Voyage to the “Island of Inversion”: 29Na
Abstract. The low energy level structure of neutron-rich 28, 29Na has been investigated through β-delayed γ spectroscopy. The present work, which presents the first detailed spectroscopy of 29Na, clearly demonstrates that for Na isotopes between 28Na (N = 17) and 29Na (N = 18), intruder configuratio...
Ausführliche Beschreibung
Autor*in: |
Tripathi, V. [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
2005 |
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Anmerkung: |
© Società Italiana di Fisica and Springer-Verlag 2005 |
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Übergeordnetes Werk: |
Enthalten in: The European physical journal / A - Società Italiana di Fisica, 1998, 25(2005), Suppl 1 vom: 29. Juni, Seite 101-103 |
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Übergeordnetes Werk: |
volume:25 ; year:2005 ; number:Suppl 1 ; day:29 ; month:06 ; pages:101-103 |
Links: |
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DOI / URN: |
10.1140/epjad/i2005-06-124-y |
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Katalog-ID: |
OLC2051742561 |
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10.1140/epjad/i2005-06-124-y doi (DE-627)OLC2051742561 (DE-He213)i2005-06-124-y-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Tripathi, V. verfasserin aut Voyage to the “Island of Inversion”: 29Na 2005 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica and Springer-Verlag 2005 Abstract. The low energy level structure of neutron-rich 28, 29Na has been investigated through β-delayed γ spectroscopy. The present work, which presents the first detailed spectroscopy of 29Na, clearly demonstrates that for Na isotopes between 28Na (N = 17) and 29Na (N = 18), intruder configurations start dominating the low lying excited states, suggestive of the small N = 20 shell gap. Tabor, S. L. aut Mantica, P. F. aut Hoffman, C. R. aut Wiedeking, M. aut Davies, A. D. aut Liddick, S. N. aut Mueller, W. F. aut Stolz, A. aut Tomlin, B. E. aut Volya, A. aut Enthalten in The European physical journal / A Società Italiana di Fisica, 1998 25(2005), Suppl 1 vom: 29. Juni, Seite 101-103 (DE-627)239430387 (DE-600)1413603-X (DE-576)064448398 1434-6001 nnns volume:25 year:2005 number:Suppl 1 day:29 month:06 pages:101-103 https://doi.org/10.1140/epjad/i2005-06-124-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_30 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_105 GBV_ILN_267 GBV_ILN_2002 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4116 GBV_ILN_4277 GBV_ILN_4307 AR 25 2005 Suppl 1 29 06 101-103 |
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10.1140/epjad/i2005-06-124-y doi (DE-627)OLC2051742561 (DE-He213)i2005-06-124-y-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Tripathi, V. verfasserin aut Voyage to the “Island of Inversion”: 29Na 2005 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica and Springer-Verlag 2005 Abstract. The low energy level structure of neutron-rich 28, 29Na has been investigated through β-delayed γ spectroscopy. The present work, which presents the first detailed spectroscopy of 29Na, clearly demonstrates that for Na isotopes between 28Na (N = 17) and 29Na (N = 18), intruder configurations start dominating the low lying excited states, suggestive of the small N = 20 shell gap. Tabor, S. L. aut Mantica, P. F. aut Hoffman, C. R. aut Wiedeking, M. aut Davies, A. D. aut Liddick, S. N. aut Mueller, W. F. aut Stolz, A. aut Tomlin, B. E. aut Volya, A. aut Enthalten in The European physical journal / A Società Italiana di Fisica, 1998 25(2005), Suppl 1 vom: 29. Juni, Seite 101-103 (DE-627)239430387 (DE-600)1413603-X (DE-576)064448398 1434-6001 nnns volume:25 year:2005 number:Suppl 1 day:29 month:06 pages:101-103 https://doi.org/10.1140/epjad/i2005-06-124-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_30 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_105 GBV_ILN_267 GBV_ILN_2002 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4116 GBV_ILN_4277 GBV_ILN_4307 AR 25 2005 Suppl 1 29 06 101-103 |
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10.1140/epjad/i2005-06-124-y doi (DE-627)OLC2051742561 (DE-He213)i2005-06-124-y-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Tripathi, V. verfasserin aut Voyage to the “Island of Inversion”: 29Na 2005 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica and Springer-Verlag 2005 Abstract. The low energy level structure of neutron-rich 28, 29Na has been investigated through β-delayed γ spectroscopy. The present work, which presents the first detailed spectroscopy of 29Na, clearly demonstrates that for Na isotopes between 28Na (N = 17) and 29Na (N = 18), intruder configurations start dominating the low lying excited states, suggestive of the small N = 20 shell gap. Tabor, S. L. aut Mantica, P. F. aut Hoffman, C. R. aut Wiedeking, M. aut Davies, A. D. aut Liddick, S. N. aut Mueller, W. F. aut Stolz, A. aut Tomlin, B. E. aut Volya, A. aut Enthalten in The European physical journal / A Società Italiana di Fisica, 1998 25(2005), Suppl 1 vom: 29. Juni, Seite 101-103 (DE-627)239430387 (DE-600)1413603-X (DE-576)064448398 1434-6001 nnns volume:25 year:2005 number:Suppl 1 day:29 month:06 pages:101-103 https://doi.org/10.1140/epjad/i2005-06-124-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_30 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_105 GBV_ILN_267 GBV_ILN_2002 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4116 GBV_ILN_4277 GBV_ILN_4307 AR 25 2005 Suppl 1 29 06 101-103 |
