How useful are indefinite state spaces?

In summary, the conversation discusses the use of Nevanlinna space and Krein space in generalized quantum mechanics. The speaker argues that bounded operators are not natural and too limited, and instead suggests using Nevanlinna spaces which allow for unbounded unitary operators. They also mention that in their opinion, bounded operators are not used much in quantum mechanics. The other person in the conversation disagrees, citing the success of bounded operators in quantum information theory and nonrelativistic quantum mechanics. They also mention that most rigorously studied QFTs are constructed in Hilbert space. The speaker responds that these examples do not belong to proper Lorentz covariant physics and that they have successfully constructed a nonperturbatively defined quantum gravity theory using
  • #36
A. Neumaier said:
The work for which Gromov received the prizes is commonly agreed to be rigorous according to the standards of today. (I don't care about prizes, but they reflect the recognition of the community, and hence are useful for comparison. Those who select the prize winners don't care about prizes either, they care about brains.) Gaps do not matter as long as the community agrees that they can be filled. Hardly any mathematician aspires to rigor in the sense of the logicians, where even the smallest gap is filled.
So perhaps then, it is just a matter of people actually having studied his work and thought about it in great detail for a long while? Note that Gromov often doesn't even care about giving proper definitions. God praise those people who have actually taken the effort for that and not just thrown away the manuscript because not everything was written down in what they conceive as a very precise way. :wink: So, what was our discussion again about? Nevanlinna spaces which are not rigorous, unbounded operators which are troublesome or eh new equations whose integrability has not been formally shown yet ? Let me tell you that even in Clifford analysis, similar, but much easier, types of equations than the ones I construct have been investigated and plenty of solutions have been found. But alas, no rigorous integrabilty theorem has been constructed yet even in those simple cases as far as I know.


A. Neumaier said:
So not even on that you have a definite account, not even at the level of rigor of theoretical physics.
If you continue to make such idiotic and manifestly false comments, our discussion is over. There is still discussion in our days about the probability interpretation of QM and the equations have been constructed 90 years ago. You constantly show that you do not understand how theoretical physics works; perhaps you should remain with those things you are educated in: mathematics. For example, none of the other quantum gravity programs suggested so far has even attempted to construct a coherent interpretation. So would you also piss on the capacities of say string theorists in that way? You would not even dare so, because you may hide in some dusty corner of your office when Edward Witten comes to you to complain. Moreover, I do have working interpretations, some of which are similar to those proposed in the literature, but you are not aware of those either as far as I understand.


A. Neumaier said:
Let me try again:

In which sense is the conventional quantum mechanics in Hilbert spaces an approximation or limiting case of your indefinite theory?
That is a different question which I do have a definite answer for (and which is also provided in the book); it is not the same one you asked before. The negative norm originates from the indefinite character of the Clifford numbers which are only turned on when there is a nonzero gravitational field. So, in case gravity vanishes, the dynamical sector leaves a Hilbert space invariant and you have the standard interpretation.
 
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  • #37
Careful said:
new equations whose integrability has not been formally shown yet ?

Has it been shown at least perturbatively to second order in the gravitational constant?
If not, the status of your theory is like that of QED in 1930, maybe with all the problems ahead that QED had to face. Or like that of string theory around 1980, where the problems still aren't overcome.


Careful said:
There is still discussion in our days about the probability interpretation of QM and the equations have been constructed 90 years ago.

But this discussion is irrelevant for the practice of quantum mechanics. The probabilistic aspect of QM is very well understood; only its origin is somewhat in the clouds.


Careful said:
The negative norm originates from the indefinite character of the Clifford numbers which are only turned on when there is a nonzero gravitational field. So, in case gravity vanishes, the dynamical sector leaves a Hilbert space invariant and you have the standard interpretation.

What happens when the gravitational field is small, bulk matter is far away, and energies are far below the Planck scale? Do you get a Hilbert space and an external gravitational field?
 
