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3 search hits
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- 238U(n, γ) reaction cross section measurement with C6D6 detectors at the n_TOF CERN facility (2014)
- Federica Mingrone Cristian Massimi Gianni Vannini Sebastian Altstadt Józef Andrzejewski Ludmila Audouin Massimo Barbagallo Vicente Bécares František Bečvář Fabio Belloni Eric Berthoumieux Jonathan Billowes Damir Bosnar Markus Brugger Marco Calviani Francisco Calviño Tavares Daniel Cano-Ott Carlos Carrapiço Francesco Cerutti Enrico Chiaveri Mary Chin Nicola Colonna Guillem Cortés Miguel Antonio Cortés-Giraldo Mary Diakaki César Domingo-Pardo Ignacio Duran Rugard Dressler Christos Eleftheriadis Alfredo Ferrari Kevin Fraval Srinivasan Ganesan Aczel Regino García Giuseppe Giubrone Isabel F. Gonçalves Enrique González Romero Erich Griesmayer Carlos Guerrero Frank Gunsing Alvaro Hernández Prieto David G. Jenkins Erwin Jericha Yacine Kadi Franz Käppeler Dimitri Karadimos Nikolai Kivel Paul Edward Koehler Milan Krtička Jiří Kroll Christos Lampoudis Christoph Langer Esther Leal Cidoncha Claudia Lederer Helmut Leeb Lou Sai Leong Roberto Losito Amod K. Mallick Athanasios Manousos Justyna Marganiec Trinitario Martínez Pier Francesco Mastinu Mario Mastromarco Emilio Mendoza Cembranos Alberto Mengoni Paolo Maria Milazzo Mihail Mirea Willy Mondalaers Carlos Paradela Dobarro Andreas Pavlik Jaroslaw Perkowski Arjan J. M. Plompen Javier Praena José Manuel Quesada Molina Thomas Rauscher René Reifarth Albert Riego Pérez Marisol S. Robles Carlo Rubbia Marta Sabaté Gilarte Raul Sarmento Alok Saxena Peter Schillebeeckx Sebastian Schmidt Dorothea Schumann Giuseppe Tagliente Jose Luis Tain Diego Tarrío Laurent Tassan-Got Andrea Tsinganis Stanislav Valenta Vincenzo Variale Pedro Vaz Alberto Ventura Mark J. Vermeulen Vasilis Vlachoudis Rosa Vlastou Anton Wallner Timothy Ware Mario Weigand Christina Weiß Tobias Wright Petar Žugec
- The radiative capture cross section of 238U is very important for the developing of new reactor technologies and the safety of existing ones. Here the preliminary results of the 238U(n,γ) cross section measurement performed at n_TOF with C6D6 scintillation detectors are presented, paying particular attention to data reduction and background subtraction.
- The nucleosynthesis of heavy elements in Stars: the key isotope 25Mg (2014)
- Cristian Massimi Paul Edward Koehler Stefan Kopecky Federica Mingrone Peter Schillebeeckx Gianni Vannini Sebastian Altstadt Józef Andrzejewski Ludmila Audouin Massimo Barbagallo Vicente Bécares František Bečvář Fabio Belloni Eric Berthoumieux Jonathan Billowes Damir Bosnar Markus Brugger Marco Calviani Francisco Calviño Tavares Daniel Cano-Ott Carlos Carrapiço Francesco Cerutti Enrico Chiaveri Mary Chin Nicola Colonna Christos Eleftheriadis Alfredo Ferrari Kevin Fraval Srinivasan Ganesan Aczel Regino García Giuseppe Giubrone Isabel F. Gonçalves Enrique González Romero Erich Griesmayer Carlos Guerrero Frank Gunsing Alvaro Hernández Prieto David G. Jenkins Erwin Jericha Yacine Kadi Franz Käppeler Dimitri Karadimos Nikolai Kivel Milan Krtička Jiří Kroll Christos Lampoudis Christoph Langer Esther Leal Cidoncha Claudia Lederer Helmut Leeb Lou Sai Leong Roberto Losito Amod K. Mallick Athanasios Manousos Justyna Marganiec Trinitario Martínez Pier Francesco Mastinu Mario Mastromarco Emilio Mendoza Cembranos Alberto Mengoni Paolo Maria Milazzo Mihail Mirea Willy Mondalaers Carlos Paradela Dobarro Andreas Pavlik Jaroslaw Perkowski Arjan J. M. Plompen Javier Praena José Manuel Quesada Molina Thomas Rauscher René Reifarth Albert Riego Pérez Marisol S. Robles Carlo Rubbia Marta Sabaté Gilarte Raul Sarmento Alok Saxena Sebastian Schmidt Dorothea Schumann Giuseppe Tagliente Jose Luis Tain Diego Tarrío Laurent Tassan-Got Andrea Tsinganis Stanislav Valenta Vincenzo Variale Pedro Vaz Alberto Ventura Mark J. Vermeulen Vasilis Vlachoudis Rosa Vlastou Anton Wallner Timothy Ware Mario Weigand Christina Weiß Tobias Wright Petar Žugec
- We have measured the radiative neutron-capture cross section and the total neutron-induced cross section of one of the most important isotopes for the s process, the 25Mg. The measurements have been carried out at the neutron time-of-flight facilities n_TOF at CERN (Switzerland) and GELINA installed at the EC-JRC-IRMM (Belgium). The cross sections as a function of neutron energy have been measured up to approximately 300 keV, covering the energy region of interest to the s process. The data analysis is ongoing and preliminary results show the potential relevance for the s process.
