002913178 001__ 2913178
002913178 003__ SzGeCERN
002913178 005__ 20241029110612.0
002913178 0247_ $$2DOI$$9APS$$a10.1103/PhysRevLett.133.052702$$qpublication
002913178 0248_ $$aoai:cds.cern.ch:2913178$$pcerncds:FULLTEXT$$pcerncds:CERN:FULLTEXT$$pcerncds:CERN
002913178 035__ $$9HAL$$ahal-04668762
002913178 035__ $$9https://inspirehep.net/api/oai2d$$aoai:inspirehep.net:2815622$$d2024-10-09T13:27:22Z$$h2024-10-11T04:00:13Z$$mmarcxml
002913178 035__ $$9Inspire$$a2815622
002913178 041__ $$aeng
002913178 100__ $$aCasanovas-Hoste, A$$uBarcelona, Polytechnic U.$$uValencia U., IFIC$$uCERN$$vEuropean Organization for Nuclear Research (CERNhttps://ror.org/01ggx4157), Switzerland
002913178 245__ $$9APS$$aShedding Light on the Origin of Pb204, the Heaviest s-Process–Only Isotope in the Solar System
002913178 260__ $$c2024
002913178 300__ $$a8 p
002913178 520__ $$9APS$$aAsymptotic giant branch stars are responsible for the production of most of the heavy isotopes beyond Sr observed in the solar system. Among them, isotopes shielded from the r-process contribution by their stable isobars are defined as s-only nuclei. For a long time the abundance of Pb204, the heaviest s-only isotope, has been a topic of debate because state-of-the-art stellar models appeared to systematically underestimate its solar abundance. Besides the impact of uncertainties from stellar models and galactic chemical evolution simulations, this discrepancy was further obscured by rather divergent theoretical estimates for the neutron capture cross section of its radioactive precursor in the neutron-capture flow, Tl204 (t1/2=3.78 yr), and by the lack of experimental data on this reaction. We present the first ever neutron capture measurement on Tl204, conducted at the CERN neutron time-of-flight facility n_TOF, employing a sample of only 9 mg of Tl204 produced at the Institute Laue Langevin high flux reactor. By complementing our new results with semiempirical calculations we obtained, at the s-process temperatures of kT≈8 keV and kT≈30 keV, Maxwellian-averaged cross sections (MACS) of 580(168) mb and 260(90) mb, respectively. These figures are about 3% lower and 20% higher than the corresponding values widely used in astrophysical calculations, which were based only on theoretical calculations. By using the new Tl204 MACS, the uncertainty arising from the Tl204(n,γ) cross section on the s-process abundance of Pb204 has been reduced from ∼30% down to +8%/-6%, and the s-process calculations are in agreement with the latest solar system abundance of Pb204 reported by K. Lodders in 2021.
002913178 540__ $$3publication$$aCC BY 4.0$$fCERN-RP: APS$$uhttps://creativecommons.org/licenses/by/4.0/
002913178 542__ $$3publication$$dauthors$$g2024
002913178 65017 $$2SzGeCERN$$aAstrophysics and Astronomy
002913178 65017 $$2SzGeCERN$$aNuclear Physics - Experiment
002913178 690C_ $$aARTICLE
002913178 690C_ $$aCERN
002913178 693__ $$aCERN PS$$enTOF
002913178 700__ $$aDomingo-Pardo, C$$uValencia U., IFIC
002913178 700__ $$aLerendegui-Marco, J$$uSeville U.
002913178 700__ $$aGuerrero, C$$uSeville U.
002913178 700__ $$aTarifeño-Saldivia, A$$uValencia U., IFIC
002913178 700__ $$aKrtička, M$$uCharles U.
002913178 700__ $$aPignatari, M$$uWigner RCP, Budapest$$uHull U.$$uIndiana U.$$vE. A. Milne Centre for Astrophysics, University of Hull, Hull, United Kingdom$$vKonkoly Observatory, HUN-REN, Konkoly Thege Miklós út 15-17, H-1121 Budapest, Hungary
002913178 700__ $$aCalviño, F$$uBarcelona, Polytechnic U.
002913178 700__ $$aSchumann, D$$uPSI, Villigen
002913178 700__ $$aHeinitz, S$$uPSI, Villigen
002913178 700__ $$aDressler, R$$uPSI, Villigen
002913178 700__ $$aKöster, U$$uLaue-Langevin Inst.
002913178 700__ $$aAberle, O$$uCERN
002913178 700__ $$aAndrzejewski, J$$uLodz U.
002913178 700__ $$aAudouin, L$$uOrsay, IPN
002913178 700__ $$aBécares, V$$uMadrid, CIEMAT$$uMadrid, Escuela Tec. Sup. Ing. Ind.
002913178 700__ $$aBacak, M$$uVienna, Tech. U., Atominst.
002913178 700__ $$aBalibrea-Correa, J$$uMadrid, CIEMAT$$uMadrid, Escuela Tec. Sup. Ing. Ind.
002913178 700__ $$aBarbagallo, M$$uINFN, Bari
002913178 700__ $$aBarros, S$$uLisbon, IST
002913178 700__ $$aBečvář, F$$uCharles U.
002913178 700__ $$aBeinrucker, C$$uGoethe U., Frankfurt (main)
002913178 700__ $$aBerthoumieux, E$$uIRFU, Saclay
002913178 700__ $$aBillowes, J$$uManchester U.
002913178 700__ $$aBosnar, D$$uZagreb U., Phys. Dept.
002913178 700__ $$aBrugger, M$$uCERN
002913178 700__ $$aCaamaño, M$$uSantiago de Compostela U.
002913178 700__ $$aCalviani, M$$uCERN
002913178 700__ $$aCano-Ott, D$$uMadrid, CIEMAT$$uMadrid, Escuela Tec. Sup. Ing. Ind.
002913178 700__ $$aCardella, R$$uCERN
002913178 700__ $$aCastelluccio, D M$$uENEA, Casaccia$$uINFN, Bologna$$vIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Bologna, Italy
002913178 700__ $$aCerutti, F$$uCERN
002913178 700__ $$aChen, Y H$$uOrsay, IPN
002913178 700__ $$aChiaveri, E$$uCERN
002913178 700__ $$aColonna, N$$uINFN, Bari
002913178 700__ $$aCortés, G$$uBarcelona, Polytechnic U.
002913178 700__ $$aCortés-Giraldo, M A$$uSeville U.
002913178 700__ $$aCosentino, L$$uINFN, Catania
002913178 700__ $$aDamone, L A$$uINFN, Bari$$uBari U.$$vDipartimento Interateneo di Fisica, Università degli Studi di Bari, Bari, Italy
002913178 700__ $$aDiakaki, M$$uIRFU, Saclay
002913178 700__ $$aDupont, E$$uIRFU, Saclay
002913178 700__ $$aDurán, I$$uSantiago de Compostela U.
002913178 700__ $$aFernández-Domínguez, B$$uSantiago de Compostela U.
002913178 700__ $$aFerrari, A$$uCERN
002913178 700__ $$aFerreira, P$$uLisbon, IST
002913178 700__ $$aFinocchiaro, P$$uINFN, Catania
002913178 700__ $$aFurman, V$$uHigher Sch. of Economics, Moscow
002913178 700__ $$aGöbel, K$$uGoethe U., Frankfurt (main)
002913178 700__ $$aGarcía, A R$$uMadrid, CIEMAT$$uMadrid, Escuela Tec. Sup. Ing. Ind.
002913178 700__ $$aGawlik-Ramięga, A$$uLodz U.
002913178 700__ $$aGlodariu, T$$uBucharest, IFIN-HH
002913178 700__ $$aGonçalves, I F$$uLisbon, IST
002913178 700__ $$aGonzález-Romero, E$$uMadrid, CIEMAT$$uMadrid, Escuela Tec. Sup. Ing. Ind.
002913178 700__ $$aGoverdovski, A$$uObninsk, Inst. Phys. Power Eng.
002913178 700__ $$aGriesmayer, E$$uVienna, Tech. U., Atominst.
002913178 700__ $$aGunsing, F$$uIRFU, Saclay$$uCERN$$vCEA Irfu, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France
002913178 700__ $$aHarada, H$$uJAEA, Ibaraki
002913178 700__ $$aHeftrich, T$$uGoethe U., Frankfurt (main)
002913178 700__ $$aHeyse, J$$uGeel, JRC
002913178 700__ $$aJenkins, D G$$uYork U., England
002913178 700__ $$aJericha, E$$uVienna, Tech. U., Atominst.
002913178 700__ $$aKäppeler, F$$uKIT, Karlsruhe, IKP
002913178 700__ $$aKadi, Y$$uCERN
002913178 700__ $$aKatabuchi, T$$uTokyo Inst. Tech.
002913178 700__ $$aKavrigin, P$$uVienna, Tech. U., Atominst.
002913178 700__ $$aKetlerov, V$$uObninsk, Inst. Phys. Power Eng.
002913178 700__ $$aKhryachkov, V$$uObninsk, Inst. Phys. Power Eng.
002913178 700__ $$aKimura, A$$uJAEA, Ibaraki
002913178 700__ $$aKivel, N$$uPSI, Villigen
002913178 700__ $$aKokkoris, M$$uNatl. Tech. U., Athens
002913178 700__ $$aLeal-Cidoncha, E$$uSantiago de Compostela U.
002913178 700__ $$aLederer-Woods, C$$uEdinburgh U.
002913178 700__ $$aLeeb, H$$uVienna, Tech. U., Atominst.
002913178 700__ $$aMeo, S Lo$$uENEA, Casaccia$$uINFN, Bologna$$vIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Bologna, Italy
002913178 700__ $$aLonsdale, S J$$uEdinburgh U.
002913178 700__ $$aLosito, R$$uCERN
002913178 700__ $$aMacina, D$$uCERN
002913178 700__ $$aMarganiec, J$$uLodz U.
002913178 700__ $$aMartínez, T$$uMadrid, CIEMAT$$uMadrid, Escuela Tec. Sup. Ing. Ind.
002913178 700__ $$aMassimi, C$$uINFN, Bologna$$uBologna U.$$vDipartimento di Fisica e Astronomia, Università di Bologna, Bologna, Italy
002913178 700__ $$aMastinu, P$$uINFN, Legnaro
002913178 700__ $$aMastromarco, M$$uINFN, Bari
002913178 700__ $$aMatteucci, F$$uINFN, Trieste$$uTrieste U.$$vDipartimento di Astronomia, Università di Trieste, Trieste, Italy
002913178 700__ $$aMaugeri, E A$$uPSI, Villigen
002913178 700__ $$aMendoza, E$$uMadrid, CIEMAT$$uMadrid, Escuela Tec. Sup. Ing. Ind.
002913178 700__ $$aMengoni, A$$uENEA, Casaccia
002913178 700__ $$aMilazzo, P M$$uINFN, Trieste
002913178 700__ $$aMingrone, F$$uINFN, Bologna
002913178 700__ $$aMirea, M$$uBucharest, IFIN-HH
002913178 700__ $$aMontesano, S$$uCERN
002913178 700__ $$aMusumarra, A$$uINFN, Catania$$uCatania U.$$vDipartimento di Fisica e Astronomia, Università di Catania, Catania, Italy
002913178 700__ $$aNolte, R$$uBraunschweig, Phys. Tech. Bund.
002913178 700__ $$aOprea, A$$uBucharest, IFIN-HH
002913178 700__ $$aPatronis, N$$uIoannina U.
002913178 700__ $$aPavlik, A$$uVienna U.
002913178 700__ $$aPerkowski, J$$uLodz U.
002913178 700__ $$aPorras, I$$uCERN$$uGranada U.$$vUniversity of Granada, Granada, Spain
002913178 700__ $$aPraena, J$$uSeville U.$$uGranada U.$$vUniversidad de Sevilla, Sevilla, Spain
002913178 700__ $$aQuesada, J M$$uSeville U.
002913178 700__ $$aRajeev, K$$uBhabha Atomic Res. Ctr.
002913178 700__ $$aRauscher, T$$uHertfordshire U.$$uBasel U.$$vDepartment of Physics, University of Basel, Basel, Switzerland
002913178 700__ $$aReifarth, R$$uGoethe U., Frankfurt (main)
002913178 700__ $$aRiego-Perez, A$$uBarcelona, Polytechnic U.
002913178 700__ $$aRomanets, Y$$uLisbon, IST
002913178 700__ $$aRout, P C$$uBhabha Atomic Res. Ctr.
002913178 700__ $$aRubbia, C$$uCERN
002913178 700__ $$aRyan, J A$$uManchester U.
002913178 700__ $$aSabaté-Gilarte, M$$uCERN$$uSeville U.$$vUniversidad de Sevilla, Sevilla, Spain
002913178 700__ $$aSaxena, A$$uBhabha Atomic Res. Ctr.
002913178 700__ $$aSchillebeeckx, P$$uGeel, JRC
002913178 700__ $$aSchmidt, S$$uGoethe U., Frankfurt (main)
002913178 700__ $$aSedyshev, P$$uHigher Sch. of Economics, Moscow
002913178 700__ $$aSmith, A G$$uManchester U.
002913178 700__ $$aStamatopoulos, A$$uNatl. Tech. U., Athens
002913178 700__ $$aTagliente, G$$uINFN, Bari
002913178 700__ $$aTain, J L$$uValencia U., IFIC
002913178 700__ $$aTassan-Got, L$$uOrsay, IPN
002913178 700__ $$aTsinganis, A$$uNatl. Tech. U., Athens
002913178 700__ $$aValenta, S$$uCharles U.
002913178 700__ $$aVannini, G$$uINFN, Bologna$$uBologna U.$$vDipartimento di Fisica e Astronomia, Università di Bologna, Bologna, Italy
002913178 700__ $$aVariale, V$$uINFN, Bari
002913178 700__ $$aVaz, P$$uLisbon, IST
002913178 700__ $$aVentura, A$$uINFN, Bologna
002913178 700__ $$aVlachoudis, V$$uCERN
002913178 700__ $$aVlastou, R$$uNatl. Tech. U., Athens
002913178 700__ $$aWallner, A$$uAustralian Natl. U., Canberra
002913178 700__ $$aWarren, S$$uManchester U.
002913178 700__ $$aWeigand, M$$uGoethe U., Frankfurt (main)
002913178 700__ $$aWeiss, C$$uCERN$$uVienna, Tech. U., Atominst.$$vEuropean Organization for Nuclear Research (CERNhttps://ror.org/01ggx4157), Switzerland
002913178 700__ $$aWolf, C$$uGoethe U., Frankfurt (main)
002913178 700__ $$aWoods, P J$$uEdinburgh U.
002913178 700__ $$aWright, T$$uManchester U.
002913178 700__ $$aŽugec, P$$uZagreb U., Phys. Dept.$$uCERN$$vEuropean Organization for Nuclear Research (CERNhttps://ror.org/01ggx4157), Switzerland
002913178 710__ $$gn_TOF Collaboration
002913178 773__ $$c052702$$mpublication$$n5$$pPhys. Rev. Lett.$$v133$$y2024
002913178 8564_ $$82563726$$s568439$$uhttp://cds.cern.ch/record/2913178/files/Publication.pdf$$yFulltext
002913178 960__ $$a13
002913178 980__ $$aARTICLE