The 154Gd neutron capture cross section measured at the n_TOF facility and its astrophysical implications

The (n, γ) cross sections of the gadolinium isotopes play an important role in the study of the stellar nucleosynthesis. In particular, among the isotopes heavier than Fe, 154Gd together with 152Gd have the peculiarity to be mainly produced by the slow capture process, the so-called s-process, since...

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Main Authors: Mastromarco M., Mazzone A., Massimi C., Cristallo S., Colonna N., Aberle O., Alcayne V., Amaducci S., Andrzejewski J., Audouin L., Babiano-Suarez V, Bacak M., Barbagallo M., Bennett S., Berthoumieux E., Bosnar D., Brown A. S., Busso M., Caamaño M., Caballero L., Calviani M., Calviño F., Cano-Ott D, Casanovas A., Cerutti F., Chiaveri E., Cortés G. P., Cortés-Giraldo M. A., Cosentino L., Damone L. A., Davies P. J., Diakaki M., Dietz M., Domingo-Pardo C, Dressler R., Ducasse Q., Dupont E., Durán I., Eleme Z., Fernández-Domíngez B., Ferrari A., Ferro-Gonçalves I., Finocchiaro P., Furman V., Garg R., Gawlik A., Gilardoni S., Göbel K., González-Romero E., Guerrero C., Gunsing F., Heinitz S., Heyse J., Jenkins D. G., Jericha E., Jiri U., Junghans A., Kadi Y., Käppeler F., Kimura A., Knapová I., Kokkoris M., Kopatch Y., Krtička M., Kurtulgil D., Ladarescu I., Lederer-Woods C, Lerendegui-Marco J, Lonsdale S.-J., Macina D., Manna A., Martínez T., Masi A., Mastinu P. F., Maugeri E., Mendoza E., Mengoni A., Michalopoulou V., Milazzo P. M., Millán-Callado M. A., Mingrone F., Moreno-Soto J, Musumarra A., Negret A., Ogállar F., Oprea A., Patronis N., Pavlik A., Perkowski J., Petrone C., Piersanti L., Pirovano E., Porras I., Praena J., Quesada J. M., Doval D. Ramos, Reifarth R., Rochman D., Rubbia C., Sabaté-Gilarte M., Saxena A., Schillebeeckx P., Schumann D., Sekhar A., Smith A. G., Sosnin N., Sprung P., Stamatopoulos A., Tagliente G., Tain J. L., Tarifeño-Saldivia A. E., Tassan-Got L, Thomas B., Torres-Sánchez P., Tsinganis A., Urlass S., Valenta S., Vannini G., Variale V., Vaz P., Ventura A., Vescovi D., Vlachoudis V., Vlastou R., Wallner A., Woods P. J., Wright T. J., Žugec P.
Format: Article
Language:English
Published: EDP Sciences 2020-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2020/15/epjconf_nd2019_07003.pdf
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author Mastromarco M.
Mazzone A.
Massimi C.
Cristallo S.
Colonna N.
Aberle O.
Alcayne V.
Amaducci S.
Andrzejewski J.
Audouin L.
Babiano-Suarez V
Bacak M.
Barbagallo M.
Bennett S.
Berthoumieux E.
Bosnar D.
Brown A. S.
Busso M.
Caamaño M.
Caballero L.
Calviani M.
Calviño F.
Cano-Ott D
Casanovas A.
Cerutti F.
Chiaveri E.
Cortés G. P.
Cortés-Giraldo M. A.
Cosentino L.
Damone L. A.
Davies P. J.
Diakaki M.
Dietz M.
Domingo-Pardo C
Dressler R.
Ducasse Q.
Dupont E.
Durán I.
Eleme Z.
Fernández-Domíngez B.
Ferrari A.
Ferro-Gonçalves I.
Finocchiaro P.
Furman V.
Garg R.
Gawlik A.
Gilardoni S.
Göbel K.
González-Romero E.
Guerrero C.
Gunsing F.
Heinitz S.
Heyse J.
Jenkins D. G.
Jericha E.
Jiri U.
Junghans A.
Kadi Y.
Käppeler F.
Kimura A.
Knapová I.
Kokkoris M.
Kopatch Y.
Krtička M.
Kurtulgil D.
Ladarescu I.
Lederer-Woods C
Lerendegui-Marco J
Lonsdale S.-J.
Macina D.
Manna A.
Martínez T.
Masi A.
Mastinu P. F.
Maugeri E.
Mendoza E.
Mengoni A.
Michalopoulou V.
Milazzo P. M.
Millán-Callado M. A.
