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Measurement of the $^{154}$Gd(n,$\gamma$) cross section and its astrophysical implications
The neutron capture cross section of 154 Gd was measured from 1 eV to 300 keV in the experimental area located 185 m from the CERN n_TOF neutron spallation source, using a metallic sample of gadolinium, enriched to 67% in 154 Gd. The capture measurement, performed with four C 6 D 6 scintillation det...
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Lenguaje: | eng |
Publicado: |
2020
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/j.physletb.2020.135405 http://cds.cern.ch/record/2709469 |
_version_ | 1780965060145840128 |
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author | Mazzone, A. Cristallo, S. Massimi, C. Aberle, O. Alaerts, G. Alcayne, V. Amaducci, S. Andrzejewski, J. Audouin, L. Babiano-Suarez, V. Bacak, M. Barbagallo, M. Bécares, V. Bečvář, F. Bellia, G. Berthoumieux, E. Billowes, J. Bosnar, D. Brown, A.S. Busso, M. Caamaño, M. Caballero, L. Calviani, M. Calviño, F. Cano-Ott, D. Casanovas, A. Castelluccio, D.M. Cerutti, F. Chen, Y.H. Chiaveri, E. Clai, G. Colonna, N. Cortés, G.P. Cortés-Giraldo, M.A. Cosentino, L. Damone, L.A. Diakaki, M. Dietz, M. Domingo-Pardo, C. Dressler, R. Dupont, E. Durán, I. Eleme, Z. Fernández-Domíngez, B. Ferrari, A. Ferro-Gonçalves, I. Finocchiaro, P. Furman, V. Garg, R. Gawlik, A. Gilardoni, S. Glodariu, T. Göbel, K. González-Romero, E. Guerrero, C. Gunsing, F. Heinitz, S. Heyse, J. Jenkins, D.G. Jericha, E. Kadi, Y. Käppeler, F. Kimura, A. Kivel, N. Kokkoris, M. Kopatch, Y. Kopecky, S. Krtička, M. Kurtulgil, D. Ladarescu, I. Lederer-Woods, C. Lerendegui-Marco, J. Lo Meo, S. Lonsdale, S.-J. Macina, D. Manna, A. Martínez, T. Masi, A. Mastinu, P.F. Mastromarco, M. Matteucci, F. Maugeri, E. Mendoza, E. Mengoni, A. Michalopoulou, V. Milazzo, P.M. Mingrone, F. Mucciola, R. Musumarra, A. Negret, A. Nolte, R. Ogállar, F. Oprea, A. Patronis, N. Pavlik, A. Perkowski, J. Piersanti, L. Porras, I. Praena, J. Quesada, J.M. Radeck, D. Ramos Doval, D. Reifarth, R. Rochman, D. Rubbia, C. Sabaté-Gilarte, M. Saxena, A. Schillebeeckx, P. Schumann, D. Smith, A.G. Sosnin, N. Stamatopoulos, A. Tagliente, G. Tain, J.L. Talip, Z. Tarifeño-Saldivia, A.E. Tassan-Got, L. Torres-Sánchez, P. Tsinganis, A. Ulrich, J. Urlass, S. Valenta, S. Vannini, G. Variale, V. Vaz, P. Ventura, A. Vescovi, D. Vlachoudis, V. Vlastou, R. Wallner, A. Woods, P.J. Wynants, R. Wright, T.J. Žugec, P. |
author_facet | Mazzone, A. Cristallo, S. Massimi, C. Aberle, O. Alaerts, G. Alcayne, V. Amaducci, S. Andrzejewski, J. Audouin, L. Babiano-Suarez, V. Bacak, M. Barbagallo, M. Bécares, V. Bečvář, F. Bellia, G. Berthoumieux, E. Billowes, J. Bosnar, D. Brown, A.S. Busso, M. Caamaño, M. Caballero, L. Calviani, M. Calviño, F. Cano-Ott, D. Casanovas, A. Castelluccio, D.M. Cerutti, F. Chen, Y.H. Chiaveri, E. Clai, G. Colonna, N. Cortés, G.P. Cortés-Giraldo, M.A. Cosentino, L. Damone, L.A. Diakaki, M. Dietz, M. Domingo-Pardo, C. Dressler, R. Dupont, E. Durán, I. Eleme, Z. Fernández-Domíngez, B. Ferrari, A. Ferro-Gonçalves, I. Finocchiaro, P. Furman, V. Garg, R. Gawlik, A. Gilardoni, S. Glodariu, T. Göbel, K. González-Romero, E. Guerrero, C. Gunsing, F. Heinitz, S. Heyse, J. Jenkins, D.G. Jericha, E. Kadi, Y. Käppeler, F. Kimura, A. Kivel, N. Kokkoris, M. Kopatch, Y. Kopecky, S. Krtička, M. Kurtulgil, D. Ladarescu, I. Lederer-Woods, C. Lerendegui-Marco, J. Lo Meo, S. Lonsdale, S.-J. Macina, D. Manna, A. Martínez, T. Masi, A. Mastinu, P.F. Mastromarco, M. Matteucci, F. Maugeri, E. Mendoza, E. Mengoni, A. Michalopoulou, V. Milazzo, P.M. Mingrone, F. Mucciola, R. Musumarra, A. Negret, A. Nolte, R. Ogállar, F. Oprea, A. Patronis, N. Pavlik, A. Perkowski, J. Piersanti, L. Porras, I. Praena, J. Quesada, J.M. Radeck, D. Ramos Doval, D. Reifarth, R. Rochman, D. Rubbia, C. Sabaté-Gilarte, M. Saxena, A. Schillebeeckx, P. Schumann, D. Smith, A.G. Sosnin, N. Stamatopoulos, A. Tagliente, G. Tain, J.L. Talip, Z. Tarifeño-Saldivia, A.E. Tassan-Got, L. Torres-Sánchez, P. Tsinganis, A. Ulrich, J. Urlass, S. Valenta, S. Vannini, G. Variale, V. Vaz, P. Ventura, A. Vescovi, D. Vlachoudis, V. Vlastou, R. Wallner, A. Woods, P.J. Wynants, R. Wright, T.J. Žugec, P. |
author_sort | Mazzone, A. |
collection | CERN |
description | The neutron capture cross section of 154 Gd was measured from 1 eV to 300 keV in the experimental area located 185 m from the CERN n_TOF neutron spallation source, using a metallic sample of gadolinium, enriched to 67% in 154 Gd. The capture measurement, performed with four C 6 D 6 scintillation detectors, has been complemented by a transmission measurement performed at the GELINA time-of-flight facility (JRC-Geel), thus minimising the uncertainty related to sample composition. An accurate Maxwellian averaged capture cross section (MACS) was deduced over the temperature range of interest for s process nucleosynthesis modelling. We report a value of 880(50) mb for the MACS at kT=30 keV, significantly lower compared to values available in literature. The new adopted 154 Gd(n, γ ) cross section reduces the discrepancy between observed and calculated solar s-only isotopic abundances predicted by s-process nucleosynthesis models. |
id | cern-2709469 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2020 |
record_format | invenio |
spelling | cern-27094692022-03-16T03:13:14Zdoi:10.1016/j.physletb.2020.135405http://cds.cern.ch/record/2709469engMazzone, A.Cristallo, S.Massimi, C.Aberle, O.Alaerts, G.Alcayne, V.Amaducci, S.Andrzejewski, J.Audouin, L.Babiano-Suarez, V.Bacak, M.Barbagallo, M.Bécares, V.Bečvář, F.Bellia, G.Berthoumieux, E.Billowes, J.Bosnar, D.Brown, A.S.Busso, M.Caamaño, M.Caballero, L.Calviani, M.Calviño, F.Cano-Ott, D.Casanovas, A.Castelluccio, D.M.Cerutti, F.Chen, Y.H.Chiaveri, E.Clai, G.Colonna, N.Cortés, G.P.Cortés-Giraldo, M.A.Cosentino, L.Damone, L.A.Diakaki, M.Dietz, M.Domingo-Pardo, C.Dressler, R.Dupont, E.Durán, I.Eleme, Z.Fernández-Domíngez, B.Ferrari, A.Ferro-Gonçalves, I.Finocchiaro, P.Furman, V.Garg, R.Gawlik, A.Gilardoni, S.Glodariu, T.Göbel, K.González-Romero, E.Guerrero, C.Gunsing, F.Heinitz, S.Heyse, J.Jenkins, D.G.Jericha, E.Kadi, Y.Käppeler, F.Kimura, A.Kivel, N.Kokkoris, M.Kopatch, Y.Kopecky, S.Krtička, M.Kurtulgil, D.Ladarescu, I.Lederer-Woods, C.Lerendegui-Marco, J.Lo Meo, S.Lonsdale, S.-J.Macina, D.Manna, A.Martínez, T.Masi, A.Mastinu, P.F.Mastromarco, M.Matteucci, F.Maugeri, E.Mendoza, E.Mengoni, A.Michalopoulou, V.Milazzo, P.M.Mingrone, F.Mucciola, R.Musumarra, A.Negret, A.Nolte, R.Ogállar, F.Oprea, A.Patronis, N.Pavlik, A.Perkowski, J.Piersanti, L.Porras, I.Praena, J.Quesada, J.M.Radeck, D.Ramos Doval, D.Reifarth, R.Rochman, D.Rubbia, C.Sabaté-Gilarte, M.Saxena, A.Schillebeeckx, P.Schumann, D.Smith, A.G.Sosnin, N.Stamatopoulos, A.Tagliente, G.Tain, J.L.Talip, Z.Tarifeño-Saldivia, A.E.Tassan-Got, L.Torres-Sánchez, P.Tsinganis, A.Ulrich, J.Urlass, S.Valenta, S.Vannini, G.Variale, V.Vaz, P.Ventura, A.Vescovi, D.Vlachoudis, V.Vlastou, R.Wallner, A.Woods, P.J.Wynants, R.Wright, T.J.Žugec, P.Measurement of the $^{154}$Gd(n,$\gamma$) cross section and its astrophysical implicationsnucl-exNuclear Physics - ExperimentThe neutron capture cross section of 154 Gd was measured from 1 eV to 300 keV in the experimental area located 185 m from the CERN n_TOF neutron spallation source, using a metallic sample of gadolinium, enriched to 67% in 154 Gd. The capture measurement, performed with four C 6 D 6 scintillation detectors, has been complemented by a transmission measurement performed at the GELINA time-of-flight facility (JRC-Geel), thus minimising the uncertainty related to sample composition. An accurate Maxwellian averaged capture cross section (MACS) was deduced over the temperature range of interest for s process nucleosynthesis modelling. We report a value of 880(50) mb for the MACS at kT=30 keV, significantly lower compared to values available in literature. The new adopted 154 Gd(n, γ ) cross section reduces the discrepancy between observed and calculated solar s-only isotopic abundances predicted by s-process nucleosynthesis models.The neutron capture cross section of $^{154}$Gd was measured from 1 eV to 300 keV in the experimental area located 185 m from the CERN n\_TOF neutron spallation source, using a metallic sample of gadolinium, enriched to 67$\%$ in $^{154}$Gd. The capture measurement, performed with four C$_{6}$D$_{6}$ scintillation detectors, has been complemented by a transmission measurement performed at the GELINA time-of-flight facility (JRC-Geel), thus minimising the uncertainty related to sample composition. An accurate Maxwellian averaged capture cross section (MACS) was deduced over the temperature range of interest for s process nucleosynthesis modeling. We report a value of 880(50) mb for the MACS at $kT=30$ keV, significantly lower compared to values available in literature. The new adopted $^{154}$Gd(n,$\gamma$) cross section reduces the discrepancy between observed and calculated solar s-only isotopic abundances predicted by s-process nucleosynthesis models.arXiv:2002.02322oai:cds.cern.ch:27094692020-02-06 |
