Subject: 200 wrong theories for the cosmological constant, by Hooft 't G.
Date: Wed, 01 Oct 2003 09:18:13 +0300
From: Dimi Chakalov <dchakalov@surfeu.at>
To: "Hooft 't G." <G.tHooft@phys.uu.nl>

Dear Professor 't Hooft,

Regarding your email of Fri, 6 Apr 2001 11:04:56 +0200, I gratefully accept your suggestion to provide for the 201st reference in your intended paper on the cosmological constant problem, entitled: "200 wrong theories for the cosmological constant."

Should you decide to change the title to "201 wrong theories for the cosmological constant", by mentioning my CD ROM "Physics of Human Intention", please read the essential ideas at

http://members.aon.at/chakalov/Klauber.html

http://members.aon.at/chakalov/Granik.html#note

and in my White Paper,

http://members.aon.at/chakalov/white_paper.html

If you wish to learn more about the so-called black holes and gravitational waves, please see the paper by Angelo Loinger at

http://members.aon.at/chakalov/Loinger.html

and references therein.

As you our acknowledged in your email of Fri, 6 Apr 2001 11:04:56 +0200, our work is not finished. Please do write your paper on the cosmological constant problem.

Wishing you best of luck in your endeavors,

Yours faithfully,

Dimi Chakalov
http://members.aon.at/chakalov
 
 

On Fri, 6 Apr 2001 11:04:56 +0200, "Hooft 't G." wrote:
>
> I do not intend to continue this discussion for very long, but
> mentioning a few facts might help.
>
> As for the existence of black holes: if you take general relativity
> but leave out quantum mechanics, you get a theory that has been
> tested with great precision at the scale of the solar system
> (particularly with compact double star systems in astronomy).
> There seems to be no strong evidence against that theory.
>
> Taking it for granted, one is led inevitably to conclude that black
> holes exist. It is easy to imagine an initial state of matter that will
> lead to implosion and a black hole. Whoever denies that hasn't
> understood the theory.
> There is no reason to object "against the existence" of black holes.
> These objects, though exotic, do not violate any basic law of
> physics, have completely and uniquely predictable behavior, and
> there are several astronomical objects that seem to be quite in
> agreement with these predictions.
>
> In all known black hole solutions, the space-time singularity is
> well-hidden behind the horizon so that their existence has
> absolutely no physical consequence, so they are acceptable
> ingredients of a sound theory.
>
> However, all this applies to black holes that are so large that
> quantum mechanical effects are irrelevant to their description. For
> this to be true, these black holes must be larger than, roughly, 
> 10^(-30) cm. In the theory mentioned above, the size of a black
> hole is a free parameter, it can be anything between 10^(-30) cm
> and many light years across.
>
> Quantum mechanics sheds a different light on them. Tiny black
> holes will not only absorb but also emit particles. This still gives
> them a quite `reasonable' appearance. No reason to suspect
> anything wrong. To the contrary, QM strongly suggests that the
> very tiny black holes behave much like elementary particles, and
> perhaps there is no basic distinction between black holes and
> elementary particles.
>
> The only problem is that the details cannot (yet?) be worked out.
> We are talking about such an esoteric domain of physics that no
> experiments are possible. For doing thought experiments, a new
> mathematical language is needed that does not yet exist. No-one
> should be surprised: our work is not finished.
>
> Then the cosmological constant. it is not understood. I once
> planned to write a paper entitled: "200 wrong theories for the
> cosmological constant", with 200 references. Needless to say that
> most of these theories are also mutually exclusive. The right theory
> has not been found. You are wellcome to provide for the 201st
> reference in my paper.
>
> On some days of the week I am thinking of the possibility that
> general relativity only exists in the quantum Hilbert space that
> describes the statistics of a deterministic theory, but that it does not
> hold for the deterministic theory itself, in other words, that this
> theory shows a preference for flat coordinates. That would do
> away with the cosmological constant problem, but it would put
> many new problems in its place.
>
> Now strings. I am not a very strong supporter of string theory, but
> I do notice the remarkable coherence of the observations made by
> string theorists, and I do not want to dismiss all that as rubbish. It
> may well be that what is called string theory now will occupy an
> important corner of a future theory, but my approach is largely
> independent of that.
>
> Greetings,
>
> Gerard 't Hooft.

