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Nuclear “ bubble” structure in 34Si
Physical Review C - Nuclear Physics, 79 (2009), 3; 034318. https://doi.org/10.1103/PhysRevC.79.034318
Grasso, M.; Gaudefroy, L.; Khan, E.; Nikšić, Tamara; Piekarewicz, J.; Sorlin, O.; Giai, N. Van; Vretenar, Dario

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Grasso, M., Gaudefroy, L., Khan, E., Nikšić, T., Piekarewicz, J., Sorlin, O. ... Vretenar, D. (2009). Nuclear “ bubble” structure in 34Si. Physical Review C - Nuclear Physics, 79. (3). doi: 10.1103/PhysRevC.79.034318

Grasso, M., et al. "Nuclear “ bubble” structure in 34Si." Physical Review C - Nuclear Physics, vol. 79, br. 3, 2009. https://doi.org/10.1103/PhysRevC.79.034318

Grasso, M., L. Gaudefroy, E. Khan, Tamara Nikšić, J. Piekarewicz, O. Sorlin, N. Van Giai i Dario Vretenar. "Nuclear “ bubble” structure in 34Si." Physical Review C - Nuclear Physics 79, br. 3 (2009). https://doi.org/10.1103/PhysRevC.79.034318

Grasso, M., et al. (2009) 'Nuclear “ bubble” structure in 34Si', Physical Review C - Nuclear Physics, 79(3). doi: 10.1103/PhysRevC.79.034318

Grasso M, Gaudefroy L, Khan E, Nikšić T, Piekarewicz J, Sorlin O, i sur.. Nuclear “ bubble” structure in 34Si. Physical Review C - Nuclear Physics [Internet]. 2009. [pristupljeno 19.04.2024.];79(3). doi: 10.1103/PhysRevC.79.034318

M. Grasso, et al., "Nuclear “ bubble” structure in 34Si", Physical Review C - Nuclear Physics, vol. 79, br. 3, 2009. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:403795. [Citirano: 19.04.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:403795
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Naslov (engleski)Nuclear “ bubble” structure in 34Si
AutorM. Grasso
AutorL. Gaudefroy
AutorE. Khan
AutorTamara Nikšić
AutorJ. Piekarewicz
AutorO. Sorlin
AutorN. Van Giai
AutorDario Vretenar
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Sažetak (engleski)
Bubble nuclei are characterized by a depletion of their central density. Their existence is examined within three different theoretical frameworks: the shell model and nonrelativistic and relativistic microscopic mean-field approaches. We analyze 34Si and 22O as possible candidates for proton and neutron bubble nuclei, respectively. In the case of 22O, we observe a significant model dependence, thereby calling into question the bubble structure of 22O. In contrast, an overall agreement among the models is obtained for 34Si. Indeed, all models predict a central proton density depletion of about 40% and a central charge density depletion of 25%– 30%. This result provides strong evidence in favor of a proton bubble in 34Si.
Jezikengleski
Vrsta publikacijeZnanstveni rad - Izvorni znanstveni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaPhysical Review C - Nuclear Physics
Brojčani podacivol. 79, br. 3, 034318
p-ISSN0556-2813
e-ISSN1089-490X
DOIhttps://doi.org/10.1103/PhysRevC.79.034318
URN:NBNurn:nbn:hr:217:403795
Datum objave publikacije2009
ProjektŠifra: 119-1191005-1010
Naziv (hrvatski): Nuklearna struktura i nuklearna astrofizika
Voditelj: Dario Vretenar
Pravna nadležnost: Hrvatska
Financijer: MZOS
Linija financiranja: ZP
URL dokumentahttp://link.aps.org/doi/10.1103/PhysRevC.79.034318
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomenaCopyright (2009) by the American Physical Society. Received 22 September 2008; revised manuscript received 10 February 2009; published 26 March 2009.
Datum i vrijeme pohrane2019-10-19 19:55:44