Scientists at Princeton University and the U.S. Department of Energy’s (DOE) Princeton Plasma Physics Laboratory (PPPL) have developed a rigorous new method for modeling the accretion disk that feeds the supermassive black hole at the center of our Milky Way galaxy. The paper, published online in December in the journal Physical Review Letters, provides a much-needed foundation for simulation of the extraordinary processes involved.
M. Schatten, I. Tomicić, and B. Okreša Đurić. 38th International Convention on Information and Communication Technology, Electronics and Microelectronics (MIPRO), page 1256--1261. Opatija, HR, IEEE, (May 2015)