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Amaducci S, Colonna N, Cosentino L, Cristallo S, Finocchiaro P, Krtička M, Massimi C, Mastromarco M, Mazzone A, Maugeri EA, Mengoni A, Roederer IU, Straniero O, Valenta S, Vescovi D, Aberle O, Alcayne V, Andrzejewski J, Audouin L, Babiano-Suarez V, Bacak M, Barbagallo M, Bennett S, Berthoumieux E, Billowes J, Bosnar D, Brown A, Busso M, Caamaño M, Caballero-Ontanaya L, Calviño F, Calviani M, Cano-Ott D, Casanovas A, Cerutti F, Chiaveri E, Cortés G, Cortés-Giraldo MA, Damone LA, Davies PJ, Diakaki M, Dietz M, Domingo-Pardo C, Dressler R, Ducasse Q, Dupont E, Durán I, Eleme Z, Fernández-Domínguez B, Ferrari A, Furman V, Göbel K, Garg R, Gawlik-Ramięga A, Gilardoni S, Gonçalves IF, González-Romero E, Guerrero C, Gunsing F, Harada H, Heinitz S, Heyse J, Jenkins DG, Junghans A, Käppeler F, Kadi Y, Kimura A, Knapová I, Kokkoris M, Kopatch Y, Kurtulgil D, Ladarescu I, Lederer-Woods C, Leeb H, Lerendegui-Marco J, Lonsdale SJ, Macina D, Manna A, Martínez T, Masi A, Mastinu P, Mendoza E, Michalopoulou V, Milazzo PM, Mingrone F, Moreno-Soto J, Musumarra A, Negret A, Nolte R, Ogállar F, Oprea A, Patronis N, Pavlik A, Perkowski J, Petrone C, Piersanti L, Pirovano E, Porras I, Praena J, Quesada JM, Ramos-Doval D, Rauscher T, Reifarth R, Rochman D, Rubbia C, Sabaté-Gilarte M, Saxena A, Schillebeeckx P, Schumann D, Sekhar A, Smith AG, Sosnin NV, Sprung P, Stamatopoulos A, Tagliente G, Tain JL, Tarifeño-Saldivia A, Tassan-Got L, Thomas T, Torres-Sánchez P, Tsinganis A, Ulrich J, Urlass S, Vannini G, Variale V, Vaz P, Ventura A, Vlachoudis V, Vlastou R, Wallner A, Woods PJ, Wright T, Žugec P. Measurement of the ^{140}Ce(n,γ) Cross Section at n_TOF and Its Astrophysical Implications for the Chemical Evolution of the Universe. Phys Rev Lett 2024; 132:122701. [PMID: 38579210 DOI: 10.1103/physrevlett.132.122701] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/30/2023] [Revised: 11/09/2023] [Accepted: 01/31/2024] [Indexed: 04/07/2024]
Abstract
^{140}Ce(n,γ) is a key reaction for slow neutron-capture (s-process) nucleosynthesis due to being a bottleneck in the reaction flow. For this reason, it was measured with high accuracy (uncertainty ≈5%) at the n_TOF facility, with an unprecedented combination of a high purity sample and low neutron-sensitivity detectors. The measured Maxwellian averaged cross section is up to 40% higher than previously accepted values. Stellar model calculations indicate a reduction around 20% of the s-process contribution to the Galactic cerium abundance and smaller sizeable differences for most of the heavier elements. No variations are found in the nucleosynthesis from massive stars.
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Affiliation(s)
- S Amaducci
- INFN Laboratori Nazionali del Sud, Catania, Italy
| | - N Colonna
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Italy
| | - L Cosentino
- INFN Laboratori Nazionali del Sud, Catania, Italy
| | - S Cristallo
- Istituto Nazionale di Astrofisica - Osservatorio Astronomico d'Abruzzo, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Italy
| | | | - M Krtička
- Charles University, Prague, Czech Republic
| | - C Massimi
- Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy
- Dipartimento di Fisica e Astronomia, Università di Bologna, Italy
| | - M Mastromarco
- European Organization for Nuclear Research (CERN), Switzerland
| | - A Mazzone
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Italy
- Consiglio Nazionale delle Ricerche, Bari, Italy
| | - E A Maugeri
- Paul Scherrer Institut (PSI), Villigen, Switzerland
| | - A Mengoni
- Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy
- Agenzia nazionale per le nuove tecnologie, l'energia e lo sviluppo economico sostenibile (ENEA), Italy
| | - I U Roederer
- Department of Physics, North Carolina State University, Raleigh, Norh Carolina 27695, USA
- Department of Astronomy, University of Michigan, Ann Arbor, Michigan 48109, USA
- Joint Institute for Nuclear Astrophysics-Center for the Evolution of the Elements (JINA-CEE), USA
| | - O Straniero
- Istituto Nazionale di Astrofisica - Osservatorio Astronomico d'Abruzzo, Italy
- INFN Sezione Napoli, Napoli, Italy
| | - S Valenta
- Charles University, Prague, Czech Republic
| | - D Vescovi
- Istituto Nazionale di Astrofisica - Osservatorio Astronomico d'Abruzzo, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Italy
| | - O Aberle
- European Organization for Nuclear Research (CERN), Switzerland
| | - V Alcayne
- Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Spain
| | | | - L Audouin
- Institut de Physique Nucléaire, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-Saclay, F-91406 Orsay Cedex, France
| | - V Babiano-Suarez
- Instituto de Física Corpuscular, CSIC - Universidad de Valencia, Spain
| | - M Bacak
- European Organization for Nuclear Research (CERN), Switzerland
- TU Wien, Atominstitut, Stadionallee 2, 1020 Wien, Austria
- CEA Irfu, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France
| | - M Barbagallo
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Italy
- European Organization for Nuclear Research (CERN), Switzerland
| | - S Bennett
- University of Manchester, United Kingdom
| | - E Berthoumieux
- CEA Irfu, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France
| | - J Billowes
- University of Manchester, United Kingdom
| | - D Bosnar
- Department of Physics, Faculty of Science, University of Zagreb, Zagreb, Croatia
| | - A Brown
- University of York, United Kingdom
| | - M Busso
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Italy
- Dipartimento di Fisica e Geologia, Università di Perugia, Italy
| | - M Caamaño
- IGFAE-Universidade de Santiago de Compostela, Spain
| | | | - F Calviño
- Universitat Politècnica de Catalunya, Spain
| | - M Calviani
- European Organization for Nuclear Research (CERN), Switzerland
| | - D Cano-Ott
- Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Spain
| | | | - F Cerutti
- European Organization for Nuclear Research (CERN), Switzerland
| | - E Chiaveri
- European Organization for Nuclear Research (CERN), Switzerland
- University of Manchester, United Kingdom
| | - G Cortés
- Universitat Politècnica de Catalunya, Spain
| | | | - L A Damone
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Italy
- Dipartimento Interateneo di Fisica, Università degli Studi di Bari, Italy
| | - P J Davies
- University of Manchester, United Kingdom
| | - M Diakaki
- European Organization for Nuclear Research (CERN), Switzerland
- National Technical University of Athens, Greece
| | - M Dietz
- School of Physics and Astronomy, University of Edinburgh, United Kingdom
| | - C Domingo-Pardo
- Instituto de Física Corpuscular, CSIC - Universidad de Valencia, Spain
| | - R Dressler
- Paul Scherrer Institut (PSI), Villigen, Switzerland
| | - Q Ducasse
- Physikalisch-Technische Bundesanstalt (PTB), Bundesallee 100, 38116 Braunschweig, Germany
| | - E Dupont
- CEA Irfu, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France
| | - I Durán
- IGFAE-Universidade de Santiago de Compostela, Spain
| | - Z Eleme
- University of Ioannina, Greece
| | | | - A Ferrari
- European Organization for Nuclear Research (CERN), Switzerland
| | - V Furman
- Affiliated with an institute or an international laboratory covered by a cooperation agreement with CERN
| | - K Göbel
- Goethe University Frankfurt, Germany
| | - R Garg
- School of Physics and Astronomy, University of Edinburgh, United Kingdom
| | | | - S Gilardoni
- European Organization for Nuclear Research (CERN), Switzerland
| | | | - E González-Romero
- Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Spain
| | | | - F Gunsing
- CEA Irfu, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France
| | - H Harada
- Japan Atomic Energy Agency (JAEA), Tokai-Mura, Japan
| | - S Heinitz
- Paul Scherrer Institut (PSI), Villigen, Switzerland
| | - J Heyse
- European Commission, Joint Research Centre (JRC), Geel, Belgium
| | | | - A Junghans
- Helmholtz-Zentrum Dresden-Rossendorf, Germany
| | - F Käppeler
- Karlsruhe Institute of Technology, Campus North, IKP, 76021 Karlsruhe, Germany
| | - Y Kadi
- European Organization for Nuclear Research (CERN), Switzerland
| | - A Kimura
- Japan Atomic Energy Agency (JAEA), Tokai-Mura, Japan
| | - I Knapová
- Charles University, Prague, Czech Republic
| | - M Kokkoris
- National Technical University of Athens, Greece
| | - Y Kopatch
- Affiliated with an institute or an international laboratory covered by a cooperation agreement with CERN
| | | | - I Ladarescu
- Instituto de Física Corpuscular, CSIC - Universidad de Valencia, Spain
| | - C Lederer-Woods
- School of Physics and Astronomy, University of Edinburgh, United Kingdom
| | - H Leeb
- TU Wien, Atominstitut, Stadionallee 2, 1020 Wien, Austria
| | | | - S J Lonsdale
- School of Physics and Astronomy, University of Edinburgh, United Kingdom
| | - D Macina
- European Organization for Nuclear Research (CERN), Switzerland
| | - A Manna
- Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy
- Dipartimento di Fisica e Astronomia, Università di Bologna, Italy
| | - T Martínez
- Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Spain
| | - A Masi
- European Organization for Nuclear Research (CERN), Switzerland
| | - P Mastinu
- INFN Laboratori Nazionali di Legnaro, Italy
| | - E Mendoza
- Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Spain
| | - V Michalopoulou
- European Organization for Nuclear Research (CERN), Switzerland
- National Technical University of Athens, Greece
| | - P M Milazzo
- Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Italy
| | - F Mingrone
- European Organization for Nuclear Research (CERN), Switzerland
| | - J Moreno-Soto
- CEA Irfu, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France
| | - A Musumarra
- Istituto Nazionale di Fisica Nucleare, Sezione di Catania, Italy
- Department of Physics and Astronomy, University of Catania, Italy
| | - A Negret
- Horia Hulubei National Institute of Physics and Nuclear Engineering, Romania