  • #38
A. Neumaier said:
Has it been shown at least perturbatively to second order in the gravitational constant?
If not, the status of your theory is like that of QED in 1930, maybe with all the problems ahead that QED had to face. Or like that of string theory around 1980, where the problems still aren't overcome.
My computations (which are not in the draft yet) so far reveal no problems on the perturbative level, the hard question is whether it closes nonpertubatively. Moreover, again, you are extremely unreasonable. Your contributions to this discussion are nihil because you put me in the situation where I would have to present a fully closed theory as a single person in a single effort. Either you comment upon the proposal as it stands now (and which is much more precisely formulated than other approaches going on for many years), or you shut up. What you do not want to see is that my comments regarding your work are embedded in a historical series of failed attempts while my approach is fully fresh and has no evidence against it at this moment in time. If you refuse to understand this dynamics and important difference in your next post, I will report it as obstructive. My patience with your nonsensical comments is over.

A. Neumaier said:
But this discussion is irrelevant for the practice of quantum mechanics. The probabilistic aspect of QM is very well understood; only its origin is somewhat in the clouds.
Again, you do not understand the point here. It is alas like that with professors who think that God likes them in all aspects. In a theory of quantum gravity, the probability aspect becomes different because you do not dispose anymore of the classical observer. Hence, what you calculate is an ''absolute'' probability which has nothing to do with observation which requires relative probabilities. This aspect is just an example of the very many things which are alive still. You may also wish to study the work of Sorkin who tries to construct dynamical probability interpretations starting from the quantum measure. Here you actually have to prove some decoherence for ''macroscopic'' bodies in order for the Born rule to emerge.


A. Neumaier said:
What happens when the gravitational field is small, bulk matter is far away, and energies are far below the Planck scale? Do you get a Hilbert space and an external gravitational field?
Probably not, the dynamics will go slightly outside any fixed sub-Hilbert space, but that is not a problem is it ? Point is, that the pure Hilbert space picture does not exist because G is nonzero.
 
  • #39
To summarize, you are only pleased with Noldus when he performs the work of Heisenberg, Von Neumann, Wigner (regarding a fully complete and rigorous foundation of a new quantum theory) and Feynman, 't Hooft (showing that the theory makes sense - although there is no renormalization issue in my approach) in one book. And then, I did not even speak about the gravitational theory. Otherwise, you deem it unworthy of theoretical physics. Please, go back to your mathematical desk and fill in epsilon's and delta's in proofs of people who have real ideas and don't bother people who do work hard to get a genuine new insight.

You constantly refuse to see or understand or acknowledge the point I am making to you. The level of irrationality (and this is a very mild word) which you display here (in many ways) is beyond comprehension for someone who has an actual responsability towards the intellectual capital he teaches to every year.

Careful
 
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  • #40
Careful said:
you put me in the situation where I would have to present a fully closed theory as a single person in a single effort.

Great and radical claims are measured by much higher standards than minor main stream contributions.

And asking for a finite second order perturbation theory is far from asking for a closed theory.

Careful said:
If [...] I will report it as obstructive. My patience with your nonsensical comments is over.

Your derisive comments would be worthy of reporting, too. I'd never challenge a humble mind like I challenge you!

Careful said:
It is alas like that with professors who think that God likes them in all aspects.

Well, why shouldn't he like his children? He gives them freedom of thought and power to think independently.

Careful said:
In a theory of quantum gravity, the probability aspect becomes different because you do not dispose anymore of the classical observer.

Even in flat space quantum field theory, one doesn't have (or need) a classical observer.
As is well-known, all known observers are quantum objects, though macroscopic ones.


Careful said:
Hence, what you calculate is an ''absolute'' probability which has nothing to do with observation which requires relative probabilities.

What should an absolute probability mean, if it cannot be observed and hence tested?


Careful said:
Probably not, the dynamics will go slightly outside any fixed sub-Hilbert space, but that is not a problem is it ? Point is, that the pure Hilbert space picture does not exist because G is nonzero.

One needs to be able to recover to first order in G the standard Hilbert space quantum mechanics in an external gravitational field, under the assumption that an observer inside the system observes another subsystem - since this is what we observe as real observers.

I hope you are at least able to do first order perturbation theory...

I am looking for _some_ things that you can explain without a 160 page overhead...
 
  • #41
Careful said:
The level of irrationality (and this is a very mild word) which you display here (in many ways) is beyond comprehension for someone who has an actual responsibility towards the intellectual capital he teaches to every year.

Well, it seems that you are the only one who perceives me as being irrational.
Others here appreciate a lot my way of imparting understanding:

kof9595995 said:
BTW it'd be really nice to have a teacher like you : )

kote said:
^ That was a surprisingly good (and concise) explanation.
 