===========
 

Subject: 201 wrong theories for the cosmological constant, by Hooft 't G.
Date: Wed, 07 Dec 2005 21:43:53 +0200
From: Dimi Chakalov <dimi@chakalov.net>
To: "Hooft 't G." <G.tHooft@phys.uu.nl>
CC: Wilma van Egmond <w.j.m.vanegmond@phys.uu.nl>,
     Stefan Nobbenhuis <S.J.B.Nobbenhuis@phys.uu.nl>,
     Mihaela Iftime <mihaela.iftime@bos.mcphs.edu>,
     John Stachel <stachel@bu.edu>,
     Gennadi Sardanashvily <sard@grav.phys.msu.su>,
     Vincent Moncrief <vincent.moncrief@yale.edu>,
     Oliver Pooley <oliver.pooley@philosophy.ox.ac.uk>,
     Paul Steinhardt <steinh@princeton.edu>,
     Piotr Chrusciel <chrusciel@univ-tours.fr>

Hi Gerard,

I very much hope you will complete your paper, entitled: "200 wrong theories for the cosmological constant", and will comment my proposal, as you stated in your email from Fri, 6 Apr 2001 11:04:56 +0200,

http://www.God-does-not-play-dice.net/Gerard.html#201

Back on April 6, 2001, you were certain that my proposal will turn out to be wrong. I don't question your expertise in paranormal phenomena,

http://www.phys.uu.nl/~thooft/para.html

but let me briefly explain my idea, just in case your mind-reading and other ESP skills were not entirely accurate (it happens).

I will try to elaborate on your unpublished idea [Ref. 1], but from a different perspective on the main issue -- "the discovery of a symmetry that forbids a cosmological constant term to appear". More on this fundamental symmetry at

http://www.God-does-not-play-dice.net/Professor_X.html#Negative_Mass

It should be *the* largest possible symmetry group, but I wouldn't
speculate on any boundary conditions [Ref. 1], since there couldn't be
any boundary conditions in the putative global mode of spacetime. The
latter enables the theory to be "invariant under all permutations of the
basic elements, out of which the theory is constructed", as suggested by
Mihaela Iftime and John Stachel [Ref. 2]. More on the hypothetical 'global mode of spacetime' at

http://www.God-does-not-play-dice.net/Wald.html#note

Do you or any of your colleagues believe GR can be properly applied at scales larger than 10^14 cm, the size of the solar system [Ref. 1]? There is a lot of "dark" stuff there, which I believe are effects of the global mode of spacetime,

http://www.God-does-not-play-dice.net/Minchin.html

It cannot be visualized, just as we cannot imagine the "spin" of elementary particles, nor the "spin" of the whole universe,

http://map.gsfc.nasa.gov/ContentMedia/map_model_2.gif

To cut the long story short, I do believe in your hunch [Ref. 1], and regret that it wasn't published. How come you set the right track [Ref. 1, Eq. 10] with your 'intuitive knowledge' (scientia intuitiva, Benedict De Spinoza), but couldn't see the path?

Anyway, once you're ready with your fundamental paper, please drop me a line and I'll send you my proposal for your consideration.

Regards,

Dimi
--
http://www.God-does-not-play-dice.net
http://www.God-does-not-play-dice.net/download.html

References

[Ref. 1] Stefan Nobbenhuis, Categorizing Different Approaches to the
Cosmological Constant Problem, 5 December 2005, gr-qc/0411093 v3.