| | - R Nolte
- Physikalisch-Technische Bundesanstalt (PTB), Bundesallee 100, 38116 Braunschweig, Germany
| | | | - A Oprea
- Horia Hulubei National Institute of Physics and Nuclear Engineering, Romania
| | | | - A Pavlik
- University of Vienna, Faculty of Physics, Vienna, Austria
| | | | - C Petrone
- Horia Hulubei National Institute of Physics and Nuclear Engineering, Romania
| | - L Piersanti
- Istituto Nazionale di Astrofisica - Osservatorio Astronomico d'Abruzzo, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Italy
| | - E Pirovano
- Physikalisch-Technische Bundesanstalt (PTB), Bundesallee 100, 38116 Braunschweig, Germany
| | | | | | | | - D Ramos-Doval
- Institut de Physique Nucléaire, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-Saclay, F-91406 Orsay Cedex, France
| | - T Rauscher
- Department of Physics, University of Basel, Switzerland
- Centre for Astrophysics Research, University of Hertfordshire, United Kingdom
| | | | - D Rochman
- Paul Scherrer Institut (PSI), Villigen, Switzerland
| | - C Rubbia
- European Organization for Nuclear Research (CERN), Switzerland
| | - M Sabaté-Gilarte
- European Organization for Nuclear Research (CERN), Switzerland
- Universidad de Sevilla, Spain
| | - A Saxena
- Bhabha Atomic Research Centre (BARC), India
| | - P Schillebeeckx
- European Commission, Joint Research Centre (JRC), Geel, Belgium
| | - D Schumann
- Paul Scherrer Institut (PSI), Villigen, Switzerland
| | - A Sekhar
- University of Manchester, United Kingdom
| | - A G Smith
- University of Manchester, United Kingdom
| | - N V Sosnin
- University of Manchester, United Kingdom
| | - P Sprung
- Paul Scherrer Institut (PSI), Villigen, Switzerland
| | | | - G Tagliente
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Italy
| | - J L Tain
- Instituto de Física Corpuscular, CSIC - Universidad de Valencia, Spain
| | | | - L Tassan-Got
- European Organization for Nuclear Research (CERN), Switzerland
- Institut de Physique Nucléaire, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-Saclay, F-91406 Orsay Cedex, France
- National Technical University of Athens, Greece
| | - Th Thomas
- Goethe University Frankfurt, Germany
| | | | - A Tsinganis
- European Organization for Nuclear Research (CERN), Switzerland
| | - J Ulrich
- Paul Scherrer Institut (PSI), Villigen, Switzerland
| | - S Urlass
- European Organization for Nuclear Research (CERN), Switzerland
- Helmholtz-Zentrum Dresden-Rossendorf, Germany
| | - G Vannini
- Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy
- Dipartimento di Fisica e Astronomia, Università di Bologna, Italy
| | - V Variale
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Italy
| | - P Vaz
- Instituto Superior Técnico, Lisbon, Portugal
| | - A Ventura
- Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy
| | - V Vlachoudis
- European Organization for Nuclear Research (CERN), Switzerland
| | - R Vlastou
- National Technical University of Athens, Greece
| | - A Wallner
- Australian National University, Canberra, Australia
| | - P J Woods
- School of Physics and Astronomy, University of Edinburgh, United Kingdom
| | - T Wright
- University of Manchester, United Kingdom
| | - P Žugec
- Department of Physics, Faculty of Science, University of Zagreb, Zagreb, Croatia
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Babiano-Suarez V, Balibrea-Correa J, Caballero-Ontanaya L, Domingo-Pardo C, Ladarescu I, Lerendegui-Marco J, Tain JL, Calviño F, Casanovas A, Tarifeño-Saldivia A, Guerrero C, Aberle O, Alcayne V, Amaducci S, Andrzejewski J, Audouin L, Bacak M, Barbagallo M, Bennett S, Berthoumieux E, Billowes J, Bosnar D, Brown A, Busso M, Caamaño M, Calviani M, Cano-Ott D, Cerutti F, Chiaveri E, Colonna N, Cortés G, CortésGiraldo MA, Cosentino L, Cristallo S, Damone LA, Davies PJ, Diakaki M, Dietz M, Dressler R, Ducasse Q, Dupont E, Durán I, Eleme Z, Fernández-Domínguez B, Ferrari A, Finocchiaro P, Furman V, Göbel K, Garg R, Gawlik-Ramięga A, Gilardoni S, Gonçalves IF, González-Romero E, Gunsing F, Harada H, Heinitz S, Heyse J, Jenkins DG, Junghans A, Käppeler F, Kadi Y, Kimura A, Knapová I, Kokkoris M, Kopatch Y, Krtička M, Kurtulgil D, Lederer-Woods C, Leeb H, Lonsdale SJ, Macina D, Manna A, Martínez T, Masi A, Massimi C, Mastinu P, Mastromarco M, Maugeri EA, Mazzone A, Mendoza E, Mengoni A, Michalopoulou V, Milazzo PM, Mingrone F, Moreno-Soto J, Musumarra A, Negret A, Nolte R, Ogállar F, Oprea A, Patronis N, Pavlik A, Perkowski J, Persanti L, Petrone C, Pirovano E, Porras I, Praena J, Quesada JM, Ramos-Doval D, Rauscher T, Reifarth R, Rochman D, Romanets Y, Rubbia C, Sabaté-Gilarte M, Saxena A, Schillebeeckx P, Schumann D, Sekhar A, Smith AG, Sosnin NV, Sprung P, Stamatopoulos A, Tagliente G, Tassan-Got L, Thomas T, 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, Wright T, Žugec P. First 80Se(n, γ) cross section measurement with high resolution in the full stellar energy range 1 eV - 100 keV and its astrophysical implications for the s-process. EPJ Web Conf 2022. [DOI: 10.1051/epjconf/202226011026] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
Most elements heavier than iron have been generated in the stellar media by means of neutron capture reactions, approximately half are produced by the slow neutron capture or s-process. Radiative neutron capture cross section measurements are of fundamental importance for the study of this mechanism. In this contribution we present a brief summary on the measurement and results for the 80Se(n,γ) cross-section. The experiment was carried out at CERN n_TOF EAR1 via the time of flight (ToF) technique, using four C6D6 scintillation detectors with very fast response. More than a hundred new resonances have been analyzed for the first time with a high accuracy. The MACS obtained at kT = 8 keV is 36% smaller than the recommended value in KADo-NiS. Some of the astrophysical implications of this result are elucidated in this contribution.
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3
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Guerrero C, Lerendegui-Marco J, Paul M, Tessler M, Heinitz S, Domingo-Pardo C, Cristallo S, Dressler R, Halfon S, Kivel N, Köster U, Maugeri EA, Palchan-Hazan T, Quesada JM, Rochman D, Schumann D, Weissman L, Aberle O, Amaducci S, Andrzejewski J, Audouin L, Bécares V, Bacak M, Balibrea J, Barak A, Barbagallo M, Barros S, Bečvář F, Beinrucker C, Berkovits D, Berthoumieux E, Billowes J, Bosnar D, Brugger M, Buzaglo Y, Caamaño M, Calviño F, Calviani M, Cano-Ott D, Cardella R, Casanovas A, Castelluccio DM, Cerutti F, Chen YH, Chiaveri E, Colonna N, Cortés G, Cortés-Giraldo MA, Cosentino L, Dafna H, Damone A, Diakaki M, Dietz M, Dupont E, Durán I, Eisen Y, Fernández-Domínguez B, Ferrari A, Ferreira P, Finocchiaro P, Furman V, Göbel K, García AR, Gawlik A, Glodariu T, Gonçalves IF, González-Romero E, Goverdovski A, Griesmayer E, Gunsing F, Harada H, Heftrich T, Heyse J, Hirsh T, Jenkins DG, Jericha E, Käppeler F, Kadi Y, Kaizer B, Katabuchi T, Kavrigin P, Ketlerov V, Khryachkov V, Kijel D, Kimura A, Kokkoris M, Kriesel A, Krtička M, Leal-Cidoncha E, Lederer-Woods C, Leeb H, Lo Meo S, Lonsdale SJ, Losito R, Macina D, Manna A, Marganiec J, Martínez T, Massimi C, Mastinu P, Mastromarco M, Matteucci F, Mendoza E, Mengoni A, Milazzo PM, Millán-Callado MA, Mingrone F, Mirea M, Montesano S, Musumarra A, Nolte R, Oprea A, Patronis N, Pavlik A, Perkowski J, Piersanti L, Porras I, Praena J, Rajeev K, Rauscher T, Reifarth R, Rodríguez-González T, Rout PC, Rubbia C, Ryan JA, Sabaté-Gilarte M, Saxena A, Schillebeeckx P, Schmidt S, Shor A, Sedyshev P, Smith AG, Stamatopoulos A, Tagliente G, Tain JL, Tarifeño-Saldivia A, Tassan-Got L, Tsinganis A, Valenta S, Vannini G, Variale V, Vaz P, Ventura A, Vlachoudis V, Vlastou R, Wallner A, Warren S, Weigand M, Weiss C, Wolf C, Woods PJ, Wright T, Žugec P. Neutron Capture on the s-Process Branching Point ^{171}Tm via Time-of-Flight and Activation. Phys Rev Lett 2020; 125:142701. [PMID: 33064503 DOI: 10.1103/physrevlett.125.142701] [Citation(s) in RCA: 6] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/29/2017] [Revised: 07/02/2020] [Accepted: 07/29/2020] [Indexed: 06/11/2023]
Abstract
The neutron capture cross sections of several unstable nuclides acting as branching points in the s process are crucial for stellar nucleosynthesis studies. The unstable ^{171}Tm (t_{1/2}=1.92 yr) is part of the branching around mass A∼170 but its neutron capture cross section as a function of the neutron energy is not known to date. In this work, following the production for the first time of more than 5 mg of ^{171}Tm at the high-flux reactor Institut Laue-Langevin in France, a sample was produced at the Paul Scherrer Institute in Switzerland. Two complementary experiments were carried out at the neutron time-of-flight facility (n_TOF) at CERN in Switzerland and at the SARAF liquid lithium target facility at Soreq Nuclear Research Center in Israel by time of flight and activation, respectively. The result of the time-of-flight experiment consists of the first ever set of resonance parameters and the corresponding average resonance parameters, allowing us to make an estimation of the Maxwellian-averaged cross sections (MACS) by extrapolation. The activation measurement provides a direct and more precise measurement of the MACS at 30 keV: 384(40) mb, with which the estimation from the n_TOF data agree at the limit of 1 standard deviation. This value is 2.6 times lower than the JEFF-3.3 and ENDF/B-VIII evaluations, 25% lower than that of the Bao et al. compilation, and 1.6 times larger than the value recommended in the KADoNiS (v1) database, based on the only previous experiment. Our result affects the nucleosynthesis at the A∼170 branching, namely, the ^{171}Yb abundance increases in the material lost by asymptotic giant branch stars, providing a better match to the available pre-solar SiC grain measurements compared to the calculations based on the current JEFF-3.3 model-based evaluation.
