dc.contributor.author |
Tagliente, G |
en |
dc.contributor.author |
Milazzo, PM |
en |
dc.contributor.author |
Fujii, K |
en |
dc.contributor.author |
Abbondanno, U |
en |
dc.contributor.author |
Aerts, G |
en |
dc.contributor.author |
Alvarez, H |
en |
dc.contributor.author |
Alvarez-Velarde, F |
en |
dc.contributor.author |
Andriamonje, S |
en |
dc.contributor.author |
Andrzejewski, J |
en |
dc.contributor.author |
Audouin, L |
en |
dc.contributor.author |
Badurek, G |
en |
dc.contributor.author |
Baumann, P |
en |
dc.contributor.author |
Becvar, F |
en |
dc.contributor.author |
Belloni, F |
en |
dc.contributor.author |
Berthoumieux, E |
en |
dc.contributor.author |
Calvino, F |
en |
dc.contributor.author |
Calviani, M |
en |
dc.contributor.author |
Cano-Ott, D |
en |
dc.contributor.author |
Capote, R |
en |
dc.contributor.author |
Carrapico, C |
en |
dc.contributor.author |
Cennini, P |
en |
dc.contributor.author |
Chepel, V |
en |
dc.contributor.author |
Chiaveri, E |
en |
dc.contributor.author |
Colonna, N |
en |
dc.contributor.author |
Cortes, G |
en |
dc.contributor.author |
Couture, A |
en |
dc.contributor.author |
Dahlfors, M |
en |
dc.contributor.author |
David, S |
en |
dc.contributor.author |
Dillmann, I |
en |
dc.contributor.author |
Domingo-Pardo, C |
en |
dc.contributor.author |
Dridi, W |
en |
dc.contributor.author |
Duran, I |
en |
dc.contributor.author |
Eleftheriadis, C |
en |
dc.contributor.author |
Embid-Segura, M |
en |
dc.contributor.author |
Ferrari, A |
en |
dc.contributor.author |
Ferreira-Marques, R |
en |
dc.contributor.author |
Furman, W |
en |
dc.contributor.author |
Goncalves, I |
en |
dc.contributor.author |
Gonzalez-Romero, E |
en |
dc.contributor.author |
Gramegna, F |
en |
dc.contributor.author |
Guerrero, C |
en |
dc.contributor.author |
Gunsing, F |
en |
dc.contributor.author |
Haas, B |
en |
dc.contributor.author |
Haight, R |
en |
dc.contributor.author |
Heil, M |
en |
dc.contributor.author |
Herrera-Martinez, A |
en |
dc.contributor.author |
Jericha, E |
en |
dc.contributor.author |
Kappeler, F |
en |
dc.contributor.author |
Kadi, Y |
en |
dc.contributor.author |
Karadimos, D |
en |
dc.contributor.author |
Karamanis, D |
en |
dc.contributor.author |
Kerveno, M |
en |
dc.contributor.author |
Kossionides, E |
en |
dc.contributor.author |
Krticka, M |
en |
dc.contributor.author |
Lamboudis, C |
en |
dc.contributor.author |
Leeb, H |
en |
dc.contributor.author |
Lindote, A |
en |
dc.contributor.author |
Lopes, I |
en |
dc.contributor.author |
Lukic, S |
en |
dc.contributor.author |
Marganiec, J |
en |
dc.contributor.author |
Marrone, S |
en |
dc.contributor.author |
Martinez, T |
en |
dc.contributor.author |
Massimi, C |
en |
dc.contributor.author |
Mastinu, P |
en |
dc.contributor.author |
Mengoni, A |
en |
dc.contributor.author |
Moreau, C |
en |
dc.contributor.author |
Mosconi, M |
en |
dc.contributor.author |
Neves, F |
en |
dc.contributor.author |
Oberhummer, H |
en |
dc.contributor.author |
O'Brien, S |
en |
dc.contributor.author |
Pancin, J |
en |
dc.contributor.author |
Papachristodoulou, C |
en |
dc.contributor.author |
Papadopoulos, C |
en |
dc.contributor.author |
Paradela, C |
en |
dc.contributor.author |
Patronis, N |
en |
dc.contributor.author |
