Probing the Z = 6 spin-orbit shell gap with (p,2p) quasi-free scattering reactions
The evolution of the traditional nuclear magic numbers away from the valley of stability is an active field of research. Experimental efforts focus on providing key spectroscopic information that will shed light into the structure of exotic nuclei and understanding the driving mechanism behind the s...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
I. Syndikus [verfasserIn] M. Petri [verfasserIn] A.O. Macchiavelli [verfasserIn] S. Paschalis [verfasserIn] C.A. Bertulani [verfasserIn] T. Aumann [verfasserIn] H. Alvarez-Pol [verfasserIn] L. Atar [verfasserIn] S. Beceiro-Novo [verfasserIn] J. Benlliure [verfasserIn] J.M. Boillos [verfasserIn] K. Boretzky [verfasserIn] M.J.G. Borge [verfasserIn] B.A. Brown [verfasserIn] M. Caamaño [verfasserIn] C. Caesar [verfasserIn] E. Casarejos [verfasserIn] W. Catford [verfasserIn] J. Cederkall [verfasserIn] S. Chakraborty [verfasserIn] L.V. Chulkov [verfasserIn] D. Cortina-Gil [verfasserIn] E. Cravo [verfasserIn] R. Crespo [verfasserIn] U. Datta Pramanik [verfasserIn] I. Dillmann [verfasserIn] P. Díaz Fernández [verfasserIn] Z. Elekes [verfasserIn] J. Enders [verfasserIn] F. Farinon [verfasserIn] L.M. Fraile [verfasserIn] D. Galaviz [verfasserIn] H. Geissel [verfasserIn] R. Gernhäuser [verfasserIn] P. Golubev [verfasserIn] K. Göbel [verfasserIn] M. Heil [verfasserIn] M. Heine [verfasserIn] A. Heinz [verfasserIn] A. Henriques [verfasserIn] M. Holl [verfasserIn] H.T. Johansson [verfasserIn] B. Jonson [verfasserIn] N. Kalantar-Nayestanaki [verfasserIn] R. Kanungo [verfasserIn] A. Kelic-Heil [verfasserIn] T. Kröll [verfasserIn] N. Kurz [verfasserIn] C. Langer [verfasserIn] T. Le Bleis [verfasserIn] J. Machado [verfasserIn] J. Marganiec-Gałązka [verfasserIn] E. Nacher [verfasserIn] T. Nilsson [verfasserIn] C. Nociforo [verfasserIn] V. Panin [verfasserIn] A. Perea [verfasserIn] S.B. Pietri [verfasserIn] R. Plag [verfasserIn] A. Rahaman [verfasserIn] R. Reifarth [verfasserIn] A. Revel [verfasserIn] G. Ribeiro [verfasserIn] C. Rigollet [verfasserIn] D.M. Rossi [verfasserIn] D. Savran [verfasserIn] H. Scheit [verfasserIn] H. Simon [verfasserIn] O. Sorlin [verfasserIn] O. Tengblad [verfasserIn] Y. Togano [verfasserIn] M. Vandebrouck [verfasserIn] V. Volkov [verfasserIn] F. Wamers [verfasserIn] C. Wheldon [verfasserIn] G.L. Wilson [verfasserIn] J.S. Winfield [verfasserIn] H. Weick [verfasserIn] P. Woods [verfasserIn] D. Yakorev [verfasserIn] M. Zhukov [verfasserIn] A. Zilges [verfasserIn] K. Zuber [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2020 |
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| Übergeordnetes Werk: |
In: Physics Letters B - Elsevier, 2015, 809(2020), Seite 135748- |
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| Übergeordnetes Werk: |
volume:809 ; year:2020 ; pages:135748- |
| Links: |
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| DOI / URN: |
10.1016/j.physletb.2020.135748 |
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DOAJ032157827 |
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| 100 | 0 | |a I. Syndikus |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Probing the Z = 6 spin-orbit shell gap with (p,2p) quasi-free scattering reactions |
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| 520 | |a The evolution of the traditional nuclear magic numbers away from the valley of stability is an active field of research. Experimental efforts focus on providing key spectroscopic information that will shed light into the structure of exotic nuclei and understanding the driving mechanism behind the shell evolution. In this work, we investigate the Z=6 spin-orbit shell gap towards the neutron dripline. To do so, we employed NA(p,2p)CA−1 quasi-free scattering reactions to measure the proton component of the 21+ state of 16,18,20C. The experimental findings support the notion of a moderate reduction of the proton 1p1/2−1p3/2 spin-orbit splitting, at variance to recent claims for a prevalent Z=6 magic number towards the neutron dripline. | ||