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Affiliation(s)
- C Guerrero
- Universidad de Sevilla, Seville, Spain
- Centro Nacional de Aceleradores (CNA) (Universidad de Sevilla-Junta de Andalucía-CSIC), Seville, Spain
| | | | - M Paul
- Hebrew University, Jerusalem, Israel
| | - M Tessler
- Soreq Nuclear Research Center (SNRC), Yavne, Israel
| | - S Heinitz
- Paul Scherrer Institut (PSI), Villigen, Switzerland
| | - C Domingo-Pardo
- Instituto de Física Corpuscular (CSIC-University of Valencia), Valencia, Spain
| | - S Cristallo
- INAF-Osservatorio Astronomico d'Abruzzo, Teramo, Italy
- INFN Sezione Perugia, Perugia, Italy
| | - R Dressler
- Paul Scherrer Institut (PSI), Villigen, Switzerland
| | - S Halfon
- Soreq Nuclear Research Center (SNRC), Yavne, Israel
| | - N Kivel
- Paul Scherrer Institut (PSI), Villigen, Switzerland
| | - U Köster
- Institut Laue-Langevin ILL, Grenoble, France
| | - E A Maugeri
- Paul Scherrer Institut (PSI), Villigen, Switzerland
| | | | | | - D Rochman
- Paul Scherrer Institut (PSI), Villigen, Switzerland
| | - D Schumann
- Paul Scherrer Institut (PSI), Villigen, Switzerland
| | - L Weissman
- Soreq Nuclear Research Center (SNRC), Yavne, Israel
| | - O Aberle
- European Organization for Nuclear Research (CERN), Geneva, Switzerland
| | - S Amaducci
- INFN Laboratori Nazionali del Sud, Catania, Italy
| | | | - L Audouin
- Institut de Physique Nucléaire, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-Saclay, Orsay Cedex, France
| | - V Bécares
- Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - M Bacak
- Technische Universität Wien, Vienna, Austria
| | - J Balibrea
- Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - A Barak
- Soreq Nuclear Research Center (SNRC), Yavne, Israel
| | - M Barbagallo
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Italy
| | - S Barros
- Instituto Superior Técnico, Lisbon, Portugal
| | - F Bečvář
- Charles University, Prague, Czech Republic
| | | | - D Berkovits
- Soreq Nuclear Research Center (SNRC), Yavne, Israel
| | - E Berthoumieux
- CEA Irfu, Université Paris-Saclay, Gif-sur-Yvette, France
| | - J Billowes
- University of Manchester, Manchester, United Kingdom
| | - D Bosnar
- Department of Physics, Faculty of Science, University of Zagreb, Zagreb, Croatia
| | - M Brugger
- European Organization for Nuclear Research (CERN), Geneva, Switzerland
| | - Y Buzaglo
- Soreq Nuclear Research Center (SNRC), Yavne, Israel
| | - M Caamaño
- University of Santiago de Compostela, Santiago de Conpostela, Spain
| | - F Calviño
- Universitat Politècnica de Catalunya, Barcelona, Spain
| | - M Calviani
- European Organization for Nuclear Research (CERN), Geneva, Switzerland
| | - D Cano-Ott
- Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - R Cardella
- European Organization for Nuclear Research (CERN), Geneva, Switzerland
| | - A Casanovas
- Universitat Politècnica de Catalunya, Barcelona, Spain
| | - D M Castelluccio
- Agenzia nazionale per le nuove tecnologie (ENEA), Bologna, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy
| | - F Cerutti
- European Organization for Nuclear Research (CERN), Geneva, Switzerland
| | - Y H Chen
- Institut de Physique Nucléaire, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-Saclay, Orsay Cedex, France
| | - E Chiaveri
- European Organization for Nuclear Research (CERN), Geneva, Switzerland
| | - N Colonna
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Italy
| | - G Cortés
- Universitat Politècnica de Catalunya, Barcelona, Spain
| | | | - L Cosentino
- INFN Laboratori Nazionali del Sud, Catania, Italy
| | - H Dafna
- Soreq Nuclear Research Center (SNRC), Yavne, Israel
| | - A Damone
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Italy
- Dipartimento di Fisica, Università degli Studi di Bari, Bari, Italy
| | - M Diakaki
- CEA Irfu, Université Paris-Saclay, Gif-sur-Yvette, France
| | - M Dietz
- School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom
| | - E Dupont
- CEA Irfu, Université Paris-Saclay, Gif-sur-Yvette, France
| | - I Durán
- University of Santiago de Compostela, Santiago de Conpostela, Spain
| | - Y Eisen
- Soreq Nuclear Research Center (SNRC), Yavne, Israel
| | | | - A Ferrari
- European Organization for Nuclear Research (CERN), Geneva, Switzerland
| | - P Ferreira
- Instituto Superior Técnico, Lisbon, Portugal
| | | | - V Furman
- Joint Institute for Nuclear Research (JINR), Dubna, Russia
| | - K Göbel
- Goethe University Frankfurt, Seville, Germany
| | - A R García
- Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - A Gawlik
- Soreq Nuclear Research Center (SNRC), Yavne, Israel
| | - T Glodariu
- Horia Hulubei National Institute of Physics and Nuclear Engineering, Jerusalem, Romania
| | | | - E González-Romero
- Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - A Goverdovski
- Institute of Physics and Power Engineering (IPPE), Obninsk, Russia
| | | | - F Gunsing
- Institut Laue-Langevin ILL, Grenoble, France
- CEA Irfu, Université Paris-Saclay, Gif-sur-Yvette, France
| | - H Harada
- Japan Atomic Energy Agency (JAEA), Tokai-mura, Japan
| | - T Heftrich
- Goethe University Frankfurt, Seville, Germany
| | - J Heyse
- Universitat Politècnica de Catalunya, Barcelona, Spain
- Physikalisch-Technische Bundesanstalt (PTB), Braunschweig, Germany
| | - T Hirsh
- Soreq Nuclear Research Center (SNRC), Yavne, Israel
| | | | - E Jericha
- Technische Universität Wien, Vienna, Austria
| | - F Käppeler
- Karlsruhe Institute of Technology (KIT), Karlsruhe, Germany
| | - Y Kadi
- European Organization for Nuclear Research (CERN), Geneva, Switzerland
| | - B Kaizer
- Soreq Nuclear Research Center (SNRC), Yavne, Israel
| | | | - P Kavrigin
- Technische Universität Wien, Vienna, Austria
| | - V Ketlerov
- Institute of Physics and Power Engineering (IPPE), Obninsk, Russia
| | - V Khryachkov
- Institute of Physics and Power Engineering (IPPE), Obninsk, Russia
| | - D Kijel
- Soreq Nuclear Research Center (SNRC), Yavne, Israel
| | - A Kimura
- Japan Atomic Energy Agency (JAEA), Tokai-mura, Japan
| | - M Kokkoris
- National Technical University of Athens, Athens, Greece
| | - A Kriesel
- Soreq Nuclear Research Center (SNRC), Yavne, Israel
| | - M Krtička
- Charles University, Prague, Czech Republic
| | - E Leal-Cidoncha
- University of Santiago de Compostela, Santiago de Conpostela, Spain
| | - C Lederer-Woods
- School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom
| | - H Leeb
- Technische Universität Wien, Vienna, Austria
| | - S Lo Meo
- Agenzia nazionale per le nuove tecnologie (ENEA), Bologna, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy
| | - S J Lonsdale
- School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom
| | - R Losito
- European Organization for Nuclear Research (CERN), Geneva, Switzerland
| | - D Macina
- European Organization for Nuclear Research (CERN), Geneva, Switzerland
| | - A Manna
- Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy
- Dipartimento di Fisica e Astronomia, Università di Bologna, Bologna, Italy
| | | | - T Martínez
- Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - C Massimi
- Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy
- Dipartimento di Fisica e Astronomia, Università di Bologna, Bologna, Italy
| | - P Mastinu
- Istituto Nazionale di Fisica Nucleare, Sezione di Legnaro, Italy
| | - M Mastromarco
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Italy
| | - F Matteucci
- Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Italy
- Dipartimento di Astronomia, Università di Trieste, Trieste, Italy
| | - E Mendoza
- Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - A Mengoni
- Agenzia nazionale per le nuove tecnologie (ENEA), Bologna, Italy
| | - P M Milazzo
- Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Italy
| | - M A Millán-Callado
- Institut de Physique Nucléaire, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-Saclay, Orsay Cedex, France
| | - F Mingrone
- Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy
| | - M Mirea
- Horia Hulubei National Institute of Physics and Nuclear Engineering, Jerusalem, Romania
| | - S Montesano
- European Organization for Nuclear Research (CERN), Geneva, Switzerland
| | - A Musumarra
- INFN Laboratori Nazionali del Sud, Catania, Italy
- Dipartimento di Fisica e Astronomia, Università di Catania, Catania, Italy
| | - R Nolte
- Physikalisch-Technische Bundesanstalt (PTB), Braunschweig, Germany
| | - A Oprea
- Horia Hulubei National Institute of Physics and Nuclear Engineering, Jerusalem, Romania
| | - N Patronis
- University of Ioannina, Ioannina, Greece
| | - A Pavlik
- University of Vienna, Faculty of Physics, Vienna, Austria