Mingrone F.
Moreno-Soto J
Musumarra A.
Negret A.
Ogállar F.
Oprea A.
Patronis N.
Pavlik A.
Perkowski J.
Petrone C.
Piersanti L.
Pirovano E.
Porras I.
Praena J.
Quesada J. M.
Doval D. Ramos
Reifarth R.
Rochman D.
Rubbia C.
Sabaté-Gilarte M.
Saxena A.
Schillebeeckx P.
Schumann D.
Sekhar A.
Smith A. G.
Sosnin N.
Sprung P.
Stamatopoulos A.
Tagliente G.
Tain J. L.
Tarifeño-Saldivia A. E.
Tassan-Got L
Thomas B.
Torres-Sánchez P.
Tsinganis A.
Urlass S.
Valenta S.
Vannini G.
Variale V.
Vaz P.
Ventura A.
Vescovi D.
Vlachoudis V.
Vlastou R.
Wallner A.
Woods P. J.
Wright T. J.
Žugec P.
author_facet Mastromarco M.
Mazzone A.
Massimi C.
Cristallo S.
Colonna N.
Aberle O.
Alcayne V.
Amaducci S.
Andrzejewski J.
Audouin L.
Babiano-Suarez V
Bacak M.
Barbagallo M.
Bennett S.
Berthoumieux E.
Bosnar D.
Brown A. S.
Busso M.
Caamaño M.
Caballero L.
Calviani M.
Calviño F.
Cano-Ott D
Casanovas A.
Cerutti F.
Chiaveri E.
Cortés G. P.
Cortés-Giraldo M. A.
Cosentino L.
Damone L. A.
Davies P. J.
Diakaki M.
Dietz M.
Domingo-Pardo C
Dressler R.
Ducasse Q.
Dupont E.
Durán I.
Eleme Z.
Fernández-Domíngez B.
Ferrari A.
Ferro-Gonçalves I.
Finocchiaro P.
Furman V.
Garg R.
Gawlik A.
Gilardoni S.
Göbel K.
González-Romero E.
Guerrero C.
Gunsing F.
Heinitz S.
Heyse J.
Jenkins D. G.
Jericha E.
Jiri U.
Junghans A.
Kadi Y.
Käppeler F.
Kimura A.
Knapová I.
Kokkoris M.
Kopatch Y.
Krtička M.
Kurtulgil D.
Ladarescu I.
Lederer-Woods C
Lerendegui-Marco J
Lonsdale S.-J.
Macina D.
Manna A.
Martínez T.
Masi A.
Mastinu P. F.
Maugeri E.
Mendoza E.
Mengoni A.
Michalopoulou V.
Milazzo P. M.
Millán-Callado M. A.
Mingrone F.
Moreno-Soto J
Musumarra A.
Negret A.
Ogállar F.
Oprea A.
Patronis N.
Pavlik A.
Perkowski J.
Petrone C.
Piersanti L.
Pirovano E.
Porras I.
Praena J.
Quesada J. M.
Doval D. Ramos
Reifarth R.
Rochman D.
Rubbia C.
Sabaté-Gilarte M.
Saxena A.
Schillebeeckx P.
Schumann D.
Sekhar A.
Smith A. G.
Sosnin N.
Sprung P.
Stamatopoulos A.
Tagliente G.
Tain J. L.
Tarifeño-Saldivia A. E.
Tassan-Got L
Thomas B.
Torres-Sánchez P.
Tsinganis A.
Urlass S.
Valenta S.
Vannini G.
Variale V.
Vaz P.
Ventura A.
Vescovi D.
Vlachoudis V.
Vlastou R.
Wallner A.
Woods P. J.
Wright T. J.
Žugec P.
author_sort Mastromarco M.
collection DOAJ
description The (n, γ) cross sections of the gadolinium isotopes play an important role in the study of the stellar nucleosynthesis. In particular, among the isotopes heavier than Fe, 154Gd together with 152Gd have the peculiarity to be mainly produced by the slow capture process, the so-called s-process, since they are shielded against the β-decay chains from the r-process region by their stable samarium isobars. Such a quasi pure s-process origin makes them crucial for testing the robustness of stellar models in galactic chemical evolution (GCE). According to recent models, the 154Gd and 152Gd abundances are expected to be 15-20% lower than the reference un-branched s-process 150Sm isotope. The close correlation between stellar abundances and neutron capture cross sections prompted for an accurate measurement of 154Gd cross section in order to reduce the uncertainty attributable to nuclear physics input and eventually rule out one of the possible causes of present discrepancies between observation and model predictions. To this end, the neutron capture cross section of 154Gd was measured in a wide neutron energy range (from thermal up to some keV) with high resolution in the first experimental area of the neutron time-of-flight facility n_TOF (EAR1) at CERN. In this contribution, after a brief description of the motivation and of the experimental setup used in the measurement, the preliminary results of the 154Gd neutron capture reaction as well as their astrophysical implications are presented.
