Constraints on the high-density nuclear equation of state from the phenomenology of compact stars and heavy-ion collisions

T. Klähn, 2, ∗ D. Blaschke, 4, † S. Typel, E.N.E. van Dalen, A. Faessler, C. Fuchs, T. Gaitanos, H. Grigorian, 6 A. Ho, E.E. Kolomeitsev, M.C. Miller, G. Röpke, J. Trümper, D.N. Voskresensky, 11 F. Weber, and H.H. Wolter 1 Institut für Physik, Universität Rostock, 18051 Rostock, Germany 2 Institut für Theoretische Physik, Universität Tübingen, 72076 Tübingen, Germany 3 Gesellschaft für Schwerionenforschung mbH (GSI), 64291 Darmstadt, Germany 4 Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, 141980 Dubna, Russia 5 Department für Physik, Universität München, 85748 Garching, Germany 6 Department of Physics, Yerevan State University, 375049 Yerevan, Armenia 7 Department of Physics, San Diego State University, 5500 Campanile Drive, San Diego, California 92182, USA 8 School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455, USA 9 Department of Astronomy, University of Maryland, College Park, MD 20742-2421, USA 10 Max-Planck-Institut für extraterrestrische Physik, 85741 Garching, Germany 11 Moscow Engineering Physical Institute, Kashirskoe Shosse 31,11549 Moscow, Russia (Dated: February 14, 2006)