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197Au(n,y) - Towards a new standard for energies relevant to stellar nucleosynthesis

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dc.contributor.authorLederer, C
dc.contributor.authorColonna, N.
dc.contributor.authorDillmann, I.
dc.contributor.authorDomingo-Pardo, C.
dc.contributor.authorGiesen, U
dc.contributor.authorHeil, M.
dc.contributor.authorGunsing, F.
dc.contributor.authorKappeler, F
dc.contributor.authorMassimi, C
dc.contributor.authorMengoni, A.
dc.contributor.authorWallner, Anton
dc.contributor.authorMosconi, M.
dc.contributor.authorNolte, R.
dc.contributor.authorSchmidt, S.
dc.coverage.spatialEilat Israel
dc.date.accessioned2015-12-13T22:56:13Z
dc.date.createdApril 3-8 2011
dc.date.issued2012
dc.date.updated2016-02-24T08:37:35Z
dc.description.abstractTwo experiments were performed to resolve a discrepancy of the197Au(n, γ) cross section between the IAEA standard evaluation and the reference cross section for astrophysical experiments in the lower keV energy region. We measured the197Au(n, γ) reactio
dc.identifier.urihttp://hdl.handle.net/1885/82725
dc.publisherIOP Publishing
dc.relation.ispartofseries5th Bi-Annual Nuclear Physics in Astrophysics, NPA5
dc.sourceJournal of Physics: Conference Series 337
dc.subjectKeywords: Cross section; Energy regions; Neutron spectra; Resonance region; Standard evaluations; Stellar nucleosynthesis; Time-of-flight techniques; Chemical elements; Experiments; Neutron sources; Neutron spectrometers; Nuclear physics; Standards; Astrophysics
dc.title197Au(n,y) - Towards a new standard for energies relevant to stellar nucleosynthesis
dc.typeConference paper
local.contributor.affiliationLederer, C, University of Vienna
local.contributor.affiliationColonna, N., INFN
local.contributor.affiliationDillmann, I., Physik Department E12 and Excellence Cluster Universe
local.contributor.affiliationDomingo-Pardo, C., Instituto de Fisica Corpuscular
local.contributor.affiliationGiesen, U, TRIUMF
local.contributor.affiliationHeil, M., GSI Helmholtzzentrum fur Schwerionenforschung
local.contributor.affiliationGunsing, F., CEA-Saclay
local.contributor.affiliationKappeler, F, Karlsruhe Institute of Technology
local.contributor.affiliationMassimi, C, Universita di Bologna
local.contributor.affiliationMengoni, A., University of Vienna
local.contributor.affiliationWallner, Anton, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationWallner, Anton, University of Vienna
local.contributor.affiliationMosconi, M., Physikalisch-Technische Bundesanstalt
local.contributor.affiliationNolte, R., Physikalisch-Technische Bundesanstalt
local.contributor.affiliationSchmidt, S., Goethe University Frankfurt
local.contributor.authoruidWallner, Anton, u5124538
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor029904 - Synchrotrons; Accelerators; Instruments and Techniques
local.identifier.ariespublicationf5625xPUB10936
local.identifier.doi10.1088/1742-6596/337/1/012045
local.identifier.scopusID2-s2.0-84857945366
local.type.statusPublished Version

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