| 650 | 4 | |a Quasi-free scattering reactions | |
| 650 | 4 | |a Magic numbers | |
| 650 | 4 | |a Spin-orbit splitting | |
| 650 | 4 | |a Tensor force | |
| 650 | 4 | |a Shell evolution | |
| 650 | 4 | |a Exotic nuclei | |
| 653 | 0 | |a Physics | |
| 700 | 0 | |a M. Petri |e verfasserin |4 aut | |
| 700 | 0 | |a A.O. Macchiavelli |e verfasserin |4 aut | |
| 700 | 0 | |a S. Paschalis |e verfasserin |4 aut | |
| 700 | 0 | |a C.A. Bertulani |e verfasserin |4 aut | |
| 700 | 0 | |a T. Aumann |e verfasserin |4 aut | |
| 700 | 0 | |a H. Alvarez-Pol |e verfasserin |4 aut | |
| 700 | 0 | |a L. Atar |e verfasserin |4 aut | |
| 700 | 0 | |a S. Beceiro-Novo |e verfasserin |4 aut | |
| 700 | 0 | |a J. Benlliure |e verfasserin |4 aut | |
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| 700 | 0 | |a E. Cravo |e verfasserin |4 aut | |
| 700 | 0 | |a R. Crespo |e verfasserin |4 aut | |
| 700 | 0 | |a U. Datta Pramanik |e verfasserin |4 aut | |
| 700 | 0 | |a I. Dillmann |e verfasserin |4 aut | |
| 700 | 0 | |a P. Díaz Fernández |e verfasserin |4 aut | |
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| 700 | 0 | |a M. Heine |e verfasserin |4 aut | |
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10.1016/j.physletb.2020.135748 doi (DE-627)DOAJ032157827 (DE-599)DOAJdd22e2ae0d6d43a99113913dec8be2ff DE-627 ger DE-627 rakwb eng QC1-999 I. Syndikus verfasserin aut Probing the Z = 6 spin-orbit shell gap with (p,2p) quasi-free scattering reactions 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The evolution of the traditional nuclear magic numbers away from the valley of stability is an active field of research. Experimental efforts focus on providing key spectroscopic information that will shed light into the structure of exotic nuclei and understanding the driving mechanism behind the shell evolution. In this work, we investigate the Z=6 spin-orbit shell gap towards the neutron dripline. To do so, we employed NA(p,2p)CA−1 quasi-free scattering reactions to measure the proton component of the 21+ state of 16,18,20C. The experimental findings support the notion of a moderate reduction of the proton 1p1/2−1p3/2 spin-orbit splitting, at variance to recent claims for a prevalent Z=6 magic number towards the neutron dripline. Quasi-free scattering reactions Magic numbers Spin-orbit splitting Tensor force Shell evolution Exotic nuclei Physics M. Petri verfasserin aut A.O. Macchiavelli verfasserin aut S. Paschalis verfasserin aut C.A. Bertulani verfasserin aut T. Aumann verfasserin aut H. Alvarez-Pol verfasserin aut L. Atar verfasserin aut S. Beceiro-Novo verfasserin aut J. Benlliure verfasserin aut J.M. Boillos verfasserin aut K. Boretzky verfasserin aut M.J.G. Borge verfasserin aut B.A. Brown verfasserin aut M. Caamaño verfasserin aut C. Caesar verfasserin aut E. Casarejos verfasserin aut W. Catford verfasserin aut J. Cederkall verfasserin aut S. Chakraborty verfasserin aut L.V. Chulkov verfasserin aut D. Cortina-Gil verfasserin aut E. Cravo verfasserin aut R. Crespo verfasserin aut U. Datta Pramanik verfasserin aut I. Dillmann verfasserin aut P. Díaz Fernández verfasserin aut Z. Elekes verfasserin aut J. Enders verfasserin aut F. Farinon verfasserin aut L.M. Fraile verfasserin aut D. Galaviz verfasserin aut H. Geissel verfasserin aut R. Gernhäuser