  • #42
If you think a post deserves to be reported, you should report it, rather than responding to it...
 
  • #43
A. Neumaier said:
Great and radical claims are measured by much higher standards than minor main stream contributions.
Yes, it requires 5 nobels in one book :smile::smile:

A. Neumaier said:
Your derisive comments would be worthy of reporting, too. I'd never challenge a humble mind like I challenge you!
There are two points:
A. I am actually more humble than you are it seems to me.
B. You did not challenge me at any instant: all you did was mentioning projects which I did not finish yet for very understandable reasons. This is fun in the beginning, but gets very annoying in the end.


A. Neumaier said:
Even in flat space quantum field theory, one doesn't have (or need) a classical observer.
As is well-known, all known observers are quantum objects, though macroscopic ones.
Nonsense, in that case you need a super observer and the state of the system is not directly discribing the probabilities of measurements you make. Actually, this superobserver would first have to measure you and then the system under study and apply the Bayesian rule.


A. Neumaier said:
One needs to be able to recover to first order in G the standard Hilbert space quantum mechanics in an external gravitational field, under the assumption that an observer inside the system observes another subsystem - since this is what we observe as real observers.
Sure, this is the standard analytical perturbative argument no? If you shut off G, you get standard QFT with all it's limitations, if G is turned on, then first order corrections arise.

A. Neumaier said:
I am looking for _some_ things that you can explain without a 160 page overhead...
It is difficult, of similar order than explaining general relativity to Newtonian physicists. You must accept that some ideas are not trivial and that 160 pages is sometimes not too much. For example, I once send you a summary and you found it full of buzzwords, while for QG physicists it was very clear what I wrote. You think you can decouple gravity from QM and what I have learned is that both need each other for a consistent formulation.
 
  • #44
A. Neumaier said:
Well, it seems that you are the only one who perceives me as being irrational.
Others here appreciate a lot my way of imparting understanding:
Well, I thought the same when I got to know you. And indeed, you explain standard stuff impartial and in a good way - we had never a dispute about that (we are both intelligent enough for this). However, you get irrational when some bold, new ideas are launched; you understand very well the process of repetition, but alas not of innovation.

Let us quit here with our little fight. I guess we both understand that battles can be fought without any need for casualties ... an art which is not too well understood. :wink:
 
  • #45
Careful said:
You did not challenge me at any instant: all you did was mentioning projects which I did not finish yet for very understandable reasons. This is fun in the beginning, but gets very annoying in the end.

I challenged your patience to the point where you threatened to report me.
Careful said:
Nonsense, in that case you need a super observer and the state of the system is not directly describing the probabilities of measurements you make. Actually, this superobserver would first have to measure you and then the system under study and apply the Bayesian rule.

Nonsense. There are no such superobservers.

But we routinely observe as quantum systems other quantum systems at energies where quantum corrections to gravity are completely negligible.

Careful said:
Sure, this is the standard analytical perturbative argument no? If you shut off G, you get standard QFT with all it's limitations, if G is turned on, then first order corrections arise.

Of course. But since you start with indefinite space, the question is whether or not you end up in a Hilbert space - as it must be in this case, since it is very well known how to describe this situation.[/QUOTE]

Careful said:
I once send you a summary and you found it full of buzzwords, while for QG physicists it was very clear what I wrote.

It is very easy to claim clarity. It is much more difficult to make it believable.

Please have some QG physicist comment here in PF on your book, to confirm your claim that for QG physicists it was very clear what you wrote.
 
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  • #46
A. Neumaier said:
I challenged your patience to the point where you threatened to report me.
Yes that is true, you managed to raise my bloodpressure !


A. Neumaier said:
Nonsense. There are no such superobservers.
Sure there are, if you have only quantum systems and the observers are quantum themselves, you need something which breaks the superpostion of this observer. You may call this a second classical observer, but it will only lead to the conclusion of a superobserver.

A. Neumaier said:
But we routinely observe as quantum systems other quantum systems at energies where quantum corrections to gravity are completely negligible.
Of course. But since you start with indefinite space, the question is whether or not you end up in a Hilbert space - as it must be in this case, since it is very well known how to describe this situation.
Didn't we have this whole discussion that you should not end up in Hilbert spaces in the first place because gauge theories in 4-D strongly appear to resist such formulation ? You are right in the sense that the dynamics should approximately leave some Hilbert space invariant, but not exactly.

A. Neumaier said:
It is very easy to claim clarity. It is much more difficult to make it believable.

Please have some QG physicist comment here in PF on your book, to confirm your claim that for QG physicists it was very clear what I wrote.
I know this due to personal communication. Why would I say this if this were not the case ? Have I ever tried to conceal a fact from you? I think all my responses were fair... what content is concerned. You may actually check the forum and you will see that tom.stoer found an almost complete copy of this document helpful and actually requested for me to put it on te web (but this is not the communication I was talking about).
 
  • #47
Careful said:
Sure there are, if you have only quantum systems and the observers are quantum themselves, you need something which breaks the superposition of this observer.

Only if one subscribes to von Neumann's very idealized description of the measurement process. I don't, because it is very inadequate to account for the practice of measurement. It applies only to certain idealized model measurements capable of treatment in the 1930's.

Careful said:
Didn't we have this whole discussion that you should not end up in Hilbert spaces in the first place because gauge theories in 4-D strongly appear to resist such formulation ?
This doesn't relieve you from the need to recover the traditional framework (which adequately expresses almost everything we can measure at ordinary distances and energies) in some very good approximation. If you can't, your predictions will be inconsistent with experiment.
 
  • #48
A. Neumaier said:
Only if one subscribes to von Neumann's very idealized description of the measurement process. I don't, because it is very inadequate to account for the practice of measurement. It applies only to certain idealized model measurements capable of treatment in the 1930's.
Von Neumann's is the only sensible one. Moreover, there exists no interpretation which can do what you want it to do. If you think there is, please provide all details; I will be happy to shoot them down.
 
  • #49
Careful said:
Von Neumann's is the only sensible one.

Von Neumann's cannot be sensible since for consistency it requires a hierarchy of bigger and bigger superobservers, which is nonsense.


Careful said:
Moreover, there exists no interpretation which can do what you want it to do. If you think there is, please provide all details; I will be happy to shoot them down.

See Sections 7.3 - 7.5 of http://lanl.arxiv.org/abs/0810.1019
 
  • #50
A. Neumaier said:
Von Neumann's cannot be sensible since for consistency it requires a hierarchy of bigger and bigger superobservers, which is nonsense.



You have a viable second option that doesn't resort to miracles?
 
  • #51
Maui said:
You have a viable second option that doesn't resort to miracles?

Yes. See the reference given in #49.
 
  • #52
A. Neumaier said:
Yes. See the reference given in #49.



You have a no go theorem that explicitly restricts deterministic models. My layman opinion says that if you are proposing another non-local HV theory, that'd be just another case of magic.
 
  • #53
A. Neumaier said:
See Sections 7.3 - 7.5 of http://lanl.arxiv.org/abs/0810.1019
There is no way in conventional QM do to what you claim, there are actually theorems about this. If you think you have something, please summarize in a few lines. I am sure it will be great fun.
 
  • #54
Careful said:
There is no way in conventional QM do to what you claim, there are actually theorems about this. If you think you have something, please summarize in a few lines. I am sure it will be great fun.

Oh, I thought you'd understand the need for more than a few lines to do something beyond what conventional QM can do:

Careful said:
no, I cannot explain these things even on one full A4 page since it requires many subtle considerations and additional concepts.
 
  • #55
Maui said:
You have a no go theorem that explicitly restricts deterministic models. My layman opinion says that if you are proposing another non-local HV theory, that'd be just another case of magic.

It requires no magic to avoid a no-go theorem by not satisfying its assumptions or conclusions.
 
  • #56
A. Neumaier said:
It requires no magic to avoid a no-go theorem by not satisfying its assumptions or conclusions.



The locality assumption or the realism(determinsim) assumption? Or do you propose some caveat? You are either too good or too naive(we most are anyway).
 
  • #57
Maui said:
The locality assumption or the realism(determinsim) assumption? Or do you propose some caveat? You are either too good or too naive(we most are anyway).

Let me propose that you first look at the reference and try to understand it. Unlike Careful's treatise, it is not technical.
 
