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Neutron spectroscopy of $^{26}$Mg states: constraining the stellar neutron source $^{22}$Ne($\alpha, n$)$^{25}$Mg
This work reports on accurate, high-resolution measurements of the 25 Mg( n,γ ) 26 Mg and 25 Mg( n,tot ) cross sections in the neutron energy range from thermal to about 300 keV, leading to a significantly improved 25 Mg( n,γ ) 26 Mg parametrization. The relevant resonances for n+25 Mg were characte...
| Autores principales: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Lenguaje: | eng |
| Publicado: |
2017
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1016/j.physletb.2017.02.025 http://cds.cern.ch/record/2253417 |
| _version_ | 1780953555737247744 |
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| author | Massimi, C. Altstadt, S. Andrzejewski, J. Audouin, L. Barbagallo, M. Bécares, V. Bečvář, F. Belloni, F. Berthoumieux, E. Billowes, J. Bisterzo, S. Bosnar, D. Brugger, M. Calviani, M. Calviño, F. Cano-Ott, D. Carrapiço, C. Castelluccio, D.M. Cerutti, F. Chiaveri, E. Cosentino, L. Chin, M. Clai, G. Colonna, N. Cortés, G. Cortés-Giraldo, M.A. Cristallo, S. Diakaki, M. Domingo-Pardo, C. Duran, I. Dressler, R. Eleftheriadis, C. Ferrari, A. Finocchiaro, P. Fraval, K. Ganesan, S. García, A.R. Giubrone, G. Gonçalves, I.F. González-Romero, E. Griesmayer, E. Guerrero, C. Gunsing, F. Hernández-Prieto, A. Jenkins, D.G. Jericha, E. Kadi, Y. Käppeler, F. Karadimos, D. Kivel, N. Koehler, P. Kokkoris, M. Kopecky, S. Krtička, M. Kroll, J. Lampoudis, C. Langer, C. Leal-Cidoncha, E. Lederer, C. Leeb, H. Leong, L.S. Lo Meo, S. Losito, R. Mallick, A. Manousos, A. Marganiec, J. Martínez, T. Mastinu, P.F. Mastromarco, M. Mendoza, E. Mengoni, A. Milazzo, P.M. Mingrone, F. Mirea, M. Mondelaers, W. Musumarra, A. Paradela, C. Pavlik, A. Perkowski, J. Pignatari, M. Piersanti, L. Plompen, A. Praena, J. Quesada, J.M. Rauscher, T. Reifarth, R. Riego, A. Robles, M.S. Rubbia, C. Sabaté-Gilarte, M. Sarmento, R. Saxena, A. Schillebeeckx, P. Schmidt, S. Schumann, D. Tagliente, G. Tain, J.L. Tarrío, D. Tassan-Got, L. Tsinganis, A. Valenta, S. Vannini, G. Van Rijs, I. Variale, V. Vaz, P. Ventura, A. Vermeulen, M.J. Vlachoudis, V. Vlastou, R. Wallner, A. Ware, T. Weigand, M. Weiß, C. Wynants, R. Wright, T. Žugec, P. |
| author_facet | Massimi, C. Altstadt, S. Andrzejewski, J. Audouin, L. Barbagallo, M. Bécares, V. Bečvář, F. Belloni, F. Berthoumieux, E. Billowes, J. Bisterzo, S. Bosnar, D. Brugger, M. Calviani, M. Calviño, F. Cano-Ott, D. Carrapiço, C. Castelluccio, D.M. Cerutti, F. Chiaveri, E. Cosentino, L. Chin, M. Clai, G. Colonna, N. Cortés, G. Cortés-Giraldo, M.A. Cristallo, S. Diakaki, M. Domingo-Pardo, C. Duran, I. Dressler, R. Eleftheriadis, C. Ferrari, A. Finocchiaro, P. Fraval, K. Ganesan, S. García, A.R. Giubrone, G. Gonçalves, I.F. González-Romero, E. Griesmayer, E. Guerrero, C. Gunsing, F. Hernández-Prieto, A. Jenkins, D.G. Jericha, E. Kadi, Y. Käppeler, F. Karadimos, D. Kivel, N. Koehler, P. Kokkoris, M. Kopecky, S. Krtička, M. Kroll, J. Lampoudis, C. Langer, C. Leal-Cidoncha, E. Lederer, C. Leeb, H. Leong, L.S. Lo Meo, S. Losito, R. Mallick, A. Manousos, A. Marganiec, J. Martínez, T. Mastinu, P.F. Mastromarco, M. Mendoza, E. Mengoni, A. Milazzo, P.M. Mingrone, F. Mirea, M. Mondelaers, W. Musumarra, A. Paradela, C. Pavlik, A. Perkowski, J. Pignatari, M. Piersanti, L. Plompen, A. Praena, J. Quesada, J.M. Rauscher, T. Reifarth, R. Riego, A. Robles, M.S. Rubbia, C. Sabaté-Gilarte, M. Sarmento, R. Saxena, A. Schillebeeckx, P. Schmidt, S. Schumann, D. Tagliente, G. Tain, J.L. Tarrío, D. Tassan-Got, L. Tsinganis, A. Valenta, S. Vannini, G. Van Rijs, I. Variale, V. Vaz, P. Ventura, A. Vermeulen, M.J. Vlachoudis, V. Vlastou, R. Wallner, A. Ware, T. Weigand, M. Weiß, C. Wynants, R. Wright, T. Žugec, P. |
