3D Collapse of Rotating Stellar Iron Cores in General Relativity with Microphysics
نویسنده
چکیده
C. D. Ott, H. Dimmelmeier, A. Marek, H.-T. Janka, I. Hawke, B. Zink, 4 and E. Schnetter Max-Planck-Institut für Gravitationsphysik, Albert-Einstein-Institut, Am Mühlenberg 1, D-14476 Potsdam, Germany Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, D-85741 Garching, Germany School of Mathematics, University of Southampton, Southampton SO17 1BJ, UK Center for Computation and Technology, Louisiana State University, Baton Rouge, LA 70803, USA
منابع مشابه
3D collapse of rotating stellar iron cores in general relativity including deleptonization and a nuclear equation of state.
We present 2D and 3D simulations of the collapse of rotating stellar iron cores in general relativity employing a nuclear equation of state and an approximate treatment of deleptonization. We compare fully general relativistic and conformally flat evolutions and find that the latter treatment is sufficiently accurate for the core-collapse supernova problem. We focus on gravitational wave (GW) e...
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