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Scientific paper - Original scientific paper
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, no. 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 and Dario Vretenar. "Nuclear “ bubble” structure in 34Si." Physical Review C - Nuclear Physics 79, no. 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, and sur.. Nuclear “ bubble” structure in 34Si. Physical Review C - Nuclear Physics [Internet]. 2009 [cited 2024 November 19];79(3). doi: 10.1103/PhysRevC.79.034318

M. Grasso, et al., "Nuclear “ bubble” structure in 34Si", Physical Review C - Nuclear Physics, vol. 79, no. 3, 2009. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:403795. [Accessed: 19 November 2024]

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Metadata
Title (english)Nuclear “ bubble” structure in 34Si
AuthorM. Grasso
AuthorL. Gaudefroy
AuthorE. Khan
AuthorTamara Nikšić
AuthorJ. Piekarewicz
AuthorO. Sorlin
AuthorN. Van Giai
AuthorDario Vretenar
Author's institutionUniversity of Zagreb
Faculty of Science
(Department of Physics)
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Abstract (english)
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.
Languageenglish
Publication typeScientific paper - Original scientific paper
Publication statusPublished
Peer reviewPeer review - international
Publication versionPublished version
Journal titlePhysical Review C - Nuclear Physics
Numberingvol. 79, no. 3, 034318
p-ISSN0556-2813
e-ISSN1089-490X
DOIhttps://doi.org/10.1103/PhysRevC.79.034318
URN:NBNurn:nbn:hr:217:403795
Publication2009
ProjectNumber: 119-1191005-1010
Title (croatian): Nuklearna struktura i nuklearna astrofizika
Leader: Dario Vretenar
Jurisdiction: Croatia
Funding stream: ZP
Document URLhttp://link.aps.org/doi/10.1103/PhysRevC.79.034318
Type of resourceText
Access conditionsOpen access
Terms of useLicence In copyright icon
Public noteCopyright (2009) by the American Physical Society. Received 22 September 2008; revised manuscript received 10 February 2009; published 26 March 2009.
Created on2019-10-19 19:55:44