Constraints on the high-density nuclear equation of state from the phenomenology of compact stars and heavy-ion collisions T Klähn, D Blaschke, S Typel, ENE Van Dalen, A Faessler, C Fuchs, ... Physical Review C—Nuclear Physics 74 (3), 035802, 2006 | 512 | 2006 |
Phase diagram of three-flavor quark matter under compact star constraints D Blaschke, S Fredriksson, H Grigorian, AM Öztaş, F Sandin Physical Review D—Particles, Fields, Gravitation, and Cosmology 72 (6), 065020, 2005 | 246 | 2005 |
Modern compact star observations and the quark matter equation of state T Klähn, D Blaschke, F Sandin, C Fuchs, A Faessler, H Grigorian, ... Physics Letters B 654 (5-6), 170-176, 2007 | 190 | 2007 |
Cooling of neutron stars. Hadronic model D Blaschke, H Grigorian, DN Voskresensky Astronomy & Astrophysics 424 (3), 979-992, 2004 | 131 | 2004 |
New class of hybrid EoS and Bayesian M-R data analysis D Alvarez-Castillo, A Ayriyan, S Benic, D Blaschke, H Grigorian, S Typel The European Physical Journal A 52, 1-11, 2016 | 124 | 2016 |
Cooling of neutron stars with color superconducting quark cores H Grigorian, D Blaschke, D Voskresensky Physical Review C—Nuclear Physics 71 (4), 045801, 2005 | 117 | 2005 |
Cooling of hybrid neutron stars and hypothetical self-bound objects with superconducting quark cores D Blaschke, H Grigorian, DN Voskresensky Astronomy & Astrophysics 368 (2), 561-568, 2001 | 105 | 2001 |
Cooling of the neutron star in Cassiopeia A D Blaschke, H Grigorian, DN Voskresensky, F Weber Physical Review C—Nuclear Physics 85 (2), 022802, 2012 | 103 | 2012 |
Strangeness in the cores of neutron stars R Lastowiecki, D Blaschke, H Grigorian, S Typel arXiv preprint arXiv:1112.6430, 2011 | 83 | 2011 |
Deconfinement transition in rotating compact stars E Chubarian, H Grigorian, G Poghosyan, D Blaschke Astronomy and Astrophysics, v. 357, p. 968-976 (2000) 357, 968-976, 2000 | 79 | 2000 |
Population synthesis as a probe of neutron star thermal evolution S Popov, H Grigorian, R Turolla, D Blaschke Astronomy & Astrophysics 448 (1), 327-334, 2006 | 77 | 2006 |
A dynamical, confining model and hot quark stars D Blaschke, H Grigorian, G Poghosyan, CD Roberts, S Schmidt Physics Letters B 450 (1-3), 207-214, 1999 | 75 | 1999 |
Was GW170817 a canonical neutron star merger? Bayesian analysis with a third family of compact stars D Blaschke, A Ayriyan, DE Alvarez-Castillo, H Grigorian Universe 6 (6), 81, 2020 | 73 | 2020 |
Status and initial physics performance studies of the MPD experiment at NICA V Abgaryan, R Acevedo Kado, SV Afanasyev, GN Agakishiev, E Alpatov, ... The European Physical Journal A 58 (7), 140, 2022 | 71 | 2022 |
Hybrid equation of state with pasta phases, and third family of compact stars K Maslov, N Yasutake, D Blaschke, A Ayriyan, H Grigorian, T Maruyama, ... Physical Review C 100 (2), 025802, 2019 | 70 | 2019 |
Hybrid stars with color superconductivity within a nonlocal chiral quark model H Grigorian, D Blaschke, DN Aguilera Physical Review C—Nuclear Physics 69 (6), 065802, 2004 | 66 | 2004 |
Nuclear medium cooling scenario in light of new Cas A cooling data and the pulsar mass measurements D Blaschke, H Grigorian, DN Voskresensky Physical Review C 88 (6), 065805, 2013 | 59 | 2013 |
Neutron star cooling constraints for color superconductivity in hybrid stars SB Popov, H Grigorian, D Blaschke Physical Review C—Nuclear Physics 74 (2), 025803, 2006 | 55 | 2006 |
Bayesian analysis of multimessenger MR data with interpolated hybrid EoS A Ayriyan, D Blaschke, AG Grunfeld, D Alvarez-Castillo, H Grigorian, ... The European Physical Journal A 57 (11), 318, 2021 | 52 | 2021 |
Robustness of third family solutions for hybrid stars against mixed phase effects A Ayriyan, NU Bastian, D Blaschke, H Grigorian, K Maslov, ... Physical Review C 97 (4), 045802, 2018 | 52 | 2018 |