verfasserin aut P. Golubev verfasserin aut K. Göbel verfasserin aut M. Heil verfasserin aut M. Heine verfasserin aut A. Heinz verfasserin aut A. Henriques verfasserin aut M. Holl verfasserin aut H.T. Johansson verfasserin aut B. Jonson verfasserin aut N. Kalantar-Nayestanaki verfasserin aut R. Kanungo verfasserin aut A. Kelic-Heil verfasserin aut T. Kröll verfasserin aut N. Kurz verfasserin aut C. Langer verfasserin aut T. Le Bleis verfasserin aut J. Machado verfasserin aut J. Marganiec-Gałązka verfasserin aut E. Nacher verfasserin aut T. Nilsson verfasserin aut C. Nociforo verfasserin aut V. Panin verfasserin aut A. Perea verfasserin aut S.B. Pietri verfasserin aut R. Plag verfasserin aut A. Rahaman verfasserin aut R. Reifarth verfasserin aut A. Revel verfasserin aut G. Ribeiro verfasserin aut C. Rigollet verfasserin aut D.M. Rossi verfasserin aut D. Savran verfasserin aut H. Scheit verfasserin aut H. Simon verfasserin aut O. Sorlin verfasserin aut O. Tengblad verfasserin aut Y. Togano verfasserin aut M. Vandebrouck verfasserin aut V. Volkov verfasserin aut F. Wamers verfasserin aut C. Wheldon verfasserin aut G.L. Wilson verfasserin aut J.S. Winfield verfasserin aut H. Weick verfasserin aut P. Woods verfasserin aut D. Yakorev verfasserin aut M. Zhukov verfasserin aut A. Zilges verfasserin aut K. Zuber verfasserin aut In Physics Letters B Elsevier, 2015 809(2020), Seite 135748- (DE-627)266015360 (DE-600)1466612-1 18732445 nnns volume:809 year:2020 pages:135748- https://doi.org/10.1016/j.physletb.2020.135748 kostenfrei https://doaj.org/article/dd22e2ae0d6d43a99113913dec8be2ff kostenfrei http://www.sciencedirect.com/science/article/pii/S0370269320305517 kostenfrei https://doaj.org/toc/0370-2693 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 809 2020 135748- |
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10.1016/j.physletb.2020.135748 doi (DE-627)DOAJ032157827 (DE-599)DOAJdd22e2ae0d6d43a99113913dec8be2ff DE-627 ger DE-627 rakwb eng QC1-999 I. Syndikus verfasserin aut Probing the Z = 6 spin-orbit shell gap with (p,2p) quasi-free scattering reactions 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The evolution of the traditional nuclear magic numbers away from the valley of stability is an active field of research. Experimental efforts focus on providing key spectroscopic information that will shed light into the structure of exotic nuclei and understanding the driving mechanism behind the shell evolution. In this work, we investigate the Z=6 spin-orbit shell gap towards the neutron dripline. To do so, we employed NA(p,2p)CA−1 quasi-free scattering reactions to measure the proton component of the 21+ state of 16,18,20C. The experimental findings support the notion of a moderate reduction of the proton 1p1/2−1p3/2 spin-orbit splitting, at variance to recent claims for a prevalent Z=6 magic number towards the neutron dripline. Quasi-free scattering reactions Magic numbers Spin-orbit splitting Tensor force Shell evolution Exotic nuclei Physics M. Petri verfasserin aut A.O. Macchiavelli verfasserin aut S. Paschalis verfasserin aut C.A. Bertulani verfasserin aut T. Aumann verfasserin aut H. Alvarez-Pol verfasserin aut L. Atar verfasserin aut S. Beceiro-Novo verfasserin aut J. Benlliure verfasserin aut J.M. Boillos verfasserin aut K. Boretzky verfasserin aut M.J.G. Borge verfasserin aut B.A. Brown verfasserin aut M. Caamaño verfasserin aut C. Caesar verfasserin aut E. Casarejos verfasserin aut W. Catford verfasserin aut J. Cederkall verfasserin aut S. Chakraborty verfasserin aut L.V. Chulkov verfasserin aut D. Cortina-Gil verfasserin aut E. Cravo verfasserin aut R. Crespo verfasserin aut U. Datta Pramanik