| Subject: Trying to paint a painting without
any canvas
Date: Sat, 31 Aug 2002 14:35:11 +0300 From: Dimi Chakalov <dchakalov@surfeu.at> To: Nikolaos Mavromatos <nm@phpd56.ph.kcl.ac.uk>, Nikos Mavromatos <Nikolaos.Mavromatos@cern.ch> CC: Mario Everaldo de Souza <msouza@fisica.ufs.br>, Angelo Loinger <Angelo.Loinger@mi.infn.it>, Craig Hogan <hogan@u.washington.edu>, Giovanni Amelino-Camelia <Giovanni.Amelino-Camelia@cern.ch>, James Gillies <cern.courier@cern.ch>, David Ehrenstein <focus@aps.org>, JR Minkel <minkel@aps.org>, P Ball <p.ball@nature.com> BCC: [snip] Dear Dr. Mavromatos, In your recent article "Testing models for quantum gravity" [Ref. 1], you mentioned the problem of background-dependence, the notorious problem of string theory. I'm sure you and your colleagues at CERN are fully aware of this highly complex problem and its implications [Refs. 2-5]. May I ask you to explain, prior to the experiments on the supposed "loss of quantum coherence" [Ref. 1], your view on the background-dependence problem in quantum gravity. Suppose, just hypothetically, that you observe loss of quantum coherence. How would you then relate such evidence to the whole bundle of problems [Refs. 2-5]? That I was never able to figure out. Hope you and your colleagues will help -- before you run the experiments. Thank you very much in advance. You can read this email also at http://members.aon.at/chakalov/Mavromatos.html Regards, Dimiter G. Chakalov
References [Ref. 1] Nick Mavromatos (September 2002).
Testing models for quantum gravity. CERN Courier,
"In the framework of local field theory, John Wheeler and Stephen Hawking have suggested that microscopic quantum space-time fluctuations of black hole type, with size of the order of the Planck length (10^35 m), characterize the quantum-gravity vacuum, giving it a "space-time foamy" nature (figure 1). Interaction of matter with such backgrounds may result in the loss of quantum coherence. This in turn could lead to significant deviations from the standard quantum-mechanical behaviour of matter particles, even at scales much lower than the characteristic quantum-gravity (Planck) energy scale of 10^19 GeV. "This is because gravity is a non-renormalizable interaction,
with a dimensionful coupling constant, and so it may manifest itself at
much lower scales. An example of such a phenomenon is provided by the so-called
charge-parity (CP) discrete symmetry, whose violation manifests itself
at scales much lower than the characteristic scale of the underlying weak
interactions responsible for the effect.
"For the time being, however, string theories seem to
suffer from an important drawback, which probably prevents a complete understanding
of quantum gravity issues within this framework. This is their background
dependence - the fact that the whole formalism of strings, at least so
far, is based on specific space-time backgrounds."
[Ref. 2] John
Baez (May 5, 2000). What is a background-free theory?
"Personally I think one can dig oneself into a hole by trying to do physics without any background structure - it's a bit like trying to paint a painting without any canvas." See also:
[Ref. 3] Peter Woit (2001). String Theory:
An Evaluation.
[Ref. 4] Angelo Loinger (2001). The generation
of gravitational waves.
See also
[Ref. 5] Mário Everaldo de Souza.
Gravity cannot be quantized. Tue, 27 Aug 2002 20:43:37
GMT,
"And if the fermionic mass carrier exists each mass is a multiple of the fermion mass. Otherwise, mass cannot be quantized because without a fermionic mass carrier there cannot be mass currents. How can gravity be quantized without quantizing mass and without fermionic currents? "The quantization of gravity has to exist either in curved spacetime or in flat spacetime. For example, it is expected that *if a body is excited gravitationally it should emit gravitational charge carriers into space and it is also expected that when a body is gravitationally excited the charge carriers (fermions) should change quantum states. When particles change mass in a high energ y collision there should exist such fermion currents*. "Let us admit the existence of such mass carrier and let
us call it *masson*.
"These two equations clearly show that the *masson* mass
depends on the metric. In curved space-time we can always choose a small
region where space-time is approximately flat. Hence, we can extend the
meaning of [g] to include curved space-time. Doing this we
notice that since the masson mass depends on the metric it can not be unique,
that is, it has different values in different curved space-times. Since
flat space time is a local approximation of curved space-time its mass
has only a local meaning. Therefore, we stumbled into another obstacle
in quantizing gravity.
