Measurement of the 154Gd(n,γ) cross section and its astrophysical implications

A. Mazzone; S. Cristallo; O. Aberle; G. Alaerts; V. Alcayne; S. Amaducci; J. Andrzejewski; L. Audouin; V. Babiano-Suarez; M. Bacak; M. Barbagallo; V. Bécares; F. Bečvář; G. Bellia; E. Berthoumieux; J. Billowes; D. Bosnar; A. S. Brown; M. Busso; M. Caamaño; L. Caballero; M. Calviani; F. Calviño; D. Cano-Ott; A. Casanovas; D. M. Castelluccio; F. Cerutti; Y. H. Chen; E. Chiaveri; G. Clai; N. Colonna; G. P. Cortés; M. A. Cortés-Giraldo; L. Cosentino; L. A. Damone; M. Diakaki; M. Dietz; C. Domingo-Pardo; R. Dressler; E. Dupont; I. Durán; Z. Eleme; B. Fernández-Domíngez; A. Ferrari; I. Ferro-Gonçalves; P. Finocchiaro; V. Furman; R. Garg; A. Gawlik; S. Gilardoni; T. Glodariu; K. Göbel; E. González-Romero; C. Guerrero; F. Gunsing; S. Heinitz; J. Heyse; D. G. Jenkins; E. Jericha; Y. Kadi; F. Käppeler; A. Kimura; N. Kivel; M. Kokkoris; Y. Kopatch; S. Kopecky; M. Krtička; D. Kurtulgil; I. Ladarescu; C. Lederer-Woods; J. Lerendegui-Marco; S. Lo Meo; S. J. Lonsdale; D. Macina; A. Manna; T. Martínez; A. Masi; C. Massimi; P. F. Mastinu; M. Mastromarco; F. Matteucci; E. Maugeri; E. Mendoza; A. Mengoni; V. Michalopoulou; P. M. Milazzo; F. Mingrone; R. Mucciola; A. Musumarra; A. Negret; R. Nolte; F. Ogállar; A. Oprea; N. Patronis; A. Pavlik; J. Perkowski; L. Piersanti; I. Porras; J. Praena; J. M. Quesada; D. Radeck; D. Ramos Doval; R. Reifarth; D. Rochman; C. Rubbia; M. Sabaté-Gilarte; A. Saxena; P. Schillebeeckx; D. Schumann; A. G. Smith; N. Sosnin; A. Stamatopoulos; G. Tagliente; J. L. Tain; Z. Talip; A. E. Tarifeño-Saldivia; L. Tassan-Got; P. Torres-Sánchez; A. Tsinganis; J. Ulrich; S. Urlass; S. Valenta; G. Vannini; V. Variale; P. Vaz; A. Ventura; D. Vescovi; V. Vlachoudis; R. Vlastou; A. Wallner; P. J. Woods; R. Wynants; T. J. Wright; P. Žugec