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10.1140/epjad/i2005-06-124-y doi (DE-627)OLC2051742561 (DE-He213)i2005-06-124-y-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Tripathi, V. verfasserin aut Voyage to the “Island of Inversion”: 29Na 2005 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica and Springer-Verlag 2005 Abstract. The low energy level structure of neutron-rich 28, 29Na has been investigated through β-delayed γ spectroscopy. The present work, which presents the first detailed spectroscopy of 29Na, clearly demonstrates that for Na isotopes between 28Na (N = 17) and 29Na (N = 18), intruder configurations start dominating the low lying excited states, suggestive of the small N = 20 shell gap. Tabor, S. L. aut Mantica, P. F. aut Hoffman, C. R. aut Wiedeking, M. aut Davies, A. D. aut Liddick, S. N. aut Mueller, W. F. aut Stolz, A. aut Tomlin, B. E. aut Volya, A. aut Enthalten in The European physical journal / A Società Italiana di Fisica, 1998 25(2005), Suppl 1 vom: 29. Juni, Seite 101-103 (DE-627)239430387 (DE-600)1413603-X (DE-576)064448398 1434-6001 nnns volume:25 year:2005 number:Suppl 1 day:29 month:06 pages:101-103 https://doi.org/10.1140/epjad/i2005-06-124-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_30 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_105 GBV_ILN_267 GBV_ILN_2002 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4116 GBV_ILN_4277 GBV_ILN_4307 AR 25 2005 Suppl 1 29 06 101-103 |
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10.1140/epjad/i2005-06-124-y doi (DE-627)OLC2051742561 (DE-He213)i2005-06-124-y-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Tripathi, V. verfasserin aut Voyage to the “Island of Inversion”: 29Na 2005 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica and Springer-Verlag 2005 Abstract. The low energy level structure of neutron-rich 28, 29Na has been investigated through β-delayed γ spectroscopy. The present work, which presents the first detailed spectroscopy of 29Na, clearly demonstrates that for Na isotopes between 28Na (N = 17) and 29Na (N = 18), intruder configurations start dominating the low lying excited states, suggestive of the small N = 20 shell gap. Tabor, S. L. aut Mantica, P. F. aut Hoffman, C. R. aut Wiedeking, M. aut Davies, A. D. aut Liddick, S. N. aut Mueller, W. F. aut Stolz, A. aut Tomlin, B. E. aut Volya, A. aut Enthalten in The European physical journal / A Società Italiana di Fisica, 1998 25(2005), Suppl 1 vom: 29. Juni, Seite 101-103 (DE-627)239430387 (DE-600)1413603-X (DE-576)064448398 1434-6001 nnns volume:25 year:2005 number:Suppl 1 day:29 month:06 pages:101-103 https://doi.org/10.1140/epjad/i2005-06-124-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_30 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_105 GBV_ILN_267 GBV_ILN_2002 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4116 GBV_ILN_4277 GBV_ILN_4307 AR 25 2005 Suppl 1 29 06 101-103 |
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Tripathi, V. Tabor, S. L. Mantica, P. F. Hoffman, C. R. Wiedeking, M. Davies, A. D. Liddick, S. N. Mueller, W. F. Stolz, A. Tomlin, B. E. Volya, A. |
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Tripathi, V. |
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10.1140/epjad/i2005-06-124-y |
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530 |
title_sort |
voyage to the “island of inversion”: 29na |
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Voyage to the “Island of Inversion”: 29Na |
abstract |
Abstract. The low energy level structure of neutron-rich 28, 29Na has been investigated through β-delayed γ spectroscopy. The present work, which presents the first detailed spectroscopy of 29Na, clearly demonstrates that for Na isotopes between 28Na (N = 17) and 29Na (N = 18), intruder configurations start dominating the low lying excited states, suggestive of the small N = 20 shell gap. © Società Italiana di Fisica and Springer-Verlag 2005 |
abstractGer |
Abstract. The low energy level structure of neutron-rich 28, 29Na has been investigated through β-delayed γ spectroscopy. The present work, which presents the first detailed spectroscopy of 29Na, clearly demonstrates that for Na isotopes between 28Na (N = 17) and 29Na (N = 18), intruder configurations start dominating the low lying excited states, suggestive of the small N = 20 shell gap. © Società Italiana di Fisica and Springer-Verlag 2005 |
abstract_unstemmed |
Abstract. The low energy level structure of neutron-rich 28, 29Na has been investigated through β-delayed γ spectroscopy. The present work, which presents the first detailed spectroscopy of 29Na, clearly demonstrates that for Na isotopes between 28Na (N = 17) and 29Na (N = 18), intruder configurations start dominating the low lying excited states, suggestive of the small N = 20 shell gap. © Società Italiana di Fisica and Springer-Verlag 2005 |
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Voyage to the “Island of Inversion”: 29Na |
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