The spectroscopy of neutron-rich sdf-shell nuclei using the CLARA-PRISMA setup

X. Liang; A. Hodsdon; F. Azaiez; R. Chapman; F. Haas; D. Bazzacco; S. Beghini; B.R. Behera; L. Berti; M. Burns; E. Caurier; L. Corradi; D. Curien; A. Deacon; G. de Angelis; Zs. Dombradi; E. Farnea; E. Fioretto; A. Gadea; F. Ibrahim; A. Jungclaus; K. Keyes; A. Latina; N. Margineau; R. Menegazzo; G. Montagnoli; D.R. Napoli; F. Nowacki; J. Ollier; A. Papenberg; G. Pollarolo; V.F.E. Pucknell; M.-D. Salsac; F. Scarlassara; J.F. Smith; K. Spohr; M. Stanoiu; A.M. Stefanini; S. Szilner; N. Toniolo; M. Trotta; D. Verney; Z. Wang; J. Wrzesinski

doi:10.1063/1.2338352

The spectroscopy of neutron-rich sdf-shell nuclei using the CLARA-PRISMA setup

X. Liang, A. Hodsdon, F. Azaiez, R. Chapman, F. Haas, D. Bazzacco, S. Beghini, B.R. Behera, L. Berti, M. Burns, E. Caurier, L. Corradi, D. Curien, A. Deacon, G. de Angelis, Zs. Dombradi, E. Farnea, E. Fioretto, A. Gadea, F. IbrahimA. Jungclaus, K. Keyes, A. Latina, N. Margineau, R. Menegazzo, G. Montagnoli, D.R. Napoli, F. Nowacki, J. Ollier, A. Papenberg, G. Pollarolo, V.F.E. Pucknell, M.-D. Salsac, F. Scarlassara, J.F. Smith, K. Spohr, M. Stanoiu, A.M. Stefanini, S. Szilner, N. Toniolo, M. Trotta, D. Verney, Z. Wang, J. Wrzesinski

Research output: Contribution to journal › Article › peer-review

Abstract

Since the discovery of the breakdown of shell effects in very neutron‐rich N=20 and 28 nuclei, studies of the properties of nuclei far from stability have been of intense interest since they provide a unique opportunity to increase our understanding of nuclear interactions in extreme conditions and often challenge our theoretical models.

Deep‐inelastic processes can be used to populated high spin states of neutron‐rich nuclei. In the deep‐inelastic processes, an equilibration in N/Z between the target and projectile nuclei is achieved. For most heavy neutron‐rich target nuclei, the N/Z ratio is 1.5 – 1.6, while for the possible neutron‐rich sdf‐shell projectile it is about 1.2. Thus by using deep‐inelastic processes one can populate neutron‐rich nuclei around N=20 and N=28.

New results for the spectroscopy of neutron‐rich N=22 36Si and 37P are presented here.

Original language	English
Pages (from-to)	37-42
Number of pages	6
Journal	AIP Conference Proceedings
Volume	853
Issue number	37
DOIs	https://doi.org/10.1063/1.2338352
Publication status	Published - Aug 2006

Keywords

neutron spectroscopy
shell model
properties of nuclei
nuclear interactions

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10.1063/1.2338352

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Liang, X., Hodsdon, A., Azaiez, F., Chapman, R., Haas, F., Bazzacco, D., Beghini, S., Behera, B. R., Berti, L., Burns, M., Caurier, E., Corradi, L., Curien, D., Deacon, A., de Angelis, G., Dombradi, Z., Farnea, E., Fioretto, E., Gadea, A., ... Wrzesinski, J. (2006). The spectroscopy of neutron-rich sdf-shell nuclei using the CLARA-PRISMA setup. AIP Conference Proceedings, 853(37), 37-42. https://doi.org/10.1063/1.2338352

@article{f64149d807204426bb0970bc68291ffb,

title = "The spectroscopy of neutron-rich sdf-shell nuclei using the CLARA-PRISMA setup",

abstract = "Since the discovery of the breakdown of shell effects in very neutron‐rich N=20 and 28 nuclei, studies of the properties of nuclei far from stability have been of intense interest since they provide a unique opportunity to increase our understanding of nuclear interactions in extreme conditions and often challenge our theoretical models.Deep‐inelastic processes can be used to populated high spin states of neutron‐rich nuclei. In the deep‐inelastic processes, an equilibration in N/Z between the target and projectile nuclei is achieved. For most heavy neutron‐rich target nuclei, the N/Z ratio is 1.5 – 1.6, while for the possible neutron‐rich sdf‐shell projectile it is about 1.2. Thus by using deep‐inelastic processes one can populate neutron‐rich nuclei around N=20 and N=28.New results for the spectroscopy of neutron‐rich N=22 36Si and 37P are presented here.",

keywords = "neutron spectroscopy, shell model, properties of nuclei, nuclear interactions",

author = "X. Liang and A. Hodsdon and F. Azaiez and R. Chapman and F. Haas and D. Bazzacco and S. Beghini and B.R. Behera and L. Berti and M. Burns and E. Caurier and L. Corradi and D. Curien and A. Deacon and {de Angelis}, G. and Zs. Dombradi and E. Farnea and E. Fioretto and A. Gadea and F. Ibrahim and A. Jungclaus and K. Keyes and A. Latina and N. Margineau and R. Menegazzo and G. Montagnoli and D.R. Napoli and F. Nowacki and J. Ollier and A. Papenberg and G. Pollarolo and V.F.E. Pucknell and M.-D. Salsac and F. Scarlassara and J.F. Smith and K. Spohr and M. Stanoiu and A.M. Stefanini and S. Szilner and N. Toniolo and M. Trotta and D. Verney and Z. Wang and J. Wrzesinski",

