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

Klähn, T.; Blaschke, D.; Typel, S.; N. E. van Dalen, E.; Faessler, Amand; Fuchs, Christian; Gaitanos, T.; Grigorian, H.; Ho, A.; É. Kolomeitsev, E.; Coleman Miller, M.; Röpke, G.; Trümper, J.; N. Voskresensky, D.; Weber, Fridolin; Wolter, H.H.

doi:10.1103/physrevc.74.035802

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

Published in Physical Review C • Sep 21, 2006

Authors:

T. Klähn

D. Blaschke

S. Typel

Abstract

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 $1.5{M...

Subject

Physics

Neutron star

Nuclear matter

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