Measurement of the 
Se77(n,γ)
 cross section up to 200 keV at the n_TOF facility at CERN

Sosnin, N. V.; Lederer-Woods, C.; Krtička, M.; Garg, R.; Dietz, M.; Bacak, M.; Barbagallo, M.; Battino, U.; Cristallo, S.; Damone, L. A.; Diakaki, M.; Heinitz, S.; Macina, D.; Mastromarco, M.; Mingrone, F.; Murphy, A. St. J.; Tagliente, G.; Valenta, S.; Vescovi, D.; Aberle, O.; Alcayne, V.; Amaducci, S.; Andrzejewski, J.; Audouin, L.; Bécares, V.; Babiano-Suarez, V.; Bečvář, F.; Bellia, G.; Berthoumieux, E.; Billowes, J.; Bosnar, D.; Brown, A.; Busso, M.; Caamaño, M.; Caballero, L.; Calviño, F.; Calviani, M.; Cano-Ott, D.; Casanovas, A.; Cerutti, F.; Chen, Y. H.; Chiaveri, E.; Colonna, N.; Cortés, G.; Cortés-Giraldo, M. A.; Cosentino, L.; Domingo-Pardo, C.; Dressler, R.; Dupont, E.; Durán, I.; Eleme, Z.; Fernández-Domínguez, B.; Ferrari, A.; Finocchiaro, P.; Göbel, K.; Gawlik-Ramięga, A.; Gilardoni, S.; Glodariu, T.; Gonçalves, I. F.; González-Romero, E.; Guerrero, C.; Gunsing, F.; Harada, H.; Heyse, J.; Jenkins, D. G.; Jericha, E.; Käppeler, F.; Kadi, Y.; Kimura, A.; Kivel, N.; Kokkoris, M.; Kurtulgil, D.; Ladarescu, I.; Leeb, H.; Lerendegui-Marco, J.; Lo Meo, S.; Lonsdale, S. J.; Manna, A.; Martínez, T.; Masi, A.; Massimi, C.; Mastinu, P.; Matteucci, F.; Maugeri, E. A.; Mazzone, A.; Mendoza, E.; Mengoni, A.; Michalopoulou, V.; Milazzo, P. M.; Musumarra, A.; Negret, A.; Nolte, R.; Ogállar, F.; Oprea, A.; Patronis, N.; Pavlik, A.; Perkowski, J.; Piersanti, L.; Porras, I.; Praena, J.; Quesada, J. M.; Radeck, D.; Ramos-Doval, D.; Rauscher, T.; Reifarth, R.; Rochman, D.; Rubbia, C.; Sabaté-Gilarte, M.; Saxena, A.; Schillebeeckx, P.; Schumann, D.; Smith, A. G.; Stamatopoulos, A.; Tain, J. L.; Talip, T.; Tarifeño-Saldivia, A.; Tassan-Got, L.; Torres-Sánchez, P.; Tsinganis, A.; Ulrich, J.; Urlass, S.; Vannini, G.; Variale, V.; Vaz, P.; Ventura, A.; Vlachoudis, V.; Vlastou, R.; Wallner, A.; Woods, P. J.; Wright, T.; Žugec, P.; Null, Null

doi:10.1103/physrevc.107.065805

The 77Se(n, & gamma;) reaction is of importance for 77Se abundance during the slow neutron capture process in massive stars. We have performed a new measurement of the 77Se radiative neutron capture cross section at the Neutron Time-of-Flight facility at CERN. Resonance capture kernels were derived up to 51 keV and cross sections up to 200 keV. Maxwellian-averaged cross sections were calculated for stellar temperatures between kT = 5 keV and kT = 100 keV, with uncertainties between 4.2% and 5.7%. Our results lead to substantial decreases of 14% and 19% in 77Se abundances produced through the slow neutron capture process in selected stellar models of 15M0 and 2M0, respectively, compared to using previous recommendation of the cross section.

Sosnin, N.V., Lederer-Woods, C., Krtička, M., Garg, R., Dietz, M., Bacak, M., et al. (2023). Measurement of the Se77(n,γ) cross section up to 200 keV at the n_TOF facility at CERN. PHYSICAL REVIEW C, 107(6), 1-9 [10.1103/physrevc.107.065805].

Measurement of the Se77(n,γ) cross section up to 200 keV at the n_TOF facility at CERN

