
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