hovik grigorian dubna, jinr yerevan 2008 international symposium the modern physics of compact stars
Post on 21-Dec-2015
215 views
TRANSCRIPT
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?