spellingShingle | nucl-ex Nuclear Physics - Experiment Mazzone, A. Cristallo, S. Massimi, C. Aberle, O. Alaerts, G. Alcayne, V. Amaducci, S. Andrzejewski, J. Audouin, L. Babiano-Suarez, V. Bacak, M. Barbagallo, M. Bécares, V. Bečvář, F. Bellia, G. Berthoumieux, E. Billowes, J. Bosnar, D. Brown, A.S. Busso, M. Caamaño, M. Caballero, L. Calviani, M. Calviño, F. Cano-Ott, D. Casanovas, A. Castelluccio, D.M. Cerutti, F. Chen, Y.H. Chiaveri, E. Clai, G. Colonna, N. Cortés, G.P. Cortés-Giraldo, M.A. Cosentino, L. Damone, L.A. Diakaki, M. Dietz, M. Domingo-Pardo, C. Dressler, R. Dupont, E. Durán, I. Eleme, Z. Fernández-Domíngez, B. Ferrari, A. Ferro-Gonçalves, I. Finocchiaro, P. Furman, V. Garg, R. Gawlik, A. Gilardoni, S. Glodariu, T. Göbel, K. González-Romero, E. Guerrero, C. Gunsing, F. Heinitz, S. Heyse, J. Jenkins, D.G. Jericha, E. Kadi, Y. Käppeler, F. Kimura, A. Kivel, N. Kokkoris, M. Kopatch, Y. Kopecky, S. Krtička, M. Kurtulgil, D. Ladarescu, I. Lederer-Woods, C. Lerendegui-Marco, J. Lo Meo, S. Lonsdale, S.-J. Macina, D. Manna, A. Martínez, T. Masi, A. Mastinu, P.F. Mastromarco, M. Matteucci, F. Maugeri, E. Mendoza, E. Mengoni, A. Michalopoulou, V. Milazzo, P.M. Mingrone, F. Mucciola, R. Musumarra, A. Negret, A. Nolte, R. Ogállar, F. Oprea, A. Patronis, N. Pavlik, A. Perkowski, J. Piersanti, L. Porras, I. Praena, J. Quesada, J.M. Radeck, D. Ramos Doval, D. Reifarth, R. Rochman, D. Rubbia, C. Sabaté-Gilarte, M. Saxena, A. Schillebeeckx, P. Schumann, D. Smith, A.G. Sosnin, N. Stamatopoulos, A. Tagliente, G. Tain, J.L. Talip, Z. Tarifeño-Saldivia, A.E. Tassan-Got, L. Torres-Sánchez, P. Tsinganis, A. Ulrich, J. Urlass, S. Valenta, S. Vannini, G. Variale, V. Vaz, P. Ventura, A. Vescovi, D. Vlachoudis, V. Vlastou, R. Wallner, A. Woods, P.J. Wynants, R. Wright, T.J. Žugec, P. Measurement of the $^{154}$Gd(n,$\gamma$) cross section and its astrophysical implications |
title | Measurement of the $^{154}$Gd(n,$\gamma$) cross section and its astrophysical implications |
title_full | Measurement of the $^{154}$Gd(n,$\gamma$) cross section and its astrophysical implications |
title_fullStr | Measurement of the $^{154}$Gd(n,$\gamma$) cross section and its astrophysical implications |
title_full_unstemmed | Measurement of the $^{154}$Gd(n,$\gamma$) cross section and its astrophysical implications |
title_short | Measurement of the $^{154}$Gd(n,$\gamma$) cross section and its astrophysical implications |
title_sort | measurement of the $^{154}$gd(n,$\gamma$) cross section and its astrophysical implications |
topic | nucl-ex Nuclear Physics - Experiment |
url | https://dx.doi.org/10.1016/j.physletb.2020.135405 http://cds.cern.ch/record/2709469 |
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