Sec. 3.2, Imaginary Space, p. 9:
"As was first observed by 't Hooft (unpublished), we can forbid the
cosmological constant term by postulating that the transformations
(...).
...
"there exists a copy of all known matter particles with negative mass
squared"
...
Sec. 3.3, Energy -->  - Energy, p. 10: "Crucial in this reasoning is that there is no coupling other than gravitational between the normal matter fields and their ghost counterparts, otherwise the Minkowski vacuum would not be stable."
...
p. 30: "Besides, it is conceivable that the need to introduce a very small cosmological constant or some other form of dark energy to explain an accelerating universe nowadays, is a signal that general relativity breaks down at very large distance scales. General relativity however, works very well on scales from 10^-1 mm to at least 10^14 cm, the size of the solar system.
...
p. 48: "Since even the sometimes very drastic modifications advocated in the proposals we discussed do not lead to a satisfactory answer, this seems to imply that the ultimate theory of quantum gravity might very well be based on very different grounds than imagined so far. The only way out could be the discovery of a symmetry that forbids a cosmological constant term to appear.
...
"Throughout this work I have benefited a lot from many valuable discussions with my supervisor Gerard 't Hooft."
 

[Ref. 2] Mihaela Iftime, John Stachel, The Hole Argument for Covariant Theories, gr-qc/0512021 v1.

"Informally this means that if everything is carried along, nothing is changed. The hole argument can only apply to background independent theories!
...
"Therefore, the following principle of generalized covariance should be a requirement on any fundamental theory: The theory should be invariant under all permutations of the basic elements, out of which the theory is constructed."
 

Note: It goes without saying that Prof. 't Hooft does not approve of my understanding of Einstein's GR: he believes that there is no problem with energy conservation (details here), while I believe energy conservation in GR is impossible in principle, because it requires a 'well-defined notion of time'. The latter is, however, the absolute time of Newton. The treatment of the coordinate "time" parameter in GR is entirely different, hence there is no 'back bone' on which you can stack a chain of physical states with well-defined energy states. See also the quasi-local nature of the gravitational analogs of the classical conserved quantities, from Laszlo Szabados here.

If you want math, click here and see the shortest explanation of 'global mode of spacetime' here, and wait for the fundamental paper by Hooft 't G., entitled: "201 wrong theories for the cosmological constant".

The last time I heard from him, he wrote (Mon, 15 Mar 2004 09:24:48 +0100): "I apologetically terminate this discussion." I wonder why. I think his idea [Ref. 1] is fantastic, only he needs help.

"It is extremely difficult to induce penguins to drink warm water", says John Coleman.
 

D. Chakalov
December 8, 2005
 

============

From: "Hooft 't G." <G.tHooft@phys.uu.nl>
To: 'Dimi Chakalov' <dchakalov@gmail.com>
Subject: RE: If time is discrete, ..., if time is continuous, ...
Date: Tue, 4 Apr 2006 15:12:24 +0200 

Yes, but I am considerably more selective than that; the site you mention
contains too much obvious nonsense.
Cordially,
G. 't Hooft

-----Original Message-----
From: Dimi Chakalov [mailto:dchakalov@gmail.com] 
Sent: dinsdag 4 april 2006 3:45
To: g.thooft@phys.uu.nl
Subject: If time is discrete, ..., if time is continuous, ...

Dear Dr. 't Hooft,

RE your quant-ph/0604008 v1, perhaps you may wish to see what other people have said on the issue,

http://www.god-does-not-play-dice.net/download.html

D.C.

===========

Date: Tue, 4 Apr 2006 23:43:30 +0300
From: "Dimi Chakalov" <dchakalov@gmail.com>
To: "Hooft 't G." <G.tHooft@phys.uu.nl>
Subject: Re: If time is discrete, ..., if time is continuous, ...
 

On 4/4/06, Hooft 't G. <G.tHooft@phys.uu.nl> wrote:
> Yes, but I am considerably more selective than that

Like Eq. 2.1, the "clock that gives a tick at every time step" maybe?

"For simplicity we therefore omit specific references to any clock 
(footnote 1)". Footnote 1: "Thus, we do, as yet, use an absolute notion of time. Special and general relativistic transformations are left for future
studies."

