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Nuclear Energy Density Functionals and Neutron Star Properties
Acta Physica Polonica B, 46 (2015), 3; 369-378. https://doi.org/10.5506/APhysPolB.46.369
Paar, Nils; Moustakidis, Ch. C.; Lalazissis, G. A.; Marketin, Tomislav; Vretenar, Dario

Citirajte ovaj rad

Paar, N., Moustakidis, C. C., Lalazissis, G. A., Marketin, T. i Vretenar, D. (2015). Nuclear Energy Density Functionals and Neutron Star Properties. Acta Physica Polonica B, 46. (3), 369-378. doi: 10.5506/APhysPolB.46.369

Paar, Nils, et al. "Nuclear Energy Density Functionals and Neutron Star Properties." Acta Physica Polonica B, vol. 46, br. 3, 2015, str. 369-378. https://doi.org/10.5506/APhysPolB.46.369

Paar, Nils, Ch. C. Moustakidis, G. A. Lalazissis, Tomislav Marketin i Dario Vretenar. "Nuclear Energy Density Functionals and Neutron Star Properties." Acta Physica Polonica B 46, br. 3 (2015): 369-378. https://doi.org/10.5506/APhysPolB.46.369

Paar, N., et al. (2015) 'Nuclear Energy Density Functionals and Neutron Star Properties', Acta Physica Polonica B, 46(3), str. 369-378. doi: 10.5506/APhysPolB.46.369

Paar N, Moustakidis CC, Lalazissis GA, Marketin T, Vretenar D. Nuclear Energy Density Functionals and Neutron Star Properties. Acta Physica Polonica B [Internet]. 2015. [pristupljeno 04.12.2024.];46(3):369-378. doi: 10.5506/APhysPolB.46.369

N. Paar, C. C. Moustakidis, G. A. Lalazissis, T. Marketin i D. Vretenar, "Nuclear Energy Density Functionals and Neutron Star Properties", Acta Physica Polonica B, vol. 46, br. 3, str. 369-378, 2015. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:517085. [Citirano: 04.12.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:517085
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Podaci o radu
Naslov (engleski)Nuclear Energy Density Functionals and Neutron Star Properties
AutorNils Paar
AutorCh. C. Moustakidis
AutorG. A. Lalazissis
AutorTomislav Marketin
AutorDario Vretenar
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Sažetak (engleski)
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 nt and pressure Pt 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.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Pregledni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaActa Physica Polonica B
Brojčani podacivol. 46, br. 3, str. 369-378
p-ISSN0587-4254
DOIhttps://doi.org/10.5506/APhysPolB.46.369
URN:NBNurn:nbn:hr:217:517085
Datum objave publikacije2015
ProjektŠifra: 291823
Naziv (engleski): New International Fellowship Mobility Programme for Experienced Researchers
Kratica: NEWFELPRO
Pravna nadležnost: eu
Financijer: EC
Linija financiranja: FP7
URL dokumentahttp://dx.doi.org/10.5506/APhysPolB.46.369
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Imenovanje 4.0 međunarodna (CC BY 4.0)
Datum i vrijeme pohrane2020-01-11 14:10:48