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Destruction of the cosmic $\gamma$-ray emitter $^{26}$Al in massive stars: Study of the key $^{26}$Al$(n,p)$ reaction
The $^{26}$Al$(n,p)$ $^{26}$Mg reaction is the key reaction impacting on the abundances of the cosmic γ -ray emitter $^{26}$Al produced in massive stars and impacts on the potential pollution of the early solar system with $^{26}$Al by asymptotic giant branch stars. We performed a measurement...
| Autores principales: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Lenguaje: | eng |
| Publicado: |
2021
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1103/PhysRevC.104.L022803 http://cds.cern.ch/record/2780489 |
| _version_ | 1780971878517571584 |
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| author | Lederer-Woods, C Woods, P J Davinson, T Kahl, D Lonsdale, S J Aberle, O Amaducci, S Andrzejewski, J Audouin, L Bacak, M Balibrea, J Barbagallo, M Bečvář, F Berthoumieux, E Billowes, J Bosnar, D Brown, A Caamaño, M Calviño, F Calviani, M Cano-Ott, D Cardella, R Casanovas, A Cerutti, F Chen, Y H Chiaveri, E Colonna, N Cortés, G Cortés-Giraldo, M A Cosentino, L Cristallo, S Damone, L A Diakaki, M Domingo-Pardo, C Dressler, R Dupont, E Durán, I Fernández-Domínguez, B Ferrari, A Ferreira, P Ferrer, F J Finocchiaro, P Furman, V Göbel, K García, A R Gawlik, A Gilardoni, S Glodariu, T Gonçalves, I F González-Romero, E Griesmayer, E Guerrero, C Gunsing, F Harada, H Heinitz, S Heyse, J Jenkins, D G Jericha, E Käppeler, F Kadi, Y Kalamara, A Kavrigin, P Kimura, A Kivel, N Kokkoris, M Krtička, M Kurtulgil, D Leal-Cidoncha, E Leeb, H Lerendegui-Marco, J Lo Meo, S Macina, D Manna, A Marganiec, J Martínez, T Masi, A Massimi, C Mastinu, P Mastromarco, M Maugeri, E A Mazzone, A Mendoza, E Mengoni, A Milazzo, P M Mingrone, F Musumarra, A Negret, A Nolte, R Oprea, A Patronis, N Pavlik, A Perkowski, J Porras, I Praena, J Quesada, J M Radeck, D Rauscher, T Reifarth, R Rubbia, C Ryan, J A Sabaté-Gilarte, M Saxena, A Schillebeeckx, P Schumann, D Sedyshev, P Smith, A G Sosnin, N V Stamatopoulos, A Tagliente, G Tain, J L Tarifeño-Saldivia, A Tassan-Got, L Valenta, S Vannini, G Variale, V Vaz, P Ventura, A Vlachoudis, V Vlastou, R Wallner, A Warren, S Weiss, C Wright, T Žugec, P |
| author_facet | Lederer-Woods, C Woods, P J Davinson, T Kahl, D Lonsdale, S J Aberle, O Amaducci, S Andrzejewski, J Audouin, L Bacak, M Balibrea, J Barbagallo, M Bečvář, F Berthoumieux, E Billowes, J Bosnar, D Brown, A Caamaño, M Calviño, F Calviani, M Cano-Ott, D Cardella, R Casanovas, A Cerutti, F Chen, Y H Chiaveri, E Colonna, N Cortés, G Cortés-Giraldo, M A Cosentino, L Cristallo, S Damone, L A Diakaki, M Domingo-Pardo, C Dressler, R Dupont, E Durán, I Fernández-Domínguez, B Ferrari, A Ferreira, P Ferrer, F J Finocchiaro, P Furman, V Göbel, K García, A R Gawlik, A Gilardoni, S Glodariu, T Gonçalves, I F González-Romero, E Griesmayer, E Guerrero, C Gunsing, F Harada, H Heinitz, S Heyse, J Jenkins, D G Jericha, E Käppeler, F Kadi, Y Kalamara, A Kavrigin, P Kimura, A Kivel, N Kokkoris, M Krtička, M Kurtulgil, D Leal-Cidoncha, E Leeb, H Lerendegui-Marco, J Lo Meo, S Macina, D Manna, A Marganiec, J Martínez, T Masi, A Massimi, C Mastinu, P Mastromarco, M Maugeri, E A Mazzone, A Mendoza, E Mengoni, A Milazzo, P M Mingrone, F Musumarra, A Negret, A Nolte, R Oprea, A Patronis, N Pavlik, A Perkowski, J Porras, I Praena, J Quesada, J M Radeck, D Rauscher, T Reifarth, R Rubbia, C Ryan, J A Sabaté-Gilarte, M Saxena, A Schillebeeckx, P Schumann, D Sedyshev, P Smith, A G Sosnin, N V Stamatopoulos, A Tagliente, G Tain, J L Tarifeño-Saldivia, A Tassan-Got, L Valenta, S Vannini, G Variale, V Vaz, P Ventura, A Vlachoudis, V Vlastou, R Wallner, A Warren, S Weiss, C Wright, T Žugec, P |