That's sheer nonsense, although not entirely obvious, since you've left it "for future studies". Unless, of course, you have already written your fundamental paper "201 wrong theories for the cosmological constant", and have proposed the 202nd theory, which is the correct one, hence can elaborate on your tantalizing Eq. 2.1.

Cordially,

D. Chakalov

 


Addendum


On December 8, 2005, I stated that
G. 't Hooft's idea [Ref. 1] is fantastic, only he needs help. It has been delivered by his Ph.D. student, Stefan Nobbenhuis [Ref. 3], but, as it stands, it's still "not yet sufficient" (p. 149). Let me see if I can help, too.

'Why does Nature prefer a flat spacetime?', asks S. Nobbenhuis [Ref. 3].

Perhaps because the local mode of spacetime is being created as a flat spacetime and perfect continuum. It is a scale-invariant 'back bone' of the whole physical world, from the Planck scale to the cosmological horizon. Once the inflationary stage was completed, the "two elephants" have an equal and opposite "pressure", and the space is brought to a dynamical stage of being "flat". If you look at the explanation offered by Eli Michael back in 1999, our understanding of the cosmic scale factor needs to be modified, in order to resolve the coincidence problem. Eli Michael wrote (links and emphasis added):

"The coordinates [X], [X], and [X] in the metric equation are "comoving" coordinates. A comoving coordinate system is one which expands with the universe. Therefore, the comoving distant between two points remains constant during the universe's evolution. The physical distance between two points does however change as the universe expands.

"It is the cosmic scale factor a which relates the comoving coordinates to physical distances, through the relation: d = a x. With the metric defined with comoving coordinates, the time evolution of the universe is described by the time evolution of the cosmic scale factor. If the cosmic scale factor grows in time then the universe expands, if it diminishes with time then the universe collapses.
...

"It is the fact that pressure also contributes to gravity that makes the inclusion of the cosmological constant interesting. If the field equations are rewritten so the cosmological constant appears on the right hand side of the equation, the cosmological constant term can then be associated with a vacuum energy density:

[XXX]

"Because the cosmological constant term is proportional to the metric, the pressure associated with the vacuum is then given by the relation:

[XXX]

"So the cosmological constant behaves gravitationally like matter and energy except that it has negative pressure. The net effect of a positive cosmological constant is then to create a repulsive gravitational force. This repulsion acts to expand the universe.

"The vacuum energy density behaves differently from matter and energy density in another regard. As the universe expands, matter and energy are spread out over more physical space and thus their gravitational attraction is diminished. For the vacuum energy, however, the PdV work done by the vacuum during adiabatic expansion provides exactly the amount of energy to fill the new volume to the same density. Therefore the cosmological constant remains truly constant, and its gravitational repulsion (or attraction) never changes during the universe's evolution."

Only it does change during the universe's evolution, which is the crux of the coincidence problem, firstly, and secondly -- the so-called 'coincidence problem' is actually the problem of discovering the true dynamics of the gravitational field. Since the cosmological "constant" appears on the right hand side of the equation, what should be added to the left hand side to achieve the perfect balance of gravitational repulsion & attraction of the flat spacetime?

NB: This perfect balance must be achieved and sustained during an accelerated expansion of the flat spacetime. Also, we need an additional degree of freedom that would allow dynamical adjustments of [lambda] during the whole evolution of the universe. That's the real challenge. The "effective" or "net effect" of the dynamical contributions of the vacuum require a brand new degree of freedom of the spacetime: the 'global mode' of the potential reality. It is not in the right hand side, nor in the left hand side of Einstein's equation, because the latter requires [lambda] to be a constant. Moreover, if we search for explanation of the Dynamic Dark Energy (DDE) in the framework of GR, as constrained by its Hamiltonian "dynamics", we inevitably reach the following formulation of the task: DDE creates the cosmological time, and in the same time DDE evolves in the time that is being created by it. It's ridiculous. Of course we have to modify GR [Ref. 3, p. 149].

