| Topic: |
Science > Physics |
| User: |
"OsherD" |
| Date: |
01 Aug 2005 10:46:38 AM |
| Object: |
Coulomb Forces Generalized Via Newton-PI |
From Osher Doctorow
COPYRIGHT NOTICE
Coulomb Forces Generalized Via Newton-PI
Copyright By Owner Osher Doctorow Ph.D.
First Published 2005
In replacing Quantum Theory (QT) and GR by Newton-PI Theory (NP for
short), the most promising development is the pervasiveness of
generalized Coulomb forces and "Coulomb-like potentials" and simiar
variables in QT and somewhat in GR.
Expression of the form:
1) 1/r^a
where r is a distance/length variable and a is a positive constant
either underlie or approximate closely or generalize to energy and
related variables in QED, QEW, and QCD. Expressions like (1) are
specializations of the form of conditional probability expressions y/x
for x not 0, and those in turn easily convert to Probable Influence
(PI) form 1 + y - x.
A second promising avenue is the Lagrangian or Lagrangian density,
whose additive structure is directly in line with PI.
In GR, aside from the Perihelion of Mercury, most widely used
applications such as Cosmology are based on power laws or linear laws
such as those involving pressure vs density and so relate to (1) with
negative "a" or positive a.
Superstring/Brane Theory dualities involve inverse relationships in the
spirit of (1) prominently, and the only part of the Heisenberg
Uncertainty Principle (HUP) that has some accuracy, namely momentum vs
position ranges under certain conditions (and momentum vs position
themselves under certain conditions) relate to the fact that velocity
is essentially a (limiting) two-point while position is essentially a
one-point variable and these are difficult to simultaneously
measure/specify under certain microscopic conditions by the nature of
one-point vs (limiting) two-point differences in small magnitudes.
Take a look at hep-th/0201098, hep-th/9602132 for starters, and I'll
return hopefully with a much longer list.
Osher Doctorow
.
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