Evolution of the Ar isotopic chain: the N=28 shell gap south of 48Ca

D. Mengoni, J. J. Valiente-Dobón, A. Gadea, S. M. Lenzi, S. Lunardi, R. Broda, A. Dewald, T. Pissulla, L. Angus, S. Aydin, D. Bazzacco, G. Benzoni, P. G. Bizzeti, A. M. Bizzeti-Sona, L. Corradi, F. Crespi, G. de Angelis, E. Farnea, E. Fioretto, A. GoergenA. Gottardo, E. Grodner, W. Królas, S. Leoni, P. Mason, D. Montanari, G. Montagnoli, D. R. Napoli, A. Obertelli, T. Pawłat, G. Pollarolo, F. Recchia, A. Algora, B. Rubio, E. Sahin, F. Scarlassara, J. F. Smith, A. M. Stefanini, S. Szilner, C. A. Ur, P. T. Wady, J. Wrzesiński

Research output: Contribution to journalArticle

3 Citations (Scopus)

Abstract

The lifetimes of the first excited states of the Z = 18 44Ar and 46Ar isotopes have been determined using a novel technique that combines the Recoil Distance Doppler Shift method with the CLARA-PRISMA spectrometers for Multinucleon Transfer Reactions. The B(E2) values extracted for the 2+ → 0+ transitions in both nuclei, as well as for higher excites states in 44Ar, are discussed and compared with the available experimental results and with the new large-scale shell-model calculations.

Original languageEnglish
JournalNuclear Physics A
Volume834
Issue number1-4
DOIs
Publication statusPublished - Mar 1 2010

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isotopes
spectrometers
life (durability)
nuclei
shift
excitation

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

Cite this

Mengoni, D., Valiente-Dobón, J. J., Gadea, A., Lenzi, S. M., Lunardi, S., Broda, R., ... Wrzesiński, J. (2010). Evolution of the Ar isotopic chain: the N=28 shell gap south of 48Ca. Nuclear Physics A, 834(1-4). https://doi.org/10.1016/j.nuclphysa.2010.01.020

Evolution of the Ar isotopic chain : the N=28 shell gap south of 48Ca. / Mengoni, D.; Valiente-Dobón, J. J.; Gadea, A.; Lenzi, S. M.; Lunardi, S.; Broda, R.; Dewald, A.; Pissulla, T.; Angus, L.; Aydin, S.; Bazzacco, D.; Benzoni, G.; Bizzeti, P. G.; Bizzeti-Sona, A. M.; Corradi, L.; Crespi, F.; de Angelis, G.; Farnea, E.; Fioretto, E.; Goergen, A.; Gottardo, A.; Grodner, E.; Królas, W.; Leoni, S.; Mason, P.; Montanari, D.; Montagnoli, G.; Napoli, D. R.; Obertelli, A.; Pawłat, T.; Pollarolo, G.; Recchia, F.; Algora, A.; Rubio, B.; Sahin, E.; Scarlassara, F.; Smith, J. F.; Stefanini, A. M.; Szilner, S.; Ur, C. A.; Wady, P. T.; Wrzesiński, J.

In: Nuclear Physics A, Vol. 834, No. 1-4, 01.03.2010.

Research output: Contribution to journalArticle

Mengoni, D, Valiente-Dobón, JJ, Gadea, A, Lenzi, SM, Lunardi, S, Broda, R, Dewald, A, Pissulla, T, Angus, L, Aydin, S, Bazzacco, D, Benzoni, G, Bizzeti, PG, Bizzeti-Sona, AM, Corradi, L, Crespi, F, de Angelis, G, Farnea, E, Fioretto, E, Goergen, A, Gottardo, A, Grodner, E, Królas, W, Leoni, S, Mason, P, Montanari, D, Montagnoli, G, Napoli, DR, Obertelli, A, Pawłat, T, Pollarolo, G, Recchia, F, Algora, A, Rubio, B, Sahin, E, Scarlassara, F, Smith, JF, Stefanini, AM, Szilner, S, Ur, CA, Wady, PT & Wrzesiński, J 2010, 'Evolution of the Ar isotopic chain: the N=28 shell gap south of 48Ca', Nuclear Physics A, vol. 834, no. 1-4. https://doi.org/10.1016/j.nuclphysa.2010.01.020
Mengoni D, Valiente-Dobón JJ, Gadea A, Lenzi SM, Lunardi S, Broda R et al. Evolution of the Ar isotopic chain: the N=28 shell gap south of 48Ca. Nuclear Physics A. 2010 Mar 1;834(1-4). https://doi.org/10.1016/j.nuclphysa.2010.01.020
Mengoni, D. ; Valiente-Dobón, J. J. ; Gadea, A. ; Lenzi, S. M. ; Lunardi, S. ; Broda, R. ; Dewald, A. ; Pissulla, T. ; Angus, L. ; Aydin, S. ; Bazzacco, D. ; Benzoni, G. ; Bizzeti, P. G. ; Bizzeti-Sona, A. M. ; Corradi, L. ; Crespi, F. ; de Angelis, G. ; Farnea, E. ; Fioretto, E. ; Goergen, A. ; Gottardo, A. ; Grodner, E. ; Królas, W. ; Leoni, S. ; Mason, P. ; Montanari, D. ; Montagnoli, G. ; Napoli, D. R. ; Obertelli, A. ; Pawłat, T. ; Pollarolo, G. ; Recchia, F. ; Algora, A. ; Rubio, B. ; Sahin, E. ; Scarlassara, F. ; Smith, J. F. ; Stefanini, A. M. ; Szilner, S. ; Ur, C. A. ; Wady, P. T. ; Wrzesiński, J. / Evolution of the Ar isotopic chain : the N=28 shell gap south of 48Ca. In: Nuclear Physics A. 2010 ; Vol. 834, No. 1-4.
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