There still remained one interesting question. When you have the gain point, the material inside the gain point has the feature that the entropy increases steadily with distance from the center. On the other hand, once you are beyond the gain point, the entropy will decrease from there on out. You have a maximum of the entropy at the gain point, and one of the difficulties was you make the neutrino capture and therefore the energy, close to the gain point; but how do you get them out to the shock which goes out through the... through the star? And that I then suggested is... goes by convection, because once the entropy decreases with increasing radius, it is known that this is unstable to convection. This was found by Karl Schwarzschild, the father of the Martin Schwarzschild who is the [first] modern astrophysicist. So you then get convection, so as you absorb neutrinos and heat the material, that hot material goes out to the surface and drives a shock. Now, then the shock starts just with a velocity which is given to it by the amount of matter which has accreted by further material falling in, and that velocity is a few thousand kilometers per second. That seems fast enough but when you looked at the... at the numerical calculations by Jim Wilson and his collaborators, you found that after a certain time the velocity of the shock gets to be much bigger: tens of thousands, or let me say 10 to 20,000 kilometers per second. How does that come about? And there I made a wrong theory. I thought it came about because the nucleons which you have produced in the shock at high temperature begin to recombine once the temperature falls below 10 billion degrees. So you get the recombination and that recombination gives you energy and that energy I thought accelerates the shock.