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New gas-filled mode of the large-acceptance spectrometer VAMOS

dc.creatorSchmitt, C.
dc.creatorRejmund, M.
dc.creatorNavin, A.
dc.creatorLecornu, B.
dc.creatorJacquot, Bertrand
dc.creatorde France, Gilles
dc.creatorLemasson, A.
dc.creatorShrivastava, A.
dc.creatorGreenlees, P.
dc.creatorUusitalo, J.
dc.creatorSubotić, Krunoslav M.
dc.creatorGaudefroy, L.
dc.creatorTheisen, Christophe
dc.creatorSulignano, Barbara
dc.creatorDorvaux, O.
dc.creatorStuttge, L.
dc.date.accessioned2018-03-01T21:20:42Z
dc.date.available2018-03-01T21:20:42Z
dc.date.issued2010
dc.identifier.issn0168-9002
dc.identifier.issn1872-9576
dc.identifier.urihttps://vinar.vin.bg.ac.rs/handle/123456789/4084
dc.description.abstractA new gas-filled operation mode of the large-acceptance spectrometer VAMOS at GANIL is reported. A beam rejection factor greater than 10(10) is obtained for the Ca-40+Sm-150 system at 196 MeV. The unprecedented transmission efficiency for the evaporation residues produced in this reaction is estimated to be around 80% for alpha x n channels and above 95% for x ny p channels. A detailed study of the performance of the gas-filled VAMOS and future developments are discussed. This new operation mode opens avenues to explore the potential of fusion reactions in various kinematics. (C) 2010 Elsevier B.V. All rights reserved.en
dc.rightsrestrictedAccessen
dc.sourceNuclear Instruments and Methods in Physics Research. Section A: Accelerators, Spectrometers, Detectors, and Associated Equipmenten
dc.subjectGas-filled spectrometeren
dc.subjectFusion reactionsen
dc.subjectBeam rejectionen
dc.subjectTransmissionen
dc.titleNew gas-filled mode of the large-acceptance spectrometer VAMOSen
dc.typearticleen
dcterms.abstractСуботић Крунослав М; Сцхмитт, Ц.; Рејмунд, М.; Навин, A.; Лецорну, Б.; Јацqуот, Б.; де Франце, Г.; Лемассон, A.; Схривастава, A.; Греенлеес, П.; Ууситало, Ј.; Гаудефроy, Л.; Тхеисен, Цх.; Сулигнано, Б.; Дорвауx, О.; Стуттге, Л.;
dc.citation.volume621
dc.citation.issue1-3
dc.citation.spage558
dc.citation.epage565
dc.identifier.wos000281109100082
dc.identifier.doi10.1016/j.nima.2010.03.146
dc.citation.rankM21
dc.identifier.scopus2-s2.0-77957894131


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