hovik grigorian dubna, jinr yerevan 2008 international symposium the modern physics of compact stars

Hovik GrigorianDubna, JINR

Yerevan 2008International SymposiumThe Modern Physics of Compact Stars

Cooling of Compact stars Schematic introduction of simulations Configurations of Compact stars Cooling processes Crust, SC Gaps and ... Time Evolution of Surface Temperature Constraints from Observations Summary & Discussion

Quasi-Equilibrate Evolution of Compact Objects

Stellar Matter under Compact star conditions

Cooling Evolution

Phase transition to QM

Internal structure of HS

The most of pathologies of hadronic stars are descendible

C74:025801,2006

How to distinguish the different types of Hybrid star models from cooling evolution?

Statistics of Compact stars

Could the Mass Distribution of NSs be exstracted from the cooling models?

Cooling of NSs is one of testing schemes for High density matter EoS

Mass distribution of NS is extracted from the cooling model

Cooling data allowed existence of HS even with one flaver QM

DU can be consided as a problem

Do Hybrid NSs an alternative or the solution of problems of compact stars?

Do for all constraints exist a valid HNS model? Can magnetic field and surface heating modify the main conclusions on cooling of NS? Is the mass distribution of NSs an obsorvable?