verfasserin aut I. Dillmann verfasserin aut P. Díaz Fernández verfasserin aut Z. Elekes verfasserin aut J. Enders verfasserin aut F. Farinon verfasserin aut L.M. Fraile verfasserin aut D. Galaviz verfasserin aut H. Geissel verfasserin aut R. Gernhäuser verfasserin aut P. Golubev verfasserin aut K. Göbel verfasserin aut M. Heil verfasserin aut M. Heine verfasserin aut A. Heinz verfasserin aut A. Henriques verfasserin aut M. Holl verfasserin aut H.T. Johansson verfasserin aut B. Jonson verfasserin aut N. Kalantar-Nayestanaki verfasserin aut R. Kanungo verfasserin aut A. Kelic-Heil verfasserin aut T. Kröll verfasserin aut N. Kurz verfasserin aut C. Langer verfasserin aut T. Le Bleis verfasserin aut J. Machado verfasserin aut J. Marganiec-Gałązka verfasserin aut E. Nacher verfasserin aut T. Nilsson verfasserin aut C. Nociforo verfasserin aut V. Panin verfasserin aut A. Perea verfasserin aut S.B. Pietri verfasserin aut R. Plag verfasserin aut A. Rahaman verfasserin aut R. Reifarth verfasserin aut A. Revel verfasserin aut G. Ribeiro verfasserin aut C. Rigollet verfasserin aut D.M. Rossi verfasserin aut D. Savran verfasserin aut H. Scheit verfasserin aut H. Simon verfasserin aut O. Sorlin verfasserin aut O. Tengblad verfasserin aut Y. Togano verfasserin aut M. Vandebrouck verfasserin aut V. Volkov verfasserin aut F. Wamers verfasserin aut C. Wheldon verfasserin aut G.L. Wilson verfasserin aut J.S. Winfield verfasserin aut H. Weick verfasserin aut P. Woods verfasserin aut D. Yakorev verfasserin aut M. Zhukov verfasserin aut A. Zilges verfasserin aut K. Zuber verfasserin aut In Physics Letters B Elsevier, 2015 809(2020), Seite 135748- (DE-627)266015360 (DE-600)1466612-1 18732445 nnns volume:809 year:2020 pages:135748- https://doi.org/10.1016/j.physletb.2020.135748 kostenfrei https://doaj.org/article/dd22e2ae0d6d43a99113913dec8be2ff kostenfrei http://www.sciencedirect.com/science/article/pii/S0370269320305517 kostenfrei https://doaj.org/toc/0370-2693 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 809 2020 135748- |
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10.1016/j.physletb.2020.135748 doi (DE-627)DOAJ032157827 (DE-599)DOAJdd22e2ae0d6d43a99113913dec8be2ff DE-627 ger DE-627 rakwb eng QC1-999 I. Syndikus verfasserin aut Probing the Z = 6 spin-orbit shell gap with (p,2p) quasi-free scattering reactions 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The evolution of the traditional nuclear magic numbers away from the valley of stability is an active field of research. Experimental efforts focus on providing key spectroscopic information that will shed light into the structure of exotic nuclei and understanding the driving mechanism behind the shell evolution. In this work, we investigate the Z=6 spin-orbit shell gap towards the neutron dripline. To do so, we employed NA(p,2p)CA−1 quasi-free scattering reactions to measure the proton component of the 21+ state of 16,18,20C. The experimental findings support the notion of a moderate reduction of the proton 1p1/2−1p3/2 spin-orbit splitting, at variance to recent claims for a prevalent Z=6 magic number towards the neutron dripline. Quasi-free scattering reactions Magic numbers Spin-orbit splitting Tensor force Shell evolution Exotic nuclei Physics M. Petri verfasserin aut A.O. Macchiavelli verfasserin aut S. Paschalis verfasserin aut C.A. Bertulani verfasserin aut T. Aumann verfasserin aut H. Alvarez-Pol verfasserin aut L. Atar verfasserin aut S. Beceiro-Novo verfasserin aut J. Benlliure verfasserin aut J.M. Boillos verfasserin aut K. Boretzky verfasserin aut M.J.G. Borge verfasserin aut B.A. Brown verfasserin aut M. Caamaño verfasserin aut C. Caesar verfasserin aut E. Casarejos