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spelling doaj.art-33ff6003ec56445cbde998ff4a6a0d142022-12-21T20:15:04ZengEDP SciencesEPJ Web of Conferences2100-014X2020-01-012390700310.1051/epjconf/202023907003epjconf_nd2019_07003The 154Gd neutron capture cross section measured at the n_TOF facility and its astrophysical implicationsMastromarco M.0Mazzone A.1Massimi C.Cristallo S.Colonna N.2Aberle O.3Alcayne V.4Amaducci S.Andrzejewski J.5Audouin L.6Babiano-Suarez V7Bacak M.Barbagallo M.8Bennett S.9Berthoumieux E.10Bosnar D.11Brown A. S.12Busso M.Caamaño M.13Caballero L.14Calviani M.15Calviño F.16Cano-Ott D17Casanovas A.18Cerutti F.19Chiaveri E.Cortés G. P.20Cortés-Giraldo M. A.21Cosentino L.22Damone L. A.Davies P. J.23Diakaki M.24Dietz M.25Domingo-Pardo C26Dressler R.27Ducasse Q.28Dupont E.29Durán I.30Eleme Z.31Fernández-Domíngez B.32Ferrari A.33Ferro-Gonçalves I.34Finocchiaro P.35Furman V.36Garg R.37Gawlik A.38Gilardoni S.39Göbel K.40González-Romero E.41Guerrero C.42Gunsing F.43Heinitz S.44Heyse J.45Jenkins D. G.46Jericha E.47Jiri U.48Junghans A.49Kadi Y.50Käppeler F.51Kimura A.52Knapová I.53Kokkoris M.54Kopatch Y.55Krtička M.56Kurtulgil D.57Ladarescu I.58Lederer-Woods C59Lerendegui-Marco J60Lonsdale S.-J.61Macina D.62Manna A.Martínez T.63Masi A.64Mastinu P. F.65Maugeri E.66Mendoza E.67Mengoni A.Michalopoulou V.Milazzo P. M.68Millán-Callado M. A.69Mingrone F.70Moreno-Soto J71Musumarra A.Negret A.72Ogállar F.73Oprea A.74Patronis N.75Pavlik A.76Perkowski J.77Petrone C.78Piersanti L.Pirovano E.79Porras I.80Praena J.81Quesada J. M.82Doval D. Ramos83Reifarth R.84Rochman D.85Rubbia C.86Sabaté-Gilarte M.Saxena A.87Schillebeeckx P.88Schumann D.89Sekhar A.90Smith A. G.91Sosnin N.92Sprung P.93Stamatopoulos A.94Tagliente G.95Tain J. L.96Tarifeño-Saldivia A. E.97Tassan-Got LThomas B.98Torres-Sánchez P.99Tsinganis A.100Urlass S.Valenta S.101Vannini G.Variale V.102Vaz P.103Ventura A.104Vescovi D.Vlachoudis V.105Vlastou R.106Wallner A.107Woods P. J.108Wright T. J.109Žugec P.110University of LodzKarlsruhe Institute of Technology, Campus North, IKPIstituto Nazionale di Fisica NucleareEuropean Organization for Nuclear Research (CERN)Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT)University of LodzIPN, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-SaclayInstituto de Física Corpuscular, CSIC - Universidad de ValenciaIPN, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-SaclayUniversity of ManchesterCEA Saclay, Irfu, Université Paris-SaclayDepartment of Physics, Faculty of Science, University of ZagrebUniversity of YorkUniversity of Santiago de CompostelaInstituto de Física Corpuscular, CSIC - Universidad de ValenciaEuropean Organization for Nuclear Research (CERN)Universitat Politècnica de CatalunyaCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT)Universitat Politècnica de CatalunyaEuropean Organization for Nuclear Research (CERN)Universitat Politècnica de CatalunyaUniversidad de SevillaINFN Laboratori Nazionali del SudUniversity of ManchesterNational Technical University of AthensSchool of Physics and Astronomy, University of EdinburghInstituto de Física Corpuscular, CSIC - Universidad de ValenciaPaul Scherrer Institut (PSI)Physikalisch-Technische Bundesanstalt (PTB), Bundesallee 100CEA Saclay, Irfu, Université Paris-SaclayUniversity of Santiago de CompostelaUniversity of IoanninaUniversity of Santiago de CompostelaEuropean Organization for Nuclear Research (CERN)Instituto Superior TécnicoINFN Laboratori Nazionali del SudJoint Institute for Nuclear Research (JINR)School of Physics and Astronomy, University of EdinburghUniversity of LodzEuropean Organization for Nuclear Research (CERN)Goethe University FrankfurtCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT)Universidad de SevillaCEA Saclay, Irfu, Université Paris-SaclayPaul Scherrer Institut (PSI)European Commission, Joint Research Centre, GeelUniversity of YorkTechnische Universität WienPaul Scherrer Institut (PSI)Helmholtz-Zentrum Dresden-RossendorfEuropean Organization