The sphere is locally homeomorphic to the plane. Which is a better description than saying the plane is an infinite sphere- which I suggest is mathematically meaningless.
I think I formally disagree here too. The plane wave approximation is a good approximation far from the source. It is not a spherical wave. (Or vice versa)robphy said:is analogous to describing a plane as a sphere of infinite radius [as one does when describing plane waves].
robphy said:E=1 is Minkowski, E=0 is Galilean.
Call the terms whatever you want.
This construction is consistent with the physics. Feel free to suggest what may be better descriptions.
Source:Einstein said:The Galilei transformation can be obtained from the Lorentz transformation by substituting an infinitely large value for the velocity of light ##c## in the latter transformation.
Sagittarius A-Star said:I think, mathematicians would use a formulation with limit at infinity.
## \lim_{c \rightarrow \infty}{(\gamma (x-vt))} = x-vt, \ \ \ \ \ ## ## \lim_{c \rightarrow \infty}{(\gamma (t-vx/c^2))} = t##
No matter how large you make ##c## I can choose a large ##v## and we see there is actually no physical difference in the geometry depending on the value of ##c##.Sagittarius A-Star said:Also Einstein used a sloppy formulation. I understand, what he meant:
Source:
https://en.wikisource.org/wiki/Rela...art_I#Section_11_-_The_Lorentz_Transformation
I think, mathematicians would use a formulation with limit at infinity.
## \lim_{c \rightarrow \infty}{(\gamma (x-vt))} = x-vt, \ \ \ \ \ ## ## \lim_{c \rightarrow \infty}{(\gamma (t-vx/c^2))} = t##
In that sense, of course!PeroK said:In that sense the limit as ##c \to \infty## is not the Galilean geometry.
In a way that's right. You can derive the Lorentz transformation from the assumption that the special principle of relativity holds and assuming that for inertial observers space is Euclidean and time is homogeneous. Using these assumptions you get either the Galilei transformation and from this you can reconstruct Newtonian spacetime (having no limiting speed) or Minkowski spacetime (having a limiting speed). The Euclidean metric also occurs formally in the solutions, but then you want the transformations between inertial frames to form a group, and when using the Euclidean-metric solution then you'd not be able to set up a causality structure. That's possible in Minkowski spacetime, because for time- or light-like separated events the part of the Lorentz group that is continuously connected with the identity, the proper orthochronous Lorentz group ##\mathrm{SO}(3,1)## (in your sign convention for the metric) the time ordering is invariant, and that's why only time- or light-like separated events can be causally connected. For more details, see. e.g.,accdd said:Isn't the fact that the spacetime metric is not Euclidean due to the fact that there is a maximum velocity in our universe?
maximum velocity ##\implies## everyone agrees on its value ##\implies## derivation of spacetime interval (##ds^2=-dt^2+dx^2+dy^2+dz^2##)
Is this reasoning wrong? Doesn't the fact that spacetime is not Euclidean derive from the fact that there is a maximum velocity?
For me individually, spacetime is clearly non-Euclidean since spacetime "distances" are measured with both clocks and rulers. I don't know how the distinction could possibly be more blatant.Trysse said:I am interested to see, what individual people take as a good explanation respectively as a good answer to the question. I am interested to see what people take as a meaningful explanation. Or what they think is necessary for a meaningful explanation.
I usually use the convention ##ds^2=-c^2 dt^2+dx^2+dy^2+dz^2## and ##c^2 d\tau^2 = c^2 dt^2 - dx^2 - dy^2 - dz^2##, so I can easily switch between the timelike and spacelike conventions.Thadriel said:Why, may I ask, do you prefer this sign convention over the other one?
vanhees71 said:V. Berzi and V. Gorini, Reciprocity Principle and the Lorentz Transformations, Jour. Math.
Phys. 10, 1518 (1969), https://doi.org/10.1063/1.1665000
Well, while this is true as stated, there is a sense in which it is meaningful to talk about such a limit. Given any physical set up (distances in terms of reference objects, speeds define from these plus a notion of ideal clock), then as c is taken to approach infinity, the error of any observation compared to Galilean approaches zero. This is important because having speeds very low compared to c does not make relativistic effects arbitrarily small. No matter how small the speeds compared to c, if the system is large enough, relativistic effects are also large. Both speeds and distances must be 'small' compared to c or ct for relativistic effects to be insignificant.PeroK said:No matter how large you make ##c## I can choose a large ##v## and we see there is actually no physical difference in the geometry depending on the value of ##c##.
