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
514 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
254 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
193 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
130 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
119 2005 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
107 2012 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
106 2001 Strangeness in the cores of neutron stars R Lastowiecki, D Blaschke, H Grigorian, S Typel
arXiv preprint arXiv:1112.6430, 2011
86 2011 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
84 2022 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
81 2000 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
80 2020 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
78 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 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
72 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 D Blaschke, H Grigorian, DN Voskresensky
Physical Review C 88 (6), 065805, 2013
62 2013 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
57 2021 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
57 2006 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
54 2018 
David BlaschkeProfessor for Theoretical Physics, University of WroclawBestätigte E-Mail-Adresse bei ift.uni.wroc.pl