| author_sort | Massimi, C. |
| collection | CERN |
| description | This work reports on accurate, high-resolution measurements of the 25 Mg( n,γ ) 26 Mg and 25 Mg( n,tot ) cross sections in the neutron energy range from thermal to about 300 keV, leading to a significantly improved 25 Mg( n,γ ) 26 Mg parametrization. The relevant resonances for n+25 Mg were characterized from a combined R-matrix analysis of the experimental data. This resulted in an unambiguous spin/parity assignment of the corresponding excited states in 26 Mg. With this information experimental upper limits of the reaction rates for 22 Ne( α,n ) 25 Mg and 22 Ne( α,γ ) 26 Mg were established, potentially leading to a significantly higher (α,n)/(α,γ) ratio than previously evaluated. The impact of these results has been studied for stellar models in the mass range 2 to 25 M⊙ . |
| id | cern-2253417 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 2017 |
| record_format | invenio |
| spelling | cern-22534172022-08-10T12:32:27Zdoi:10.1016/j.physletb.2017.02.025http://cds.cern.ch/record/2253417engMassimi, C.Altstadt, S.Andrzejewski, J.Audouin, L.Barbagallo, M.Bécares, V.Bečvář, F.Belloni, F.Berthoumieux, E.Billowes, J.Bisterzo, S.Bosnar, D.Brugger, M.Calviani, M.Calviño, F.Cano-Ott, D.Carrapiço, C.Castelluccio, D.M.Cerutti, F.Chiaveri, E.Cosentino, L.Chin, M.Clai, G.Colonna, N.Cortés, G.Cortés-Giraldo, M.A.Cristallo, S.Diakaki, M.Domingo-Pardo, C.Duran, I.Dressler, R.Eleftheriadis, C.Ferrari, A.Finocchiaro, P.Fraval, K.Ganesan, S.García, A.R.Giubrone, G.Gonçalves, I.F.González-Romero, E.Griesmayer, E.Guerrero, C.Gunsing, F.Hernández-Prieto, A.Jenkins, D.G.Jericha, E.Kadi, Y.Käppeler, F.Karadimos, D.Kivel, N.Koehler, P.Kokkoris, M.Kopecky, S.Krtička, M.Kroll, J.Lampoudis, C.Langer, C.Leal-Cidoncha, E.Lederer, C.Leeb, H.Leong, L.S.Lo Meo, S.Losito, R.Mallick, A.Manousos, A.Marganiec, J.Martínez, T.Mastinu, P.F.Mastromarco, M.Mendoza, E.Mengoni, A.Milazzo, P.M.Mingrone, F.Mirea, M.Mondelaers, W.Musumarra, A.Paradela, C.Pavlik, A.Perkowski, J.Pignatari, M.Piersanti, L.Plompen, A.Praena, J.Quesada, J.M.Rauscher, T.Reifarth, R.Riego, A.Robles, M.S.Rubbia, C.Sabaté-Gilarte, M.Sarmento, R.Saxena, A.Schillebeeckx, P.Schmidt, S.Schumann, D.Tagliente, G.Tain, J.L.Tarrío, D.Tassan-Got, L.Tsinganis, A.Valenta, S.Vannini, G.Van Rijs, I.Variale, V.Vaz, P.Ventura, A.Vermeulen, M.J.Vlachoudis, V.Vlastou, R.Wallner, A.Ware, T.Weigand, M.Weiß, C.Wynants, R.Wright, T.Žugec, P.Neutron spectroscopy of $^{26}$Mg states: constraining the stellar neutron source $^{22}$Ne($\alpha, n$)$^{25}$Mgnucl-exNuclear Physics - ExperimentThis work reports on accurate, high-resolution measurements of the 25 Mg( n,γ ) 26 Mg and 25 Mg( n,tot ) cross sections in the neutron energy range from thermal to about 300 keV, leading to a significantly improved 25 Mg( n,γ ) 26 Mg parametrization. The relevant resonances for n+25 Mg were characterized from a combined R-matrix analysis of the experimental data. This resulted in an unambiguous spin/parity assignment of the corresponding excited states in 26 Mg. With this information experimental upper limits of the reaction rates for 22 Ne( α,n ) 25 Mg and 22 Ne( α,γ ) 26 Mg were established, potentially leading to a significantly higher (α,n)/(α,γ) ratio than previously evaluated. The impact of these results has been studied for stellar models in the mass range 2 to 