for Nuclear Research (CERN)Karlsruhe Institute of Technology, Campus North, IKPJapan Atomic Energy Agency (JAEA)Charles UniversityNational Technical University of AthensJoint Institute for Nuclear Research (JINR)Charles UniversityGoethe University FrankfurtInstituto de Física Corpuscular, CSIC - Universidad de ValenciaSchool of Physics and Astronomy, University of EdinburghUniversidad de SevillaSchool of Physics and Astronomy, University of EdinburghEuropean Organization for Nuclear Research (CERN)Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT)European Organization for Nuclear Research (CERN)Istituto Nazionale di Fisica NuclearePaul Scherrer Institut (PSI)Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT)Istituto Nazionale di Fisica NazionaleUniversidad de SevillaEuropean Organization for Nuclear Research (CERN)CEA Saclay, Irfu, Université Paris-SaclayHoria Hulubei National Institute of Physics and Nuclear Engineering (IFIN-HH)University of GranadaHoria Hulubei National Institute of Physics and Nuclear Engineering (IFIN-HH)University of IoanninaUniversity of Vienna, Faculty of PhysicsUniversity of LodzHoria Hulubei National Institute of Physics and Nuclear Engineering (IFIN-HH)Physikalisch-Technische Bundesanstalt (PTB), Bundesallee 100University of GranadaUniversity of GranadaUniversidad de SevillaIPN, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-SaclayGoethe University FrankfurtPaul Scherrer Institut (PSI)European Organization for Nuclear Research (CERN)Bhabha Atomic Research Centre (BARC)European Commission, Joint Research Centre, GeelPaul Scherrer Institut (PSI)University of ManchesterUniversity of ManchesterUniversity of ManchesterPaul Scherrer Institut (PSI)National Technical University of AthensIstituto Nazionale di Fisica NucleareInstituto de Física Corpuscular, CSIC - Universidad de ValenciaUniversitat Politècnica de CatalunyaGoethe University FrankfurtUniversity of GranadaEuropean Organization for Nuclear Research (CERN)Charles UniversityIstituto Nazionale di Fisica NucleareInstituto Superior TécnicoIstituto Nazionale di Fisica Nucleare, Sezione di BolognaEuropean Organization for Nuclear Research (CERN)National Technical University of AthensAustralian National UniversitySchool of Physics and Astronomy, University of EdinburghUniversity of ManchesterDepartment of Physics, Faculty of Science, University of ZagrebThe (n, γ) cross sections of the gadolinium isotopes play an important role in the study of the stellar nucleosynthesis. In particular, among the isotopes heavier than Fe, 154Gd together with 152Gd have the peculiarity to be mainly produced by the slow capture process, the so-called s-process, since they are shielded against the β-decay chains from the r-process region by their stable samarium isobars. Such a quasi pure s-process origin makes them crucial for testing the robustness of stellar models in galactic chemical evolution (GCE). According to recent models, the 154Gd and 152Gd abundances are expected to be 15-20% lower than the reference un-branched s-process 150Sm isotope. The close correlation between stellar abundances and neutron capture cross sections prompted for an accurate measurement of 154Gd cross section in order to reduce the uncertainty attributable to nuclear physics input and eventually rule out one of the possible causes of present discrepancies between observation and model predictions. To this end, the neutron capture cross section of 154Gd was measured in a wide neutron energy range (from thermal up to some keV) with high resolution in the first experimental area of the neutron time-of-flight facility n_TOF (EAR1) at CERN. In this contribution, after a brief description of the motivation and of the experimental setup used in the measurement, the preliminary results of the 154Gd neutron capture reaction as well as their astrophysical implications are presented.https://www.epj-conferences.org/articles/epjconf/pdf/2020/15/epjconf_nd2019_07003.pdf
spellingShingle Mastromarco M.