verfasserin aut W. Catford verfasserin aut J. Cederkall verfasserin aut S. Chakraborty verfasserin aut L.V. Chulkov verfasserin aut D. Cortina-Gil verfasserin aut E. Cravo verfasserin aut R. Crespo verfasserin aut U. Datta Pramanik verfasserin aut I. Dillmann verfasserin aut P. Díaz Fernández verfasserin aut Z. Elekes verfasserin aut J. Enders verfasserin aut F. Farinon verfasserin aut L.M. Fraile verfasserin aut D. Galaviz verfasserin aut H. Geissel verfasserin aut R. Gernhäuser verfasserin aut P. Golubev verfasserin aut K. Göbel verfasserin aut M. Heil verfasserin aut M. Heine verfasserin aut A. Heinz verfasserin aut A. Henriques verfasserin aut M. Holl verfasserin aut H.T. Johansson verfasserin aut B. Jonson verfasserin aut N. Kalantar-Nayestanaki verfasserin aut R. Kanungo verfasserin aut A. Kelic-Heil verfasserin aut T. Kröll verfasserin aut N. Kurz verfasserin aut C. Langer verfasserin aut T. Le Bleis verfasserin aut J. Machado verfasserin aut J. Marganiec-Gałązka verfasserin aut E. Nacher verfasserin aut T. Nilsson verfasserin aut C. Nociforo verfasserin aut V. Panin verfasserin aut A. Perea verfasserin aut S.B. Pietri verfasserin aut R. Plag verfasserin aut A. Rahaman verfasserin aut R. Reifarth verfasserin aut A. Revel verfasserin aut G. Ribeiro verfasserin aut C. Rigollet verfasserin aut D.M. Rossi verfasserin aut D. Savran verfasserin aut H. Scheit verfasserin aut H. Simon verfasserin aut O. Sorlin verfasserin aut O. Tengblad verfasserin aut Y. Togano verfasserin aut M. Vandebrouck verfasserin aut V. Volkov verfasserin aut F. Wamers verfasserin aut C. Wheldon verfasserin aut G.L. Wilson verfasserin aut J.S. Winfield verfasserin aut H. Weick verfasserin aut P. Woods verfasserin aut D. Yakorev verfasserin aut M. Zhukov verfasserin aut A. Zilges verfasserin aut K. Zuber verfasserin aut In Physics Letters B Elsevier, 2015 809(2020), Seite 135748- (DE-627)266015360 (DE-600)1466612-1 18732445 nnns volume:809 year:2020 pages:135748- https://doi.org/10.1016/j.physletb.2020.135748 kostenfrei https://doaj.org/article/dd22e2ae0d6d43a99113913dec8be2ff kostenfrei http://www.sciencedirect.com/science/article/pii/S0370269320305517 kostenfrei https://doaj.org/toc/0370-2693 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 809 2020 135748- |
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10.1016/j.physletb.2020.135748 doi (DE-627)DOAJ032157827 (DE-599)DOAJdd22e2ae0d6d43a99113913dec8be2ff DE-627 ger DE-627 rakwb eng QC1-999 I. Syndikus verfasserin aut Probing the Z = 6 spin-orbit shell gap with (p,2p) quasi-free scattering reactions 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The evolution of the traditional nuclear magic numbers away from the valley of stability is an active field of research. Experimental efforts focus on providing key spectroscopic information that will shed light into the structure of exotic nuclei and understanding the driving mechanism behind the shell evolution. In this work, we investigate the Z=6 spin-orbit shell gap towards the neutron dripline. To do so, we employed NA(p,2p)CA−1 quasi-free scattering reactions to measure the proton component of the 21+ state of 16,18,20C. The experimental findings support the notion of a moderate reduction of the proton 1p1/2−1p3/2 spin-orbit splitting, at variance to recent claims for a prevalent Z=6 magic number towards the neutron dripline. Quasi-free scattering reactions Magic numbers Spin-orbit splitting Tensor force Shell evolution Exotic nuclei Physics M. Petri verfasserin aut A.O. Macchiavelli verfasserin aut S. Paschalis verfasserin aut C.A. Bertulani verfasserin aut T. Aumann verfasserin aut H. Alvarez-Pol verfasserin aut L. Atar verfasserin