Now here is a post quite recently done by me, concerning how many
Coulomb Interactions exist
in the 231Pu Atom Totality in order to hold together the Universe and
make it work:
Newsgroups: sci.physics, sci.math
From: "a_plutonium" <a_pluton...@hotmail.com>
Date: 24 Jan 2007 00:40:51 -0800
Local: Wed, Jan 24 2007 3:40 am
Subject: *5* new book "ATOM TOTALITY THEORY Replaces Big Bang Theory
in PHYSICS" ; Cosmic blackbody microwave radiation
a_plutonium wrote:
> Now I have listed these supporting evidences according to what I deem
> the greatest weight of support
[quoted text clipped - 13 lines]
> 10) inverse fine structure constant and proton to electron mass ratio
> 11) pi e explained
Atom Totality theory explains uniform blackbody 2.71 K cosmic
microwave
background radiation
First question to those who know physics, can you
really have a
blackbody radiation such as the ones that Planck had
studied and
had researched and used to form the foundation of
quantum mechanics
that is not uniform? That it may have fluctuations?
Second question,
can the Cosmos really have a blackbody radiation and
not be a cavity?
Such as the cavity of the 5f6 of 231Pu?
Third question, can you really have a blackbody cavity
as the Cosmos itself and not be an Atom?
-------
From: Archimedes Plutonium
Newsgroups:
sci.physics,sci.physics.
particle,sci.chem,sci.physics.electromag,sci.astro
Subject: Re: Minimum Coulomb Interactions for
plutonium
Date: 30 Sep 1995 02:39:12 GMT
Lines: 92
In article (44e36n...@rzsun02.rrz.uni-hamburg.de>
fc3a...@AMRISC03.math.uni-hamburg.de (Hauke Reddmann)
writes:
> And Pu is then the case where even the Schroedinger
> equation can't be written out. (Remember that Pu has
a so high
> mass number that relativistic effects come in.) In
this case you
> use approximations, like treating closed shells as a
spherically
> symmetric potential. Of course the calculations then
are not
> nearly exact as in the H case.
> So, which value should YOU use? As you are sort of a
> neopythagorean, I fear you won't be satisfied with
approximations
> and must use the 95!/2 value. Even worse, this only
nails down
> the coulomb interactions. There are loads of
second-order effects
> due to spin dependent interactions.
> Hope this helps. This post got very long, but you
see what happens
> when you get into the realm of "dirty" science, with
all sorts of
> models, approximations and calculations.
Thank you very much both Hauke Reddmann and Gerald
L. Hurst.
The Coulombic states is a very large number indeed.
And it is
commonsense and intuition that says that a neon atom
is held in
place by lots more than just 190 things going on. Neon
is held up
by at least 10^7 things going on.
I can use any of these large numbers for plutonium,
(2^188 x2x2x2) of (n,L,M_L,m_s), or the 95!/2, or the
one which
I favor the most since as of recent it comes from the
Hydrogen
Atom Systems where all the forces are either Coulombic
or
Radioactivity. Thus 231PU is ((2^231) x2x2x2) or
232!/2.
With those large numbers it really does not matter
for the
difference of one more electron and proton in the next
element
after plutonium, which is element 95. These numbers
are so huge
and that is what is needed in order to compose a
thermodynamics.
> Archimedes Plutonium
> www.iw.net/~a_plutonium
> whole entire Universe is just one big atom
> where dots of the electron-dot-cloud are galaxies