"Thus, the gravitational field cannot be scalar, pseudoscalar,
vectorial, pseudovectorial, and symmetric tensorial field. The only possibility
left is to be an antisymmetric tensorial field which is a result that agrees
well with general relativity. Misner, Thorne and Wheeler [2] have proven
that the classical gravitational field is an antisymmetric tensorial field.
This work shows that the same should hold quantum mechanically. But since
elementary fermions are spin 1/2 particles we expect the *masson* to be
also an elementary fermion. But this means that the graviton should have
spin equal to 0 or 1 because bosons intermediate states between fermions.
In other words if the *masson* is in a state with spin [X]
it can only go to a state with [X] and this means that there
should be the emission of a graviton with spin equal to 1 or 0 but as was
shown above this possibility cannot happen.
"Therefore, the gravitational field can not be quantized
and, of course, neither the masson nor the graviton exists. This leads
us to say that the gravitational field is always a static field which is
in line with the null results of gravitational waves."
==============
Subject: Re: Trying to paint a painting
without any canvas
Dear Nick, Thank you for your kind and thoughtful reply and for explaining your viewpoint on the background dependence of quantum gravity, as I requested in my preceding email from Sat, 31 Aug 2002 14:35:11 +0300, http://members.aon.at/chakalov/Mavromatos.html On Fri, 6 Sep 2002 12:46:14 +0200 (MET DST), you wrote: [snip] > In models my colleagues and I have been involved with
Please see my reply below. > I would be very much interested in seeing how you view this It seems to me that your specific model is based on string theory and general relativity (as I gathered from your "Quantum Gravity and Dirichlet-Brane Phenomenology"), and hence it has a background *ab initio*. I can not comment on your model because I was never able to understand it. I had the rare privilege to discuss the spacetime "foam" and "It from Bit" with Prof. John Wheeler in Princeton on 22 May 1989, but I'm afraid it didn't help a bit. To understand your ideas, I respectfully asked you in my previous email for help. I wrote: "Suppose, just hypothetically, that you observe loss of quantum coherence. How would you then relate such evidence to the whole bundle of problems [Refs. 2-5]? That I was never able to figure out. Hope you and your colleagues will help -- before you run the experiments." In addition to [Refs. 2-5], which you can find in my previous email, http://members.aon.at/chakalov/Mavromatos.html please see also Steve Carlip at http://www.physics.ucdavis.edu/Text/Carlip.html#problems > So experiments NEED TO BE CARRIED OUT in order to guide I fully agree that experiments need to be carried out, but I have no idea how to interpret the results, even if you observe loss of quantum coherence. Perhaps you may wish to consult Steve Carlip by email and, during your forthcoming conference, Steve Adler http://members.aon.at/chakalov/Adler.html#NB and Carlos Barcelo http://members.aon.at/chakalov/Wald.html#3 Stephen Hawking wrote in 1995: "Unless quantum gravity can make contact with observation, it will become as academic as arguments about how many angels can dance on the head of a pin." http://members.aon.at/chakalov/Gerardus.html#Hawking In brief, unless you solve the puzzles in [Refs. 2-5] from my previous email and crack the problems listed by Steve Carlip, I personally will remain very skeptical about your interpretation of loss of quantum coherence as "quantum gravity effects". We don't have a full-blown theory of quantum gravity, and everything we say is pretty much like "How do we know that Father Christmas has a beard? Because snow falls when he shakes it!" BTW the story about Father Christmas' beard applies to my efforts as well. I sent today a copy from my CD ROM to Prof. Sarben Sarkar, accompanied by a letter (printed below). Should you find my CD interesting, please feel free to clone and pass it to your colleagues. I will highly appreciate all critical comments and suggestions. Kind regards, Dimi
TO
Tuesday, 10 September 2002 Dear Professor Sarkar, I am taking the liberty of sending you the first beta
version of my CD ROM "Physics of Human Intention". You and your colleagues
can find there my email to Dr. Nick Mavromatos (Mavromatos.html) and other
material which, I believe, is relevant to your forthcoming conference "Branes,
Gravity, Condensed Matter and Nonlinear Quantum Mechanics", September 11-14,
2002,
I wish I knew earlier about this very important event. Anyway, I hope you and/or some colleague of yours might find the subject of my CD ROM interesting. I mention there the research done by some of the participants of your conference. Please convey my kind regards to Dr. Nick Mavromatos and Professor John G. Taylor. Sincerely yours, D. Chakalov Encl.: 1
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