aut S. Beceiro-Novo verfasserin aut J. Benlliure verfasserin aut J.M. Boillos verfasserin aut K. Boretzky verfasserin aut M.J.G. Borge verfasserin aut B.A. Brown verfasserin aut M. Caamaño verfasserin aut C. Caesar verfasserin aut E. Casarejos verfasserin aut W. Catford verfasserin aut J. Cederkall verfasserin aut S. Chakraborty verfasserin aut L.V. Chulkov verfasserin aut D. Cortina-Gil verfasserin aut E. Cravo verfasserin aut R. Crespo verfasserin aut U. Datta Pramanik verfasserin aut I. Dillmann verfasserin aut P. Díaz Fernández verfasserin aut Z. Elekes verfasserin aut J. Enders verfasserin aut F. Farinon verfasserin aut L.M. Fraile verfasserin aut D. Galaviz verfasserin aut H. Geissel verfasserin aut R. Gernhäuser verfasserin aut P. Golubev verfasserin aut K. Göbel verfasserin aut M. Heil verfasserin aut M. Heine verfasserin aut A. Heinz verfasserin aut A. Henriques verfasserin aut M. Holl verfasserin aut H.T. Johansson verfasserin aut B. Jonson verfasserin aut N. Kalantar-Nayestanaki verfasserin aut R. Kanungo verfasserin aut A. Kelic-Heil verfasserin aut T. Kröll verfasserin aut N. Kurz verfasserin aut C. Langer verfasserin aut T. Le Bleis verfasserin aut J. Machado verfasserin aut J. Marganiec-Gałązka verfasserin aut E. Nacher verfasserin aut T. Nilsson verfasserin aut C. Nociforo verfasserin aut V. Panin verfasserin aut A. Perea verfasserin aut S.B. Pietri verfasserin aut R. Plag verfasserin aut A. Rahaman verfasserin aut R. Reifarth verfasserin aut A. Revel verfasserin aut G. Ribeiro verfasserin aut C. Rigollet verfasserin aut D.M. Rossi verfasserin aut D. Savran verfasserin aut H. Scheit verfasserin aut H. Simon verfasserin aut O. Sorlin verfasserin aut O. Tengblad verfasserin aut Y. Togano verfasserin aut M. Vandebrouck verfasserin aut V. Volkov verfasserin aut F. Wamers verfasserin aut C. Wheldon verfasserin aut G.L. Wilson verfasserin aut J.S. Winfield verfasserin aut H. Weick verfasserin aut P. Woods verfasserin aut D. Yakorev verfasserin aut M. Zhukov verfasserin aut A. Zilges verfasserin aut K. Zuber verfasserin aut In Physics Letters B Elsevier, 2015 809(2020), Seite 135748- (DE-627)266015360 (DE-600)1466612-1 18732445 nnns volume:809 year:2020 pages:135748- https://doi.org/10.1016/j.physletb.2020.135748 kostenfrei https://doaj.org/article/dd22e2ae0d6d43a99113913dec8be2ff kostenfrei http://www.sciencedirect.com/science/article/pii/S0370269320305517 kostenfrei https://doaj.org/toc/0370-2693 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 809 2020 135748- |
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I. Syndikus @@aut@@ M. Petri @@aut@@ A.O. Macchiavelli @@aut@@ S. Paschalis @@aut@@ C.A. Bertulani @@aut@@ T. Aumann @@aut@@ H. Alvarez-Pol @@aut@@ L. Atar @@aut@@ S. Beceiro-Novo @@aut@@ J. Benlliure @@aut@@ J.M. Boillos @@aut@@ K. Boretzky @@aut@@ M.J.G. Borge @@aut@@ B.A. Brown @@aut@@ M. Caamaño @@aut@@ C. Caesar @@aut@@ E. Casarejos @@aut@@ W. Catford @@aut@@ J. Cederkall @@aut@@ S. Chakraborty @@aut@@ L.V. Chulkov @@aut@@ D. Cortina-Gil @@aut@@ E. Cravo @@aut@@ R. Crespo @@aut@@ U. Datta Pramanik @@aut@@ I. Dillmann @@aut@@ P. Díaz Fernández @@aut@@ Z. Elekes @@aut@@ J. Enders @@aut@@ F. Farinon @@aut@@ L.M. Fraile @@aut@@ D. Galaviz @@aut@@ H. Geissel @@aut@@ R. Gernhäuser @@aut@@ P. Golubev @@aut@@ K. Göbel @@aut@@ M. Heil @@aut@@ M. Heine @@aut@@ A. Heinz @@aut@@ A. Henriques @@aut@@ M. Holl @@aut@@ H.T. Johansson @@aut@@ B. Jonson @@aut@@ N. Kalantar-Nayestanaki @@aut@@ R. Kanungo @@aut@@ A. Kelic-Heil @@aut@@ T. Kröll @@aut@@ N. Kurz @@aut@@ C. Langer @@aut@@ T. Le Bleis @@aut@@ J. Machado @@aut@@ J. Marganiec-Gałązka @@aut@@ E. Nacher @@aut@@ T. Nilsson @@aut@@ C. Nociforo @@aut@@ V. Panin @@aut@@ A. Perea @@aut@@ S.B. Pietri @@aut@@ R. Plag @@aut@@ A. Rahaman @@aut@@ R. Reifarth @@aut@@ A. Revel @@aut@@ G. Ribeiro @@aut@@ C. Rigollet @@aut@@ D.M. Rossi @@aut@@ D. Savran @@aut@@ H. Scheit @@aut@@ H. Simon @@aut@@ O. Sorlin @@aut@@ O. Tengblad @@aut@@ Y. Togano @@aut@@ M. Vandebrouck @@aut@@ V. Volkov @@aut@@ F. Wamers @@aut@@ C. Wheldon @@aut@@ G.L. Wilson @@aut@@ J.S. Winfield @@aut@@ H. Weick @@aut@@ P. Woods @@aut@@ D. Yakorev @@aut@@ M. Zhukov @@aut@@ A. Zilges @@aut@@ K. Zuber @@aut@@ |