doi:10.1016/j.physletb.2020.135405

Measurement of the ¹⁵⁴Gd(n,γ) cross section and its astrophysical implications

A. Mazzone, S. Cristallo, O. Aberle, G. Alaerts, V. Alcayne, S. Amaducci, J. Andrzejewski, L. Audouin, V. Babiano-Suarez, M. Bacak, M. Barbagallo, V. Bécares, F. Bečvář, G. Bellia, E. Berthoumieux, J. Billowes, D. Bosnar, A. S. Brown, M. Busso, M. CaamañoL. Caballero, M. Calviani, F. Calviño, D. Cano-Ott, A. Casanovas, D. M. Castelluccio, F. Cerutti, Y. H. Chen, E. Chiaveri, G. Clai, N. Colonna, G. P. Cortés, M. A. Cortés-Giraldo, L. Cosentino, L. A. Damone, M. Diakaki, M. Dietz, C. Domingo-Pardo, R. Dressler, E. Dupont, I. Durán, Z. Eleme, B. Fernández-Domíngez, A. Ferrari, I. Ferro-Gonçalves, P. Finocchiaro, V. Furman, R. Garg, A. Gawlik, S. Gilardoni, T. Glodariu, K. Göbel, E. González-Romero, C. Guerrero, F. Gunsing, S. Heinitz, J. Heyse, D. G. Jenkins, E. Jericha, Y. Kadi, F. Käppeler, A. Kimura, N. Kivel, M. Kokkoris, Y. Kopatch, S. Kopecky, M. Krtička, D. Kurtulgil, I. Ladarescu, C. Lederer-Woods, J. Lerendegui-Marco, S. Lo Meo, S. J. Lonsdale, D. Macina, A. Manna, T. Martínez, A. Masi, C. Massimi^*, P. F. Mastinu, M. Mastromarco, F. Matteucci, E. Maugeri, E. Mendoza, A. Mengoni, V. Michalopoulou, P. M. Milazzo, F. Mingrone, R. Mucciola, A. Musumarra, A. Negret, R. Nolte, F. Ogállar, A. Oprea, N. Patronis, A. Pavlik, J. Perkowski, L. Piersanti, I. Porras, J. Praena, J. M. Quesada, D. Radeck, D. Ramos Doval, R. Reifarth, D. Rochman, C. Rubbia, M. Sabaté-Gilarte, A. Saxena, P. Schillebeeckx, D. Schumann, A. G. Smith, N. Sosnin, A. Stamatopoulos, G. Tagliente, J. L. Tain, Z. Talip, A. E. Tarifeño-Saldivia, L. Tassan-Got, P. Torres-Sánchez, A. Tsinganis, J. Ulrich, S. Urlass, S. Valenta, G. Vannini, V. Variale, P. Vaz, A. Ventura, D. Vescovi, V. Vlachoudis, R. Vlastou, A. Wallner, P. J. Woods, R. Wynants, T. J. Wright, P. Žugec

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

6 Citations (Scopus)

Abstract

The neutron capture cross section of ¹⁵⁴Gd 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 ¹⁵⁴Gd. The capture measurement, performed with four C₆D₆ 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 ¹⁵⁴Gd(n,γ) cross section reduces the discrepancy between observed and calculated solar s-only isotopic abundances predicted by s-process nucleosynthesis models.

Original language	English
Article number	135405
Journal	Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume	804
DOIs	https://doi.org/10.1016/j.physletb.2020.135405
Publication status	Published - 10 May 2020

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Mazzone, A., Cristallo, S., 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., ... Žugec, P. (2020). Measurement of the ¹⁵⁴Gd(n,γ) cross section and its astrophysical implications. Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, 804, Article 135405. https://doi.org/10.1016/j.physletb.2020.135405

@article{4e624a92a7ef4cc4a53d1542c795c072,

title = "Measurement of the 154Gd(n,γ) cross section and its astrophysical implications",

abstract = "The neutron capture cross section of 154Gd 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 154Gd. The capture measurement, performed with four C6D6 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 154Gd(n,γ) cross section reduces the discrepancy between observed and calculated solar s-only isotopic abundances predicted by s-process nucleosynthesis models.",

