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Statements

Subject Item
n2:RIV%2F61389005%3A_____%2F13%3A00391535%21RIV14-MSM-61389005
rdf:type
skos:Concept n13:Vysledek
rdfs:seeAlso
http://prc.aps.org/pdf/PRC/v87/i1/e012801
dcterms:description
The reaction O-17(n, alpha)C-14 was studied at energies from E-c.m. = 0 to E-c.m. = 350 keV by using the quasifree deuteron breakup in the three-body reaction O-17 + d -> alpha + C-14 + p, which extended the Trojan Horse indirect method (THM) to neutron-induced reactions. It is found that the O-18 excited state at E* = 8.125 +/- 0.002 MeV, observed in THM experiments, is absent in the direct measurement because of its high centrifugal barrier. The angular distributions of the populated resonances have been measured by using this method. The results unambiguously indicate the ability of the THM to overcome the centrifugal barrier suppression effect and to pick out the contribution of the bare nuclear interaction. The reaction O-17(n, alpha)C-14 was studied at energies from E-c.m. = 0 to E-c.m. = 350 keV by using the quasifree deuteron breakup in the three-body reaction O-17 + d -> alpha + C-14 + p, which extended the Trojan Horse indirect method (THM) to neutron-induced reactions. It is found that the O-18 excited state at E* = 8.125 +/- 0.002 MeV, observed in THM experiments, is absent in the direct measurement because of its high centrifugal barrier. The angular distributions of the populated resonances have been measured by using this method. The results unambiguously indicate the ability of the THM to overcome the centrifugal barrier suppression effect and to pick out the contribution of the bare nuclear interaction.
dcterms:title
Suppression of the centrifugal barrier effects in the off-energy-shell neutron plus O-17 interaction Suppression of the centrifugal barrier effects in the off-energy-shell neutron plus O-17 interaction
skos:prefLabel
Suppression of the centrifugal barrier effects in the off-energy-shell neutron plus O-17 interaction Suppression of the centrifugal barrier effects in the off-energy-shell neutron plus O-17 interaction
skos:notation
RIV/61389005:_____/13:00391535!RIV14-MSM-61389005
n13:predkladatel
n14:ico%3A61389005
n3:aktivita
n19:I n19:P
n3:aktivity
I, P(GAP203/10/0310), P(LH11001), P(LM2011019)
n3:cisloPeriodika
1
n3:dodaniDat
n11:2014
n3:domaciTvurceVysledku
n12:6547362 n12:1494090 n12:9723633 n12:3528871
n3:druhVysledku
n16:J
n3:duvernostUdaju
n6:S
n3:entitaPredkladatele
n15:predkladatel
n3:idSjednocenehoVysledku
109058
n3:idVysledku
RIV/61389005:_____/13:00391535
n3:jazykVysledku
n17:eng
n3:klicovaSlova
cross-section; nuclear astrophysics; Trojan Horse
n3:klicoveSlovo
n5:nuclear%20astrophysics n5:cross-section n5:Trojan%20Horse
n3:kodStatuVydavatele
US - Spojené státy americké
n3:kontrolniKodProRIV
[68732DE20E2D]
n3:nazevZdroje
Physical Review. C
n3:obor
n18:BG
n3:pocetDomacichTvurcuVysledku
4
n3:pocetTvurcuVysledku
29
n3:projekt
n4:LH11001 n4:LM2011019 n4:GAP203%2F10%2F0310
n3:rokUplatneniVysledku
n11:2013
n3:svazekPeriodika
87
n3:tvurceVysledku
Sergi, M. L. Fang, X. Couder, M. Rapisarda, G. G. Cherubini, S. Mrázek, Jaromír Wiescher, M. Gulino, M. Ma, C. Mukhamedzhanov, A. M. Lamm, L. Spitaleri, C. Tang, X D. de Boer, R. Notani, M. Tan, W. Guardo, G. L. Goldberg, V. Z. Kroha, Václav Pizzone, R. G. O'Brien, S. Davies, P. Lamia, L. Roberson, D. Thompson, I. J. Hons, Zdeněk Burjan, Václav Li, C. La Cognata, M.
n3:wos
000313159100001
s:issn
0556-2813
s:numberOfPages
5
n10:doi
10.1103/PhysRevC.87.012801