On Aug 3, 2005, at 11:48 AM, Jack Sarfatti wrote:

http://xxx.lanl.gov/PS_cache/astro-p...07/0507619.pdf

First of all suppose we eliminate ALL the stellar rotation curve data.
By how much will that change Omega(Dark Matter) from ~ 0.23? I will ask
P. Natarajan who is just about to lecture on

Probing Dark Matter Using Gravitational Lensing

here at SLAC Panofsky Auditorium.

Secty DOE coming here tomorrow BTW.

These guys http://xxx.lanl.gov/PS_cache/astro-p...07/0507619.pdf

assume w = 0. My model assumes w = -1 that I also need to explain the
Pioneer anomaly.


On Jul 28, 2005, at 10:07 AM, art wagner wrote:


After recently coming across these two papers, I thought it
worthwhile to bring them to your attention vis-a-vis the current
discussions .....
(http://xxx.lanl.gov/PS_cache/cond-ma...07/0507454.pdf) and
(http://xxx.lanl.gov/PS_cache/astro-p...7/0507619.pdf). The
Weyl field source model is quite interesting, no....?