Pavlik, A |
en |
dc.contributor.author |
Pavlopoulos, P |
en |
dc.contributor.author |
Perrot, L |
en |
dc.contributor.author |
Pigni, MT |
en |
dc.contributor.author |
Plag, R |
en |
dc.contributor.author |
Plompen, A |
en |
dc.contributor.author |
Plukis, A |
en |
dc.contributor.author |
Poch, A |
en |
dc.contributor.author |
Praena, J |
en |
dc.contributor.author |
Pretel, C |
en |
dc.contributor.author |
Quesada, J |
en |
dc.contributor.author |
Reifarth, R |
en |
dc.contributor.author |
Rosetti, M |
en |
dc.contributor.author |
Rubbia, C |
en |
dc.contributor.author |
Rudolf, G |
en |
dc.contributor.author |
Rullhusen, P |
en |
dc.contributor.author |
Salgado, J |
en |
dc.contributor.author |
Santos, C |
en |
dc.contributor.author |
Sarchiapone, L |
en |
dc.contributor.author |
Savvidis, I |
en |
dc.contributor.author |
Stephan, C |
en |
dc.contributor.author |
Tain, JL |
en |
dc.contributor.author |
Tassan-Got, L |
en |
dc.contributor.author |
Tavora, L |
en |
dc.contributor.author |
Terlizzi, R |
en |
dc.contributor.author |
Vannini, G |
en |
dc.contributor.author |
Vaz, P |
en |
dc.contributor.author |
Ventura, A |
en |
dc.contributor.author |
Villamarin, D |
en |
dc.contributor.author |
Vincente, MC |
en |
dc.contributor.author |
Vlachoudis, V |
en |
dc.contributor.author |
Vlastou, R |
en |
dc.contributor.author |
Voss, F |
en |
dc.contributor.author |
Walter, S |
en |
dc.contributor.author |
Wiescher, M |
en |
dc.contributor.author |
Wisshak, K |
en |
dc.date.accessioned |
2014-03-01T02:07:08Z |
|
dc.date.available |
2014-03-01T02:07:08Z |
|
dc.date.issued |
2011 |
en |
dc.identifier.issn |
0556-2813 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/29522 |
|
dc.subject.classification |
Physics, Nuclear |
en |
dc.subject.other |
GIANT BRANCH STARS |
en |
dc.subject.other |
CAPTURE CROSS-SECTIONS |
en |
dc.subject.other |
S-PROCESS NUCLEOSYNTHESIS |
en |
dc.subject.other |
NEUTRON-CAPTURE |
en |
dc.subject.other |
MASSIVE STARS |
en |
dc.subject.other |
PRIMITIVE METEORITES |
en |
dc.subject.other |
STATISTICAL-MODEL |
en |
dc.subject.other |
NUCLEAR-SCIENCE |
en |
dc.subject.other |
SILICON-CARBIDE |
en |
dc.subject.other |
ELEMENTS |
en |
dc.title |
Zr-96(n,gamma) measurement at the n_TOF facility at CERN |
en |
heal.type |
journalArticle |
en |
heal.identifier.secondary |
055802 |
en |
heal.language |
English |
en |
heal.publicationDate |
2011 |
en |
heal.abstract |
The (n,gamma) cross section of Zr-96 has been investigated at the CERN n_TOF spallation neutron source. High-resolution time-of-flight measurements using an enriched ZrO2 sample allowed us to analyze 15 resonances below 40 keV with improved accuracy. On average, the capture widths were found to be 25% smaller than reported in earlier experiments. If complemented with the contribution by direct radiative capture, the derived Maxwellian averaged cross sections are consistent with activation data at kT = 25 keV. The present results confirm the astrophysical implications for the s-process branching at Zr-95. |
en |
heal.publisher |
AMER PHYSICAL SOC |
en |
heal.journalName |
PHYSICAL REVIEW C |
en |
dc.identifier.isi |
ISI:000297121100005 |
en |
dc.identifier.volume |
84 |
en |
dc.identifier.issue |
5 |
en |