| author_sort | Lederer-Woods, C |
| collection | CERN |
| description | The
$^{26}$Al$(n,p)$ $^{26}$Mg reaction is the key reaction impacting on the abundances of the cosmic
γ
-ray emitter
$^{26}$Al
produced in massive stars and impacts on the potential pollution of the early solar system with
$^{26}$Al
by asymptotic giant branch stars. We performed a measurement of the
$^{26}$Al$(n,p)$ $^{26}$Mg
cross section at the high-flux beam line EAR-2 at the n_TOF facility (CERN). We report resonance strengths for eleven resonances, nine being measured for the first time, while there is only one previous measurement for the other two. Our resonance strengths are significantly lower than the only previous values available. Our cross-section data range to 150 keV neutron energy, which is sufficient for a reliable determination of astrophysical reactivities up to 0.5 GK stellar temperature. |
| id | cern-2780489 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 2021 |
| record_format | invenio |
| spelling | cern-27804892022-06-30T12:03:21Zdoi:10.1103/PhysRevC.104.L022803http://cds.cern.ch/record/2780489engLederer-Woods, CWoods, P JDavinson, TKahl, DLonsdale, S JAberle, OAmaducci, SAndrzejewski, JAudouin, LBacak, MBalibrea, JBarbagallo, MBečvář, FBerthoumieux, EBillowes, JBosnar, DBrown, ACaamaño, MCalviño, FCalviani, MCano-Ott, DCardella, RCasanovas, ACerutti, FChen, Y HChiaveri, EColonna, NCortés, GCortés-Giraldo, M ACosentino, LCristallo, SDamone, L ADiakaki, MDomingo-Pardo, CDressler, RDupont, EDurán, IFernández-Domínguez, BFerrari, AFerreira, PFerrer, F JFinocchiaro, PFurman, VGöbel, KGarcía, A RGawlik, AGilardoni, SGlodariu, TGonçalves, I FGonzález-Romero, EGriesmayer, EGuerrero, CGunsing, FHarada, HHeinitz, SHeyse, JJenkins, D GJericha, EKäppeler, FKadi, YKalamara, AKavrigin, PKimura, AKivel, NKokkoris, MKrtička, MKurtulgil, DLeal-Cidoncha, ELeeb, HLerendegui-Marco, JLo Meo, SMacina, DManna, AMarganiec, JMartínez, TMasi, AMassimi, CMastinu, PMastromarco, MMaugeri, E AMazzone, AMendoza, EMengoni, AMilazzo, P MMingrone, FMusumarra, ANegret, ANolte, ROprea, APatronis, NPavlik, APerkowski, JPorras, IPraena, JQuesada, J MRadeck, DRauscher, TReifarth, RRubbia, CRyan, J ASabaté-Gilarte, MSaxena, ASchillebeeckx, PSchumann, DSedyshev, PSmith, A GSosnin, N VStamatopoulos, ATagliente, GTain, J LTarifeño-Saldivia, ATassan-Got, LValenta, SVannini, GVariale, VVaz, PVentura, AVlachoudis, VVlastou, RWallner, AWarren, SWeiss, CWright, TŽugec, PDestruction of the cosmic $\gamma$-ray emitter $^{26}$Al in massive stars: Study of the key $^{26}$Al$(n,p)$ reactionAstrophysics and AstronomyNuclear Physics - ExperimentThe $^{26}$Al$(n,p)$ $^{26}$Mg reaction is the key reaction impacting on the abundances of the cosmic γ -ray emitter $^{26}$Al produced in massive stars and impacts on the potential pollution of the early solar system with $^{26}$Al