NSR Query Results
Output year order : Descending NSR database version of May 2, 2024. Search: Author = H.Grigorian Found 17 matches. 2021AY07 Eur.Phys.J. A 57, 318 (2021) A.Ayriyan, D.Blaschke, A.G.Grunfeld, D.Alvarez-Castillo, H.Grigorian, V.Abgaryan Bayesian analysis of multimessenger M-R data with interpolated hybrid EoS
doi: 10.1140/epja/s10050-021-00619-0
2019MA60 Phys.Rev. C 100, 025802 (2019) K.Maslov, N.Yasutake, D.Blaschke, A.Ayriyan, H.Grigorian, T.Maruyama, T.Tatsumi, D.N.Voskresensky Hybrid equation of state with pasta phases, and third family of compact stars
doi: 10.1103/PhysRevC.100.025802
2018AY01 Phys.Rev. C 97, 045802 (2018) A.Ayriyan, N.-U.Bastian, D.Blaschke, H.Grigorian, K.Maslov, D.N.Voskresensky Robustness of third family solutions for hybrid stars against mixed phase effects
doi: 10.1103/PhysRevC.97.045802
2018GR10 Nucl.Phys. A980, 105 (2018) H.Grigorian, D.N.Voskresensky, K.A.Maslov Cooling of neutron stars in "nuclear medium cooling scenario" with stiff equation of state including hyperons
doi: 10.1016/j.nuclphysa.2018.10.014
2016AL07 Eur.Phys.J. A 52, 69 (2016) D.Alvarez-Castillo, A.Ayriyan, S.Benic, D.Blaschke, H.Grigorian, S.Typel New class of hybrid EoS and Bayesian M - R data analysis
doi: 10.1140/epja/i2016-16069-2
2016GR02 Eur.Phys.J. A 52, 67 (2016) H.Grigorian, D.N.Voskresensky, D.Blaschke Influence of the stiffness of the equation of state and in-medium effects on the cooling of compact stars
doi: 10.1140/epja/i2016-16067-4
2013BL12 Phys.Rev. C 88, 065805 (2013) D.Blaschke, H.Grigorian, D.N.Voskresensky Nuclear medium cooling scenario in light of new Cas A cooling data and the 2M(.)pulsar mass measurements
doi: 10.1103/PhysRevC.88.065805
2012BL02 Phys.Rev. C 85, 022802 (2012) D.Blaschke, H.Grigorian, D.N.Voskresensky, F.Weber Cooling of the neutron star in Cassiopeia A
doi: 10.1103/PhysRevC.85.022802
2006BL19 Nucl.Phys. A774, 815 (2006) D.Blaschke, D.Voskresensky, H.Grigorian Cooling of Neutron Stars with Color Superconducting Quark Cores
doi: 10.1016/j.nuclphysa.2006.06.142
2006GR18 Phys.Rev. C 74, 025801 (2006) Brightness constraint for cooling models of young neutron stars
doi: 10.1103/PhysRevC.74.025801
2006KL08 Phys.Rev. C 74, 035802 (2006) T.Klahn, D.Blaschke, S.Typel, E.N.E.van Dalen, A.Faessler, C.Fuchs, T.Gaitanos, H.Grigorian, A.Ho, E.E.Kolomeitsev, M.C.Miller, G.Ropke, J.Trumper, D.N.Voskresensky, F.Weber, H.H.Wolter Constraints on the high-density nuclear equation of state from the phenomenology of compact stars and heavy-ion collisions
doi: 10.1103/PhysRevC.74.035802
2006PO12 Phys.Rev. C 74, 025803 (2006) S.B.Popov, H.Grigorian, D.Blaschke Neutron star cooling constraints for color superconductivity in hybrid stars
doi: 10.1103/PhysRevC.74.025803
2005AG13 Nucl.Phys. A757, 527 (2005) D.N.Aguilera, D.Blaschke, H.Grigorian How robust is a 2SC quark matter phase under compact star constraints?
doi: 10.1016/j.nuclphysa.2005.04.009
2005GR08 Phys.Rev. C 71, 045801 (2005) H.Grigorian, D.Blaschke, D.Voskresensky Cooling of neutron stars with color superconducting quark cores
doi: 10.1103/PhysRevC.71.045801
2004BL07 Nucl.Phys. A736, 203 (2004) D.Blaschke, S.Fredriksson, H.Grigorian, A.M.Oztas Diquark condensation effects on hot quark star configurations
doi: 10.1016/j.nuclphysa.2004.02.022
2004GR19 Phys.Rev. C 69, 065802 (2004) H.Grigorian, D.Blaschke, D.N.Aguilera Hybrid stars with color superconductivity within a nonlocal chiral quark model
doi: 10.1103/PhysRevC.69.065802
2003GR07 Nucl.Phys. A715, 831c (2003) H.Grigorian, D.Blaschke, G.Poghosyan Mapping Deconfinement with a Compact Star Phase Diagram
doi: 10.1016/S0375-9474(02)01513-0
Back to query form |