prof. dr hab. David Blaschke
 profesor
                    Zakład Fizyki Cząstek i Astrofizyki Jądrowej                
Z-ca Dyrektora ds. naukowych 
                        Instytut Fizyki Teoretycznej                    
pl. M. Borna 9
                                                    david.blaschke@uwr.edu.pl
                                                                            tel. +48 71 375 92 52, +48 71 375 93 55
                                                                    
Zainteresowania
- particle physics
 - theoretical nuclear physics
 - nuclear matter
 - quark matter
 - equation of state
 - neutron stars
 - stars neutron
 - phase transition
 - neutron star
 - neutron star matter
 
Dyscyplina naukowa
- nauki fizyczne
 
Najnowsze publikacje
- Unperturbed inverse kinematics nucleon knockout measurements with a carbon beam
 - Dense nuclear matter equation of state from heavy-ion collisions
 - Identifying a First-Order Phase Transition in Neutron-Star Mergers through Gravitational Waves
 - Equation of State Constraints from the Threshold Binary Mass for Prompt Collapse of Neutron Star Mergers
 - Neutron stars with crossover to color superconducting quark matter
 - Toward a unified equation of state for multi-messenger astronomy
 - Third family of compact stars within a nonlocal chiral quark model equation of state
 - Density functional approach to quark matter with confinement and color superconductivity
 - Effect of color superconductivity on the mass of hybrid neutron stars in an effective model with perturbative QCD asymptotics
 - Constraining the onset density of the hadron-quark phase transition with gravitational-wave observations
 - Sexaquark dilemma in neutron stars and its solution by quark deconfinement
 - Update of the three-fluid hydrodynamics-based event simulator: Light-nuclei production in heavy-ion collisions
 - Effect of mesonic off-shell correlations in the PNJL equation of state
 - Constraining free parameters of a color superconducting nonlocal Nambu–Jona-Lasinio model using Bayesian analysis of neutron stars mass and radius measurements
 - Ionization potential depression and Pauli blocking in degenerate plasmas at extreme densities
 - Hybrid star phenomenology from the properties of the special point
 - First-order phase transition from hypernuclear matter to deconfined quark matter obeying new constraints from compact star observations
 - Universal relations for rapidly rotating cold and hot hybrid stars
 - Ab Initio Static Exchange–Correlation Kernel across Jacob’s Ladder without Functional Derivatives
 - Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations
 
