Friday, May 14, 2004

Gary, I took a first quick look at the Diaz paper. It looks good! It is consistent with my idea. It has w = -1 eq. (2.7) p. 3. Excellent. Of course we already knew from Bohmian NRQM theory that the quantum potential Q is a way of representing zero point energy,
e.g. Bohm's solution of the hydrogen atom ground state.

Yes, I will reference this paper from now on. Good find! A+!
Looks like you are learning something. That's the right paper at the right time. God is subtle, but not malicious. He is describing I think only the random residual micro-quantum ZPE "noise" or "normal fluid" part. I don't see any "vacuum coherence" yet in his model or any connection to "dark matter" with positive pressure and the stability of the single electron. I will study all these papers after I get the book out the door.

Keep me posted on spin off from those two PRAVDA articles. They should stir things up a bit. Awaken The Pundits from their dogmatic slumbers from the hallowed Halls of Ivy to the dark corridors of Power at Langley and The Kremlin. ;-) The Russians and Ukranians may not have a lot of money, but they still have superior intellects and this sort of stuff does not need expensive machines with huge energy outputs. Eric Davis is wrong about that. It's all micro-nanotech with a fine mesh-phase array of LC oscillators with really high Tc coils on micron to nanoscale imbedded all over the thin smart computing material of the fuselage. Each little solenoid current controls the local Josephson phase difference between the high Tc SC coil and the vacuum it occupies. Hence, the coherent phased array Theta(x)
controls induced /\zpf, i.e.

Induced /\zpf(s) ~ (Effective Area)^-1(Effective Volume)(virtual electron-positron vacuum condensate density)^1/2(real electron-pair control superconductor density)^1/2 cos[Theta(x)]

Where gauge invariant Theta(x) is sensitive to magnetic fluxes,, rotations and other Berry phase effects in the usual well known ways.

The local zero point stress-energy density tensor at scale s is

tuv (ZPF) =[ c^4/8piG*(s)]/\zpf(s)guv(x,s)

where we want s-regions such that G*(s) >> G(Newton) i.e. increasing Andrei Sakharov's "metric elasticity."



On May 14, 2004, at 5:11 AM, Jack Sarfatti wrote:

Interesting if true. If he means off-mass shell virtual particles inside vacuum off mass shell then maybe. Seems to fit with Valentini?
I haven't read it yet. His scalar field should be my vacuum coherence. Remember I have a local nonrandom signal c-number ODLRO macro-quantum order parameter controlling the residual random micro-quantum zero point noise whose pressure, positive or negative, is gravitating dark matter or antigravitating dark energy phases of exotic vacuum respectively.

Non-equilbrium of the virtual particles gives signal nonlocality (Valentini).

On May 13, 2004, at 10:19 PM, Gary S. Bekkum wrote:

Hi Jack,

Before I respond to your comments, I am wondering if you might comment on your theory vs Pedro F. Gonzalez-Diaz theory of "subquantum dark energy"; specifically:

"...the subquantum potential Vsq can take on both positive and negative values, the associated field theory can lead to positive or negative pressure, respectively...the subquantum potential is interpreted as that potential associated to the hidden dynamics of the particles which are homogenously and isotropically distributed in the universe...dark energy appears to at least partly correspond to the overall work which is done by all of the particles along their hidden trajectories associated through the Bohm's interpretation with the essential quantum indeterminancy of the observable matter in the universe...non gravitational components, i.e. dark matter and dark energy are both unitarily described by just the scalar field ..."

http://arxiv.org/abs/astro-ph/0311244


Sub-Quantum Dark Energy
Authors: Pedro F. Gonzalez-Diaz (IMAFF, CSIC, Madrid)
Comments: 7 pages, RevTex, some minor changes and references added, to appear in Phys. Rev. D
Report-no: IMAFF-RCA-03-03

A procedure is considered which upgrades the Lagrangian description of quantum relativistic particles to the Lagrangian of a proper field theory in the case that the Klein-Gordon wave equation is classically interpreted in terms of a relativistic sub-quantum potential. We apply the resulting field theory to cosmology and show that the relativistic version of the Bohm's subquantum potential which can be associated with a homogeneous and isotropic distribution of particles behaves like though it was a cosmological constant responsible for the current accelerating expansion of the universe, at least in the limit where the field potential vanishes.



Gary S. Bekkum
garysbekkum@hotmail.com


From: gaoshan.iqm@263.net
To: garysbekkum@hotmail.com
Subject: my new homepage
Date: Thu, 13 May 2004 16:40:21 +0800

Dear Gary,

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Best wishes,

Gao Shan

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