On Jan 8, 2008, at 1:56 PM, OrionWorks wrote:
Hi Horace,
Thank you for taking the time to wade through my CM report. I've
downloaded your documents, the "Gravimagnetism" and "Creating a new
Formula" portion - all for my reading pleasure. ;-)
I'm interested in your work on the controversial MOND issue. My first
initial skim left me wondering about the ramifications of normal and
cosmic matter. I'm sure I need to read it several more times, because
at present I don't quite understand the mechanisms involved in why all
that negative gravity cosmic matter still seems to want to hang around
as spherical halos at the peripheral of galaxies. If one of cosmic
matter's properties is negative gravity (from our perspective within
the galaxy) why doesn't it simply wander off into dark space? Why does
it collect as a "halo"?
It is an outward moving Halo. It takes a long time to cross a galaxy
even at the speed of light. The halo is continuously created, so
represents a continuous flow, and at an accelerating flow rate at that.
Here is an interesting observation I noted by classifying about 3500
galaxies on galaxy zoo. The bar galaxies tend to have long flat
segments to the bars. I think this might be due to the outflow of
negative gravitation mass mirror matter weakly interacting with
outward flowing jets of real matter. There is a powerful
gravimagnetic field cast by the central black holes. The
gravimagnetic Lorentz force on the two outward matter types is in
opposed directions! The counter flow of the two weakly interacting
matter types tends to straighten the bar near the central part of the
galaxy. The gravimagnetic force drops of as the 4th power, and the
flow of the mirror matter diminishes in the outreaches, so the bar
then warps tangentially. Eventually the bar disappears and only an
ordinary ring of matter remains around the galaxy. I don't know if
this is all correct, but this is what continually pops into my head
as I view some of the many great views of bar galaxies that are
available on the web. It is certainly true that fairly rapid
precession rates must be involved for the jets of ordinary matter to
spew out radially to the gravimagnetic field, but you can see
evidence for such precession in photos of nearby bar galaxies. The
gravimagnetic axis and the pole (the pole is the line normal to the
plane of the galaxy) of bar galaxies thus must tend to be askew, and
thus the Lorentz force is manifest by the outward flow of the jets
and the mirror matter.
As for the suggestion of applying 1/r^4, Egads! My computer programs
can easily incorporate any power I wish to enter, but as you have also
mentiond, the results will be even more unstable than my 1/r^3
simulations. I'm currently at a loss as to how I might go about
incorporating overlapping Broglie wavelengths. 8-0
That's a creation of de Broglie, as in Louis-Victor-Pierre-Raymond,
7th duc de Broglie:
http://en.wikipedia.org/wiki/Louis_de_Broglie
http://en.wikipedia.org/wiki/De_broglie_wavelength
The wavelength lambda is a function of momentum:
lambda = h / p = h / (gamma*m*v)
Divide by 2 and you have the apparent radius of the particle. When
two particle's wavelengths overlap, you can estimate the force as
due to dividing the charge according to the proportion of the volume
of the chords of a sphere of radius lamda/2 on the either side of
the center of the neighboring particle. A better approach is to
compute a simple table of charge factors (or a least squares fit
curve) by ratio of distance between centers to lambda/2, and do the
complete integration of forces throughout the volume of charge on
either side of the centers of the particles.
Hopefully in due course I may eventually be able to come up with some
intelligent follow-up questions.
I may not be able to answer them in a timely fashion or even at all
for that matter, either due to lack of time or general ignorance.
PS: How in the world do you keep all those equations straight in
your head!
That one is easy to answer. I can't. It gets worse by the year.
8^) If it weren't for my Mac I couldn't find anything.
Horace Heffner
http://www.mtaonline.net/~hheffner/