year = "2006",

month = aug,

doi = "10.1063/1.2338352",

language = "English",

volume = "853",

pages = "37--42",

journal = "AIP Conference Proceedings",

issn = "0094-243X",

publisher = "American Institute of Physics",

number = "37",

}

Liang, X, Hodsdon, A, Azaiez, F, Chapman, R, Haas, F, Bazzacco, D, Beghini, S, Behera, BR, Berti, L, Burns, M, Caurier, E, Corradi, L, Curien, D, Deacon, A, de Angelis, G, Dombradi, Z, Farnea, E, Fioretto, E, Gadea, A, Ibrahim, F, Jungclaus, A, Keyes, K, Latina, A, Margineau, N, Menegazzo, R, Montagnoli, G, Napoli, DR, Nowacki, F, Ollier, J, Papenberg, A, Pollarolo, G, Pucknell, VFE, Salsac, M-D, Scarlassara, F, Smith, JF, Spohr, K, Stanoiu, M, Stefanini, AM, Szilner, S, Toniolo, N, Trotta, M, Verney, D, Wang, Z & Wrzesinski, J 2006, 'The spectroscopy of neutron-rich sdf-shell nuclei using the CLARA-PRISMA setup', AIP Conference Proceedings, vol. 853, no. 37, pp. 37-42. https://doi.org/10.1063/1.2338352

TY - JOUR

T1 - The spectroscopy of neutron-rich sdf-shell nuclei using the CLARA-PRISMA setup

AU - Liang, X.

AU - Hodsdon, A.

AU - Azaiez, F.

AU - Chapman, R.

AU - Haas, F.

AU - Bazzacco, D.

AU - Beghini, S.

AU - Behera, B.R.

AU - Berti, L.

AU - Burns, M.

AU - Caurier, E.

AU - Corradi, L.

AU - Curien, D.

AU - Deacon, A.

AU - de Angelis, G.

AU - Dombradi, Zs.

AU - Farnea, E.

AU - Fioretto, E.

AU - Gadea, A.

AU - Ibrahim, F.

AU - Jungclaus, A.

AU - Keyes, K.

AU - Latina, A.

AU - Margineau, N.

AU - Menegazzo, R.

AU - Montagnoli, G.

AU - Napoli, D.R.

AU - Nowacki, F.

AU - Ollier, J.

AU - Papenberg, A.

AU - Pollarolo, G.

AU - Pucknell, V.F.E.

AU - Salsac, M.-D.

AU - Scarlassara, F.

AU - Smith, J.F.

AU - Spohr, K.

AU - Stanoiu, M.

AU - Stefanini, A.M.

AU - Szilner, S.

AU - Toniolo, N.

AU - Trotta, M.

AU - Verney, D.

AU - Wang, Z.

AU - Wrzesinski, J.

PY - 2006/8

Y1 - 2006/8

N2 - Since the discovery of the breakdown of shell effects in very neutron‐rich N=20 and 28 nuclei, studies of the properties of nuclei far from stability have been of intense interest since they provide a unique opportunity to increase our understanding of nuclear interactions in extreme conditions and often challenge our theoretical models.Deep‐inelastic processes can be used to populated high spin states of neutron‐rich nuclei. In the deep‐inelastic processes, an equilibration in N/Z between the target and projectile nuclei is achieved. For most heavy neutron‐rich target nuclei, the N/Z ratio is 1.5 – 1.6, while for the possible neutron‐rich sdf‐shell projectile it is about 1.2. Thus by using deep‐inelastic processes one can populate neutron‐rich nuclei around N=20 and N=28.New results for the spectroscopy of neutron‐rich N=22 36Si and 37P are presented here.

AB - Since the discovery of the breakdown of shell effects in very neutron‐rich N=20 and 28 nuclei, studies of the properties of nuclei far from stability have been of intense interest since they provide a unique opportunity to increase our understanding of nuclear interactions in extreme conditions and often challenge our theoretical models.Deep‐inelastic processes can be used to populated high spin states of neutron‐rich nuclei. In the deep‐inelastic processes, an equilibration in N/Z between the target and projectile nuclei is achieved. For most heavy neutron‐rich target nuclei, the N/Z ratio is 1.5 – 1.6, while for the possible neutron‐rich sdf‐shell projectile it is about 1.2. Thus by using deep‐inelastic processes one can populate neutron‐rich nuclei around N=20 and N=28.New results for the spectroscopy of neutron‐rich N=22 36Si and 37P are presented here.

KW - neutron spectroscopy

KW - shell model

KW - properties of nuclei

KW - nuclear interactions

U2 - 10.1063/1.2338352

DO - 10.1063/1.2338352

M3 - Article

SN - 0094-243X

VL - 853

SP - 37

EP - 42

JO - AIP Conference Proceedings

JF - AIP Conference Proceedings

IS - 37

ER -

The spectroscopy of neutron-rich sdf-shell nuclei using the CLARA-PRISMA setup

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Keywords

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