  • #58
A. Neumaier said:
Von Neumann's cannot be sensible since for consistency it requires a hierarchy of bigger and bigger superobservers, which is nonsense.
:confused: Accepting for the sake of argument it requires a hierarchy of superobservers, I really don't see why such a thing should be nonsensical.

I could easily imagine an argument that in reality that such a hierarchy would contain much more information than is accessible to us, but that's a rather normal state of affairs for physical theories, rather than being nonsense.
 
  • #59
Hurkyl said:
:confused: Accepting for the sake of argument it requires a hierarchy of superobservers, I really don't see why such a thing should be nonsensical.

I could easily imagine an argument that in reality that such a hierarchy would contain much more information than is accessible to us, but that's a rather normal state of affairs for physical theories, rather than being nonsense.

Let the first order observer observe a single particle, and for k>1, let the k-th order observer observe the (k-1)-st order observer.

We first fix the situation von Neumann is talking about: ideal measurements that put the system instantaneously into a well-defined eigenstate, hence measure a complete set of observables of the system.

An observer (together with the observing equipment) must therefore be much larger than the object it observes, since it must have essentially classical pointer readings for each particular observable in the complete set. If the observed system consists of n quantum particles, it has 3n continuous quantum degrees of freedom. hence the observer must have 3n classical pointers, each comprising at least N atoms, where for a reasonable accuracy, N>>100. Therefore the observer consists of a system consisting of n particles consists of at least 300n particles. But this is an extremely conservative estimate, since we ignore all the logistics that is necessary to make such complete measurements with some reliability.

The k-th order observer of a single particle (n=1) therefore contains at least 300^k particles. Assuming the number of particles in the universe to be U, we see that the existence of the k-th observer implies
[tex] k\le log U/log 300 < 33[/tex]
when U=10^81. Even allowing lots of unknown dark matter will not change the resulting upper bound by much.

The only escape to this argument is to assume that the number of particles is infinite.
But even then there appear to be unsurmountable problems with the k-th observer measuring all details approximately instantaneously, given that the single particle observed by the lowest order observer is on the Earth and we know quite well the distribution of particles close enough to the Earth to be able to neglect relativistic delays.
 
  • #60
Dear Arnold,

Your scheme needs a superobserver as well, you cannot escape that. Let me hint you were the devil is: you uncritically assume that a ''macroscopic'' ''apparatus'' behaves more or less classically. This goes straight against Schrodinger's cat argument of course; whatever way you chose to escape, I guarantuee you upfront that you won't escape Von Neumann's conclusion. It appears to me that you did not follow the logical implications of your own writings far enough.

Moreover, your reasoning about the tower of observations is ''ganz falsch''.

Johan
 
  • #61
A. Neumaier said:
We first fix the situation von Neumann is talking about: ideal measurements that put the system instantaneously into a well-defined eigenstate, hence measure a complete set of observables of the system.
So you're not talking about this at all?


The only escape to this argument is to assume that the number of particles is infinite.
That's to be expected from an infinite hierarchy of observers. :-p We were expecting "nearly infinite" particles anyways anyways, so that thermodynamics could become relevant.


But even then there appear to be unsurmountable problems with the k-th observer measuring all details approximately instantaneously, given that the single particle observed by the lowest order observer is on the Earth and we know quite well the distribution of particles close enough to the Earth to be able to neglect relativistic delays.
I can't figure out what you're trying to argue here. I will make a comment that may or may not be relevant, though: how close to instantaneous "approximately instantaneously" must be depends on scale. Someone observing an experiment in a lab would probably require it to be less than a millisecond, whereas a couple hours probably counts for someone observing the solar system.
 
  • #62
Hurkyl said:
So you're not talking about this at all?

fix was meant in the sense of ''make precise'', not of ''correct''.


Hurkyl said:
That's to be expected from an infinite hierarchy of observers. :-p We were expecting "nearly infinite" particles anyways anyways, so that thermodynamics could become relevant.

The point is the exponential increase in the size of the k-th observer. Actually the factor 300 should be more like 10^8 or so, so that thermodynamics applies and produces approximately classical pointer readings. Indeed, if we consider an everyday measurement of the presence of a particle by a Geiger counter, the factor is already 10^20, and it is completely impossible to install machinery that measures the complete state of a Geiger counter. Interactions beyond the Earth are far too weak to gain significant information about the counter, except perhaps to photograph it from space, which gives < 10^7 degrees of freedom while >10^20 are needed, and no amount of namotechnology can change this significantly.

