Matches in SemOpenAlex for { <https://semopenalex.org/work/W1528584793> ?p ?o ?g. }
Showing items 1 to 81 of
81
with 100 items per page.
- W1528584793 abstract "Isotopically enriched {sup 129}I (85% {sup 129}I and 15% {sup 127}I), {sup 237}Np, and {sup 241}Am targets were irradiated with a beam of 660-MeV protons at the JINR DLNP Phasotron and cross sections of formation of 207 residual products (74 from {sup 129}I, 53 from {sup 237}Np, and 80 from {sup 241}Am) were determined using the {gamma}-spectrometry method. Here, they analyze all these data using eleven different models, realized in eight codes: LAHET (Bertini, ISABEL, INCL+ABLA, and INCL+RAL options), CASCADE, CEM95, CEM2k, LAQGSM+GEM2, CEM2k+GEM2, LAQGSM+GEMINI, and CEM2k+GEMINI, in order to validate the tested models against the experimental data and to understand better the mechanisms for production of residual nuclei. The agreement of different models with the data varies quite a bit. They find that most of the codes are fairly reliable in predicting cross sections for nuclides not too far away in mass from the targets, but differ greatly in the deep spallation, fission, and fragmentation regions. None of the codes tested here except GEMINI allow fission of nuclei as light as iodine, therefore the best agreement with the {sup 129}I data, especially in the A = 40-90 region, is shown by the codes CEM2k and LAQGSM when they aremore » merged with GEMINI. At the same time, GEMINI is not yet very reliable for an accurate description of actinides and the {sup 237}Np and {sup 241}Am data are reproduced better by LAHET (Bertini, ISABEL, or INCL+RAL/ABLA options), and by CEM2k and LAQGSM merged with GEM2 and not so well when using GEMINI. They conclude that none of the codes tested here are able to reproduce well all these data and all of them need to be further improved; development of a better universal evaporation/fission model should be of a high priority.« less" @default.
- W1528584793 created "2016-06-24" @default.
- W1528584793 creator A5006471132 @default.
- W1528584793 creator A5013159315 @default.
- W1528584793 creator A5014392551 @default.
- W1528584793 creator A5015700144 @default.
- W1528584793 creator A5027393147 @default.
- W1528584793 creator A5036979736 @default.
- W1528584793 creator A5044537097 @default.
- W1528584793 creator A5053541100 @default.
- W1528584793 creator A5060944739 @default.
- W1528584793 creator A5064635321 @default.
- W1528584793 creator A5064851399 @default.
- W1528584793 creator A5072277718 @default.
- W1528584793 creator A5076268307 @default.
- W1528584793 creator A5091513176 @default.
- W1528584793 date "2004-01-01" @default.
- W1528584793 modified "2023-09-29" @default.
- W1528584793 title "Analysis of the JINR p(660 MeV) + [sup 129]I, [sup 23]Np, and [sup 231]Am measurements with eleven different models" @default.
- W1528584793 hasPublicationYear "2004" @default.
- W1528584793 type Work @default.
- W1528584793 sameAs 1528584793 @default.
- W1528584793 citedByCount "0" @default.
- W1528584793 crossrefType "journal-article" @default.
- W1528584793 hasAuthorship W1528584793A5006471132 @default.
- W1528584793 hasAuthorship W1528584793A5013159315 @default.
- W1528584793 hasAuthorship W1528584793A5014392551 @default.
- W1528584793 hasAuthorship W1528584793A5015700144 @default.
- W1528584793 hasAuthorship W1528584793A5027393147 @default.
- W1528584793 hasAuthorship W1528584793A5036979736 @default.
- W1528584793 hasAuthorship W1528584793A5044537097 @default.
- W1528584793 hasAuthorship W1528584793A5053541100 @default.
- W1528584793 hasAuthorship W1528584793A5060944739 @default.
- W1528584793 hasAuthorship W1528584793A5064635321 @default.
- W1528584793 hasAuthorship W1528584793A5064851399 @default.
- W1528584793 hasAuthorship W1528584793A5072277718 @default.
- W1528584793 hasAuthorship W1528584793A5076268307 @default.
- W1528584793 hasAuthorship W1528584793A5091513176 @default.
- W1528584793 hasConcept C121332964 @default.
- W1528584793 hasConcept C12294094 @default.
- W1528584793 hasConcept C152568617 @default.
- W1528584793 hasConcept C164304813 @default.
- W1528584793 hasConcept C177322064 @default.
- W1528584793 hasConcept C177571023 @default.
- W1528584793 hasConcept C185544564 @default.
- W1528584793 hasConcept C185592680 @default.
- W1528584793 hasConceptScore W1528584793C121332964 @default.
- W1528584793 hasConceptScore W1528584793C12294094 @default.
- W1528584793 hasConceptScore W1528584793C152568617 @default.
- W1528584793 hasConceptScore W1528584793C164304813 @default.
- W1528584793 hasConceptScore W1528584793C177322064 @default.
- W1528584793 hasConceptScore W1528584793C177571023 @default.
- W1528584793 hasConceptScore W1528584793C185544564 @default.
- W1528584793 hasConceptScore W1528584793C185592680 @default.
- W1528584793 hasLocation W15285847931 @default.
- W1528584793 hasOpenAccess W1528584793 @default.
- W1528584793 hasPrimaryLocation W15285847931 @default.
- W1528584793 hasRelatedWork W117475610 @default.
- W1528584793 hasRelatedWork W12188258 @default.
- W1528584793 hasRelatedWork W1525320582 @default.
- W1528584793 hasRelatedWork W1603989454 @default.
- W1528584793 hasRelatedWork W164001124 @default.
- W1528584793 hasRelatedWork W181055028 @default.
- W1528584793 hasRelatedWork W1964988841 @default.
- W1528584793 hasRelatedWork W1973403808 @default.
- W1528584793 hasRelatedWork W1974513153 @default.
- W1528584793 hasRelatedWork W2005912696 @default.
- W1528584793 hasRelatedWork W2040881273 @default.
- W1528584793 hasRelatedWork W2065026200 @default.
- W1528584793 hasRelatedWork W2268267114 @default.
- W1528584793 hasRelatedWork W2273410770 @default.
- W1528584793 hasRelatedWork W2273483805 @default.
- W1528584793 hasRelatedWork W2281670235 @default.
- W1528584793 hasRelatedWork W2281916912 @default.
- W1528584793 hasRelatedWork W2285286332 @default.
- W1528584793 hasRelatedWork W320313209 @default.
- W1528584793 hasRelatedWork W347760638 @default.
- W1528584793 isParatext "false" @default.
- W1528584793 isRetracted "false" @default.
- W1528584793 magId "1528584793" @default.
- W1528584793 workType "article" @default.