This HTML5 document contains 68 embedded RDF statements represented using HTML+Microdata notation.

The embedded RDF content will be recognized by any processor of HTML5 Microdata.

Namespace Prefixes

PrefixIRI
n19http://linked.opendata.cz/ontology/domain/vavai/riv/typAkce/
dctermshttp://purl.org/dc/terms/
n17http://purl.org/net/nknouf/ns/bibtex#
n4http://linked.opendata.cz/resource/domain/vavai/riv/tvurce/
n18http://linked.opendata.cz/ontology/domain/vavai/
n15http://linked.opendata.cz/resource/domain/vavai/zamer/
n12https://schema.org/
shttp://schema.org/
skoshttp://www.w3.org/2004/02/skos/core#
n3http://linked.opendata.cz/ontology/domain/vavai/riv/
n20http://linked.opendata.cz/resource/domain/vavai/vysledek/RIV%2F61389005%3A_____%2F10%3A00350640%21RIV11-AV0-61389005/
n2http://linked.opendata.cz/resource/domain/vavai/vysledek/
rdfhttp://www.w3.org/1999/02/22-rdf-syntax-ns#
n14http://linked.opendata.cz/ontology/domain/vavai/riv/klicoveSlovo/
n16http://linked.opendata.cz/ontology/domain/vavai/riv/duvernostUdaju/
xsdhhttp://www.w3.org/2001/XMLSchema#
n13http://linked.opendata.cz/ontology/domain/vavai/riv/aktivita/
n5http://linked.opendata.cz/ontology/domain/vavai/riv/jazykVysledku/
n9http://linked.opendata.cz/ontology/domain/vavai/riv/obor/
n7http://linked.opendata.cz/ontology/domain/vavai/riv/druhVysledku/
n6http://reference.data.gov.uk/id/gregorian-year/

Statements

Subject Item
n2:RIV%2F61389005%3A_____%2F10%3A00350640%21RIV11-AV0-61389005
rdf:type
skos:Concept n18:Vysledek
dcterms:description
The use of quasi-free reactions in studying nuclear reactions between charged particles of astrophysical interest has received much attention over the last two decades. The Trojan Horse Method is based on this approach and it has been used to study a number of reactions relevant for Nuclear Astrophysics. Recently we applied this method to the study of nuclear reactions that involve radioactive species, namely to the study of the F-18+p -> O-15+alpha process at temperatures corresponding to the energies available in the classical novae scenario. Quasi-free reactions can also be exploited to study processes induced by neutrons. This technique is particularly interesting when applied to reaction induced by neutrons on unstable short-lived nuclei. Such processes are very important in the nucleosynthesis of elements in the sand r-processes scenarios and this technique can give hints for solving key questions in nuclear astrophysics where direct measurements are practically impossible. The use of quasi-free reactions in studying nuclear reactions between charged particles of astrophysical interest has received much attention over the last two decades. The Trojan Horse Method is based on this approach and it has been used to study a number of reactions relevant for Nuclear Astrophysics. Recently we applied this method to the study of nuclear reactions that involve radioactive species, namely to the study of the F-18+p -> O-15+alpha process at temperatures corresponding to the energies available in the classical novae scenario. Quasi-free reactions can also be exploited to study processes induced by neutrons. This technique is particularly interesting when applied to reaction induced by neutrons on unstable short-lived nuclei. Such processes are very important in the nucleosynthesis of elements in the sand r-processes scenarios and this technique can give hints for solving key questions in nuclear astrophysics where direct measurements are practically impossible.
dcterms:title
Nuclear Astrophysics and Neutron Induced Reactions: Quasi-Free Reactions and RIBs Nuclear Astrophysics and Neutron Induced Reactions: Quasi-Free Reactions and RIBs
skos:prefLabel
Nuclear Astrophysics and Neutron Induced Reactions: Quasi-Free Reactions and RIBs Nuclear Astrophysics and Neutron Induced Reactions: Quasi-Free Reactions and RIBs
skos:notation
RIV/61389005:_____/10:00350640!RIV11-AV0-61389005
n3:aktivita
n13:Z
n3:aktivity
Z(AV0Z10480505)
n3:dodaniDat
n6:2011
n3:domaciTvurceVysledku
n4:6547362 n4:1494090
n3:druhVysledku
n7:D
n3:duvernostUdaju
n16:S
n3:entitaPredkladatele
n20:predkladatel
n3:idSjednocenehoVysledku
275548
n3:idVysledku
RIV/61389005:_____/10:00350640
n3:jazykVysledku
n5:eng
n3:klicovaSlova
Quasi-free reaction; nuclear astrophysics; neutron induced reaction
n3:klicoveSlovo
n14:neutron%20induced%20reaction n14:nuclear%20astrophysics n14:Quasi-free%20reaction
n3:kontrolniKodProRIV
[5980E89FD600]
n3:mistoKonaniAkce
Osaka
n3:mistoVydani
MELVILLE, NY
n3:nazevZdroje
10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES
n3:obor
n9:BG
n3:pocetDomacichTvurcuVysledku
2
n3:pocetTvurcuVysledku
29
n3:rokUplatneniVysledku
n6:2010
n3:tvurceVysledku
Kroha, Václav Lamiaa, L. Nishimura, S. Iwasa, N. Tumino, A. Sergi, M. L. Hammache, F. Coc, A. Spitaleri, C. La Cognata, M. Crucilla, V. Cherubini, S. Rapisarda, G. G. Puglia, S. De Sereville, N. Elekes, Z. Pizzone, R. G. Romano, S. Gulino, M. Kubono, S. Yamaguchi, H. Li, C. B. Komatsubara, H. Binh, D. N. Kato, S. Burjan, Václav Somorjai, E. Wakabayashi, Y. Hayakawa, S.
n3:typAkce
n19:WRD
n3:wos
000281986900014
n3:zahajeniAkce
2010-03-08+01:00
n3:zamer
n15:AV0Z10480505
s:numberOfPages
6
n17:hasPublisher
AMER INST PHYSICS, 2 HUNTINGTON QUADRANGLE, STE 1NO1
n12:isbn
978-0-7354-0819-7