The nucleosynthesis of heavy elements in Stars: The key isotope 25Mg

Massimi, Cristian; Koehler, P.; Kopecky, S.; Mingrone, Federica; Schillebeeckx, P.; Vannini, G.; Altstadt, S.; Andrzejewski, J.; Audouin, L.; Barbagallo, M.; Bécares, V.; Bečvář, F.; Belloni, F.; Berthoumieux, E.; Billowes, J.; Bosnar, D.; Brugger, M.; Calviani, M.; Calviño, F.; Cano Ott, D.; Carrapiço, C.; Cerutti, F.; Chiaveri, E.; Chin, M.; Colonna, N.; Cortés, G.; Cortés Giraldo, M. A.; Diakaki, M.; Domingo Pardo, C.; Duran, I.; Dressler, R.; Eleftheriadis, C.; Ferrari, A.; Fraval, K.; Ganesan, S.; García, A. R.; Giubrone, G.; Gonçalves, I. F.; González Romero, E.; Griesmayer, E.; Guerrero, C.; Gunsing, F.; Hernández Prieto, A.; Jenkins, D. G.; Jericha, E.; Kadi, Y.; Käppeler, F.; Karadimos, D.; Kivel, N.; Krtička, M.; Kroll, J.; Lampoudis, C.; Langer, C.; Leal Cidoncha, E.; Lederer, C.; Leeb, H.; Leong, L. S.; Losito, R.; Mallick, A.; Manousos, A.; Marganiec, J.; Martínez, T.; Mastinu, P. F.; Mastromarco, M.; Mendoza, E.; Mengoni, A.; Milazzo, P. M.; Mirea, M.; Mondalaers, W.; Paradela, C.; Pavlik, A.; Perkowski, J.; Plompen, A.; Praena, J.; Quesada, J. M.; Rauscher, T.; Reifarth, R.; Riego, A.; Robles, M. S.; Rubbia, C.; Sabaté Gilarte, M.; Sarmento, R.; Saxena, A.; Schmidt, S.; Schumann, D.; Tagliente, G.; Tain, J. L.; Tarrío, D.; Tassan Got, L.; Tsinganis, A.; Valenta, S.; Variale, V.; Vaz, P.; Ventura, A.; Vermeulen, M. J.; Vlachoudis, V.; Vlastou, R.; Wallner, A.; Ware, T.; Weigand, M.; Weiß, C.; Wright, T.; Žugec, P.

doi:10.1051/epjconf/20146607016

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. © Owned by the authors, published by EDP Sciences, 2014.

Massimi, C., Koehler, P., Kopecky, S., Mingrone, F., Schillebeeckx, P., Vannini, G., et al. (2014). The nucleosynthesis of heavy elements in Stars: The key isotope 25Mg [10.1051/epjconf/20146607016].

The nucleosynthesis of heavy elements in Stars: The key isotope 25Mg

MASSIMI, CRISTIAN;Koehler, P.;Kopecky, S.;MINGRONE, FEDERICA;Schillebeeckx, P.;Vannini, G.;Altstadt, S.;Andrzejewski, J.;Audouin, L.;Barbagallo, M.;Bécares, V.;Bečvář, F.;Belloni, F.;Berthoumieux, E.;Billowes, J.;Bosnar, D.;Brugger, M.;Calviani, M.;Calviño, F.;Cano Ott, D.;Carrapiço, C.;Cerutti, F.;Chiaveri, E.;Chin, M.;Colonna, N.;Cortés, G.;Cortés Giraldo, M. A.;Diakaki, M.;Domingo Pardo, C.;Duran, I.;Dressler, R.;Eleftheriadis, C.;Ferrari, A.;Fraval, K.;Ganesan, S.;García, A. R.;Giubrone, G.;Gonçalves, I. F.;González Romero, E.;Griesmayer, E.;Guerrero, C.;Gunsing, F.;Hernández Prieto, A.;Jenkins, D. G.;Jericha, E.;Kadi, Y.;Käppeler, F.;Karadimos, D.;Kivel, N.;Krtička, M.;Kroll, J.;Lampoudis, C.;Langer, C.;Leal Cidoncha, E.;Lederer, C.;Leeb, H.;Leong, L. S.;Losito, R.;Mallick, A.;Manousos, A.;Marganiec, J.;Martínez, T.;Mastinu, P. F.;Mastromarco, M.;Mendoza, E.;Mengoni, A.;Milazzo, P. M.;Mirea, M.;Mondalaers, W.;Paradela, C.;Pavlik, A.;Perkowski, J.;Plompen, A.;Praena, J.;Quesada, J. M.;Rauscher, T.;Reifarth, R.;Riego, A.;Robles, M. S.;Rubbia, C.;Sabaté Gilarte, M.;Sarmento, R.;Saxena, A.;Schmidt, S.;Schumann, D.;Tagliente, G.;Tain, J. L.;Tarrío, D.;Tassan Got, L.;Tsinganis, A.;Valenta, S.;Variale, V.;Vaz, P.;Ventura, A.;Vermeulen, M. J.;Vlachoudis, V.;Vlastou, R.;Wallner, A.;Ware, T.;Weigand, M.;Weiß, C.;Wright, T.;Žugec, P.

2014

Abstract

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. © Owned by the authors, published by EDP Sciences, 2014.

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	Anno
	
				2014
			
	Titolo del volume
	
				EPJ Web of Conferences
			
	Pagina iniziale
	
				07016
			
	Pagina finale
	
				07019
			
	Rivista
	
				EPJ WEB OF CONFERENCES
			
	Codice DOI
	
				https://dx.doi.org/10.1051/epjconf/20146607016
			
	Citazione
	
				Massimi, C., Koehler, P., Kopecky, S., Mingrone, F., Schillebeeckx, P., Vannini, G., et al. (2014). The nucleosynthesis of heavy elements in Stars: The key isotope 25Mg [10.1051/epjconf/20146607016].
			
	Tutti gli autori
	
						Massimi, C.; Koehler, P.; Kopecky, S.; Mingrone, F.; Schillebeeckx, P.; Vannini, G.; Altstadt, S.; Andrzejewski, J.; Audouin, L.; Barbagallo, M.; Béca...espandi
						
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/571873

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