prikaz prve stranice dokumenta Nuclear Energy Density Functionals and Neutron Star Properties
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Scientific paper - review paper
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

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Paar, N., Moustakidis, C. C., Lalazissis, G. A., Marketin, T. & 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, no. 3, 2015, pp. 369-378. https://doi.org/10.5506/APhysPolB.46.369

Paar, Nils, Ch. C. Moustakidis, G. A. Lalazissis, Tomislav Marketin and Dario Vretenar. "Nuclear Energy Density Functionals and Neutron Star Properties." Acta Physica Polonica B 46, no. 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), pp. 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 [cited 2024 June 14];46(3):369-378. doi: 10.5506/APhysPolB.46.369

N. Paar, C. C. Moustakidis, G. A. Lalazissis, T. Marketin and D. Vretenar, "Nuclear Energy Density Functionals and Neutron Star Properties", Acta Physica Polonica B, vol. 46, no. 3, pp. 369-378, 2015. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:517085. [Accessed: 14 June 2024]

Metadata
Title (english)Nuclear Energy Density Functionals and Neutron Star Properties
AuthorNils Paar
AuthorCh. C. Moustakidis
AuthorG. A. Lalazissis
AuthorTomislav Marketin
AuthorDario Vretenar
Author's institutionUniversity of Zagreb
Faculty of Science
(Department of Physics)
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Abstract (english)
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.
Keywords (english)
Languageenglish
Publication typeScientific paper - review paper
Publication statusPublished
Peer reviewPeer review - international
Publication versionPublished version
Journal titleActa Physica Polonica B
Numberingvol. 46, no. 3, pp. 369-378
p-ISSN0587-4254
DOIhttps://doi.org/10.5506/APhysPolB.46.369
URN:NBNurn:nbn:hr:217:517085
Publication2015
ProjectNumber: 291823
Title (english): New International Fellowship Mobility Programme for Experienced Researchers
Acronym: NEWFELPRO
Jurisdiction: eu
Funding stream: FP7
Document URLhttp://dx.doi.org/10.5506/APhysPolB.46.369
Type of resourceText
Access conditionsOpen access
Terms of useLicence Attribution 4.0 International (CC BY 4.0) icon
Created on2020-01-11 14:10:48