In that sense the limit as ##c \to \infty## is not the Galilean geometry.
This is why mathematical analysis is needed so that we know which limits are valid and which are not.
Why invent something (an infinite or near infinite ##c##) that is simply unnecessary?PAllen said:Well, while this is true as stated, there is a sense in which it is meaningful to talk about such a limit. Given any physical set up (distances in terms of reference objects, speeds define from these plus a notion of ideal clock), then as c is taken to approach infinity, the error of any observation compared to Galilean approaches zero. This is important because having speeds very low compared to c does not make relativistic effects arbitrarily small. No matter how small the speeds compared to c, if the system is large enough, relativistic effects are also large. Both speeds and distances must be 'small' compared to c or ct for relativistic effects to be insignificant.
In the "limit-equations" in posting #41, c is not set to infinite, nor to a finite value "near infinite", as can be see from the definition of limit at infinity.PeroK said:Why invent something (an infinite or near infinite ##c##) that is simply unnecessary?
In post #41 you reach the sort of contradiction I am talking about. You show that, if we choose a fixed ##v##, then in the limit as ##c \to \infty##, we have ##\gamma \to 1##.Sagittarius A-Star said:In the "limit-equations" in posting #41, c is not set to infinite, nor to a finite value "near infinite", as can be see from the definition of limit at infinity.
That is what you wrote already in #43 and I replied to in #45.PeroK said:In those terms Galilean relativity is not a continuous limit of Special Relativity as ##c \to \infty##.
I don't agree with post #45. The conclusion that if you increase the invariant speed ##c## then you approach Galilean relativity in some limiting sense is false. The limit argument doesn't work, IMO.Sagittarius A-Star said:That is what you wrote already in #43 and I replied to in #45.
I didn't write or conclude this in #45.PeroK said:The conclusion that if you increase the invariant speed ##c## then you approach Galilean relativity in some limiting sense ...
That is the sloppy formulation from Einstein, I wanted to avoid.PeroK said:You only get Galilean relativity by plugging ##c = \infty## directly into the equations.
You can't avoid it. That's my point. The limit argument fails because the Lorentz Transformation entails transforming between any IRFs. And, however large you make ##c## you have all ##v < c## to consider.Sagittarius A-Star said:That is the sloppy formulation from Einstein, I wanted to avoid.
That is again, what you wrote already in #43 and I replied to in #45:PeroK said:You can't avoid it. That's my point. The limit argument fails because the Lorentz Transformation entails transforming between any IRFs. And, however large you make ##c## you have all ##v < c## to consider.
Sagittarius A-Star said:... The "limit-equations" in posting #41 are valid, if they are regarded as purely mathematical equations, without any reference to physics.
For example, no dependency between the mathematical quantities "c" and "v" is assumed, besides the dependencies stated in those equations. You can't write down the GT and assume at the same time, that actual physics, like described in postulate 2 of SR, is valid.
But, there is a mathematical dependency between ##v## and ##c##. Relativity is about the group of Lorentz transformations. Not just a transformation for a given ##v##.Sagittarius A-Star said:That is again, what you wrote already in #43 and I replied to in #45:
PeroK said:What is valid is that, for a fixed ##c##, as ##v \to 0## then the LT does tend to the Galilean transformation.
You're missing the point. If ##v## is small, then ##\gamma \approx 1##. And you can study a subset of SR where ##v## is small and you have approximately the Galilean transformation.Sagittarius A-Star said:If you mean ## \lim_{v \rightarrow 0}{}##, then you get only a special case of the GT
## \lim_{v \rightarrow 0}{(\gamma (x-vt))} = x-0 \cdot t = x, \ \ \ \ \ ## ## \lim_{v \rightarrow 0}{(\gamma (t-vx/c^2))} = t##
That's correct, except if the ##x## in ##\gamma (t-vx/c^2)## is very large, as @PAllen mentioned in #50.PeroK said:If ##v## is small, then ##\gamma \approx 1##. And you can study a subset of SR where ##v## is small and you have approximately the Galilean transformation.
This is really the scientifically important fact. For SR to be a valid theory the differences between it and Galilean relativity must be smaller than the experimental uncertainty in any domain where Galilean relativity has been experimentally validated. You can express that requirement with several different limits, but the important fact is that in any of those limits the difference must approach zero.PAllen said:as c is taken to approach infinity, the error of any observation compared to Galilean approaches zero