by asymptotic giant branch stars. We performed a measurement of the $^{26}$Al$(n,p)$ $^{26}$Mg cross section at the high-flux beam line EAR-2 at the n_TOF facility (CERN). We report resonance strengths for eleven resonances, nine being measured for the first time, while there is only one previous measurement for the other two. Our resonance strengths are significantly lower than the only previous values available. Our cross-section data range to 150 keV neutron energy, which is sufficient for a reliable determination of astrophysical reactivities up to 0.5 GK stellar temperature.oai:cds.cern.ch:27804892021 |
| spellingShingle | Astrophysics and Astronomy Nuclear Physics - Experiment Lederer-Woods, C Woods, P J Davinson, T Kahl, D Lonsdale, S J Aberle, O Amaducci, S Andrzejewski, J Audouin, L Bacak, M Balibrea, J Barbagallo, M Bečvář, F Berthoumieux, E Billowes, J Bosnar, D Brown, A Caamaño, M Calviño, F Calviani, M Cano-Ott, D Cardella, R Casanovas, A Cerutti, F Chen, Y H Chiaveri, E Colonna, N Cortés, G Cortés-Giraldo, M A Cosentino, L Cristallo, S Damone, L A Diakaki, M Domingo-Pardo, C Dressler, R Dupont, E Durán, I Fernández-Domínguez, B Ferrari, A Ferreira, P Ferrer, F J Finocchiaro, P Furman, V Göbel, K García, A R Gawlik, A Gilardoni, S Glodariu, T Gonçalves, I F González-Romero, E Griesmayer, E Guerrero, C Gunsing, F Harada, H Heinitz, S Heyse, J Jenkins, D G Jericha, E Käppeler, F Kadi, Y Kalamara, A Kavrigin, P Kimura, A Kivel, N Kokkoris, M Krtička, M Kurtulgil, D Leal-Cidoncha, E Leeb, H Lerendegui-Marco, J Lo Meo, S Macina, D Manna, A Marganiec, J Martínez, T Masi, A Massimi, C Mastinu, P Mastromarco, M Maugeri, E A Mazzone, A Mendoza, E Mengoni, A Milazzo, P M Mingrone, F Musumarra, A Negret, A Nolte, R Oprea, A Patronis, N Pavlik, A Perkowski, J Porras, I Praena, J Quesada, J M Radeck, D Rauscher, T Reifarth, R Rubbia, C Ryan, J A Sabaté-Gilarte, M Saxena, A Schillebeeckx, P Schumann, D Sedyshev, P Smith, A G Sosnin, N V Stamatopoulos, A Tagliente, G Tain, J L Tarifeño-Saldivia, A Tassan-Got, L Valenta, S Vannini, G Variale, V Vaz, P Ventura, A Vlachoudis, V Vlastou, R Wallner, A Warren, S Weiss, C Wright, T Žugec, P Destruction of the cosmic $\gamma$-ray emitter $^{26}$Al in massive stars: Study of the key $^{26}$Al$(n,p)$ reaction |
| title | Destruction of the cosmic $\gamma$-ray emitter $^{26}$Al in massive stars: Study of the key $^{26}$Al$(n,p)$ reaction |
| title_full | Destruction of the cosmic $\gamma$-ray emitter $^{26}$Al in massive stars: Study of the key $^{26}$Al$(n,p)$ reaction |
| title_fullStr | Destruction of the cosmic $\gamma$-ray emitter $^{26}$Al in massive stars: Study of the key $^{26}$Al$(n,p)$ reaction |
| title_full_unstemmed | Destruction of the cosmic $\gamma$-ray emitter $^{26}$Al in massive stars: Study of the key $^{26}$Al$(n,p)$ reaction |
| title_short | Destruction of the cosmic $\gamma$-ray emitter $^{26}$Al in massive stars: Study of the key $^{26}$Al$(n,p)$ reaction |
| title_sort | destruction of the cosmic $\gamma$-ray emitter $^{26}$al in massive stars: study of the key $^{26}$al$(n,p)$ reaction |
| topic | Astrophysics and Astronomy Nuclear Physics - Experiment |
| url | https://dx.doi.org/10.1103/PhysRevC.104.L022803 http://cds.cern.ch/record/2780489 |
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