First Measurement of 72Ge(n, γ) at n-TOF

M. Dietz; C. Lederer-Woods; O. Aberle; J. Andrzejewski; L. Audouin; M. Bacak; J. Balibrea; M. Barbagallo; F. Bečvář; E. Berthoumieux; J. Billowes; D. Bosnar; A. Brown; M. Caamaño; F. Calviño; M. Calviani; D. Cano-Ott; R. Cardella; A. Casanovas; F. Cerutti; Y. H. Chen; E. Chiaveri; N. Colonna; G. Cortés; M. A. Cortés-Giraldo; L. Cosentino; L. A. Damone; M. Diakaki; C. Domingo-Pardo; R. Dressler; E. Dupont; I. Durán; B. Fernández-Domínguez; A. Ferrari; P. Ferreira; P. Finocchiaro; V. Furman; K. Göbel; A. R. García; R. Garg; A. Gawlik; S. Gilardoni; T. Glodariu; I. F. Gonçalves; E. González-Romero; E. Griesmayer; C. Guerrero; F. Gunsing; H. Harada; T. Rauscher

doi:10.1051/epjconf/201718402005

First Measurement of ⁷²Ge(n, γ) at n-TOF

M. Dietz
, C. Lederer-Woods
, O. Aberle
, J. Andrzejewski
, L. Audouin
, M. Bacak
, J. Balibrea
, M. Barbagallo
, F. Bečvář
, E. Berthoumieux
, J. Billowes
, D. Bosnar
, A. Brown
, M. Caamaño
, F. Calviño
, M. Calviani
, D. Cano-Ott
, R. Cardella
, A. Casanovas
, F. Cerutti

Y. H. Chen, E. Chiaveri, N. Colonna, G. Cortés, M. A. Cortés-Giraldo, L. Cosentino, L. A. Damone, M. Diakaki, C. Domingo-Pardo, R. Dressler, E. Dupont, I. Durán, B. Fernández-Domínguez, A. Ferrari, P. Ferreira, P. Finocchiaro, V. Furman, K. Göbel, A. R. García, R. Garg, A. Gawlik, S. Gilardoni, T. Glodariu, I. F. Gonçalves, E. González-Romero, E. Griesmayer, C. Guerrero, F. Gunsing, H. Harada, T. Rauscher

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Abstract

The slow neutron capture process (s-process) is responsible for producing about half of the elemental abundances heavier than iron in the universe. Neutron capture cross sections on stable isotopes are a key nuclear physics input for s-process studies. The ⁷²Ge(n, γ) cross section has an important influence on production of isotopes between Ge and Zr during s-process in massive stars and therefore experimental data are urgently required. ⁷²Ge(n, γ) was measured at the neutron time-of-flight facility n-TOF (CERN) for the first time at stellar energies. The measurement was performed using an enriched ⁷²GeO₂ sample at a flight path of 185m with a set of liquid scintillation detectors (C₆D₆). The motivation, experiment and current status of the data analysis are reported.

Original language	English
Article number	02005
Journal	EPJ Web of Conferences
Volume	184
DOIs	https://doi.org/10.1051/epjconf/201718402005
Publication status	Published - 29 Jun 2018
Event	9th European Summer School on Experimental Nuclear Astrophysics, ENNAS 2017 - Santa Tecla, Catania, Italy Duration: 17 Sept 2017 → 24 Sept 2017

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© The Authors, published by EDP Sciences. This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).
Final published version, 328 KBLicence: CC BY

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Dietz, M., Lederer-Woods, C., Aberle, O., 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., ... Rauscher, T. (2018). First Measurement of ⁷²Ge(n, γ) at n-TOF. EPJ Web of Conferences, 184, Article 02005. https://doi.org/10.1051/epjconf/201718402005

@article{e6dc8e2f642e4953b1f9da75405be77f,

title = "First Measurement of 72Ge(n, γ) at n-TOF",

abstract = "The slow neutron capture process (s-process) is responsible for producing about half of the elemental abundances heavier than iron in the universe. Neutron capture cross sections on stable isotopes are a key nuclear physics input for s-process studies. The 72Ge(n, γ) cross section has an important influence on production of isotopes between Ge and Zr during s-process in massive stars and therefore experimental data are urgently required. 72Ge(n, γ) was measured at the neutron time-of-flight facility n-TOF (CERN) for the first time at stellar energies. The measurement was performed using an enriched 72GeO2 sample at a flight path of 185m with a set of liquid scintillation detectors (C6D6). The motivation, experiment and current status of the data analysis are reported.",

author = "M. Dietz and C. Lederer-Woods and O. Aberle and J. Andrzejewski and L. Audouin and M. Bacak and J. Balibrea and M. Barbagallo and F. Be{\v c}v{\'a}{\v r} and E. Berthoumieux and J. Billowes and D. Bosnar and A. Brown and M. Caama{\~n}o and F. Calvi{\~n}o and M. Calviani and D. Cano-Ott and R. Cardella and A. Casanovas and F. Cerutti and Chen, \{Y. H.\} and E. Chiaveri and N. Colonna and G. Cort{\'e}s and Cort{\'e}s-Giraldo, \{M. A.\} and L. Cosentino and Damone, \{L. A.\} and M. Diakaki and C. Domingo-Pardo and R. Dressler and E. Dupont and I. Dur{\'a}n and B. Fern{\'a}ndez-Dom{\'i}nguez and A. Ferrari and P. Ferreira and P. Finocchiaro and V. Furman and K. G{\"o}bel and Garc{\'i}a, \{A. R.\} and R. Garg and A. Gawlik and S. Gilardoni and T. Glodariu and Gon{\c c}alves, \{I. F.\} and E. Gonz{\'a}lez-Romero and E. Griesmayer and C. Guerrero and F. Gunsing and H. Harada and T. Rauscher",

