Q-reeus wrote:Mikko wrote:Be careful with the definitions. Would you call a space where ds² = r² (dr² + df²) "locally Euclidean"?
Depends on what f stands for, and whether one considers a truly differential spatial expansion about some given point.
Mikko wrote:It is one of the coordinates, the other one is r.
Q-reeus wrote:Which cannot be logically reconciled with the 'equally valid' finding in part 1 that zero interior spatial 'redshift' must apply.
Now if you think there is a logical or arithmetical error in parts 1 or 2 of current v3 of viXra article (sans any reference therein to ISM), it's long overdue for you to point to it.
Mikko wrote:Most of the part 1 looks good, from the beginning to formula 1-7. From that point on the discussion is affected by your confusion about coordinate systems. As you have now sorted that out, you should be able to fix it. Just be careful that your updated conclusion follows from your calculations. At that point new errors easily slip in.
At that point it clicked - even though all spatial metric components expand equally as a function of r, the mean change of r metric component between r and r+dr is just half that of the circumferential components which are evaluated only at the radial end-points r and r+dr.
Q-reeus wrote:Where in part 3 the provision that ISM 'isotropy' might be entirely illusory was already given (now confirmed).
Mikko wrote:The isotropy of isotropic coordinates is not illusory.
It is a property of a coordinate system, not of space.
But the space has an important property, too: some spaces allow isotropic coordinate systems, some don't. That way having an isotropic coordinate system tells something about the space, whereas having an anisotropic coordinate system does not tell the opposite.
The prose after the equation 1-7 needs correction. As written v3, it refers to spatial anisotropy as if it were a property of the space.
I cannot really comment the corrected text that I havn't seen, and there is no point to comment the erroneous text now that you understand at least the most obvious error.
The weak field calculations in section 2 are easier with isotropic coordinates. In a weak field the difference between the two coordinate systems is neglible.
The calculation is still easier in Cartesian coordinates. The spherical coordinates do not work that well for off-center masses. With isotropic coordinates the transition to Cartesian coordinates is simple.
The comparison to Yilmaz gravity is also easier in isotropic coordinates as the expression of the line element is much simpler than in Schwarzschild coordinates. Just make sure that you have the thin shell at the right place, which is defined in terms of the Schwarzschild coordinates. The isotropic radial coordinate is different, and in Yilmaz space different from Schwarzschild space.
If the analysis of the situation in Yilmaz space were properly written, it would be the most interesting part of the paper.
Mikko wrote:If you only compare Schwarzschild space with Schwarzschild coordinates to Yilmaz space with isotropic coordinates, you may get two kinds of differences: some are consequences of different coordinate systems, other of different spaces. You need to sort out which is which.
It might be easier to avoid conceptual confusions if different symbols are used for Schwarzschild's and insotropic radial coordinates. Perhaps you could use ŕ or ř or ȓ (and for the coordinate of the shell Ŕ or Ř or Ȓ) or some other decoration.
Q-reeus wrote:Ignoring mechanical strains, for SM the diameter or circumference of shell is on both a proper and coordinate basis totally unaffected by gravity.
Mikko wrote:[The diameter of the shell is R because that is how the situation is specified. If you wish, you may consider that the definition of R. Anyway, that truth is unaffected by anything, for nothing can override the specification.
If you don't appreciate what that last bit means in context of spherical shell scenario, recall that by definition the shell 'areal radius' R is defined in terms of proper area A (or equivalently circumference C) - i.e. R = √(A/(4π)) = C/(2π).
The circumference is 2πR because space is euclidean in the interior. No choice of coordinates can alter that.
Of course, in a different theory with non-zero gravity in at least a part of the interior would have a different relation between the radius and the circumference.
Q-reeus wrote:The circumference is 2πR because space is euclidean in the interior. No choice of coordinates can alter that.
Well for sure in SM the above reproduced 'areal radius' definition can only consistently hold if the interior is not just Euclidean but spatially non-depressed Euclidean i.e. √(g_rr) = 1 exactly for all r<R.
Mikko wrote:In Euclidean geometry the ratio of circumference to radius is always 2π. If you find anything else then your geometry is non-Euclidean.
Q-reeus wrote:As per part 1 of article, there must be an asymptotic correspondence in the weak gravity regime between Newtonian gravity and any reasonable metric theory. So we know the interior will be equipotential thus Euclidean barring just maybe a vanishingly small correction in some higher order powers/derivatives of metric. YM demonstrably has no issue with that.
Mikko wrote:In GR the interior spatial metric is not merely asymptotically Euclidean but exactly. This corresponds exactly to the Newtonian zero gravity.
But you have not made it clear why do you consider is as any anomaly, nor how would YG be any better (or otherwise different). The only difference you have shown is that you prefer to use Schwarzschild coordinates with GR but not with YG and isotropic coordinates with YG but not with GR.
As both coordinate systems are quite reasonable in for both GR and YG, this hardly constitute any anomaly, even in your preferences.
Q-reeus wrote:The natural metric choices - the ones appearing as originally derived, are anisotropic SM and isotropic YM respectively.
Numbers of times over this now six pages of dialogue I have asked you to specifically find fault with in particular the math derivation (and underlying assumptions) of part 2 of v3 article.
Mikko wrote:One coordinate system is not more natural than another, they are all artificial. We often say that same choice is "natural" if it makes something simpler than any other choice, but saying so does not make it so -- we just are sloppy with the language.
And anyway, simplicity depends on purpose. It your intent is to compare two spaces, it is not natural to choose different coordinate systems and let the difference obscure the comparison.
There are still problems in part 1 and in those parts of part 3 that do not depend on part 2.
Discussion of part 2 does not solve them.
Anyway, if you write explicitely the formula for ds² in the interior region (in the same style as you have for the exterior region), that would clarify the part 1 and probably part 2, too.
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