keywords = "Gd, Neutron time of flight, n_TOF, s process",

author = "A. Mazzone and S. Cristallo and O. Aberle and G. Alaerts and V. Alcayne and S. Amaducci and J. Andrzejewski and L. Audouin and V. Babiano-Suarez and M. Bacak and M. Barbagallo and V. B{\'e}cares and F. Be{\v c}v{\'a}{\v r} and G. Bellia and E. Berthoumieux and J. Billowes and D. Bosnar and Brown, {A. S.} and M. Busso and M. Caama{\~n}o and L. Caballero and M. Calviani and F. Calvi{\~n}o and D. Cano-Ott and A. Casanovas and Castelluccio, {D. M.} and F. Cerutti and Chen, {Y. H.} and E. Chiaveri and G. Clai and N. Colonna and Cort{\'e}s, {G. P.} and Cort{\'e}s-Giraldo, {M. A.} and L. Cosentino and Damone, {L. A.} and M. Diakaki and M. Dietz and C. Domingo-Pardo and R. Dressler and E. Dupont and I. Dur{\'a}n and Z. Eleme and B. Fern{\'a}ndez-Dom{\'i}ngez and A. Ferrari and I. Ferro-Gon{\c c}alves and P. Finocchiaro and V. Furman and R. Garg and A. Gawlik and S. Gilardoni and T. Glodariu and K. G{\"o}bel and E. Gonz{\'a}lez-Romero and C. Guerrero and F. Gunsing and S. Heinitz and J. Heyse and Jenkins, {D. G.} and E. Jericha and Y. Kadi and F. K{\"a}ppeler and A. Kimura and N. Kivel and M. Kokkoris and Y. Kopatch and S. Kopecky and M. Krti{\v c}ka and D. Kurtulgil and I. Ladarescu and C. Lederer-Woods and J. Lerendegui-Marco and {Lo Meo}, S. and Lonsdale, {S. J.} and D. Macina and A. Manna and T. Mart{\'i}nez and A. Masi and C. Massimi and Mastinu, {P. F.} and M. Mastromarco and F. Matteucci and E. Maugeri and E. Mendoza and A. Mengoni and V. Michalopoulou and Milazzo, {P. M.} and F. Mingrone and R. Mucciola and A. Musumarra and A. Negret and R. Nolte and F. Og{\'a}llar and A. Oprea and N. Patronis and A. Pavlik and J. Perkowski and L. Piersanti and I. Porras and J. Praena and Quesada, {J. M.} and D. Radeck and {Ramos Doval}, D. and R. Reifarth and D. Rochman and C. Rubbia and M. Sabat{\'e}-Gilarte and A. Saxena and P. Schillebeeckx and D. Schumann and Smith, {A. G.} and N. Sosnin and A. Stamatopoulos and G. Tagliente and Tain, {J. L.} and Z. Talip and Tarife{\~n}o-Saldivia, {A. E.} and L. Tassan-Got and P. Torres-S{\'a}nchez and A. Tsinganis and J. Ulrich and S. Urlass and S. Valenta and G. Vannini and V. Variale and P. Vaz and A. Ventura and D. Vescovi and V. Vlachoudis and R. Vlastou and A. Wallner and Woods, {P. J.} and R. Wynants and Wright, {T. J.} and P. {\v Z}ugec",

note = "Publisher Copyright: {\textcopyright} 2020 The Author(s)",

year = "2020",

month = may,

day = "10",

doi = "10.1016/j.physletb.2020.135405",

language = "English",

volume = "804",

journal = "Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics",

issn = "0370-2693",

publisher = "Elsevier B.V.",

}

Mazzone, A, Cristallo, S, 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, AS, Busso, M, Caamaño, M, Caballero, L, Calviani, M, Calviño, F, Cano-Ott, D, Casanovas, A, Castelluccio, DM, Cerutti, F, Chen, YH, Chiaveri, E, Clai, G, Colonna, N, Cortés, GP, Cortés-Giraldo, MA, Cosentino, L, Damone, LA, 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, DG, 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, SJ, Macina, D, Manna, A, Martínez, T, Masi, A, Massimi, C, Mastinu, PF, Mastromarco, M, Matteucci, F, Maugeri, E, Mendoza, E, Mengoni, A, Michalopoulou, V, Milazzo, PM, 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, JM, Radeck, D, Ramos Doval, D, Reifarth, R, Rochman, D, Rubbia, C, Sabaté-Gilarte, M, Saxena, A, Schillebeeckx, P, Schumann, D, Smith, AG, Sosnin, N, Stamatopoulos, A, Tagliente, G, Tain, JL, Talip, Z, Tarifeño-Saldivia, AE, 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, PJ, Wynants, R, Wright, TJ & Žugec, P 2020, 'Measurement of the ¹⁵⁴Gd(n,γ) cross section and its astrophysical implications', Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, vol. 804, 135405. https://doi.org/10.1016/j.physletb.2020.135405

TY - JOUR

T1 - Measurement of the 154Gd(n,γ) cross section and its astrophysical implications

AU - Mazzone, A.

AU - Cristallo, S.

AU - Aberle, O.

AU - Alaerts, G.

AU - Alcayne, V.

AU - Amaducci, S.

AU - Andrzejewski, J.

AU - Audouin, L.

AU - Babiano-Suarez, V.

AU - Bacak, M.

AU - Barbagallo, M.

AU - Bécares, V.

AU - Bečvář, F.

AU - Bellia, G.

AU - Berthoumieux, E.

AU - Billowes, J.

AU - Bosnar, D.

AU - Brown, A. S.

AU - Busso, M.

AU - Caamaño, M.

AU - Caballero, L.

AU - Calviani, M.

AU - Calviño, F.

AU - Cano-Ott, D.

AU - Casanovas, A.

AU - Castelluccio, D. M.

AU - Cerutti, F.

AU - Chen, Y. H.

AU - Chiaveri, E.

