Matches in UGent Biblio for { <https://biblio.ugent.be/publication/1076253#aggregation> ?p ?o. }
Showing items 1 to 38 of
38
with 100 items per page.
- aggregation classification "C1".
- aggregation creator B33922.
- aggregation creator B33923.
- aggregation creator B33924.
- aggregation creator B33925.
- aggregation creator B33926.
- aggregation creator B33927.
- aggregation creator B33928.
- aggregation creator person.
- aggregation creator person.
- aggregation date "2010".
- aggregation format "application/pdf".
- aggregation hasFormat 1076253.bibtex.
- aggregation hasFormat 1076253.csv.
- aggregation hasFormat 1076253.dc.
- aggregation hasFormat 1076253.didl.
- aggregation hasFormat 1076253.doc.
- aggregation hasFormat 1076253.json.
- aggregation hasFormat 1076253.mets.
- aggregation hasFormat 1076253.mods.
- aggregation hasFormat 1076253.rdf.
- aggregation hasFormat 1076253.ris.
- aggregation hasFormat 1076253.txt.
- aggregation hasFormat 1076253.xls.
- aggregation hasFormat 1076253.yaml.
- aggregation isPartOf urn:isbn:9789814322737.
- aggregation language "eng".
- aggregation publisher "World Scientific".
- aggregation rights "I have transferred the copyright for this publication to the publisher".
- aggregation subject "Physics and Astronomy".
- aggregation title "Characteristics of light charged particle emission in the ternary fission of 250Cf and 252Cf at different excitation energies".
- aggregation abstract "The emission probabilities and the energy distributions of tritons, α and ^6He particles emitted in the spontaneous ternary fission (zero excitation energy) of ^250Cf and ^252Cf and in the cold neutron induced fission (excitation energy ≈ 6.5 MeV) of ^249Cf and 251Cf are determined. The particle identification was done with suited ΔE-E telescope detectors, at the IRMM (Geel, Belgium) for the spontaneous fission and at the ILL (Grenoble, France) for the neutron induced fission measurements. Hence particle emission characteristics of the fissioning systems ^250Cf and ^252Cf are obtained at zero and at about 6.5 MeV excitation energies. While the triton emission probability is hardly influenced by the excitation energy, the ^4He and ^6He emission probability in spontaneous fission is higher than for neutron induced fission. This can be explained by the strong influence of the cluster preformation probability on the ternary particle emission probability.".
- aggregation authorList BK85493.
- aggregation endPage "153".
- aggregation startPage "145".
- aggregation aggregates 1139570.
- aggregation isDescribedBy 1076253.
- aggregation similarTo LU-1076253.