
dr Oleksii Ivanytskyi
pl. M. Borna 9
oleksii.ivanytskyi@uwr.edu.pl
tel. +48 71 375 92 52, +48 71 375 94 08
Zainteresowania
- particle physics
- quark matter
- neutron stars
- stars neutron
- dark matter
- neutron star
- equation of state
- compact stars
- astronomy astrophysics
- heavy ion collisions
Dyscyplina naukowa
- nauki fizyczne
Najnowsze publikacje
- 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
- The Effects of Self-interacting Bosonic Dark Matter on Neutron Star Properties
- Hybrid star phenomenology from the properties of the special point
- What Is the Nature of the HESS J1731-347 Compact Object?
- Bosonic dark matter in neutron stars and its effect on gravitational wave signal
- Rapid neutron star cooling triggered by dark matter
- A new class of hybrid EoS with multiple critical endpoints for simulations of supernovae, neutron stars and their mergers
- Thermodynamics of quark matter with multiquark clusters in an effective Beth-Uhlenbeck type approach
- Status and initial physics performance studies of the MPD experiment at NICA
- Thermal production of sexaquarks in heavy-ion collisions
- Induced surface and curvature tension equation of state for hadron resonance gas in finite volumes and its relation to morphological thermodynamics
- Recovering the Conformal Limit of Color Superconducting Quark Matter within a Confining Density Functional Approach
- Colliding and Fixed Target Mode in a Single Experiment—A Novel Approach to Study the Matter under New Extreme Conditions
- Early Quark Deconfinement in Compact Star Astrophysics and Heavy-ion Collisions
- Quark Deconfinement in Compact Stars Through Sexaquark Condensation
- The Impact of Asymmetric Dark Matter on the Thermal Evolution of Nucleonic and Hyperonic Compact Stars
- Constraints on the fermionic dark matter from observations of neutron stars
- Special point "trains" in the M-R diagram of hybrid stars
- Early deconfinement of asymptotically conformal color-superconducting quark matter in neutron stars