Mazzone A.
Massimi C.
Cristallo S.
Colonna N.
Aberle O.
Alcayne V.
Amaducci S.
Andrzejewski J.
Audouin L.
Babiano-Suarez V
Bacak M.
Barbagallo M.
Bennett S.
Berthoumieux E.
Bosnar D.
Brown A. S.
Busso M.
Caamaño M.
Caballero L.
Calviani M.
Calviño F.
Cano-Ott D
Casanovas A.
Cerutti F.
Chiaveri E.
Cortés G. P.
Cortés-Giraldo M. A.
Cosentino L.
Damone L. A.
Davies P. J.
Diakaki M.
Dietz M.
Domingo-Pardo C
Dressler R.
Ducasse Q.
Dupont E.
Durán I.
Eleme Z.
Fernández-Domíngez B.
Ferrari A.
Ferro-Gonçalves I.
Finocchiaro P.
Furman V.
Garg R.
Gawlik A.
Gilardoni S.
Göbel K.
González-Romero E.
Guerrero C.
Gunsing F.
Heinitz S.
Heyse J.
Jenkins D. G.
Jericha E.
Jiri U.
Junghans A.
Kadi Y.
Käppeler F.
Kimura A.
Knapová I.
Kokkoris M.
Kopatch Y.
Krtička M.
Kurtulgil D.
Ladarescu I.
Lederer-Woods C
Lerendegui-Marco J
Lonsdale S.-J.
Macina D.
Manna A.
Martínez T.
Masi A.
Mastinu P. F.
Maugeri E.
Mendoza E.
Mengoni A.
Michalopoulou V.
Milazzo P. M.
Millán-Callado M. A.
Mingrone F.
Moreno-Soto J
Musumarra A.
Negret A.
Ogállar F.
Oprea A.
Patronis N.
Pavlik A.
Perkowski J.
Petrone C.
Piersanti L.
Pirovano E.
Porras I.
Praena J.
Quesada J. M.
Doval D. Ramos
Reifarth R.
Rochman D.
Rubbia C.
Sabaté-Gilarte M.
Saxena A.
Schillebeeckx P.
Schumann D.
Sekhar A.
Smith A. G.
Sosnin N.
Sprung P.
Stamatopoulos A.
Tagliente G.
Tain J. L.
Tarifeño-Saldivia A. E.
Tassan-Got L
Thomas B.
Torres-Sánchez P.
Tsinganis A.
Urlass S.
Valenta S.
Vannini G.
Variale V.
Vaz P.
Ventura A.
Vescovi D.
Vlachoudis V.
Vlastou R.
Wallner A.
Woods P. J.
Wright T. J.
Žugec P.
The 154Gd neutron capture cross section measured at the n_TOF facility and its astrophysical implications
EPJ Web of Conferences
title The 154Gd neutron capture cross section measured at the n_TOF facility and its astrophysical implications
title_full The 154Gd neutron capture cross section measured at the n_TOF facility and its astrophysical implications
title_fullStr The 154Gd neutron capture cross section measured at the n_TOF facility and its astrophysical implications
title_full_unstemmed The 154Gd neutron capture cross section measured at the n_TOF facility and its astrophysical implications
title_short The 154Gd neutron capture cross section measured at the n_TOF facility and its astrophysical implications
title_sort 154gd neutron capture cross section measured at the n tof facility and its astrophysical implications
url https://www.epj-conferences.org/articles/epjconf/pdf/2020/15/epjconf_nd2019_07003.pdf
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AT gonzalezromeroe 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
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AT junghansa 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
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AT kimuraa 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT knapovai 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT kokkorism 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT kopatchy 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT krtickam 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
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AT mastinupf 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
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AT patronisn 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT pavlika 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT perkowskij 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
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AT piersantil 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
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AT porrasi 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT praenaj 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT quesadajm 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT dovaldramos 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
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AT rochmand 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT rubbiac 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT sabategilartem 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT saxenaa 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT schillebeeckxp 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT schumannd 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT sekhara 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT smithag 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT sosninn 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT sprungp 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT stamatopoulosa 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT taglienteg 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT tainjl 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT tarifenosaldiviaae 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT tassangotl 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT thomasb 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT torressanchezp 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT tsinganisa 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT urlasss 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT valentas 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT vanninig 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT varialev 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT vazp 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT venturaa 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT vescovid 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT vlachoudisv 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT vlastour 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT wallnera 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT woodspj 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT wrighttj 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications
AT zugecp 154gdneutroncapturecrosssectionmeasuredatthentoffacilityanditsastrophysicalimplications