G'day ramparts
In a nutshell
Compact matter has properties that allow it to form a vortex, the stability of the vortex is dependent on the size and type of matter. This vortex is able to eject matter from the core of the compact matter as subatomic particles carried in a magnetic field close to the speed of light, we also know that atoms form from a memory property. This process can explain the formation of supernovas and the giant jets of AGN that are able to eject matter and reform galaxies near and far. What ever images that we see can be explained without using the BBT that relies on ad hoc theories to make it work.
Some people think that I'm trying to prove a point. Far from it. I'm several years from really even thinking of proving any points.
The next Ten years are very promissing from NASA to research compact matter and the various frequencies of phase transition during a supernova and AGN.
This may be of interest:
http://arxiv.org/abs/0909.4201
Symmetry breaking patterns and collective modes of spin-one color superconductors
Authors: Tomas Brauner, Jin-yi Pang, Qun Wang
(Submitted on 23 Sep 2009)
Abstract: Spin-one color superconductor is a viable candidate phase of dense matter in the interiors of compact stars. Its low-energy excitations will influence the transport properties of such matter and thus have impact on late-stage evolution of neutron stars. It also provides a good example of spontaneous symmetry breaking with rich breaking patterns. In this contribution, we reanalyze the phase diagram of a spin-one color superconductor and point out that a part of it is occupied by noninert states, which have been neglected in literature so far. We classify the collective Nambu--Goldstone modes, which are essential to the transport phenomena.
and
http://arxiv.org/abs/0906.3043
The Meissner Effect and Vortex Expulsion in Color-Superconducting Quark stars, and its Role for Re-heating of Magnetars
Authors: Brian Niebergal, Rachid Ouyed, Rodrigo Negreiros, Fridolin Weber
(Submitted on 16 Jun 2009)
Abstract: Compact stars made of quark matter rather than confined hadronic matter, are expected to form a color superconductor. This superconductor ought to be threaded with rotational vortex lines within which the star's interior magnetic field is confined. The vortices (and thus magnetic flux) would be expelled from the star during stellar spin-down, leading to magnetic reconnection at the surface of the star and the prolific production of thermal energy. In this Letter, we show that this energy release can re-heat quark stars to exceptionally high temperatures, such as observed for Soft Gamma Repeaters (SGRs), Anomalous X-Ray pulsars (AXPs), and X-ray dim isolated neutron stars (XDINs). Moreover, our numerical investigations of the temperature evolution, spin-down rate, and magnetic field behavior of such superconducting quark stars suggest that SGRs, AXPs, and XDINs may be linked ancestrally. Finally, we discuss the possibility of a time delay before the star enters the color superconducting phase, which can be used to estimate the density at which quarks deconfine. We find this density to be five times that of nuclear saturation.