- Destruction of the cosmic γ-ray emitter 26Al in massive stars: study of the key 26Al(n,p) reaction (2021)
- Claudia Lederer-Woods Philip John Woods Thomas Davinson David Kahl Sarah Jane Lonsdale Oliver Aberle Simone Amaducci Józef Andrzejewski Laurent Audouin Michael Bacak Javier Balibrea-Correa Massimo Barbagallo František Bečvář Eric Berthoumieux Jon Billowes Damir Bosnar Adam Brown Manuel Caamaño Francisco Calviño Marco Calviani Daniel Cano-Ott Roberto Cardella Adria Casanovas Francesco Cerutti Y. H. Chen Enrico Chiaveri Nicola Colonna Guillem Cortés Miguel Antonio Cortés-Giraldo Luigi Cosentino Sergio Cristallo Lucia Anna Damone Maria Diakaki Cesar Domingo-Pardo Rugard Dressler Emmeric Dupont Ignacio Durán Beatriz Fernández-Domínguez Alfredo Ferrari Paulo Ferreira Francesc J. Ferrer Paolo Finocchiaro Valter Furman Kathrin Göbel Aczel Regino García Aleksandra Gawlik Simone Gilardoni Tudor Glodariu Isabel F. Gonçalves Enrique González-Romero Erich Griesmayer Carlos Guerrero Frank Gunsing Hideo Harada Stephan Heinitz Jan Heyse David G. Jenkins Erwin Jericha Franz Käppeler Yacine Kadi Antigoni Kalamara Pavel Kavrigin Atsushi Kimura Nikolai Kivel Michael Kokkoris Milan Krtička Deniz Kurtulgil E. Leal-Cidoncha Helmut Leeb Jorge Lerendegui-Marco Sergio Lo Meo Daniela Macina Alice Manna Justyna Marganiec Trinitario Martínez Alessandro Masi Cristian Massimi Pierfrancesco Mastinu Mario Mastromarco Emilio-Andrea Maugeri Annamaria Mazzone Emilio Mendoza Alberto Mengoni Paolo M. Milazzo Federica Mingrone Agatino Musumarra Alexandru Negret Ralf Nolte Andreea Oprea Nikolas Patronis Andreas Pavlik Jarosław Perkowski Ignacio Porras Javier Praena José-Manuel Quesada Desiree Radeck Thomas Rauscher René Reifarth Carlo Rubbia James A. Ryan Marta Sabaté-Gilarte Alok Saxena Peter Schillebeeckx Dorothea Schumann Pavel V. Sedyshev Alastair G. Smith Nikolay V. Sosnin Athanasios Stamatopoulos Giuseppe Tagliente José L. Tain Ariel Tarifeño-Saldivia Laurent Tassan-Got Stanislav Valenta Gianni Vannini Vincenzo Variale Pedro Vaz Alberto Ventura Vasilis Vlachoudis Rosa Vlastou Anton Wallner Stuart Warren Christina Weß Tobias Wright Petar Žugec
- The 26Al(n,p)26Mg reaction is the key reaction impacting on the abundances of the cosmic γ-ray emitter 26Al produced in massive stars and impacts on the potential pollution of the early solar system with 26Al by asymptotic giant branch stars. We performed a measurement of the 26Al(n,p)26Mg cross section at the high-flux beam line EAR-2 at the n_TOF facility (CERN). We report resonance strengths for eleven resonances, nine being measured for the first time, while there is only one previous measurement for the other two. Our resonance strengths are significantly lower than the only previous values available. Our cross-section data range to 150 keV neutron energy, which is sufficient for a reliable determination of astrophysical reactivities up to 0.5 GK stellar temperature.
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