Sosnin, N. V.;Lederer-Woods, C.;Krtička, M.;Garg, R.;Dietz, M.;Bacak, M.;Barbagallo, M.;Battino, U.;Cristallo, S.;Damone, L. A.;Diakaki, M.;Heinitz, S.;Macina, D.;Mastromarco, M.;Mingrone, F.;Murphy, A. St. J.;Tagliente, G.;Valenta, S.;Vescovi, D.;Aberle, O.;Alcayne, V.;Amaducci, S.;Andrzejewski, J.;Audouin, L.;Bécares, V.;Babiano-Suarez, V.;Bečvář, F.;Bellia, G.;Berthoumieux, E.;Billowes, J.;Bosnar, D.;Brown, A.;Busso, M.;Caamaño, M.;Caballero, L.;Calviño, F.;Calviani, M.;Cano-Ott, D.;Casanovas, A.;Cerutti, F.;Chen, Y. H.;Chiaveri, E.;Colonna, N.;Cortés, G.;Cortés-Giraldo, M. A.;Cosentino, L.;Domingo-Pardo, C.;Dressler, R.;Dupont, E.;Durán, I.;Eleme, Z.;Fernández-Domínguez, B.;Ferrari, A.;Finocchiaro, P.;Göbel, K.;Gawlik-Ramięga, A.;Gilardoni, S.;Glodariu, T.;Gonçalves, I. F.;González-Romero, E.;Guerrero, C.;Gunsing, F.;Harada, H.;Heyse, J.;Jenkins, D. G.;Jericha, E.;Käppeler, F.;Kadi, Y.;Kimura, A.;Kivel, N.;Kokkoris, M.;Kurtulgil, D.;Ladarescu, I.;Leeb, H.;Lerendegui-Marco, J.;Lo Meo, S.;Lonsdale, S. J.;Manna, A.;Martínez, T.;Masi, A.;Massimi, C.^{Writing – Review & Editing};Mastinu, P.;Matteucci, F.;Maugeri, E. A.;Mazzone, A.;Mendoza, E.;Mengoni, A.;Michalopoulou, V.;Milazzo, P. M.;Musumarra, A.;Negret, A.;Nolte, R.;Ogállar, F.;Oprea, A.;Patronis, N.;Pavlik, A.;Perkowski, J.;Piersanti, L.;Porras, I.;Praena, J.;Quesada, J. M.;Radeck, D.;Ramos-Doval, D.;Rauscher, T.;Reifarth, R.;Rochman, D.;Rubbia, C.;Sabaté-Gilarte, M.;Saxena, A.;Schillebeeckx, P.;Schumann, D.;Smith, A. G.;Stamatopoulos, A.;Tain, J. L.;Talip, T.;Tarifeño-Saldivia, A.;Tassan-Got, L.;Torres-Sánchez, P.;Tsinganis, A.;Ulrich, J.;Urlass, S.;Vannini, G.;Variale, V.;Vaz, P.;Ventura, A.;Vlachoudis, V.;Vlastou, R.;Wallner, A.;Woods, P. J.;Wright, T.;Žugec, P.;null, null

2023

Abstract

The 77Se(n, & gamma;) reaction is of importance for 77Se abundance during the slow neutron capture process in massive stars. We have performed a new measurement of the 77Se radiative neutron capture cross section at the Neutron Time-of-Flight facility at CERN. Resonance capture kernels were derived up to 51 keV and cross sections up to 200 keV. Maxwellian-averaged cross sections were calculated for stellar temperatures between kT = 5 keV and kT = 100 keV, with uncertainties between 4.2% and 5.7%. Our results lead to substantial decreases of 14% and 19% in 77Se abundances produced through the slow neutron capture process in selected stellar models of 15M0 and 2M0, respectively, compared to using previous recommendation of the cross section.

Scheda breve

Scheda completa

Scheda completa (DC)

	Anno
	
				2023
			
	Rivista
	
				PHYSICAL REVIEW C
			
	Codice DOI
	
				https://dx.doi.org/10.1103/physrevc.107.065805
			
	Citazione
	
				Sosnin, N.V., Lederer-Woods, C., Krtička, M., Garg, R., Dietz, M., Bacak, M., et al. (2023). Measurement of the 
Se77(n,γ)
 cross section up to 200 keV at the n_TOF facility at CERN. PHYSICAL REVIEW C, 107(6), 1-9 [10.1103/physrevc.107.065805].
			
	Tutti gli autori
	
						Sosnin, N. V.; Lederer-Woods, C.; Krtička, M.; Garg, R.; Dietz, M.; Bacak, M.; Barbagallo, M.; Battino, U.; Cristallo, S.; Damone, L. A.; Diakaki, M.;...espandi
						
	Appare nelle tipologie:
	
				1.01 Articolo in rivista

File in questo prodotto:

File	Dimensione	Formato
PhysRevC.107.065805.pdf accesso aperto Tipo: Versione (PDF) editoriale Licenza: Licenza per Accesso Aperto. Creative Commons Attribuzione (CCBY) Dimensione 698.91 kB Formato Adobe PDF Visualizza/Apri	698.91 kB	Adobe PDF	Visualizza/Apri

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/961164

Citazioni

ND

0

0

CRIS Current Research Information System

Measurement of the Se77(n,γ) cross section up to 200 keV at the n_TOF facility at CERN

Writing – Review & Editing

2023

Abstract

Scheda breve

Scheda completa

Scheda completa (DC)

Citazioni

social impact

CRIS Current Research Information System

Measurement of the Se77(n,γ) cross section up to 200 keV at the n_TOF facility at CERN

Writing – Review & Editing

2023

Abstract

Scheda breve Scheda completa Scheda completa (DC)

Informazioni

Citazioni

social impact

Conferma cancellazione

Scheda breve

Scheda completa

Scheda completa (DC)