25 M⊙ .This work reports on accurate, high-resolution measurements of the $^{25}$Mg($n, \gamma$)$^{26}$Mg and $^{25}$Mg($n, tot$) cross sections in the neutron energy range from thermal to about 300 keV, leading to a significantly improved $^{25}$Mg($n, \gamma$)$^{26}$Mg parametrization. The relevant resonances for $n+^{25}$Mg were characterized from a combined R-matrix analysis of the experimental data. This resulted in an unambiguous spin/parity assignment of the corresponding excited states in $^{26}$Mg. With this information experimental upper limits of the reaction rates for $^{22}$Ne($\alpha, n$)$^{25}$Mg and $^{22}$Ne($\alpha, \gamma$)$^{26}$Mg were established, potentially leading to a significantly higher ($\alpha, n$)/($\alpha, \gamma$) ratio than previously evaluated. The impact of these results have been studied for stellar models in the mass range 2 to 25 $M_{\odot}$.arXiv:1702.04520oai:cds.cern.ch:22534172017-02-15 |
| spellingShingle | nucl-ex Nuclear Physics - Experiment Massimi, C. Altstadt, S. Andrzejewski, J. Audouin, L. Barbagallo, M. Bécares, V. Bečvář, F. Belloni, F. Berthoumieux, E. Billowes, J. Bisterzo, S. Bosnar, D. Brugger, M. Calviani, M. Calviño, F. Cano-Ott, D. Carrapiço, C. Castelluccio, D.M. Cerutti, F. Chiaveri, E. Cosentino, L. Chin, M. Clai, G. Colonna, N. Cortés, G. Cortés-Giraldo, M.A. Cristallo, S. Diakaki, M. Domingo-Pardo, C. Duran, I. Dressler, R. Eleftheriadis, C. Ferrari, A. Finocchiaro, P. Fraval, K. Ganesan, S. García, A.R. Giubrone, G. Gonçalves, I.F. González-Romero, E. Griesmayer, E. Guerrero, C. Gunsing, F. Hernández-Prieto, A. Jenkins, D.G. Jericha, E. Kadi, Y. Käppeler, F. Karadimos, D. Kivel, N. Koehler, P. Kokkoris, M. Kopecky, S. Krtička, M. Kroll, J. Lampoudis, C. Langer, C. Leal-Cidoncha, E. Lederer, C. Leeb, H. Leong, L.S. Lo Meo, S. Losito, R. Mallick, A. Manousos, A. Marganiec, J. Martínez, T. Mastinu, P.F. Mastromarco, M. Mendoza, E. Mengoni, A. Milazzo, P.M. Mingrone, F. Mirea, M. Mondelaers, W. Musumarra, A. Paradela, C. Pavlik, A. Perkowski, J. Pignatari, M. Piersanti, L. Plompen, A. Praena, J. Quesada, J.M. Rauscher, T. Reifarth, R. Riego, A. Robles, M.S. Rubbia, C. Sabaté-Gilarte, M. Sarmento, R. Saxena, A. Schillebeeckx, P. Schmidt, S. Schumann, D. Tagliente, G. Tain, J.L. Tarrío, D. Tassan-Got, L. Tsinganis, A. Valenta, S. Vannini, G. Van Rijs, I. Variale, V. Vaz, P. Ventura, A. Vermeulen, M.J. Vlachoudis, V. Vlastou, R. Wallner, A. Ware, T. Weigand, M. Weiß, C. Wynants, R. Wright, T. Žugec, P. Neutron spectroscopy of $^{26}$Mg states: constraining the stellar neutron source $^{22}$Ne($\alpha, n$)$^{25}$Mg |
| title | Neutron spectroscopy of $^{26}$Mg states: constraining the stellar neutron source $^{22}$Ne($\alpha, n$)$^{25}$Mg |
| title_full | Neutron spectroscopy of $^{26}$Mg states: constraining the stellar neutron source $^{22}$Ne($\alpha, n$)$^{25}$Mg |
| title_fullStr | Neutron spectroscopy of $^{26}$Mg states: constraining the stellar neutron source $^{22}$Ne($\alpha, n$)$^{25}$Mg |
| title_full_unstemmed | Neutron spectroscopy of $^{26}$Mg states: constraining the stellar neutron source $^{22}$Ne($\alpha, n$)$^{25}$Mg |
| title_short | Neutron spectroscopy of $^{26}$Mg states: constraining the stellar neutron source $^{22}$Ne($\alpha, n$)$^{25}$Mg |
| title_sort | neutron spectroscopy of $^{26}$mg states: constraining the stellar neutron source $^{22}$ne($\alpha, n$)$^{25}$mg |
| topic | nucl-ex Nuclear Physics - Experiment |
| url | https://dx.doi.org/10.1016/j.physletb.2017.02.025 http://cds.cern.ch/record/2253417 |
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