| | | | - L Piersanti
- INAF-Osservatorio Astronomico d'Abruzzo, Teramo, Italy
| | - I Porras
- University of Granada, Granada, Spain
| | - J Praena
- Universidad de Sevilla, Seville, Spain
- University of Granada, Granada, Spain
| | - K Rajeev
- Bhabha Atomic Research Centre (BARC), Mumbai, India
| | - T Rauscher
- Centre for Astrophysics Research, University of Hertfordshire, Hatfield, United Kingdom
- Department of Physics, University of Basel, Basel, Switzerland
| | - R Reifarth
- Goethe University Frankfurt, Seville, Germany
| | - T Rodríguez-González
- Universidad de Sevilla, Seville, Spain
- Centro Nacional de Aceleradores (CNA) (Universidad de Sevilla-Junta de Andalucía-CSIC), Seville, Spain
| | - P C Rout
- Bhabha Atomic Research Centre (BARC), Mumbai, India
| | - C Rubbia
- European Organization for Nuclear Research (CERN), Geneva, Switzerland
| | - J A Ryan
- University of Manchester, Manchester, United Kingdom
| | - M Sabaté-Gilarte
- Universidad de Sevilla, Seville, Spain
- European Organization for Nuclear Research (CERN), Geneva, Switzerland
| | - A Saxena
- Bhabha Atomic Research Centre (BARC), Mumbai, India
| | | | - S Schmidt
- Goethe University Frankfurt, Seville, Germany
| | - A Shor
- Soreq Nuclear Research Center (SNRC), Yavne, Israel
| | - P Sedyshev
- Joint Institute for Nuclear Research (JINR), Dubna, Russia
| | - A G Smith
- University of Manchester, Manchester, United Kingdom
| | | | - G Tagliente
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Italy
| | - J L Tain
- Instituto de Física Corpuscular (CSIC-University of Valencia), Valencia, Spain
| | | | - L Tassan-Got
- Institut de Physique Nucléaire, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-Saclay, Orsay Cedex, France
| | - A Tsinganis
- National Technical University of Athens, Athens, Greece
| | - S Valenta
- Charles University, Prague, Czech Republic
| | - G Vannini
- Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy
- Dipartimento di Fisica e Astronomia, Università di Bologna, Bologna, Italy
| | - V Variale
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Italy
| | - P Vaz
- Instituto Superior Técnico, Lisbon, Portugal
| | - A Ventura
- Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy
| | - V Vlachoudis
- European Organization for Nuclear Research (CERN), Geneva, Switzerland
| | - R Vlastou
- National Technical University of Athens, Athens, Greece
| | - A Wallner
- Australian National University, Canberra, Australia
| | - S Warren
- University of Manchester, Manchester, United Kingdom
| | - M Weigand
- Goethe University Frankfurt, Seville, Germany
| | - C Weiss
- European Organization for Nuclear Research (CERN), Geneva, Switzerland
- Technische Universität Wien, Vienna, Austria
| | - C Wolf
- Goethe University Frankfurt, Seville, Germany
| | - P J Woods
- School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom
| | - T Wright
- University of Manchester, Manchester, United Kingdom
| | - P Žugec
- European Organization for Nuclear Research (CERN), Geneva, Switzerland
- Department of Physics, Faculty of Science, University of Zagreb, Zagreb, Croatia
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4
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Manna A, Aberle O, Alcayne V, Amaducci S, Andrzejewski J, Audouin L, Babiano VS, Bacak M, Barbagallo M, Bennett S, Berthoumieux E, Bosnar D, Brown AS, Busso M, Caamaño M, Caballero L, Calviani M, Calvi F, Cano-Ott D, Casanovas A, Cerutti F, Chiaveri E, Colonna N, Cortés GP, Cortés-Giraldo MA, Coséntino L, Cristallo S, Damone LA, Davies PJ, Diakaki M, Dietz M, Domingo-Pardo C, Dressler R, Ducasse Q, Dupont E, Durán I, Eleme Z, Fernández-Domíngez B, Ferrari A, Ferro-Goncalves 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 DG, Jericha E, Jiri U, Junghans A, Kadi Y, Käppeler F, Kimura A, Knapová I, Kokkoris M, Kopatch Y, Krtiička M, Kurtulgil D, Ladarescu I, Lederer-Woods C, Lerendegui-Marco J, Lonsdale SJ, Macina D, Martínez T, Masi A, Massimi C, Mastinu PF, Mastromarco M, Maugeri E, Mazzone A, Mendoza E, Mengoni A, Michalopoulou V, Milazzo PM, Millán-Callado MA, Mingrone F, Moreno-Soto J, Musumarra A, Negret A, Nolte R, Ogállar F, Oprea A, Patronis N, Pavlik A, Perkowski J, Petrone C, Piersanti L, Pirovano E, Porras I, Praena J, Quesada J, Ramos D, Reifarth R, Rochman D, Rubbia C, Sabaté-Gilarte M, Saxena A, Schillebeeckx P, Schumann D, Sekhar A, Smith A, Sosnin N, Sprung P, Stamatopoulos A, Tagliente G, Tain JL, Tarifeno-Saldivia AE, 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 PJ, Wright TJ, Žugec P. Setup for the measurement of the 235U(n, f) cross section relative to n-p scattering up to 1 GeV. EPJ Web Conf 2020. [DOI: 10.1051/epjconf/202023901008] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
The neutron induced fission of 235U is extensively used as a reference for neutron fluence measurements in various applications, ranging from the investigation of the biological effectiveness of high energy neutrons, to the measurement of high energy neutron cross sections of relevance for accelerator driven nuclear systems. Despite its widespread use, no data exist on neutron induced fission of 235U above 200 MeV. The neutron facility n_TOF offers the possibility to improve the situation. The measurement of 235U(n,f) relative to the differential n-p scattering cross-section, was carried out in September 2018 with the aim of providing accurate and precise cross section data in the energy range from 10 MeV up to 1 GeV. In such measurements, Recoil Proton Telescopes (RPTs) are used to measure the neutron flux while the fission events are detected and counted with dedicated detectors. In this paper the measurement campaign and the experimental set-up are illustrated.
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5
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Terranova 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 AS, Busso M, Caamaño M, Caballero L, Calviani M, Calviño F, Cano-Ott D, Casanovas A, Cerutti F, Chiaveri E, Colonna N, Cortés GP, Cortés-Giraldo MA, Cosentino L, Cristallo S, Damone LA, Davies PJ, 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 DG, 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 SJ, Macina D, Manna A, Martínez T, Masi A, Massimi C, Mastinu PF, Mastromarco M, Maugeri E, Mazzone A, Mendoza E, Mengoni A, Michalopoulou V, Milazzo PM, Millán-Callado MA, 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 JM, Doval DR, Reifarth R, Rochman D, Rubbia C, Sabaté-Gilarte M, Saxena A, Schillebeeckx P, Schumann D, Sekhar A, Smith AG, Sosnin N, Sprung P, Stamatopoulos A, Tagliente G, Tain JL, Tarifeño-Saldivia AE, 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 PJ, Wright TJ, Žugec P. Monte Carlo simulations and n-p differential scattering data measured with Proton Recoil Telescopes. EPJ Web Conf 2020. [DOI: 10.1051/epjconf/202023901024] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022] Open
Abstract
The neutron-induced fission cross section of 235U, a standard at thermal energy and between 0.15 MeV and 200 MeV, plays a crucial role in nuclear technology applications. The long-standing need of improving cross section data above 20 MeV and the lack of experimental data above 200 MeV motivated a new experimental campaign at the n_TOF facility at CERN. The measurement has been performed in 2018 at the experimental area 1 (EAR1), located at 185 m from the neutron-producing target (the experiment is presented by A. Manna et al. in a contribution to this conference). The 235U(n,f) cross section from 20 MeV up to about 1 GeV has been measured relative to the 1H(n,n)1H reaction, which is considered the primary reference in this energy region. The neutron flux impinging on the 235U sample (a key quantity for determining the fission events) has been obtained by detecting recoil protons originating from n-p scattering in a C2H4 sample. Two Proton Recoil Telescopes (PRT), consisting of several layers of solid-state detectors and fast plastic scintillators, have been located at proton scattering angles of 25.07° and 20.32°, out of the neutron beam. The PRTs exploit the ΔE-E technique for particle identification, a basic requirement for the rejection of charged particles from neutron-induced reactions in carbon. Extensive Monte Carlo simulations were performed to characterize proton transport through the different slabs of silicon and scintillation detectors, to optimize the experimental set-up and to deduce the efficiency of the whole PRT detector. In this work we compare measured data collected with the PRTs with a full Monte Carlo simulation based on the Geant-4 toolkit.
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6
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Barbagallo M, Aberle O, Alcayne V, Amaducci S, Andrzejewski J, Audouin L, Babiano-Suarez V, Bacak M, Bennett S, Berthoumieux E, Bosnar D, Brown AS, Busso M, Caamaño M, Caballero L, Calviani M, Calviño F, Cano-Ott D, Casanovas A, Cerutti F, Chiaveri E, Colonna N, Cortés GP, Cortés-Giraldo MA, Cosentino L, Cristallo S, Damone LA, Davies PJ, 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 DG, 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 SJ, Macina D, Manna A, Martínez T, Masi A, Massimi C, Mastinu PF, Mastromarco M, Maugeri E, Mazzone A, Mendoza E, Mengoni A, Michalopoulou V, Milazzo PM, Millán-Callado MA, 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 JM, Ramos Doval D, Reifarth R, Rochman D, Rubbia C, Sabaté- Gilarte M, Saxena A, Schillebeeckx P, Schumann D, Sekhar A, Smith AG, Sosnin N, Sprung P, Stamatopoulos A, Tagliente G, Tain JL, Tarifeño-Saldivia AE, 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 PJ, Wright TJ, Žugec P. Measurement of the energy-differential cross-section of the 12C(n,p) 12B and 12C(n,d) 11B reactions at the n_TOF facility at CERN. EPJ Web Conf 2020. [DOI: 10.1051/epjconf/202023901045] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
Although the 12C(n,p)12B and 12C(n,d)11B reactions are of interest in several fields of basic and applied Nuclear Physics the present knowledge of these two cross-sections is far from being accurate and reliable, with both evaluations and data showing sizable discrepancies. As part of the challenging n_TOF program on (n,cp) nuclear reactions study, the energy differential cross-sections of the 12C(n,p)12B and 12C(n,d)11 B reactions have been measured at CERN from the reaction thresholds up to 30 MeV neutron energy. Both measurements have been recently performed at the long flight-path (185 m) experimental area of the n_TOF facility at CERN using a pure (99.95%) rigid graphite target and two silicon telescopes. In this paper an overview of the experiment is presented together with a few preliminary results.
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7
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Chiaveri E, 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, Busso M, Caamaño M, Caballero L, Calviani M, Calviño F, Cano-Ott D, Casanovas A, Cerutti F, Colonna N, Cortés G, Cortés-Giraldo M, Cosentino L, Cristallo S, Damone L, Davies P, 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, 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 SJ, Macina D, Manna A, Martínez T, Masi A, Massimi C, Mastinu P, Mastromarco M, Maugeri E, Mazzone A, Mendoza E, Mengoni A, Michalopoulou V, Milazzo P, Millán-Callado M, 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, Ramos Doval D, Reifarth R, Rochman D, Rubbia C, Sabaté-Gilarte M, Saxena A, Schillebeeckx P, Schumann D, Sekhar A, Smith A, Sosnin N, Sprung P, Stamatopoulos A, Tagliente G, Tain J, Tarifeño-Saldivia A, 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, Wright T, Žugec P. Status and perspectives of the neutron time-of-flight facility n_TOF at CERN. EPJ Web Conf 2020. [DOI: 10.1051/epjconf/202023917001] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
Since the start of its operation in 2001, based on an idea of Prof. Carlo Rubbia [1], the neutron time of-flight facility of CERN, n_TOF, has become one of the most forefront neutron facilities in the world for wide-energy spectrum neutron cross section measurements. Thanks to the combination of excellent neutron energy resolution and high instantaneous neutron flux available in the two experimental areas, the second of which has been constructed in 2014, n_TOF is providing a wealth of new data on neutron-induced reactions of interest for nuclear astrophysics, advanced nuclear technologies and medical applications. The unique features of the facility will continue to be exploited in the future, to perform challenging new measurements addressing the still open issues and long-standing quests in the field of neutron physics. In this document the main characteristics of the n_TOF facility and their relevance for neutron studies in the different areas of research will be outlined, addressing the possible future contribution of n_TOF in the fields of nuclear astrophysics, nuclear technologies and medical applications. In addition, the future perspectives of the facility will be described including the upgrade of the spallation target, the setup of an imaging installation and the construction of a new irradiation area.
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8
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Oprea A, Gunsing F, Schillebeeckx P, Aberle O, Bacak M, Berthoumieux E, Cano-Ott D, Diakaki M, Dupont E, Geslot B, Glodariu T, Heyse J, Mendoza E, Negret A, Alcayne V, Amaducci S, Andrzejewski J, Audouin L, Bécares V, Babiano-Suarez V, Barbagallo M, Becčvář F, Bellia G, Billowes J, Bosnar D, Brown A, Busso M, Caamaño M, Caballero-Ontanaya L, Calviño F, Calviani M, Casanovas A, Cerutti F, Chen YH, Chiaveri E, Colonna N, Cortés G, Cortés-Giraldo MA, Cosentino L, Cristallo S, Damone LA, Dietz M, Domingo-Pardo C, Dressler R, Durán I, Eleme Z, Femández-Domínguez B, Ferrari A, Finocchiaro P, Furman V, Göbel K, Garg R, Gawlik A, Gilardoni S, Goncalves IF, González-Romero E, Guerrero C, Harada H, Heinitz S, Jenkins DG, Jericha E, Käppeler F, Kadi Y, Kimura A, Kivel N, Kokkoris M, Kopatch Y, Krtička M, Kurtulgil D, Ladarescu I, Lederer-Woods C, Lerendegui-Marco J, Meo SL, Lonsdale SJ, Macina D, Manna A, Martínez T, Masi A, Massimi C, Mastinu P, Mastromarco M, Matteucci F, Maugeri EA, Mazzone A, Mengoni A, Michalopoulou V, Milazzo PM, Mingrone F, Musumarra A, Nolte R, Ogállar F, Patronis N, Pavlik A, Perkowski J, Persanti L, Porras I, Praena J, Quesada JM, Radeck D, Ramos-Doval D, Reifarth R, Rochman D, Rubbia C, Sabaté-Gilarte M, Saxena A, Schumann D, Smith AG, Sosnin NV, Stamatopoulos A, Tagliente G, Tain JL, Talip T, Tarifeño-Saldivia A, Tassan-Got L, Torres-Sánchez P, Tsinganis A, Ulrich J, Urlass S, Valenta S, Vannini G, Variale V, Vaz P, Ventura A, Vlachoudis V, Vlastou R, Wallner A, Woods PJ, Wright T, Žugec P. Neutron capture cross section measurements of 241Am at the n_TOF facility. EPJ Web Conf 2020. [DOI: 10.1051/epjconf/202023901009] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022] Open
Abstract
Neutron capture on 241Am plays an important role in the nuclear energy production and also provides valuable information for the improvement of nuclear models and the statistical interpretation of the nuclear properties. A new experiment to measure the 241Am(n, γ) cross section in the thermal region and the first few resonances below 10 eV has been carried out at EAR2 of the n_TOF facility at CERN. Three neutron-insensitive C6D6 detectors have been used to measure the neutron-capture gamma cascade as a function of the neutron time of flight, and then deduce the neutron capture yield. Preliminary results will be presented and compared with previously obtained results at the same facility in EAR1. In EAR1 the gamma-ray background at thermal energies was about 90% of the signal while in EAR2 is up to a 25 factor much more favorable signal to noise ratio. We also extended the low energy limit down to subthermal energies. This measurement will allow a comparison with neutron capture measurements conducted at reactors and using a different experimental technique.
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Mendoza E, Alcayne V, Cano-Ott D, Kimura A, Skarbeli AV, Aberle O, 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, Casanovas A, Cerutti F, Chen YH, Chiaveri E, Colonna N, Cortés GP, Cortés-Giraldo MA, Cosentino L, Cristallo S, 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, Kivel N, Kokkoris M, Kopatch Y, Krtička M, Kurtulgil D, Ladarescu I, Lederer-Woods C, Lerendegui-Marco J, Meo SL, Lonsdale SJ, Macina D, Manna A, Martínez T, Masi A, Massimi C, Mastinu PF, Mastromarco M, Matteucci F, Maugeri E, Mazzone A, Mengoni A, Michalopoulou V, Milazzo PM, Mingrone F, 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, Doval DR, 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, Vlachoudis V, Vlastou R, Wallner A, Woods PJ, Wright TJ, Žugec P. Study of photon strength functions of 241Pu and 245Cm from neutron capture measurements. EPJ Web Conf 2020. [DOI: 10.1051/epjconf/202023901015] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
We have measured theγ-rays following neutron capture on240Pu and244Cm at the n_TOF facility at CERN with the Total Absorption Calorimeter (TAC) and with C6D6 organic scintillators. The TAC is made of 40 BaF2 crystals operating in coincidence and covering almost the entire solid angle. This allows to obtain information concerning the energy spectra and the multiplicity of the measured captureγ-ray cascades. Additional information is also obtained from the C6D6 detectors. We have analyzed the measured data in order to draw conclusions about the Photon Strength Functions (PSFs) of241Pu and245Cm below their neutron separation energies. The analysis has been performed by fitting the PSFs to the experimental results, using the differential evolution method, in order to find neutron capture cascades capable of reproducing at the same time a great variety of deposited energy spectra.
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Amaducci S, 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-Girardo 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, Gawlik A, Gilardoni S, Glodariu T, Gonçalves IF, González-Romero E, Griesmayer E, Guerrero C, Gunsing F, Harada H, Heinitz S, Heyse J, Jenkins DG, Jericha E, Käppeler F, Kadi Y, Kalamara A, Kavrigin P, Kimura A, Kivel N, Knapova I, Kokkoris M, Krtička M, Kurtulgil D, Leal-Cidoncha E, Lederer C, Leeb H, Lerendegui-Marco J, Lo Meo S, Lonsdale SJ, Macina D, Manna A, Marganiec J, Martínez T, Masi A, Massimi C, Mastinu P, Mastromarco M, Maugeri EA, Mazzone A, Mendoza E, Mengoni A, Milazzo PM, Mingrone F, Musumarra A, Negret A, Nolte R, Oprea A, Patronis N, Pavlik A, Perkowski J, Porras I, Praena J, Quesada JM, Radeck D, Rauscher T, Reifarth R, Rubbia C, Ryan JA, Sabaté-Gilarte M, Saxena A, Schillebeeckx P, Schumann D, Sedyshev P, Smith AG, Sosnin NV, Stamatopoulos A, Tagliente G, Tain JL, 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, Woods PJ, Wright T, Žugec P. Accurate measurement of the standard 235U(n,f) cross section from thermal to 170 keV neutron energy. EPJ Web Conf 2020. [DOI: 10.1051/epjconf/202023908002] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
An accurate measurement of the 235U(n,f) cross section from thermal to 170 keV of neutron energy has recently been performed at n_TOF facility at CERN using 6Li(n,t)4He and 10B(n,α)7Li as references. This measurement has been carried out in order to investigate a possible overestimation of the 235U fission cross section evaluation provided by most recent libraries between 10 and 30 keV. A custom experimental apparatus based on in-beam silicon detectors has been used, and a Monte Carlo simulation in GEANT4 has been employed to characterize the setup and calculate detectors efficiency. The results evidenced the presence of an overestimation in the interval between 9 and 18 keV and the new data may be used to decrease the uncertainty of 235U(n,f) cross section in the keV region.
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Michalopoulou V, Stamatopoulos A, Vlastou R, Kokkoris M, Tsinganis A, Diakaki M, Eleme Z, Patronis N, Heyse J, Schillebeeckx P, Tassan-Got L, Barbagallo M, Colonna N, Urlass S, Macina D, Chiaveri E, Aberle O, Alcayne V, Amaducci S, Andrzejewski J, Audouin L, Babiano-Suarez V, Bacak M, Bennett S, Berthoumieux E, Bosnar D, Brown AS, Busso M, Caamaño M, Caballero L, Calviani M, Calviño F, Cano-Ott D, Casanovas A, Cerutti F, Cortés GP, Cortés-Giraldo MA, Cosentino L, Cristallo S, Damone LA, Davies PJ, Dietz M, Domingo-Pardo C, Dressler R, Ducasse Q, Dupont E, Durán I, Femández-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, Jenkins DG, Jericha E, Jiri U, Junghans A, Kadi Y, Käppeler F, Kimura A, Knapová I, Kopatch Y, Krtiička M, Kurtulgil D, Ladarescu I, Lederer-Woods C, Lerendegui-Marco J, Lonsdale SJ, Manna A, Martínez T, Masi A, Massimi C, Mastinu PF, Mastromarco M, Maugeri E, Mazzone A, Mendoza E, Mengoni A, Milazzo PM, Millán-Callado MA, Mingrone F, Moreno-Soto J, Musumarra A, Negret A, Ogállar F, Oprea A, Pavlik A, Perkowski J, Petrone C, Piersanti L, Pirovano E, Porras I, Praena J, Quesada JM, Ramos Doval D, Reifarth R, Rochman D, Rubbia C, Sabaté-Gilarte M, Saxena A, Schumann D, Sekhar A, Smith AG, Sosnin N, Sprung P, Tagliente G, Tain JL, Tarifeño-Saldivia AE, Thomas B, Torres-Sánchez P, Valenta S, Vannini G, Variale V, Vaz P, Ventura A, Vescovi D, Vlachoudis V, Wallner A, Woods PJ, Wright TJ, Žugec P. First results of the 230Th(n,f) cross section measurements at the CERN n_TOF facility. EPJ Web Conf 2020. [DOI: 10.1051/epjconf/202023905004] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
The study of neutron-induced reactions on actinides is of considerable importance for the design of advanced nuclear systems and alternative fuel cycles. Specifically, 230Th is produced from the α-decay of 234U as a byproduct of the 232Th/233U fuel cycle, thus the accurate knowledge of its fission cross section is strongly required. However, few experimental datasets exist in literature with large deviations among them, covering the energy range between 0.2 to 25 MeV. In addition, the study of the 230Th(n,f) cross-section is of great interest in the research on the fission process related to the structure of the fission barriers. Previous measurements have revealed a large resonance at En=715 keV and additional fine structures, but with high discrepancies among the cross-section values of these measurements. This contribution presents preliminary results of the 230Th(n,f) cross-section measurements at the CERN n_TOF facility. The high purity targets of the natural, but very rare isotope 230Th, were produced at JRC-Geel in Belgium. The measurements were performed at both experimental areas (EAR-1 and EAR-2) of the n_TOF facility, covering a very broad energy range from thermal up to at least 100 MeV. The experimental setup was based on Micromegas detectors with the 235U(n,f) and 238U(n,f) reaction cross-sections used as reference.
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Mengoni A, Damone L, Barbagallo M, Aberle O, Alcayne V, Amaducci S, Andrzejewski J, Audouin L, Babiano-Suarez V, Bacak M, Bennett S, Berthoumieux E, Bosnar D, Brown A, Busso M, Caamaño M, Caballero L, Calviani M, Calviño F, Cano-Ott D, Casanovas A, Cerutti F, Chiaveri E, Colonna N, Cortés G, Cortés-Giraldo M, Cosentino L, Cristallo S, Davies P, 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, 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 SJ, Macina D, Manna A, Martínez T, Masi A, Massimi C, Mastinu P, Mastromarco M, Maugeri E, Mazzone A, Mendoza E, Michalopoulou V, Milazzo P, Millán-Callado M, 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, Doval DR, Reifarth R, Rochman D, Rubbia C, Sabaté-Gilarte M, Saxena A, Schillebeeckx P, Schumann D, Sekhar A, Smith A, Sosnin N, Sprung P, Stamatopoulos A, Tagliente G, Tain J, Tarifeño-Saldivia A, 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, Wright T, Žugec P. New reaction rates for the destruction of 7Be during big bang nucleosynthesis measured at CERN/n_TOF and their implications on the cosmological lithium problem. EPJ Web Conf 2020. [DOI: 10.1051/epjconf/202023907001] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
New measurements of the7Be(n,α)4He and7Be(n,p)7Li reaction cross sections from thermal to keV neutron energies have been recently performed at CERN/n_TOF. Based on the new experimental results, astrophysical reaction rates have been derived for both reactions, including a proper evaluation of their uncertainties in the thermal energy range of interest for big bang nucleosynthesis studies. The new estimate of the7Be destruction rate, based on these new results, yields a decrease of the predicted cosmological7Li abundance insufficient to provide a viable solution to the cosmological lithium problem.
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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 AS, Busso M, Caamaño M, Caballero L, Calviani M, Calviño F, Cano-Ott D, Casanovas A, Cerutti F, Chiaveri E, Cortés GP, Cortés-Giraldo MA, Cosentino L, Damone LA, Davies PJ, 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 DG, 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 SJ, Macina D, Manna A, Martínez T, Masi A, Mastinu PF, Maugeri E, Mendoza E, Mengoni A, Michalopoulou V, Milazzo PM, Millán-Callado MA, 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 JM, Doval DR, Reifarth R, Rochman D, Rubbia C, Sabaté-Gilarte M, Saxena A, Schillebeeckx P, Schumann D, Sekhar A, Smith AG, Sosnin N, Sprung P, Stamatopoulos A, Tagliente G, Tain JL, Tarifeño-Saldivia AE, 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 PJ, Wright TJ, Žugec P. The 154Gd neutron capture cross section measured at the n_TOF facility and its astrophysical implications. EPJ Web Conf 2020. [DOI: 10.1051/epjconf/202023907003] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
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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Alcayne V, Mendoza E, Cano-Ott D, Kimura A, Aberle O, 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, Casanovas A, Cerutti F, Chen YH, Chiaveri E, Colonna N, Cortés GP, Cortés-Giraldo MA, Cosentino L, Cristallo S, 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, Kivel N, Kokkoris M, Kopatch Y, 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, Mazzone A, Mengoni A, Michalopoulou V, Milazzo PM, Mingrone F, 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, Vlachoudis V, Vlastou R, Wallner A, Woods PJ, Wright TJ, Žugec P. Measurement of the 244Cm capture cross sections at both CERN n_TOF experimental areas. EPJ Web Conf 2020. [DOI: 10.1051/epjconf/202023901034] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
Accurate neutron capture cross section data for minor actinides (MAs) are required to estimate the production and transmutation rates of MAs in light water reactors with a high burnup, critical fast reactors like Gen-IV systems and other innovative reactor systems such as accelerator driven systems (ADS). Capture reactions of244Cm open the path for the formation of heavier Cm isotopes and of heavier elements such as Bk and Cf. In addition,244Cm shares nearly 50% of the total actinide decay heat in irradiated reactor fuels with a high burnup, even after three years of cooling.Experimental data for this isotope are very scarce due to the difficulties of providing isotopically enriched samples and because the high intrinsic activity of the samples requires the use of neutron facilities with high instantaneous flux. The only two previous experimental data sets for this neutron capture cross section have been obtained in 1969 using a nuclear explosion and, more recently, at J-PARC in 2010. The neutron capture cross sections have been measured at n_TOF with the same samples that the previous experiments in J-PARC. The samples were measured at n_TOF Experimental Area 2 (EAR-2) with three C6D6detectors and also in Experimental Area 1 (EAR-1) with the Total Absorption Calorimeter (TAC). Preliminary results assessing the quality and limitations of these new experimental datasets are presented for the experiments in both areas. Preliminary yields of both measurements will be compared with evaluated libraries for the first time.
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Eleme Z, Patronis N, Stamatopoulos A, Tsinganis A, Kokkoris M, Michalopoulou V, Diakaki M, Vlastou R, Tassan-Got L, Colonna N, Heyse J, Barbagallo M, Mastromarco M, Macina D, Chiaveri E, Aberle O, Alcayne V, Amaducci S, Andrzejewski J, Audouin L, Babiano-Suarez V, Bacak M, Bennett S, Berthoumieux E, Bosnar D, Brown AS, Busso M, Caamaño M, Caballero L, Calviani M, Calviño F, Cano-Ott D, Casanovas A, Cerutti F, Cortés GP, Cortés-Giraldo MA, Cosentino L, Cristallo S, Damone LA, Davies PJ, Dietz M, Domingo-Pardo C, Dressler R, Ducasse Q, Dupont E, Durán I, 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, Jenkins DG, Jericha E, Jiri U, Junghans A, Kadi Y, Käppeler F, Kimura A, Knapová I, Kopatch Y, Krticˇka M, Kurtulgil D, Ladarescu I, Lederer-Woods C, Lerendegui-Marco J, Lonsdale SJ, Manna A, Martínez T, Masi A, Massimi C, Mastinu PF, Maugeri E, Mazzone A, Mendoza E, Mengoni A, Milazzo PM, Millán-Callado MA, Mingrone F, Moreno-Soto J, Musumarra A, Negret A, Ogállar F, Oprea A, Pavlik A, Perkowski J, Petrone C, Piersanti L, Pirovano E, Porras I, Praena J, Quesada JM, Ramos Doval D, Reifarth R, Rochman D, Rubbia C, Sabaté-Gilarte M, Saxena A, Schillebeeckx P, Schumann D, Sekhar A, Smith AG, Sosnin N, Sprung P, Tagliente G, Tain JL, Tarifeño-Saldivia AE, Thomas B, Torres-Sánchez P, Urlass S, Valenta S, Vannini G, Variale V, Vaz P, Ventura A, Vescovi D, Vlachoudis V, Wallner A, Woods PJ, Wright TJ, Žugec P. First results of the 241Am(n,f) cross section measurement at the Experimental Area 2 of the n_TOF facility at CERN. EPJ Web Conf 2020. [DOI: 10.1051/epjconf/202023905014] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022] Open
Abstract
Feasibility, design and sensitivity studies on innovative nuclear reactors that could address the issue of nuclear waste transmutation using fuels enriched in minor actinides, require high accuracy cross section data for a variety of neutron-induced reactions from thermal energies to several tens of MeV. The isotope 241Am (T1/2= 433 years) is present in high-level nuclear waste (HLW), representing about 1.8 % of the actinide mass in spent PWR UOx fuel. Its importance increases with cooling time due to additional production from the β-decay of 241Pu with a half-life of 14.3 years. The production rate of 241 Am in conventional reactors, including its further accumulation through the decay of 241Pu and its destruction through transmutation/incineration are very important parameters for the design of any recycling solution. In the present work, the 241 Am(n,f) reaction cross-section was measured using Micromegas detectors at the Experimental Area 2 of the n_TOF facility at CERN. For the measurement, the 235U(n,f) and 238U(n,f) reference reactions were used for the determination of the neutron flux. In the present work an overview of the experimental setup and the adopted data analysis techniques is given along with preliminary results.
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Tassan-Got L, Colonna N, Diakaki M, Eleme Z, Manna A, Sekhar A, Stamatopoulos A, Aberle O, Alcayne V, Amaducci S, Andrzejewski J, Audouin L, Babiano-Suarez V, Bacak M, Barbagallo M, Bennett S, Berthoumieux E, Bosnar D, Brown AS, Busso M, Caamaño M, Caballero L, Calviani M, Calviño F, Cano-Ott D, Casanovas A, Cerutti F, Chiaveri E, Cortés GP, Cortés-Giraldo MA, Cosentino L, Cristallo S, Damone LA, Davies PJ, Dietz M, Domingo-Pardo C, Dressler R, Ducasse Q, Dupont E, Durán I, 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 DG, Jiri U, Junghans A, Kadi Y, Käppeler F, Kimura A, Knapová I, Kokkoris M, Kopatch Y, Krticˇka M, Kurtulgil D, Ladarescu I, Lederer-Woods C, Lerendegui-Marco J, Lonsdale SJ, Macina D, Martínez T, Masi A, Massimi C, Mastinu PF, Mastromarco M, Maugeri E, Mazzone A, Mendoza E, Mengoni A, Michalopoulou V, Milazzo PM, Millán-Callado MA, 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 JM, Ramos Doval D, Reifarth R, Rochman D, Rubbia C, Sabaté-Gilarte M, Saxena A, Schillebeeckx P, Schumann D, Smith AG, Sosnin N, Sprung P, Tagliente G, Tain JL, Tarifeño-Saldivia AE, 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 PJ, Wright TJ, Žugec P. Fission program at n_TOF. EPJ Web Conf 2019. [DOI: 10.1051/epjconf/201921103006] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
Since its start in 2001 the n_TOF collaboration developed a measurement program on fission, in view of advanced fuels in new generation reactors. A special effort was made on measurement of cross sections of actinides, exploiting the peculiarity of the n_TOF neutron beam which spans a huge energy domain, from the thermal region up to GeV. Moreover fission fragment angular distributions have also been measured. An overview of the cross section results achieved with different detectors is presented, including a discussion of the 237Np case where discrepancies showed up between different detector systems. The results on the anisotropy of the fission fragments and its implication on the mechanism of neutron absorption, and in applications, are also shown.
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Battini F, Agostini A, Boulamanti AK, Giuntoli J, Amaducci S. Mitigating the environmental impacts of milk production via anaerobic digestion of manure: case study of a dairy farm in the Po Valley. Sci Total Environ 2014; 481:196-208. [PMID: 24598150 DOI: 10.1016/j.scitotenv.2014.02.038] [Citation(s) in RCA: 41] [Impact Index Per Article: 4.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/26/2013] [Revised: 02/04/2014] [Accepted: 02/09/2014] [Indexed: 06/03/2023]
Abstract
This work analyzes the environmental impacts of milk production in an intensive dairy farm situated in the Northern Italy region of the Po Valley. Three manure management scenarios are compared: in Scenario 1 the animal slurry is stored in an open tank and then used as fertilizer. In scenario 2 the manure is processed in an anaerobic digestion plant and the biogas produced is combusted in an internal combustion engine to produce heat (required by the digester) and electricity (exported). Scenario 3 is similar to scenario 2 but the digestate is stored in a gas-tight tank. In scenario 1 the GHG emissions are estimated to be equal to 1.21 kg CO2 eq.kg(-1) Fat and Protein Corrected Milk (FPCM) without allocation of the environmental burden to the by-product meat. With mass allocation, the GHG emissions associated to the milk are reduced to 1.18 kg CO2 eq.kg(-1) FPCM. Using an economic allocation approach the GHG emissions allocated to the milk are 1.13 kg CO2 eq.kg(-1) FPCM. In scenarios 2 and 3, without allocation, the GHG emissions are reduced respectively to 0.92 (-23.7%) and 0.77 (-36.5%) kg CO2 eq.kg(-1) FPCM. If land use change due to soybean production is accounted for, an additional emission of 0.53 kg CO2 eq. should be added, raising the GHG emissions to 1.74, 1.45 and 1.30 kg CO2 eq kg(-1) FPCM in scenarios 1, 2 and 3, respectively. Primary energy from non-renewable resources decreases by 36.2% and 40.6% in scenarios 2 and 3, respectively, with the valorization of the manure in the biogas plant. The other environmental impact mitigated is marine eutrophication that decreases by 8.1% in both scenarios 2 and 3, mostly because of the lower field emissions. There is, however, a trade-off between non-renewable energy and GHG savings and other environmental impacts: acidification (+6.1% and +5.5% in scenarios 2 and 3, respectively), particulate matter emissions (+1.4% and +0.7%) and photochemical ozone formation potential (+41.6% and +42.3%) increase with the adoption of a biogas plant. The cause of the increase is mostly emissions from the CHP engine. These impacts can be tackled by improving biogas combustion technologies to reduce methane and NOx emissions. Freshwater eutrophication slightly increases (+0.8% in both scenarios 2 and 3) because of the additional infrastructures needed. In conclusion, on-farm manure anaerobic digestion with the production of electricity is an effective technology to significantly reduce global environmental impacts of dairy farms (GHG emissions and non-renewable energy consumption), however local impacts may increase as a consequence (especially photochemical ozone formation).
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Affiliation(s)
- F Battini
- Institute of Agronomy, Genetics and Field Crops, Università Cattolica del Sacro Cuore, Via Emilia Parmense 84, 29122 Piacenza, Italy.
| | - A Agostini
- STU Unit, JRC-IET-European Commission, Westerduinweg 3, 1755LE Petten, The Netherlands; ENEA-Italian National Agency for New Technologies, Energy and the Environment, Via Anguillarese 301, Rome, Italy
| | - A K Boulamanti
- STU Unit, JRC-IET-European Commission, Westerduinweg 3, 1755LE Petten, The Netherlands
| | - J Giuntoli
- STU Unit, JRC-IET-European Commission, Westerduinweg 3, 1755LE Petten, The Netherlands
| | - S Amaducci
- Institute of Agronomy, Genetics and Field Crops, Università Cattolica del Sacro Cuore, Via Emilia Parmense 84, 29122 Piacenza, Italy
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Bazzi C, Arrigo G, Luciani L, Casazza F, Saviotti M, Malaspina D, Bonucci E, Ballanti P, Amaducci S, Lattuada P. Clinical features of 24 patients on regular hemodialysis treatment (RDT) for 16-23 years in a single unit. Clin Nephrol 1995; 44:96-107. [PMID: 8529316] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/31/2023] Open
Abstract
Careful investigation of the clinical conditions of patients on maintenance hemodialysis for about 20 years in a single dialysis unit was of great interest for evaluation of the pathological consequences in long-term survivors of insufficient correction of uremia and of the dialysis treatment "per se". We analyzed the outcomes for a cohort of 116 patients who started RDT before 1976 and the clinical conditions of the 24 patients still on RDT in our unit at the end of 1991 (average duration of treatment = 222 +/- 23 months). Actuarial survival was 72% at 10 years and 43% at 20 years. Rehabilitation of the 24 survivors was rather good: 13 were able to work, 8 were retired or unable to work, but able to care for most personal needs. Actual body weight, anthropometric parameters and biochemical parameters revealed a well-preserved nutritional status. Anemia improved from 23 +/- 7 at the start of RDT to 31 +/- 8 in the 21 patients never treated with erythropoietin. Blood pressure was normal without therapy in 18 patients and elevated in 6. Mild-to-moderate left ventricular hypertrophy was present in all the 6 patients with arterial hypertension and in only 6 of the 18 normotensive patients. The ratio of early diastolic filling to filling during atrial contraction (E/A ratio) was < 1 in 16 patients: it was 1.05 +/- 0.43 in 9 patients with stable intradialysis blood pressure and significantly lower (0.73 +/- 0.15) in 12 patients with recurrent intradialysis hypotension. Supraventricular arrhythmias were detected by Holter monitoring in 41% and ventricular arrhythmias in 35% of patients. Extensive vascular calcifications were present (in 100% of patients in the abdominal aorta), but only 4 patients showed clinical signs of peripheral vascular disease. Subperiosteal resorption was detected radiologically in the hands of 59% of patients. Bone histology, interpretable for only 20 patients, revealed no bone lesions in 1 case (5%), mild mixed osteodystrophy in 3 cases (15%), advanced mixed osteodystrophy in 5 cases (25%), osteodystrophy with predominant hyperparathyroidism in 2 cases (10%), osteodystrophy with predominant osteomalacia in 6 cases (30%), and aplastic bone disease in 3 cases (15%). Moderate aluminum staining was found in only 4 patients and was more marked in earlier biopsies taken before withdrawal of the aluminium-containing phosphate-binding drugs.(ABSTRACT TRUNCATED AT 400 WORDS)
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Affiliation(s)
- C Bazzi
- Division of Nephrology and Dialysis, San Carlo Borromeo Hospital, Milan, Italy
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Bazzi C, Amaducci S, Arrigo G, Colombo B, Moreni E, D'Amico G. Bronchial responsiveness in patients on regular hemodialysis treatment of very long duration. Am J Kidney Dis 1994; 24:802-5. [PMID: 7977322 DOI: 10.1016/s0272-6386(12)80674-3] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/28/2023]
Abstract
Several mechanisms (trapping of neutrophils, increased extravascular lung water, left ventricular hypertrophy, metastatic lung calcification, and iron deposition) may impair pulmonary function and alter bronchial responsiveness in patients on long-term regular dialysis treatment (RDT), but no studies have been published concerning patients on RDT for a very long time. To assess bronchial reactivity, a methacholine inhalation test was performed 2 to 24 hours after a dialysis session in 19 patients with RDT duration of almost 20 years (221 +/- 26 months) (group 1) and in 14 patients on RDT for a shorter time (24 +/- 22 months) (group 2); all patients had normal standard pulmonary function test results (group 1: forced vital capacity, 95% +/- 13% and forced expiratory volume in one second [FEV1]: 97% +/- 17%; group 2: forced vital capacity, 108% +/- 11% and FEV1, 108% +/- 9% of expected values). The methacholine provocation dose causing a 20% decrease in FEV1 was significantly lower than normal in seven (37%) group 1 patients and only in one (7%) group 2 patient; this difference was statistically significant (P = 0.049). There were no correlations between bronchial hyperresponsiveness and interdialysis weight gain, left ventricular hypertrophy, diastolic dysfunction expressed as the ratio between early diastolic filling and filling during atrial contraction, secondary hyperparathyroidism, and iron overload. Therefore, bronchial hyperresponsiveness is present in a substantial percentage of patients on RDT of very long duration, but the cause is unknown.
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Affiliation(s)
- C Bazzi
- Division of Nephrology and Dialysis, S. Carlo Borromeo Hospital, Milano,Italy
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20
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Dellafiore L, Colombo B, Del Sante M, Farina D, Zanoni C, Amaducci S, Beulcke G. [Pulmonary involvement in scleroderma assessed with high-resolution computerized tomography and functional tests]. Radiol Med 1994; 87:608-13. [PMID: 8008890] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 01/28/2023]
Abstract
This study was aimed at investigating and analyzing lung involvement in scleroderma patients with different imaging methods, toward a rational diagnostic approach. Twenty-four patients with systemic sclerosis were examined with pulmonary function tests (PFT), spirometry and diffusing capacity for carbon monoxide (DLCO), chest radiography and high-resolution Computed Tomography (HRCT). Abnormal findings were present in 42% of cases on X-ray films and in 71% of cases on HRCT images. PFT was abnormal in the spirometries of 42% of cases and in DLCO tests in 50% of cases. The most common findings at HRCT were the small reticular and the ground-glass patterns. HRCT emerged as the most effective method to evaluate lung involvement in systemic sclerosis. In our series, HRCT allowed possibly curable lung lesions to be differentiated from incurable ones. However, HRCT is suggested in the patients with impaired pulmonary function to allow treatment choice; on the contrary, in the patients with no functional impairment, HRCT adds little information to clinical findings, showing only limited focal lesions.
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Affiliation(s)
- L Dellafiore
- Servizio di Radiologia, Ente Ospedaliero S. Carlo Borromeo, Milano
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21
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Arossa W, Spinaci S, Forconi G, Concina E, Amaducci S, Mastrangelo G, Scotti PG. A survey on spirometer calibration. Part one: Census and in field control of devices. Med Lav 1981; 72:177-82. [PMID: 7300790] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 01/24/2023]
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Arossa W, Spinaci S, De Rosa C, Amaducci S, Mastrangelo G, Scotti PG. Calibration of forced expiration curves by explosive decompression. Med Lav 1980; 71:199-203. [PMID: 7453647] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 01/25/2023]
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Amaducci S, Arossa W, Mastrangelo G, Paruzzlo P, Scotti PG. [Survey on the sensitivity and reproducibility of forced expiration indices used in epidemiological investigations of obstructive lung disease carried out at local occupational health centres (author's transl)]. Med Lav 1979; 70:266- 75. [PMID: 545107] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 12/23/2022]
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Amaducci S, Mandelli V, Morpurgo M, Rampulla C. Aging, cigarette smoking, and respiratory function. Bull Eur Physiopathol Respir 1977; 13:523-32. [PMID: 912139] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 12/24/2022]
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Abstract
A syndrome, characterized by pulmonary hyperdistension (increased residual volume, closing capacity and Motley index), was observed in patients with hyperlipoproteinemias without without other known causes of pulmonary disease. This syndrome is mostly asymptomatic;hyperdistension is of variable degree and not directly correlated to plasma lipid levels. It is partially reversible after reduction of lipidemia. The cause of this syndrome is not known. It may explain a decreased pulmonary working capacity in asymptomatic hyperlipidemic patients.
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Rampulla C, Marconi C, Beulcke G, Amaducci S. Correlations between lung-transfer factor, ventilation, and cardiac output during exercise. Respiration 1976; 33:405-15. [PMID: 1005935 DOI: 10.1159/000193758] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/25/2022] Open
Abstract
In nine healthy and young subject of either sex, undergoing three or four rounds of muscular exercise of increasing severity on a bicycle ergometer, the authors investigated the behavior of the lung transfer factor (Dlco), pulmonary ventilation (V), alveolar ventilation (Va), and cardiac output (Q). In all instances they found a positive linear correlation between DLCO and oxygen consumption (VO2), at least up to 70% of maximum oxygen consumption (Vo2max) (r=0.935;p less than 0.001). Dlco was found to increase linearly as a function of increasing V (R=0.898;P LESS THAN 0.001) AND EVEN MORE SO OF INCREASING Va (r=0.919; p less than 0.001). Also the relationship between Dlco and Q appeared linear in all subjects (r=0.926; p less than 0.001). On the other hand, individual Dlco values showed considerable scatter at equal Vo2, V, Va, and Q values. Among the factors responsible for the increase of Dlco during muscular exercise, in addition to increased ventilation and cardiac output, the authors suggest the possible role of the greater desaturation of mixed venous blood and variations of hemoglobin affinity for CO.
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