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I. Syndikus misc QC1-999 misc Quasi-free scattering reactions misc Magic numbers misc Spin-orbit splitting misc Tensor force misc Shell evolution misc Exotic nuclei misc Physics Probing the Z = 6 spin-orbit shell gap with (p,2p) quasi-free scattering reactions |
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QC1-999 Probing the Z = 6 spin-orbit shell gap with (p,2p) quasi-free scattering reactions Quasi-free scattering reactions Magic numbers Spin-orbit splitting Tensor force Shell evolution Exotic nuclei |
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Probing the Z = 6 spin-orbit shell gap with (p,2p) quasi-free scattering reactions |
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I. Syndikus M. Petri A.O. Macchiavelli S. Paschalis C.A. Bertulani T. Aumann H. Alvarez-Pol L. Atar S. Beceiro-Novo J. Benlliure J.M. Boillos K. Boretzky M.J.G. Borge B.A. Brown M. Caamaño C. Caesar E. Casarejos W. Catford J. Cederkall S. Chakraborty L.V. Chulkov D. Cortina-Gil E. Cravo R. Crespo U. Datta Pramanik I. Dillmann P. Díaz Fernández Z. Elekes J. Enders F. Farinon L.M. Fraile D. Galaviz H. Geissel R. Gernhäuser P. Golubev K. Göbel M. Heil M. Heine A. Heinz A. Henriques M. Holl H.T. Johansson B. Jonson N. Kalantar-Nayestanaki R. Kanungo A. Kelic-Heil T. Kröll N. Kurz C. Langer T. Le Bleis J. Machado J. Marganiec-Gałązka E. Nacher T. Nilsson C. Nociforo V. Panin A. Perea S.B. Pietri R. Plag A. Rahaman R. Reifarth A. Revel G. Ribeiro C. Rigollet D.M. Rossi D. Savran H. Scheit H. Simon O. Sorlin O. Tengblad Y. Togano M. Vandebrouck V. Volkov F. Wamers C. Wheldon G.L. Wilson J.S. Winfield H. Weick P. Woods D. Yakorev M. Zhukov A. Zilges K. Zuber |
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10.1016/j.physletb.2020.135748 |
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probing the z = 6 spin-orbit shell gap with (p,2p) quasi-free scattering reactions |
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Probing the Z = 6 spin-orbit shell gap with (p,2p) quasi-free scattering reactions |
| abstract |
The evolution of the traditional nuclear magic numbers away from the valley of stability is an active field of research. Experimental efforts focus on providing key spectroscopic information that will shed light into the structure of exotic nuclei and understanding the driving mechanism behind the shell evolution. In this work, we investigate the Z=6 spin-orbit shell gap towards the neutron dripline. To do so, we employed NA(p,2p)CA−1 quasi-free scattering reactions to measure the proton component of the 21+ state of 16,18,20C. The experimental findings support the notion of a moderate reduction of the proton 1p1/2−1p3/2 spin-orbit splitting, at variance to recent claims for a prevalent Z=6 magic number towards the neutron dripline. |
| abstractGer |