Hurkyl said:
Someone observing an experiment in a lab would probably require it to be less than a millisecond, whereas a couple hours probably counts for someone observing the solar system.

Well, in this time, a decent quantum system has already changed its state so much that at completion of the experiment one can no longer claim to have measured the state at the beginning.

Thus even a second-order observer is an illusion.

Considering that many measurements on Earth are actually made, and _all_these_ would have to be collapsed by super-observers, things get even more fantastic. This is no longer physics but science fiction.
 
  • #63
Careful said:
you uncritically assume that a ''macroscopic'' ''apparatus'' behaves more or less classically.

I only need that the tip of the pointer behaves classically. This is a well-known empirical fact without which we couldn't do any measurement at all. This is at the basis of my interpretation.

On the other hand, von Neumann's interpretation (and the underlying Born rule) is based on assumptions that are so highly idealized that they can't be realized except for extremely tiny systems.


Careful said:
Moreover, your reasoning about the tower of observations is ''ganz falsch''.

Well, where is the mistake?
 
  • #64
A. Neumaier said:
I only need that the tip of the pointer behaves classically. This is a well-known empirical fact without which we couldn't do any measurement at all. This is at the basis of my interpretation.

On the other hand, von Neumann's interpretation (and the underlying Born rule) is based on assumptions that are so highly idealized that they can't be realized except for extremely tiny systems.




Well, where is the mistake?
Before we proceed, are you prepared to aknowledge that you made a mistake in case every sensible person can see that you are wrong? Because, the main problem resides there.
 
  • #65
Careful said:
Before we proceed, are you prepared to aknowledge that you made a mistake in case every sensible person can see that you are wrong? Because, the main problem resides there.

Strange that you ask. I never had problems with learning.
 
  • #66
A. Neumaier said:
Strange that you ask. I never had problems with learning.
First, that is a matter of perception (and I strongly disagree with your self-assesment); second, what I said is that you have problems with admitting your own shortcomings and acting rationally upon them. So, I ask again, if you are mistaken, will you as a true gentlemen admit so? I have no problems to admit when I make a mistake, but since you claim to outsmart Von Neumann and Wigner, I would think that in case you are proven wrong, a mild acknowledgment is in place.
 
  • #67
A. Neumaier said:
fix was meant in the sense of ''make precise'', not of ''correct''.
The reason I asked was because you don't really seem to be talking about the measurement I linked. You seem to be making four significant, unwarranted hypotheses that turn your argument into a straw-man.

The first is your hypothesis that a measurement be instantaneous. I have no idea about the original source, but it certainly wasn't required in the link I gave, nor is there any obvious reason why it should be so. What is expected is just that the joint object - measuring device - environment* system undergoes unitary time evolution.

The second is your hypothesis that the construction and reading of the measuring device must be practical. Again there was no such hypothesis in the link, nor any obvious reason why it should be so. Even if we wanted to consider the special case of a real-world measurement in a laboratory, we still don't even require distinguishing between all states of the device to be anything resembling feasible -- many device states will correspond to the same reading.

The third is that the observer & measuring device must resemble a human and a real-life device we could call a measuring device. (or even that there must be an observer!)

The fourth one is the hypothesis that the measurement completely distinguishes the states of the object of study. While this is included in the link I mentioned, there is no obvious reason why it should be taken as a requirement.


*: I hope you don't mind me making this obvious extension.
 
  • #68
Hurkyl said:
The reason I asked was because you don't really seem to be talking about the measurement I linked.

Indeed, I didn't realize that there was an embedded link. The context didn't say there was one, and my browser indicates embedded links only when the mouse is directly upon them.

I thought that ''this'' referred to the text you had quoted.

I'll respond to the link separately, in a different thread since the topic has no longer anything to do with the title of the thread.
 
  • #69
Hurkyl said:
What is expected is just that the joint object - measuring device - environment* system undergoes unitary time evolution.

*: I hope you don't mind me making this obvious extension.

No, I don't.

My reply to your array of comments is in post #7 of the thread https://www.physicsforums.com/showthread.php?p=3128309
 

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