Pregled bibliografske jedinice broj: 387633
Nuclear “ bubble” structure in 34Si
Nuclear “ bubble” structure in 34Si // Physical Review C, 79 (2009), 3; 034318-1 doi:10.1103/PhysRevC.79.034318 (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 387633 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Nuclear “ bubble” structure in 34Si
Autori
Grasso, M. ; Gaudefroy, L. ; Khan, E. ; Nikšić, Tamara ; Piekarewicz, J. ; Sorlin, O. ; Van Giai, N. ; Vretenar, Dario
Izvornik
Physical Review C (0556-2813) 79
(2009), 3;
034318-1
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
21.10.Ft; 21.60.-n; 25.30.Bf; 27.30.+t
Sažetak
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.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Projekti:
119-1191005-1010 - Nuklearna struktura i nuklearna astrofizika (Vretenar, Dario, MZOS ) ( CroRIS)
Ustanove:
Prirodoslovno-matematički fakultet, Zagreb
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus