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Model dependence of the neutron-skin thickness on the symmetry energy
Physical Review C, 93 (2016), 6; 064303. https://doi.org/10.1103/PhysRevC.93.064303
Mondal, C.; Agrawal, B. K.; Centelles, M.; Colò, G.; Roca-Maza, X.; Paar, Nils; Viñas, X.; Singh, S. K.; Patra, S. K.

Institucijski repozitorij: Repozitorij Prirodoslovno-matematičkog fakulteta

Citirajte ovaj rad

Mondal, C., Agrawal, B. K., Centelles, M., Colò, G., Roca Maza, X., Paar, N. ... Patra, S. K. (2016). Model dependence of the neutron-skin thickness on the symmetry energy. Physical Review C, 93. (6). doi: 10.1103/PhysRevC.93.064303

Mondal, C., et al. "Model dependence of the neutron-skin thickness on the symmetry energy." Physical Review C, vol. 93, br. 6, 2016. https://doi.org/10.1103/PhysRevC.93.064303

Mondal, C., B. K. Agrawal, M. Centelles, G. Colò, X. Roca Maza, Nils Paar, X. Viñas, S. K. Singh i S. K. Patra. "Model dependence of the neutron-skin thickness on the symmetry energy." Physical Review C 93, br. 6 (2016). https://doi.org/10.1103/PhysRevC.93.064303

Mondal, C., et al. (2016) 'Model dependence of the neutron-skin thickness on the symmetry energy', Physical Review C, 93(6). doi: 10.1103/PhysRevC.93.064303

Mondal C, Agrawal BK, Centelles M, Colò G, Roca Maza X, Paar N, i sur.. Model dependence of the neutron-skin thickness on the symmetry energy. Physical Review C [Internet]. 2016. [pristupljeno 29.11.2024.];93(6). doi: 10.1103/PhysRevC.93.064303

C. Mondal, et al., "Model dependence of the neutron-skin thickness on the symmetry energy", Physical Review C, vol. 93, br. 6, 2016. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:696608. [Citirano: 29.11.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:696608
Podaci o radu
Naslov (engleski)Model dependence of the neutron-skin thickness on the symmetry energy
AutorC. Mondal
AutorB. K. Agrawal
AutorM. Centelles
AutorG. Colò
AutorX. Roca-Maza
AutorNils Paar
AutorX. Viñas
AutorS. K. Singh
AutorS. K. Patra
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Sažetak (engleski)
The model dependence in the correlations of the neutron-skin thickness in heavy nuclei with various symmetryenergy parameters is analyzed by using several families of systematically varied microscopic mean-field models. Such correlations show a varying degree of model dependence once the results for all the different families are combined. Some mean-field models associated with similar values of the symmetry-energy slope parameter at saturation density L, and pertaining to different families, yield a greater-than-expected spread in the neutron-skin thickness of the 208Pb nucleus. The effective value of the symmetry-energy slope parameter Leff, determined by using the nucleon density profiles of the finite nucleus and the density derivative S (ρ) of the symmetry energy starting from about saturation density up to low densities typical of the surface of nuclei, seems to account for the spread in the neutron-skin thickness for the models with similar L. The differences in the values of Leff are mainly due to the small differences in the nucleon density distributions of heavy nuclei in the surface region and the behavior of the symmetry energy at subsaturation densities.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Izvorni znanstveni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaPhysical Review C
Brojčani podacivol. 93, br. 6, 064303
p-ISSN2469-9985
e-ISSN2469-9993
DOIhttps://doi.org/10.1103/PhysRevC.93.064303
URN:NBNurn:nbn:hr:217:696608
Datum objave publikacije2016
ProjektŠifra: IP-2014-09-9159
Naziv (hrvatski): Struktura i dinamika egzotičnih femto-sustava
Kratica: STRUDEF
Voditelj: Nils Paar
Pravna nadležnost: Hrvatska
Financijer: HRZZ
Linija financiranja: IP
URL dokumentahttps://journals.aps.org/prc/abstract/10.1103/PhysRevC.93.064303
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomena© 2016 American Physical Society. Received 8 April 2016; published 2 June 2016.
Datum i vrijeme pohrane2020-02-23 15:41:50