Text version.
Dynamics of Bianchi IX universe with massive scalar field.
Abstract:The dynamics of the Bianchi IX cosmological model with
minimally coupled massive real scalar field is studied. The possibility of
non-singular transition from contraction to expansion is shown. A set of
initial conditions that lead to non-singular solutions is studied
numerically.
Source(gzipped unix tape
archive), PostScript(gzipped
PostScript document).
The results of numerical computations available on this page in animated
GIF format. There are some differences between the color notation adopted in
the article and GIF animations. The correspondence between these
color notations listed below:
| Article |
GIFs |
| light-gray |
blue |
| gray |
green |
| dim-gray |
yellow |
| black |
red |
The slice in 
plane for the values of 
growing from 0.1549 to 0.1608 : bp_bm1.gif.
The slice in
plane for the values of
growing from 0.7593 to 0.7627 : bp_bm2.gif.
The slice in
plane for the values of
growing from 1.1415 to 1.1426 : bp_bm3.gif.
The slice in 
plane for the values of
growing from 0.1536 to 0.1608 : bp_bpd1.gif.
The slice in 
plane for the values of
growing from 0.1525 to 0.1610 : bm_bmd1.gif.
The slice in
plane for the values of
growing from 0.7593 to 0.7622 : bm_bmd2.gif.
These GIFs may be viewed directly from your browser but it would be
better to download them on your local disc and use appications wich allows
to view animated GIFs (for example XAnim: http://xanim.va.pubnix.com/home.html
).
All GIFs in unix tape archive are here: dynB_IXgifs.tar
.
