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

By T. Klähn, D. Blaschke, S. Typel, E. V. Dalen, A. Faessler, C. Fuchs, T. Gaitanos, H. Grigorian, A. Ho, E. Kolomeitsev and 6 more. 2006

282 citations recorded by the source corpus.

A new scheme for testing nuclear matter equations of state (EoSs) at high densities using constraints from neutron star (NS) phenomenology and a flow data analysis of heavy-ion collisions is suggested. An acceptable EoS shall not allow the direct Urca process to occur in NSs with masses below 1.5M� , and also shall not contradict flow and kaon production data of heavy-ion collisions. Compact star constraints include the mass

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/b54f97dbe810ed356fdf6c68031339371e588eee

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. I. Tews
2. E. Kolomeitsev
3. A. Ohnishi
4. J. Lattimer
5. A. Watts
6. Bao-An Li
7. A. Steiner
8. A. Schwenk

In Nuclear and High Energy Physics

1. I. Tews
2. J. Lattimer
3. E. Kolomeitsev
4. A. Ohnishi

Citations in the corpus

• Symmetry Parameter Constraints from a Lower Bound on Neutron-matter Energy (2016, background): “…show values for interactions commonly used in tabulated equations of state for astrophysical simulations (notation and data from Fischer et al. 2014), and open squares (from Klähn et al. 2006) and the inverted triangle (from Maslov et al. 2016) show those of other frequently used interactions.”