From femtonova to supernova: Heavy-ion collisions and the supernova equation of state

Hagel, K. and Hempel, M. and Natowitz, J. B. and Röpke, G. and Typel, S. and Wuenschel, S. and Wada, R. and Barbui, M. and Schmidt, K.. (2016) From femtonova to supernova: Heavy-ion collisions and the supernova equation of state. In: 12th International Conference on Nucleus-Nucleus Collisions 2015, 117.

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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.
Faculties and Departments:05 Faculty of Science > Departement Physik > Former Organization Units Physics > Astrophysik (Liebendörfer)
UniBasel Contributors:Hempel, Matthias
Item Type:Conference or Workshop Item, refereed
Conference or workshop item Subtype:Conference Paper
Publisher:EDP Sciences
Series Name:EPJ Web of Conferences
Note:Publication type according to Uni Basel Research Database: Conference paper
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Last Modified:15 Mar 2017 12:58
Deposited On:15 Mar 2017 12:58

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