note = "{\textcopyright} The Authors, published by EDP Sciences. This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).; 9th European Summer School on Experimental Nuclear Astrophysics, ENNAS 2017 ; Conference date: 17-09-2017 Through 24-09-2017",

year = "2018",

month = jun,

day = "29",

doi = "10.1051/epjconf/201718402005",

language = "English",

volume = "184",

journal = "EPJ Web of Conferences",

issn = "2101-6275",

publisher = "EDP Sciences",

}

Dietz, M, Lederer-Woods, C, Aberle, O, 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, YH, Chiaveri, E, Colonna, N, Cortés, G, Cortés-Giraldo, MA, Cosentino, L, Damone, LA, Diakaki, M, Domingo-Pardo, C, Dressler, R, Dupont, E, Durán, I, Fernández-Domínguez, B, Ferrari, A, Ferreira, P, Finocchiaro, P, Furman, V, Göbel, K, García, AR, Garg, R, Gawlik, A, Gilardoni, S, Glodariu, T, Gonçalves, IF, González-Romero, E, Griesmayer, E, Guerrero, C, Gunsing, F, Harada, H & Rauscher, T 2018, 'First Measurement of ⁷²Ge(n, γ) at n-TOF', EPJ Web of Conferences, vol. 184, 02005. https://doi.org/10.1051/epjconf/201718402005

TY - JOUR

T1 - First Measurement of 72Ge(n, γ) at n-TOF

AU - Dietz, M.

AU - Lederer-Woods, C.

AU - Aberle, O.

AU - Andrzejewski, J.

AU - Audouin, L.

AU - Bacak, M.

AU - Balibrea, J.

AU - Barbagallo, M.

AU - Bečvář, F.

AU - Berthoumieux, E.

AU - Billowes, J.

AU - Bosnar, D.

AU - Brown, A.

AU - Caamaño, M.

AU - Calviño, F.

AU - Calviani, M.

AU - Cano-Ott, D.

AU - Cardella, R.

AU - Casanovas, A.

AU - Cerutti, F.

AU - Chen, Y. H.

AU - Chiaveri, E.

AU - Colonna, N.

AU - Cortés, G.

AU - Cortés-Giraldo, M. A.

AU - Cosentino, L.

AU - Damone, L. A.

AU - Diakaki, M.

AU - Domingo-Pardo, C.

AU - Dressler, R.

AU - Dupont, E.

AU - Durán, I.

AU - Fernández-Domínguez, B.

AU - Ferrari, A.

AU - Ferreira, P.

AU - Finocchiaro, P.

AU - Furman, V.

AU - Göbel, K.

AU - García, A. R.

AU - Garg, R.

AU - Gawlik, A.

AU - Gilardoni, S.

AU - Glodariu, T.

AU - Gonçalves, I. F.

AU - González-Romero, E.

AU - Griesmayer, E.

AU - Guerrero, C.

AU - Gunsing, F.

AU - Harada, H.

AU - Rauscher, T.

N1 - © The Authors, published by EDP Sciences. This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).

PY - 2018/6/29

Y1 - 2018/6/29

N2 - The slow neutron capture process (s-process) is responsible for producing about half of the elemental abundances heavier than iron in the universe. Neutron capture cross sections on stable isotopes are a key nuclear physics input for s-process studies. The 72Ge(n, γ) cross section has an important influence on production of isotopes between Ge and Zr during s-process in massive stars and therefore experimental data are urgently required. 72Ge(n, γ) was measured at the neutron time-of-flight facility n-TOF (CERN) for the first time at stellar energies. The measurement was performed using an enriched 72GeO2 sample at a flight path of 185m with a set of liquid scintillation detectors (C6D6). The motivation, experiment and current status of the data analysis are reported.

AB - The slow neutron capture process (s-process) is responsible for producing about half of the elemental abundances heavier than iron in the universe. Neutron capture cross sections on stable isotopes are a key nuclear physics input for s-process studies. The 72Ge(n, γ) cross section has an important influence on production of isotopes between Ge and Zr during s-process in massive stars and therefore experimental data are urgently required. 72Ge(n, γ) was measured at the neutron time-of-flight facility n-TOF (CERN) for the first time at stellar energies. The measurement was performed using an enriched 72GeO2 sample at a flight path of 185m with a set of liquid scintillation detectors (C6D6). The motivation, experiment and current status of the data analysis are reported.

UR - https://www.scopus.com/pages/publications/85051043923

U2 - 10.1051/epjconf/201718402005

DO - 10.1051/epjconf/201718402005

M3 - Conference article

AN - SCOPUS:85051043923

SN - 2101-6275

VL - 184

JO - EPJ Web of Conferences

JF - EPJ Web of Conferences

M1 - 02005

T2 - 9th European Summer School on Experimental Nuclear Astrophysics, ENNAS 2017

Y2 - 17 September 2017 through 24 September 2017

ER -

First Measurement of ⁷²Ge(n, γ) at n-TOF

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