Maybe reading about Jets and there formation may explain whats in black holes.
At the end of the day, nobody really knows because we have not seen a black hole or even an event horizon.
But the folowing links for those interested in reading up, is quite fascinating.
Relativistic poynting jets
http://arxiv.org/find/all/1/all:+AND.../0/1/0/all/0/1
Accretion flow transonic
http://arxiv.org/find/all/1/all:+AND.../0/1/0/all/0/1
Than again what do you think degenerate matter is?
http://arxiv.org/abs/0811.2034
Transonic properties of the accretion disk around compact objects
Authors: Banibrata Mukhopadhyay
(Submitted on 13 Nov 2008)
.Abstract: An accretion flow is necessarily transonic around a black hole. However, around a neutron star it may or may not be transonic, depending on the inner disk boundary conditions influenced by the neutron star. I will discuss various transonic behavior of the disk fluid in general relativistic (or pseudo general relativistic) framework. I will address that there are four types of sonic/critical point possible to form in an accretion disk. It will be shown that how the fluid properties including location of sonic points vary with angular momentum of the compact object which controls the overall disk dynamics and outflows
and
http://arxiv.org/abs/0812.3401
The X-ray Jets of Active Galaxies
Authors: D.M. Worrall (University of Bristol)
(Submitted on 17 Dec 2008)
Abstract: Jet physics is again flourishing as a result of Chandra's ability to resolve high-energy emission from the radio-emitting structures of active galaxies and separate it from the X-ray-emitting thermal environments of the jets. These enhanced capabilities have coincided with an increasing interest in the link between the growth of super-massive black holes and galaxies, and an appreciation of the likely importance of jets in feedback processes. I review the progress that has been made using Chandra and XMM-Newton observations of jets and the medium in which they propagate, addressing several important questions, including: Are the radio structures in a state of minimum energy? Do powerful large-scale jets have fast spinal speeds? What keeps jets collimated? Where and how does particle acceleration occur? What is jet plasma made of? What does X-ray emission tell us about the dynamics and energetics of radio plasma/gas interactions? Is a jet's fate determined by the central engine?
and
http://arxiv.org/abs/0810.0923
Dynamics of black holes
Authors: Sean A. Hayward
(Submitted on 6 Oct 2008)
Abstract: This is a review of current theory of black-hole dynamics, concentrating on the framework in terms of trapping horizons. Summaries are given of the history, the classical theory of black holes, the defining ideas of dynamical black holes, the basic laws, conservation laws for energy and angular momentum, other physical quantities and the limit of local equilibrium. Some new material concerns how processes such as black-hole evaporation and coalescence might be described by a single trapping horizon which manifests temporally as separate horizons.
This process of forming jets will be the most important process to understand.
It will explain the phase changes in star formation and the various forms of galaxy evolution