Measurement of 73Ge(n,γ) cross sections and implications for stellar nucleosynthesis
73Ge(n,γ) cross sections were measured at the neutron time-of-flight facility n_TOF at CERN up to neutron energies of 300 keV, providing for the first time experimental data above 8 keV. Results indicate that the stellar cross section at kT=30 keV is 1.5 to 1.7 times higher than most theoretical pre...
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| Format: | Article |
| Language: | English |
| Published: |
Elsevier
2019-03-01
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| Series: | Physics Letters B |
| Online Access: | http://www.sciencedirect.com/science/article/pii/S037026931930070X |
| _version_ | 1819241869745324032 |
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| author | C. Lederer-Woods U. Battino P. Ferreira A. Gawlik C. Guerrero F. Gunsing S. Heinitz J. Lerendegui-Marco A. Mengoni R. Reifarth A. Tattersall S. Valenta C. Weiss O. Aberle J. Andrzejewski L. Audouin V. Bécares M. Bacak J. Balibrea M. Barbagallo S. Barros F. Bečvář C. Beinrucker F. Belloni E. Berthoumieux J. Billowes D. Bosnar M. Brugger M. Caamaño F. Calviño M. Calviani D. Cano-Ott F. Cerutti E. Chiaveri N. Colonna G. Cortés M.A. Cortés-Giraldo L. Cosentino L.A. Damone K. Deo M. Diakaki M. Dietz C. Domingo-Pardo R. Dressler E. Dupont I. Durán B. Fernández-Domínguez A. Ferrari P. Finocchiaro R.J.W. Frost V. Furman K. Göbel A.R. García I. Gheorghe T. Glodariu I.F. Gonçalves E. González-Romero A. Goverdovski E. Griesmayer H. Harada T. Heftrich A. Hernández-Prieto J. Heyse D.G. Jenkins E. Jericha F. Käppeler Y. Kadi T. Katabuchi P. Kavrigin V. Ketlerov V. Khryachkov A. Kimura N. Kivel I. Knapova M. Kokkoris M. Krtička E. Leal-Cidoncha H. Leeb M. Licata S. Lo Meo R. Losito D. Macina J. Marganiec T. Martínez C. Massimi P. Mastinu M. Mastromarco F. Matteucci E. Mendoza P.M. Milazzo F. Mingrone M. Mirea S. Montesano A. Musumarra R. Nolte F.R. Palomo-Pinto C. Paradela N. Patronis A. Pavlik J. Perkowski J.I. Porras J. Praena J.M. Quesada T. Rauscher A. Riego-Perez M. Robles C. Rubbia J.A. Ryan M. Sabaté-Gilarte A. Saxena P. Schillebeeckx S. Schmidt D. Schumann P. Sedyshev A.G. Smith A. Stamatopoulos S.V. Suryanarayana G. Tagliente J.L. Tain A. Tarifeño-Saldivia L. Tassan-Got A. Tsinganis G. Vannini V. Variale P. Vaz A. Ventura V. Vlachoudis R. Vlastou A. Wallner S. Warren M. Weigand T. Wright P. Žugec |
| author_facet | C. Lederer-Woods U. Battino P. Ferreira A. Gawlik C. Guerrero F. Gunsing S. Heinitz J. Lerendegui-Marco A. Mengoni R. Reifarth A. Tattersall S. Valenta C. Weiss O. Aberle J. Andrzejewski L. Audouin V. Bécares M. Bacak J. Balibrea M. Barbagallo S. Barros F. Bečvář C. Beinrucker F. Belloni E. Berthoumieux J. Billowes D. Bosnar M. Brugger M. Caamaño F. Calviño M. Calviani D. Cano-Ott F. Cerutti E. Chiaveri N. Colonna G. Cortés M.A. Cortés-Giraldo L. Cosentino L.A. Damone K. Deo M. Diakaki M. Dietz C. Domingo-Pardo R. Dressler E. Dupont I. Durán B. Fernández-Domínguez A. Ferrari P. Finocchiaro R.J.W. Frost V. Furman K. Göbel A.R. García I. Gheorghe T. Glodariu I.F. Gonçalves E. González-Romero A. Goverdovski E. Griesmayer H. Harada T. Heftrich A. Hernández-Prieto J. Heyse D.G. Jenkins E. Jericha F. Käppeler Y. Kadi T. Katabuchi P. Kavrigin V. Ketlerov V. Khryachkov A. Kimura N. Kivel I. Knapova M. Kokkoris M. Krtička E. Leal-Cidoncha H. Leeb M. Licata S. Lo Meo R. Losito D. Macina J. Marganiec T. Martínez C. Massimi P. Mastinu M. Mastromarco F. Matteucci E. Mendoza P.M. Milazzo F. Mingrone M. Mirea S. Montesano A. Musumarra R. Nolte F.R. Palomo-Pinto C. Paradela N. Patronis A. Pavlik J. Perkowski J.I. Porras J. Praena J.M. Quesada T. Rauscher A. Riego-Perez M. Robles C. Rubbia J.A. Ryan M. Sabaté-Gilarte A. Saxena P. Schillebeeckx S. Schmidt D. Schumann P. Sedyshev A.G. Smith A. Stamatopoulos S.V. Suryanarayana G. Tagliente J.L. Tain A. Tarifeño-Saldivia L. Tassan-Got A. Tsinganis G. Vannini V. Variale P. Vaz A. Ventura V. Vlachoudis R. Vlastou A. Wallner S. Warren M. Weigand T. Wright P. Žugec |
| author_sort | C. Lederer-Woods |
| collection | DOAJ |
| description | 73Ge(n,γ) cross sections were measured at the neutron time-of-flight facility n_TOF at CERN up to neutron energies of 300 keV, providing for the first time experimental data above 8 keV. Results indicate that the stellar cross section at kT=30 keV is 1.5 to 1.7 times higher than most theoretical predictions. The new cross sections result in a substantial decrease of 73Ge produced in stars, which would explain the low isotopic abundance of 73Ge in the solar system. Keywords: Nucleosynthesis, Neutron capture, s process, Germanium, n_TOF |
| first_indexed | 2024-12-23T14:30:46Z |
| format | Article |
| id | doaj.art-0cdf904b20d1412ab3ad0e3c9cf18a7e |
| institution | Directory Open Access Journal |
| issn | 0370-2693 |
| language | English |
| last_indexed | 2024-12-23T14:30:46Z |
| publishDate | 2019-03-01 |
| publisher | Elsevier |
| record_format | Article |
| series | Physics Letters B |
| spelling | doaj.art-0cdf904b20d1412ab3ad0e3c9cf18a7e2022-12-21T17:43:30ZengElsevierPhysics Letters B0370-26932019-03-01790458465Measurement of 73Ge(n,γ) cross sections and implications for stellar nucleosynthesisC. Lederer-Woods0U. Battino1P. Ferreira2A. Gawlik3C. Guerrero4F. Gunsing5S. Heinitz6J. Lerendegui-Marco7A. Mengoni8R. Reifarth9A. Tattersall10S. Valenta11C. Weiss12O. Aberle13J. Andrzejewski14L. Audouin15V. Bécares16M. Bacak17J. Balibrea18M. Barbagallo19S. Barros20F. Bečvář21C. Beinrucker22F. Belloni23E. Berthoumieux24J. Billowes25D. Bosnar26M. Brugger27M. Caamaño28F. Calviño29M. Calviani30D. Cano-Ott31F. Cerutti32E. Chiaveri33N. Colonna34G. Cortés35M.A. Cortés-Giraldo36L. Cosentino37L.A. Damone38K. Deo39M. Diakaki40M. Dietz41C. Domingo-Pardo42R. Dressler43E. Dupont44I. Durán45B. Fernández-Domínguez46A. Ferrari47P. Finocchiaro48R.J.W. Frost49V. Furman50K. Göbel51A.R. García52I. Gheorghe53T. Glodariu54I.F. Gonçalves55E. González-Romero56A. Goverdovski57E. Griesmayer58H. Harada59T. Heftrich60A. Hernández-Prieto61J. Heyse62D.G. Jenkins63E. Jericha64F. Käppeler65Y. Kadi66T. Katabuchi67P. Kavrigin68V. Ketlerov69V. Khryachkov70A. Kimura71N. Kivel72I. Knapova73M. Kokkoris74M. Krtička75E. Leal-Cidoncha76H. Leeb77M. Licata78S. Lo Meo79R. Losito80D. Macina81J. Marganiec82T. Martínez83C. Massimi84P. Mastinu85M. Mastromarco86F. Matteucci87E. Mendoza88P.M. Milazzo89F. Mingrone90M. Mirea91S. Montesano92A. Musumarra93R. Nolte94F.R. Palomo-Pinto95C. Paradela96N. Patronis97A. Pavlik98J. Perkowski99J.I. Porras100J. Praena101J.M. Quesada102T. Rauscher103A. Riego-Perez104M. Robles105C. Rubbia106J.A. Ryan107M. Sabaté-Gilarte108A. Saxena109P. Schillebeeckx110S. Schmidt111D. Schumann112P. Sedyshev113A.G. Smith114A. Stamatopoulos115S.V. Suryanarayana116G. Tagliente117J.L. Tain118A. Tarifeño-Saldivia119L. Tassan-Got120A. Tsinganis121G. Vannini122V. Variale123P. Vaz124A. Ventura125V. Vlachoudis126R. Vlastou127A. Wallner128S. Warren129M. Weigand130T. Wright131P. Žugec132School of Physics and Astronomy, University of Edinburgh, United Kingdom; Goethe University Frankfurt, Germany; Corresponding author at: School of Physics and Astronomy, University of Edinburgh, United Kingdom.School of Physics and Astronomy, University of Edinburgh, United KingdomInstituto Superior Técnico, Lisbon, PortugalUniversity of Lodz, PolandUniversidad de Sevilla, SpainCEA Irfu, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France; European Organization for Nuclear Research (CERN), SwitzerlandPaul Scherrer Institut (PSI), Villingen, SwitzerlandUniversidad de Sevilla, SpainAgenzia nazionale per le nuove tecnologie, l'energia e lo sviluppo economico sostenibile (ENEA), Bologna, ItalyGoethe University Frankfurt, GermanySchool of Physics and Astronomy, University of Edinburgh, United KingdomCharles University, Prague, Czech RepublicEuropean Organization for Nuclear Research (CERN), Switzerland; Technische Universität Wien, AustriaEuropean Organization for Nuclear Research (CERN), SwitzerlandUniversity of Lodz, PolandInstitut de Physique Nucléaire, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-Saclay, F-91406 Orsay Cedex, FranceCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), SpainTechnische Universität Wien, AustriaCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), SpainIstituto Nazionale di Fisica Nucleare, Sezione di Bari, ItalyInstituto Superior Técnico, Lisbon, PortugalCharles University, Prague, Czech RepublicGoethe University Frankfurt, GermanyCEA Irfu, Université Paris-Saclay, F-91191 Gif-sur-Yvette, FranceCEA Irfu, Université Paris-Saclay, F-91191 Gif-sur-Yvette, FranceUniversity of Manchester, United KingdomDepartment of Physics, Faculty of Science, University of Zagreb, Zagreb, CroatiaEuropean Organization for Nuclear Research (CERN), SwitzerlandUniversity of Santiago de Compostela, SpainUniversitat Politècnica de Catalunya, SpainEuropean Organization for Nuclear Research (CERN), SwitzerlandCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), SpainEuropean Organization for Nuclear Research (CERN), SwitzerlandEuropean Organization for Nuclear Research (CERN), SwitzerlandIstituto Nazionale di Fisica Nucleare, Sezione di Bari, ItalyUniversitat Politècnica de Catalunya, SpainUniversidad de Sevilla, SpainINFN Laboratori Nazionali del Sud, Catania, ItalyIstituto Nazionale di Fisica Nucleare, Sezione di Bari, Italy; Dipartimento di Fisica, Università degli Studi di Bari, ItalyBhabha Atomic Research Centre (BARC), IndiaCEA Irfu, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France; National Technical University of Athens, GreeceSchool of Physics and Astronomy, University of Edinburgh, United KingdomInstituto de Física Corpuscular, CSIC - Universidad de Valencia, SpainPaul Scherrer Institut (PSI), Villingen, SwitzerlandCEA Irfu, Université Paris-Saclay, F-91191 Gif-sur-Yvette, FranceUniversity of Santiago de Compostela, SpainUniversity of Santiago de Compostela, SpainEuropean Organization for Nuclear Research (CERN), SwitzerlandINFN Laboratori Nazionali del Sud, Catania, ItalyUniversity of Manchester, United KingdomJoint Institute for Nuclear Research (JINR), Dubna, RussiaGoethe University Frankfurt, GermanyCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), SpainHoria Hulubei National Institute of Physics and Nuclear Engineering, RomaniaHoria Hulubei National Institute of Physics and Nuclear Engineering, RomaniaInstituto Superior Técnico, Lisbon, PortugalCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), SpainInstitute of Physics and Power Engineering (IPPE), Obninsk, RussiaTechnische Universität Wien, AustriaJapan Atomic Energy Agency (JAEA), Tokai-mura, JapanGoethe University Frankfurt, GermanyEuropean Organization for Nuclear Research (CERN), Switzerland; Universitat Politècnica de Catalunya, SpainEuropean Commission, Joint Research Centre, Geel, Retieseweg 111, B-2440 Geel, BelgiumUniversity of York, United KingdomTechnische Universität Wien, AustriaKarlsruhe Institute of Technology, Campus North, IKP, 76021 Karlsruhe, GermanyEuropean Organization for Nuclear Research (CERN), SwitzerlandTokyo Institute of Technology, JapanTechnische Universität Wien, AustriaInstitute of Physics and Power Engineering (IPPE), Obninsk, RussiaInstitute of Physics and Power Engineering (IPPE), Obninsk, RussiaJapan Atomic Energy Agency (JAEA), Tokai-mura, JapanPaul Scherrer Institut (PSI), Villingen, SwitzerlandCharles University, Prague, Czech RepublicNational Technical University of Athens, GreeceCharles University, Prague, Czech RepublicUniversity of Santiago de Compostela, SpainTechnische Universität Wien, AustriaIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy; Dipartimento di Fisica e Astronomia, Università di Bologna, ItalyAgenzia nazionale per le nuove tecnologie, l'energia e lo sviluppo economico sostenibile (ENEA), Bologna, Italy; Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, ItalyEuropean Organization for Nuclear Research (CERN), SwitzerlandEuropean Organization for Nuclear Research (CERN), SwitzerlandUniversity of Lodz, PolandCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), SpainIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy; Dipartimento di Fisica e Astronomia, Università di Bologna, ItalyIstituto Nazionale di Fisica Nucleare, Sezione di Legnaro, ItalyIstituto Nazionale di Fisica Nucleare, Sezione di Bari, ItalyIstituto Nazionale di Fisica Nucleare, Sezione di Trieste, Italy; Dipartimento di Astronomia, Università di Trieste, ItalyCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), SpainIstituto Nazionale di Fisica Nucleare, Sezione di Trieste, ItalyIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, ItalyHoria Hulubei National Institute of Physics and Nuclear Engineering, RomaniaEuropean Organization for Nuclear Research (CERN), SwitzerlandINFN Laboratori Nazionali del Sud, Catania, Italy; Dipartimento di Fisica e Astronomia, Università di Catania, ItalyPhysikalisch-Technische Bundesanstalt (PTB), Bundesallee 100, 38116 Braunschweig, GermanyUniversidad de Sevilla, SpainUniversity of Santiago de Compostela, SpainUniversity of Ioannina, GreeceUniversity of Vienna, Faculty of Physics, Vienna, AustriaUniversity of Lodz, PolandEuropean Organization for Nuclear Research (CERN), Switzerland; University of Granada, SpainUniversidad de Sevilla, SpainUniversidad de Sevilla, SpainCentre for Astrophysics Research, University of Hertfordshire, United Kingdom; Department of Physics, University of Basel, SwitzerlandUniversitat Politècnica de Catalunya, SpainUniversity of Santiago de Compostela, SpainEuropean Organization for Nuclear Research (CERN), SwitzerlandUniversity of Manchester, United KingdomEuropean Organization for Nuclear Research (CERN), Switzerland; Universidad de Sevilla, SpainBhabha Atomic Research Centre (BARC), IndiaEuropean Commission, Joint Research Centre, Geel, Retieseweg 111, B-2440 Geel, BelgiumGoethe University Frankfurt, GermanyPaul Scherrer Institut (PSI), Villingen, SwitzerlandJoint Institute for Nuclear Research (JINR), Dubna, RussiaUniversity of Manchester, United KingdomNational Technical University of Athens, GreeceBhabha Atomic Research Centre (BARC), IndiaIstituto Nazionale di Fisica Nucleare, Sezione di Bari, ItalyInstituto de Física Corpuscular, CSIC - Universidad de Valencia, SpainInstituto de Física Corpuscular, CSIC - Universidad de Valencia, SpainInstitut de Physique Nucléaire, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-Saclay, F-91406 Orsay Cedex, FranceNational Technical University of Athens, GreeceIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy; Dipartimento di Fisica e Astronomia, Università di Bologna, ItalyIstituto Nazionale di Fisica Nucleare, Sezione di Bari, ItalyInstituto Superior Técnico, Lisbon, PortugalIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, ItalyEuropean Organization for Nuclear Research (CERN), SwitzerlandNational Technical University of Athens, GreeceAustralian National University, Canberra, AustraliaUniversity of Manchester, United KingdomGoethe University Frankfurt, GermanyUniversity of Manchester, United KingdomDepartment of Physics, Faculty of Science, University of Zagreb, Zagreb, Croatia73Ge(n,γ) cross sections were measured at the neutron time-of-flight facility n_TOF at CERN up to neutron energies of 300 keV, providing for the first time experimental data above 8 keV. Results indicate that the stellar cross section at kT=30 keV is 1.5 to 1.7 times higher than most theoretical predictions. The new cross sections result in a substantial decrease of 73Ge produced in stars, which would explain the low isotopic abundance of 73Ge in the solar system. Keywords: Nucleosynthesis, Neutron capture, s process, Germanium, n_TOFhttp://www.sciencedirect.com/science/article/pii/S037026931930070X |
| spellingShingle | C. Lederer-Woods U. Battino P. Ferreira A. Gawlik C. Guerrero F. Gunsing S. Heinitz J. Lerendegui-Marco A. Mengoni R. Reifarth A. Tattersall S. Valenta C. Weiss O. Aberle J. Andrzejewski L. Audouin V. Bécares M. Bacak J. Balibrea M. Barbagallo S. Barros F. Bečvář C. Beinrucker F. Belloni E. Berthoumieux J. Billowes D. Bosnar M. Brugger M. Caamaño F. Calviño M. Calviani D. Cano-Ott F. Cerutti E. Chiaveri N. Colonna G. Cortés M.A. Cortés-Giraldo L. Cosentino L.A. Damone K. Deo M. Diakaki M. Dietz C. Domingo-Pardo R. Dressler E. Dupont I. Durán B. Fernández-Domínguez A. Ferrari P. Finocchiaro R.J.W. Frost V. Furman K. Göbel A.R. García I. Gheorghe T. Glodariu I.F. Gonçalves E. González-Romero A. Goverdovski E. Griesmayer H. Harada T. Heftrich A. Hernández-Prieto J. Heyse D.G. Jenkins E. Jericha F. Käppeler Y. Kadi T. Katabuchi P. Kavrigin V. Ketlerov V. Khryachkov A. Kimura N. Kivel I. Knapova M. Kokkoris M. Krtička E. Leal-Cidoncha H. Leeb M. Licata S. Lo Meo R. Losito D. Macina J. Marganiec T. Martínez C. Massimi P. Mastinu M. Mastromarco F. Matteucci E. Mendoza P.M. Milazzo F. Mingrone M. Mirea S. Montesano A. Musumarra R. Nolte F.R. Palomo-Pinto C. Paradela N. Patronis A. Pavlik J. Perkowski J.I. Porras J. Praena J.M. Quesada T. Rauscher A. Riego-Perez M. Robles C. Rubbia J.A. Ryan M. Sabaté-Gilarte A. Saxena P. Schillebeeckx S. Schmidt D. Schumann P. Sedyshev A.G. Smith A. Stamatopoulos S.V. Suryanarayana G. Tagliente J.L. Tain A. Tarifeño-Saldivia L. Tassan-Got A. Tsinganis G. Vannini V. Variale P. Vaz A. Ventura V. Vlachoudis R. Vlastou A. Wallner S. Warren M. Weigand T. Wright P. Žugec Measurement of 73Ge(n,γ) cross sections and implications for stellar nucleosynthesis Physics Letters B |
| title | Measurement of 73Ge(n,γ) cross sections and implications for stellar nucleosynthesis |
| title_full | Measurement of 73Ge(n,γ) cross sections and implications for stellar nucleosynthesis |
| title_fullStr | Measurement of 73Ge(n,γ) cross sections and implications for stellar nucleosynthesis |
| title_full_unstemmed | Measurement of 73Ge(n,γ) cross sections and implications for stellar nucleosynthesis |
| title_short | Measurement of 73Ge(n,γ) cross sections and implications for stellar nucleosynthesis |
| title_sort | measurement of 73ge n γ cross sections and implications for stellar nucleosynthesis |
| url | http://www.sciencedirect.com/science/article/pii/S037026931930070X |
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measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT pmmilazzo measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT fmingrone measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT mmirea measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT smontesano measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT amusumarra measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT rnolte measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT frpalomopinto measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT cparadela measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT npatronis measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT apavlik measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT jperkowski measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT jiporras measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT jpraena measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT jmquesada measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT trauscher measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT ariegoperez measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT mrobles measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT crubbia measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT jaryan measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT msabategilarte measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT asaxena measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT pschillebeeckx measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT sschmidt measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT dschumann measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT psedyshev measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT agsmith measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT astamatopoulos measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT svsuryanarayana measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT gtagliente measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT jltain measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT atarifenosaldivia measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT ltassangot measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT atsinganis measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT gvannini measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT vvariale measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT pvaz measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT aventura measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT vvlachoudis measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT rvlastou measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT awallner measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT swarren measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT mweigand measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT twright measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis AT pzugec measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis |