riassunto2

MG11 
Talk detail
 

 Participant 

Cerny, Slavomir

Institution

Silesian Universuty at Opava  - Bezrucovo nam. 13 - Opava - - CZECH REPUBLIC

Session

Talk

Abstract

APT3

Equation of State of Dense Matter in Neutron Stars

We discuss recent equations of state for dense nuclear matter with possible phase transitions arising in neutron stars such a pion, kaon and hyperon condensation, superfluidity a quark matter, and their influence on the structure of neutron star. Specifically, we search for maximum and minimum mass, radius a temperature of neutron stars and compare them with observations

 

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