Shell closure N=16 in24O

Nociforo, C; Kanungo, R; Prochazka, A; Aumann, T; Boutin, D; Cortina-Gil, D; Davids, B; Diakaki, M; Farinon, F; Geissef, H; Gernhauser, R; Gerf, J; Janik, R; Jonson, B; Kindler, B; Knober, R; Krucken, R; Lantz, M; Lenske, H; Litvinov, YuA; Lommef, B; Mahata, K; Maierbeck, P; Musumarra, A; Nilsson, T; Otsuka, T; Perro, C; Scheidenberger, C; Sltar, B; Strmen, P; Sun, B; Szarka, I; Tanihata, I; Utsuno, Y; Weick, H; Winkler, M

dc.contributor.author	Nociforo, C	en
dc.contributor.author	Kanungo, R	en
dc.contributor.author	Prochazka, A	en
dc.contributor.author	Aumann, T	en
dc.contributor.author	Boutin, D	en
dc.contributor.author	Cortina-Gil, D	en
dc.contributor.author	Davids, B	en
dc.contributor.author	Diakaki, M	en
dc.contributor.author	Farinon, F	en
dc.contributor.author	Geissef, H	en
dc.contributor.author	Gernhauser, R	en
dc.contributor.author	Gerf, J	en
dc.contributor.author	Janik, R	en
dc.contributor.author	Jonson, B	en
dc.contributor.author	Kindler, B	en
dc.contributor.author	Knober, R	en
dc.contributor.author	Krucken, R	en
dc.contributor.author	Lantz, M	en
dc.contributor.author	Lenske, H	en
dc.contributor.author	Litvinov, YuA	en
dc.contributor.author	Lommef, B	en
dc.contributor.author	Mahata, K	en
dc.contributor.author	Maierbeck, P	en
dc.contributor.author	Musumarra, A	en
dc.contributor.author	Nilsson, T	en
dc.contributor.author	Otsuka, T	en
dc.contributor.author	Perro, C	en
dc.contributor.author	Scheidenberger, C	en
dc.contributor.author	Sltar, B	en
dc.contributor.author	Strmen, P	en
dc.contributor.author	Sun, B	en
dc.contributor.author	Szarka, I	en
dc.contributor.author	Tanihata, I	en
dc.contributor.author	Utsuno, Y	en
dc.contributor.author	Weick, H	en
dc.contributor.author	Winkler, M	en
dc.date.accessioned	2014-03-01T02:52:06Z
dc.date.available	2014-03-01T02:52:06Z
dc.date.issued	2009	en
dc.identifier.issn	0094243X	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/35849
dc.subject	Nuclear structure	en
dc.subject	Radioactive ion beams.	en
dc.title	Shell closure N=16 in24O	en
heal.type	conferenceItem	en
heal.identifier.primary	10.1063/1.3232161	en
heal.identifier.secondary	http://dx.doi.org/10.1063/1.3232161	en
heal.publicationDate	2009	en
heal.abstract	Advanced nuclear stracture models predict the presence of the shell closures N=14, 16 in neutron-rich O isotopes rather than N=20. Spectroscopic investigations performed at the neutron drip line have recently confirmed such predictions showing that the24O is a doubly magic nucleus (Z=8, N=16). Predictions within the shell model calculation for the23,24O ground state have been confirmed measuring their spectroscopic factors. Results obtained in one-neutron removal reactions performed by using in-flight radioactive ion beams produced at the Fragment Separator FRS of GSI are reported. © 2009 American Institute of Physics.	en
heal.journalName	AIP Conference Proceedings	en
dc.identifier.doi	10.1063/1.3232161	en
dc.identifier.volume	1165	en
dc.identifier.spage	90	en
dc.identifier.epage	93	en