Notice that the mechanism postulated for the adjustments of [lambda] is dynamical, such that the effective cosmological constant is currently "incredibly small". Just drop the presumption that the matter energy density "obviously decreases as the universe grows larger and larger" [Ref. 3], because an evolving cosmological "constant", as noted by R. Penrose, "would have to be accompanied by a compensating non-conservation of the mass-energy of the matter". We're dealing with 'potential reality', which is why "it is reasonable to look for modifications" of both GR and QM [Ref. 3, p. 149], as outlined here.

If you decide to ignore the potential reality, you'll face an insurmountable task: the second law of thermodynamics states that the universe must have started in an extremely low entropy state, and R. Penrose has argued that this makes the choice of our Initial Conditions very special indeed, namely, the probability to enjoy the universe around us, as evolving from this most special and unlikely choice, is as likely as 1 part in (1010)123. So, if you don't like miracles or "anthropic" parapsychology à la Steven Weinberg, your only way out is to employ the potential reality, to which the second law of thermodynamics simply do not apply. Why not? Because you simply cannot apply the laws of thermodynamics to 'the whole universe as ONE'.

To sum up, I think Stefan Nobbenhuis is a brilliant physicist, and I will be more than happy if he resolves the first off puzzle: the phenomenon that makes the Dynamics Dark Energy "dark". Since DDE has nothing to do with thermodynamics, perhaps Stefan Nobbenhuis would like to explore the Brans conjecture, namely, some "not smoothly embedded structure" of the spacetime manifold, which could accommodate "as many negative energy as positive energy states" [Ref. 3, p. 75]. (It's tricky, because in the local mode we don't get "negative energy" but two worlds, material and tachyonic, separated by a timeless luxonic "barrier"; more here). But I sincerely hope he will never be awarded a Nobel Prize: although it is the best thing that can happen to a man, it is the worst thing that can happen to a theoretical physicist.

Consider, for example, Gerard 't Hooft, who said above that "the site you mention contains too much obvious nonsense." Is the proposal for 'local mode of spacetime' (cf. above) "obvious nonsense"? Here's what you have to do to verify the claim by Gerard 't Hooft:

First, solve the puzzle of the classical world. Recall Asher Peres (Interpreting the Quantum World, quant-ph/9711003):

"In classical mechanics, a dynamical variable indeed has a definite value at each point of phase space. Specifying a point in phase space is the standard way of indicating the state of a physical system. However, in quantum mechanics, a dynamical variable is represented by a Hermitian matrix (or, more generally, by a self-adjoint operator). It is manifestly pointless to attribute to it a numerical value."

I believe there should exist a Lorentz-invariant, reversible, bi-directional, and smooth transition from the hidden unobservable quantum reality to the normal world of tables and chairs, and back to the hidden unobservable quantum reality. That's the puzzle of the classical world.

Please take part in the 'flipping a quantum coin' quiz here, and report your choice. (Recall that POVMs were designed to bypass, not resolve, the Pauli's argument that there is no self-adjoint time operator canonically conjugating to a Hamiltonian if the Hamiltonian spectrum is bounded from below.) More here.

Then comes the second hurdle: the dynamics of GR. It is manifestly pointless to attribute to the energy of the gravitational field a precise, numerical value: the alleged Dirac-ADM "dynamics" doesn't work. The problems are widely known, of course.

What is the common task? You need a mechanism for selecting "a definite value at each point of phase space", in both QM and GR. If your brain can do it, Mother Nature can to do it as well. Hence you get a scale-invariant 'back bone' of the whole physical world, from the Planck scale to the cosmological horizon: the local mode of spacetime. How? From the global mode, of course.

Is this "too much obvious nonsense", as Gerard 't Hooft claims?

Please follow the links, and then ask G. 't Hooft for clarification. Being a renowned mind reader and clairvoyant, he declared five and a half years ago, on April 6, 2001, that my proposal will turn out to be wrong.



D. Chakalov
September 7, 2006
Last update: September 24, 2006

 

[Ref. 3] Stefan Nobbenhuis, The Cosmological Constant Problem, an Inspiration for New Physics. Ph.D. Thesis, defended June 15, 2006. Supervisor: Prof. Dr. G. ’t Hooft. gr-qc/0609011 v1, 4 September 2006


p. 4: "No symmetry is known that can protect the cosmological constant to such a small value.
...

"In conclusion, the question is why is the effective cosmological constant
so close to zero? Or, in other words, why is the vacuum state of our
universe (at present) so close to the classical vacuum state of zero energy, or perhaps better, why is the resulting four-dimensional curvature so small, or why does Nature prefer a flat spacetime? Apparently spacetime is such, that it takes a lot of energy to curve it, while stretching it is (almost) for free, since the cosmological constant is (almost) zero.
...

p. 6: "The first, or sometimes called "old" cosmological constant problem is
why is the effective cosmological constant so incredibly small, as described in the previous section.

"The second problem is, if it is so small, then why is it not exactly equal
to zero? Often in physics it is a lot easier to understand why a parameter
is identically zero, than why it is a very small number.

"And a third question may be posed, based on the measured value of the
effective cosmological constant. The energy density of the vacuum that it
represents, appears to be of the same order of magnitude as the present
matter energy density in the universe. This is quite peculiar, since, as we
we will see in chapter (2), vacuum energy density, denoted [Ved], remains
constant during the evolution of the universe, whereas the matter energy
density, [Med] obviously decreases as the universe grows larger and larger. If the two energy densities are of the same order of magnitude
nowadays, this means that their ratio, [Ved]/[Med] had to be infinitesimal
in the early universe, but fine-tuned to become equal now. Therefore, one
obviously starts to wonder whether we are living in some special epoch, that causes these two forms of energy density to be roughly equal in magnitude. This has become known as the "cosmic coincidence problem" and is also sometimes phrased as the "Why now?" problem.
...


p. 16: "Three approaches are studied in great detail. The first can be found in chapter 4 and is based on my paper written together with Gerard ’t Hooft [50], in which we explore a new symmetry based on a transformation to imaginary space. The idea is that the laws of nature have a much wider symmetry than previously expected, and that quantum field theory can be analytically continued to the full complex plane. This generally leads to negative energy states. Positivity of energy arises only after imposing hermiticity and boundary conditions, which opens the way for a vacuum state invariant under these transformations to have zero energy, leading to zero cosmological constant.


p. 59: "We do not address the issue of non-zero cosmological constant, nor the so-called cosmic coincidence problem. We believe that a symmetry which would set the cosmological constant to exactly zero would be great progress.

p. 60: "Thus, the symmetry that we are trying to identify is a symmetry of
laws of nature prior to imposing any boundary conditions. Demanding
invariance under [XXX] where [XXX] may be real or imaginary, violates
boundary conditions at [XXX], leaving only one state invariant: the physical vacuum.

p. 75: "The symmetry proposed in this chapter is different. It is suspected that the field equations themselves have a larger symmetry than the boundary conditions for the solutions. It is the boundary conditions, and the hermiticity conditions on the fields, that force all physical states to have positive energies. If we drop these conditions, we get as many negative energy as positive energy states, and indeed, there may be a symmetry relating positive energy with negative energy. This is the most promising beginning of an argument why the vacuum state must have strictly vanishing gravitational energy.

p. 149: "So far we can only conclude that in fact none of the approaches described above is a real outstanding candidate for a solution of the ‘old’ cosmological constant problem. The most elegant solution would be a symmetry, that protects the cosmological constant. All possible candidates we can think of were treated in chapter 3 and (4). However, no symmetry, consistent with established results, was found. The symmetry analytically continuing quantum field theory and general relativity to the full complex space (chapter (4)) is interesting, but as it stands, not yet sufficient.
...

"Since the cosmological constant problem lies at the heart of a fusion
between general relativity and quantum mechanics, it is reasonable to look
for modifications of either one, or even both."