Pregled bibliografske jedinice broj: 790718
Nuclear energy density functionals and neutron star properties
Nuclear energy density functionals and neutron star properties // Acta physica Polonica B, 46 (2015), 3; 369-378 doi:10.5506/APhysPolB.46.369 (međunarodna recenzija, pregledni rad, znanstveni)
CROSBI ID: 790718 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Nuclear energy density functionals and neutron star properties
Autori
Paar, Nils ; Moustakidis, Charalampos Ch. ; Lalazissis, Georgios A. ; Marketin, Tomislav ; Vretenar, Dario
Izvornik
Acta physica Polonica B (0587-4254) 46
(2015), 3;
369-378
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, pregledni rad, znanstveni
Ključne riječi
neutron stars ; energy density functional
Sažetak
Recently, a method based on relativistic nuclear energy density functional (EDF) has been employed to study relations between collective excitations in finite nuclei with the nuclear matter symmetry energy, and the phase transition density n(t) and pressure P- t at the inner edge separating the liquid core and the solid crust of a neutron star. By using the thermodynamic method, relativistic EDF and experimental data on the properties of charge-exchange dipole transitions, isovector giant dipole and quadrupole resonances and pygmy dipole transitions, the neutron star liquid-to-solid phase transition density and pressure are constrained. The analysis shows that accurate measurements are necessary to further constrain the symmetry energy parameters and the structure of neutron star crust.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus