The<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Zr</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>92</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi></mml:mrow></mml:math>) reaction and its implications for stellar nucleosynthesis
G. Tagliente(Istituto Nazionale di Fisica Nucleare), M. Igashira(Tokyo Institute of Technology), F. Calviño(Polytechnic University of Puerto Rico), K. Fujii(Istituto Nazionale di Fisica Nucleare), F. Álvarez‐Velarde(Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas), A. Herrera-Martı́nez(European Organization for Nuclear Research), F. Bečvář(Charles University), R. C. Haight(Los Alamos National Laboratory), Brian J. Haas(Broad Institute), C. Carrapiço(DSM (Netherlands)), M. Calviani, R. Gallino(Istituto Nazionale di Fisica Nucleare, Sezione di Torino), G. Aerts(DSM (Netherlands)), G. Cortés(FC Barcelona), A. Ferrari(European Organization for Nuclear Research), J. Andrzejewski(University of Łódź), M. Dahlfors(European Organization for Nuclear Research), I. Dillmann(GSI Helmholtz Centre for Heavy Ion Research), R. Ferreira‐Marques(University of Coimbra), N. Colonna(Istituto Nazionale di Fisica Nucleare, Sezione di Bari), P. Baumann(Centre National de la Recherche Scientifique), W. Furman(Joint Institute for Nuclear Research), E. Berthoumieux(DSM (Netherlands)), C. Domingo‐Pardo(Consejo Superior de Investigaciones Científicas), D. Cano‐Ott(Unidades Centrales Científico-Técnicas), C. Eleftheriadis(Aristotle University of Thessaloniki), James W. Cox(University of Notre Dame), A. Couture(University of Notre Dame), I. F. Gonçalves(University of Coimbra), V. Chepel(University of Coimbra), I. Durán(Universidade de Santiago de Compostela), R. Capote(International Atomic Energy Agency), S. Bisterzo(University of Turin), P. Cennini(European Organization for Nuclear Research), U. Abbondanno(Istituto Nazionale di Fisica Nucleare), W. Dridi(DSM (Netherlands)), M. Embid-Segura(Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas), P. M. Milazzo(Istituto Nazionale di Fisica Nucleare, Sezione di Trieste), L. Audouin(Centre National de la Recherche Scientifique), E. González-Romero(Unidades Centrales Científico-Técnicas), F. Gunsing(DSM (Netherlands)), F. Belloni(Istituto Nazionale di Fisica Nucleare), C. Guerrero(Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas), S. Andriamonje(Commissariat à l'Énergie Atomique et aux Énergies Alternatives), M. Heil(Istituto Nazionale di Fisica Nucleare), G. Badurek(TU Wien), H. Álvarez(Universidade de Santiago de Compostela), S. David(Centre National de la Recherche Scientifique), E. Chiaveri(European Organization for Nuclear Research), F. Gramegna(Istituto Nazionale di Fisica Nucleare)
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