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dc.contributor.authorGlorius, J.
dc.contributor.authorLanger, C.
dc.contributor.authorSlavkovská, Z.
dc.contributor.authorBott, L.
dc.contributor.authorBrandau, C.
dc.contributor.authorBrückner, B.
dc.contributor.authorBlaum, K.
dc.contributor.authorChen, X.
dc.contributor.authorDababneh, S.
dc.contributor.authorDavinson, T.
dc.contributor.authorErbacher, P.
dc.contributor.authorFiebiger, S.
dc.contributor.authorGaßner, T.
dc.contributor.authorGöbel, K.
dc.contributor.authorGroothuis, M.
dc.contributor.authorGumberidze, A.
dc.contributor.authorGyürky, G.
dc.contributor.authorHeil, M.
dc.contributor.authorHess, R.
dc.contributor.authorHensch, R.
dc.contributor.authorHillmann, P.
dc.contributor.authorHillenbrand, P. M.
dc.contributor.authorHinrichs, O.
dc.contributor.authorJurado, B.
dc.contributor.authorKausch, T.
dc.contributor.authorKhodaparast, A.
dc.contributor.authorKisselbach, T.
dc.contributor.authorKlapper, N.
dc.contributor.authorKozhuharov, C.
dc.contributor.authorKurtulgil, D.
dc.contributor.authorLane, G.
dc.contributor.authorLederer-Woods, C.
dc.contributor.authorLestinsky, M.
dc.contributor.authorLitvinov, S.
dc.contributor.authorLitvinov, Yu A.
dc.contributor.authorLöher, B.
dc.contributor.authorNolden, F.
dc.contributor.authorPetridis, N.
dc.contributor.authorPopp, U.
dc.contributor.authorRauscher, T.
dc.contributor.authorReed, M.
dc.contributor.authorReifarth, R.
dc.contributor.authorSanjari, M. S.
dc.contributor.authorSavran, D.
dc.contributor.authorSimon, H.
dc.contributor.authorSpillmann, U.
dc.contributor.authorSteck, M.
dc.contributor.authorStöhlker, T.
dc.contributor.authorStumm, J.
dc.contributor.authorSurzhykov, A.
dc.contributor.authorSzücs, T.
dc.contributor.authorNguyen, T. T.
dc.contributor.authorTaremi Zadeh, A.
dc.contributor.authorThomas, B.
dc.contributor.authorTorilov, S. Yu
dc.contributor.authorTörnqvist, H.
dc.contributor.authorTräger, M.
dc.contributor.authorTrageser, C.
dc.contributor.authorTrotsenko, S.
dc.contributor.authorVarga, L.
dc.contributor.authorVolknandt, M.
dc.contributor.authorWeick, H.
dc.contributor.authorWeigand, M.
dc.contributor.authorWolf, C.
dc.contributor.authorWoods, P. J.
dc.contributor.authorXing, Y. M.
dc.date.accessioned2019-04-03T14:07:25Z
dc.date.available2019-04-03T14:07:25Z
dc.date.issued2019-03-07
dc.identifier.citationGlorius , J , Langer , C , Slavkovská , Z , Bott , L , Brandau , C , Brückner , B , Blaum , K , Chen , X , Dababneh , S , Davinson , T , Erbacher , P , Fiebiger , S , Gaßner , T , Göbel , K , Groothuis , M , Gumberidze , A , Gyürky , G , Heil , M , Hess , R , Hensch , R , Hillmann , P , Hillenbrand , P M , Hinrichs , O , Jurado , B , Kausch , T , Khodaparast , A , Kisselbach , T , Klapper , N , Kozhuharov , C , Kurtulgil , D , Lane , G , Lederer-Woods , C , Lestinsky , M , Litvinov , S , Litvinov , Y A , Löher , B , Nolden , F , Petridis , N , Popp , U , Rauscher , T , Reed , M , Reifarth , R , Sanjari , M S , Savran , D , Simon , H , Spillmann , U , Steck , M , Stöhlker , T , Stumm , J , Surzhykov , A , Szücs , T , Nguyen , T T , Taremi Zadeh , A , Thomas , B , Torilov , S Y , Törnqvist , H , Träger , M , Trageser , C , Trotsenko , S , Varga , L , Volknandt , M , Weick , H , Weigand , M , Wolf , C , Woods , P J & Xing , Y M 2019 , ' Approaching the Gamow Window with Stored Ions : Direct Measurement of Xe 124 (p,γ) in the ESR Storage Ring ' , Physical Review Letters , vol. 122 , no. 9 , 092701 . https://doi.org/10.1103/PhysRevLett.122.092701
dc.identifier.issn0031-9007
dc.identifier.urihttp://hdl.handle.net/2299/21238
dc.description© 2019 American Physical Society. All rights reserved.
dc.description.abstractWe report the first measurement of low-energy proton-capture cross sections of Xe124 in a heavy-ion storage ring. Xe12454+ ions of five different beam energies between 5.5 and 8 AMeV were stored to collide with a windowless hydrogen target. The Cs125 reaction products were directly detected. The interaction energies are located on the high energy tail of the Gamow window for hot, explosive scenarios such as supernovae and x-ray binaries. The results serve as an important test of predicted astrophysical reaction rates in this mass range. Good agreement in the prediction of the astrophysically important proton width at low energy is found, with only a 30% difference between measurement and theory. Larger deviations are found above the neutron emission threshold, where also neutron and γ widths significantly impact the cross sections. The newly established experimental method is a very powerful tool to investigate nuclear reactions on rare ion beams at low center-of-mass energies.en
dc.format.extent6
dc.format.extent472195
dc.language.isoeng
dc.relation.ispartofPhysical Review Letters
dc.subjectPhysics and Astronomy(all)
dc.titleApproaching the Gamow Window with Stored Ions : Direct Measurement of Xe 124 (p,γ) in the ESR Storage Ringen
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=85062944826&partnerID=8YFLogxK
rioxxterms.versionofrecord10.1103/PhysRevLett.122.092701
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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