The evolution of the traditional nuclear magic numbers away from the valley of stability is an active field of research. Experimental efforts focus on providing key spectroscopic information that will shed light into the structure of exotic nuclei and understanding the driving mechanism behind the shell evolution. In this work, we investigate the Z=6 spin-orbit shell gap towards the neutron dripline. To do so, we employed NA(p,2p)CA−1 quasi-free scattering reactions to measure the proton component of the 21+ state of 16,18,20C. The experimental findings support the notion of a moderate reduction of the proton 1p1/2−1p3/2 spin-orbit splitting, at variance to recent claims for a prevalent Z=6 magic number towards the neutron dripline. |
| abstract_unstemmed |
The evolution of the traditional nuclear magic numbers away from the valley of stability is an active field of research. Experimental efforts focus on providing key spectroscopic information that will shed light into the structure of exotic nuclei and understanding the driving mechanism behind the shell evolution. In this work, we investigate the Z=6 spin-orbit shell gap towards the neutron dripline. To do so, we employed NA(p,2p)CA−1 quasi-free scattering reactions to measure the proton component of the 21+ state of 16,18,20C. The experimental findings support the notion of a moderate reduction of the proton 1p1/2−1p3/2 spin-orbit splitting, at variance to recent claims for a prevalent Z=6 magic number towards the neutron dripline. |
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| title_short |
Probing the Z = 6 spin-orbit shell gap with (p,2p) quasi-free scattering reactions |
| url |
https://doi.org/10.1016/j.physletb.2020.135748 https://doaj.org/article/dd22e2ae0d6d43a99113913dec8be2ff http://www.sciencedirect.com/science/article/pii/S0370269320305517 https://doaj.org/toc/0370-2693 |
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M. Petri A.O. Macchiavelli S. Paschalis C.A. Bertulani T. Aumann H. Alvarez-Pol L. Atar S. Beceiro-Novo J. Benlliure J.M. Boillos K. Boretzky M.J.G. Borge B.A. Brown M. Caamaño C. Caesar E. Casarejos W. Catford J. Cederkall S. Chakraborty L.V. Chulkov D. Cortina-Gil E. Cravo R. Crespo U. Datta Pramanik I. Dillmann P. Díaz Fernández Z. Elekes J. Enders F. Farinon L.M. Fraile D. Galaviz H. Geissel R. Gernhäuser P. Golubev K. Göbel M. Heil M. Heine A. Heinz A. Henriques M. Holl H.T. Johansson B. Jonson N. Kalantar-Nayestanaki R. Kanungo A. Kelic-Heil T. Kröll N. Kurz C. Langer T. Le Bleis J. Machado J. Marganiec-Gałązka E. Nacher T. Nilsson C. Nociforo V. Panin A. Perea S.B. Pietri R. Plag A. Rahaman R. Reifarth A. Revel G. Ribeiro C. Rigollet D.M. Rossi D. Savran H. Scheit H. Simon O. Sorlin O. Tengblad Y. Togano M. Vandebrouck V. Volkov F. Wamers C. Wheldon G.L. Wilson J.S. Winfield H. Weick P. Woods D. Yakorev M. Zhukov A. Zilges K. Zuber |
| author2Str |
M. Petri A.O. Macchiavelli S. Paschalis C.A. Bertulani T. Aumann H. Alvarez-Pol L. Atar S. Beceiro-Novo J. Benlliure J.M. Boillos K. Boretzky M.J.G. Borge B.A. Brown M. Caamaño C. Caesar E. Casarejos W. Catford J. Cederkall S. Chakraborty L.V. Chulkov D. Cortina-Gil E. Cravo R. Crespo U. Datta Pramanik I. Dillmann P. Díaz Fernández Z. Elekes J. Enders F. Farinon L.M. Fraile D. Galaviz H. Geissel R. Gernhäuser P. Golubev K. Göbel M. Heil M. Heine A. Heinz A. Henriques M. Holl H.T. Johansson B. Jonson N. Kalantar-Nayestanaki R. Kanungo A. Kelic-Heil T. Kröll N. Kurz C. Langer T. Le Bleis J. Machado J. Marganiec-Gałązka E. Nacher T. Nilsson C. Nociforo V. Panin A. Perea S.B. Pietri R. Plag A. Rahaman R. Reifarth A. Revel G. Ribeiro C. Rigollet D.M. Rossi D. Savran H. Scheit H. Simon O. Sorlin O. Tengblad Y. Togano M. Vandebrouck V. Volkov F. Wamers C. Wheldon G.L. Wilson J.S. Winfield H. Weick P. Woods D. Yakorev M. Zhukov A. Zilges K. Zuber |
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| doi_str |
10.1016/j.physletb.2020.135748 |
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