EPJ Web of Conferences
Volume 117, 201612th International Conference on Nucleus-Nucleus Collisions 2015
|Number of page(s)||8|
|Section||VII. Equation of State of Neutron-Rich Nuclear Matter, Clusters in Nuclei and Nuclear Reactions|
|Published online||11 May 2016|
From femtonova to supernova: Heavy-ion collisions and the supernova equation of state
1 Cyclotron Institute, Texas A & M University, College Station, Texas, USA
2 Department of Physics, University of Basel, 4056 Basel, Switzerland
3 University of Rostock, FB Physik, Rostock, Germany
4 GSI Helmholtzzentrum fr Schwerionenforschung GmbH, D-64291 Darmstadt, Germany
5 Institute of Physics, Silesia University, Katowice, Poland
Published online: 11 May 2016
Calculations using astrophysical equations of state at low densities comparable to that of the neutrino emission surface in supernovae and accretion disks are confronted with experimental results from heavy ion collisions. An extension of previous work shows that it is important to include all of the measured experimental data to draw conclusions about the astrophysical equation of state. Armed with this information, the calculations of the astrophysical equation of state are significantly constrained. Predictions of temperatures and densities sampled in black hole accretion disks are compared to those sampled in the experimental data.
© Owned by the authors, published by EDP Sciences - SIF, 2016
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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