AU - Clai, G.

AU - Colonna, N.

AU - Cortés, G. P.

AU - Cortés-Giraldo, M. A.

AU - Cosentino, L.

AU - Damone, L. A.

AU - Diakaki, M.

AU - Dietz, M.

AU - Domingo-Pardo, C.

AU - Dressler, R.

AU - Dupont, E.

AU - Durán, I.

AU - Eleme, Z.

AU - Fernández-Domíngez, B.

AU - Ferrari, A.

AU - Ferro-Gonçalves, I.

AU - Finocchiaro, P.

AU - Furman, V.

AU - Garg, R.

AU - Gawlik, A.

AU - Gilardoni, S.

AU - Glodariu, T.

AU - Göbel, K.

AU - González-Romero, E.

AU - Guerrero, C.

AU - Gunsing, F.

AU - Heinitz, S.

AU - Heyse, J.

AU - Jenkins, D. G.

AU - Jericha, E.

AU - Kadi, Y.

AU - Käppeler, F.

AU - Kimura, A.

AU - Kivel, N.

AU - Kokkoris, M.

AU - Kopatch, Y.

AU - Kopecky, S.

AU - Krtička, M.

AU - Kurtulgil, D.

AU - Ladarescu, I.

AU - Lederer-Woods, C.

AU - Lerendegui-Marco, J.

AU - Lo Meo, S.

AU - Lonsdale, S. J.

AU - Macina, D.

AU - Manna, A.

AU - Martínez, T.

AU - Masi, A.

AU - Massimi, C.

AU - Mastinu, P. F.

AU - Mastromarco, M.

AU - Matteucci, F.

AU - Maugeri, E.

AU - Mendoza, E.

AU - Mengoni, A.

AU - Michalopoulou, V.

AU - Milazzo, P. M.

AU - Mingrone, F.

AU - Mucciola, R.

AU - Musumarra, A.

AU - Negret, A.

AU - Nolte, R.

AU - Ogállar, F.

AU - Oprea, A.

AU - Patronis, N.

AU - Pavlik, A.

AU - Perkowski, J.

AU - Piersanti, L.

AU - Porras, I.

AU - Praena, J.

AU - Quesada, J. M.

AU - Radeck, D.

AU - Ramos Doval, D.

AU - Reifarth, R.

AU - Rochman, D.

AU - Rubbia, C.

AU - Sabaté-Gilarte, M.

AU - Saxena, A.

AU - Schillebeeckx, P.

AU - Schumann, D.

AU - Smith, A. G.

AU - Sosnin, N.

AU - Stamatopoulos, A.

AU - Tagliente, G.

AU - Tain, J. L.

AU - Talip, Z.

AU - Tarifeño-Saldivia, A. E.

AU - Tassan-Got, L.

AU - Torres-Sánchez, P.

AU - Tsinganis, A.

AU - Ulrich, J.

AU - Urlass, S.

AU - Valenta, S.

AU - Vannini, G.

AU - Variale, V.

AU - Vaz, P.

AU - Ventura, A.

AU - Vescovi, D.

AU - Vlachoudis, V.

AU - Vlastou, R.

AU - Wallner, A.

AU - Woods, P. J.

AU - Wynants, R.

AU - Wright, T. J.

AU - Žugec, P.

PY - 2020/5/10

Y1 - 2020/5/10

N2 - The neutron capture cross section of 154Gd 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 154Gd. The capture measurement, performed with four C6D6 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 154Gd(n,γ) cross section reduces the discrepancy between observed and calculated solar s-only isotopic abundances predicted by s-process nucleosynthesis models.

AB - The neutron capture cross section of 154Gd 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 154Gd. The capture measurement, performed with four C6D6 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 154Gd(n,γ) cross section reduces the discrepancy between observed and calculated solar s-only isotopic abundances predicted by s-process nucleosynthesis models.

KW - Gd

KW - Neutron time of flight

KW - n_TOF

KW - s process

UR - http://www.scopus.com/inward/record.url?scp=85082862606&partnerID=8YFLogxK

U2 - 10.1016/j.physletb.2020.135405

DO - 10.1016/j.physletb.2020.135405

M3 - Article

SN - 0370-2693

VL - 804

JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

M1 - 135405

ER -

Measurement of the ¹⁵⁴Gd(n,γ) cross section and its astrophysical implications

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