hovik grigorian dubna, jinr yerevan 2008 international symposium the modern physics of compact stars
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Hovik GrigorianDubna, JINR
Yerevan 2008International SymposiumThe Modern Physics of Compact Stars
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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
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Quasi-Equilibrate Evolution of Compact Objects
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Stellar Matter under Compact star conditions
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Cooling Evolution
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Phase transition to QM
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Internal structure of HS
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The most of pathologies of hadronic stars are descendible
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C74:025801,2006
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How to distinguish the different types of Hybrid star models from cooling evolution?
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Statistics of Compact stars
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Could the Mass Distribution of NSs be exstracted from the cooling models?
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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
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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?