002689800 001__ 2689800
002689800 003__ SzGeCERN
002689800 005__ 20220810142337.0
002689800 0247_ $$2DOI$$9Elsevier$$a10.1016/j.physletb.2019.04.039
002689800 0248_ $$aoai:inspirehep.net:1733368$$pcerncds:CERN:FULLTEXT$$pcerncds:FULLTEXT$$pcerncds:CERN$$qINSPIRE:HEP$$qForCDS
002689800 035__ $$9http://inspirehep.net/oai2d$$aoai:inspirehep.net:1733368$$d2019-09-16T15:51:00Z$$h2019-09-17T04:18:28Z$$mmarcxml
002689800 035__ $$9Inspire$$a1733368
002689800 041__ $$aeng
002689800 100__ $$aBerry, T [email protected]$$uSurrey U.
002689800 245__ $$9Elsevier$$aInvestigation of the $\Delta n = 0$ selection rule in Gamow-Teller transitions: The $\beta$-decay of $^{207}$Hg
002689800 260__ $$c2019
002689800 300__ $$a5 p
002689800 520__ $$9Elsevier$$aGamow-Teller $\beta$ decay is forbidden if the number of nodes in the radial wave functions of the initial and final states is different. This $\Delta n=0$ requirement plays a major role in the $\beta$ decay of heavy neutron-rich nuclei, affecting the nucleosynthesis through the increased half-lives of nuclei on the astrophysical $r$-process pathway below both $Z=50$ (for $N>82$ ) and $Z=82$ (for $N>126$). The level of forbiddenness of the $\Delta n=1\ \nu 1g_{9/2} \rightarrow \pi0g_{7/2}$ transition has been investigated from the $\beta^-$ decay of the ground state of $^{207}$Hg into the single-proton-hole nucleus $^{207}$Tl in an experiment at the ISOLDE Decay Station. From statistical observational limits on possible $\gamma$-ray transitions depopulating the $\pi 0g_{7/2}^{−1}$ state in $^{207}$Tl, an upper limit of $3.9 \times 10^{−3}$% was obtained for the probability of this decay, corresponding to log$ft > 8.8$ within a 95% confidence limit. This is the most stringent test of the $\Delta n=0$ selection rule to date.
002689800 540__ $$3publication$$aCC-BY-4.0$$bElsevier$$uhttp://creativecommons.org/licenses/by/4.0/
002689800 542__ $$3publication$$dThe Authors$$g2019
002689800 65017 $$2SzGeCERN$$aNuclear Physics - Experiment
002689800 690C_ $$aCERN
002689800 693__ $$aCERN ISOLDE
002689800 700__ $$aPodolyák, Zs$$uSurrey U.
002689800 700__ $$aCarroll, R J$$uSurrey U.
002689800 700__ $$aLică, R$$uCERN$$uBucharest, IFIN-HH$$vH. Hulubei National Institute for Physics and Nuclear Engineering, Bucharest, Romania
002689800 700__ $$aGrawe, H
002689800 700__ $$aTimofeyuk, N K$$uSurrey U.
002689800 700__ $$aAlexander, T$$uSurrey U.
002689800 700__ $$aAndreyev, A N$$uYork U., England
002689800 700__ $$aAnsari, S$$uCologne U.
002689800 700__ $$aBorge, M J G$$uCERN$$uMadrid, Inst. Estructura Materia$$vInstituto de Estructura de la Materia, CSIC, Serrano 113 bis, Madrid, E-28006, Spain
002689800 700__ $$aCreswell, J$$uDaresbury
002689800 700__ $$aFahlander, C$$uLund U.
002689800 700__ $$aFraile, L M$$uUCM, Madrid, Dept. Phys.
002689800 700__ $$aFynbo, H O U$$jORCID:0000-0003-0316-4548$$uAarhus U.
002689800 700__ $$aGelletly, W$$uSurrey U.
002689800 700__ $$aGerst, R -B$$uCologne U.
002689800 700__ $$aGórska, M$$uDarmstadt, GSI
002689800 700__ $$aGredley, A$$uLiverpool U.
002689800 700__ $$aGreenlees, P$$uJyvaskyla U.
002689800 700__ $$aHarkness-Brennan, L J$$uLiverpool U.
002689800 700__ $$aHuyse, M$$uKU Leuven, Dept. Phys. Astron.
002689800 700__ $$aJudge, S M$$uTeddington, Natl. Phys. Lab
002689800 700__ $$aJudson, D S$$uLiverpool U.
002689800 700__ $$aKonki, J$$uJyvaskyla U.$$uHelsinki Inst. of Phys.$$uCERN$$vHelsinki Institute of Physics, University of Helsinki, Helsinki, FIN-00014, Finland
002689800 700__ $$aKurcewicz, J$$uCERN
002689800 700__ $$aKuti, I$$uDebrecen, Inst. Nucl. Res.
002689800 700__ $$aLalkovski, S$$uSurrey U.
002689800 700__ $$aLazarus, I$$uDaresbury
002689800 700__ $$aLund, M$$uAarhus U.
002689800 700__ $$aMadurga, M$$uCERN
002689800 700__ $$aMărginean, N$$uBucharest, IFIN-HH
002689800 700__ $$aMărginean, R$$uBucharest, IFIN-HH
002689800 700__ $$aMarroquin, I$$uMadrid, Inst. Estructura Materia
002689800 700__ $$aMihai, C$$uBucharest, IFIN-HH
002689800 700__ $$aMihai, R E$$uBucharest, IFIN-HH
002689800 700__ $$aNácher, E$$jORCID:0000-0002-2123-539X$$uMadrid, Inst. Estructura Materia
002689800 700__ $$aNae, S$$uBucharest, IFIN-HH
002689800 700__ $$aNegret, A$$uBucharest, IFIN-HH
002689800 700__ $$aNiţă, C$$uBucharest, IFIN-HH$$uBrighton U.$$vSchool of Computing, Engineering and Mathematics, University of Brighton, Brighton, BN2 4GJ, United Kingdom
002689800 700__ $$aPage, R D$$uLiverpool U.
002689800 700__ $$aPascu, S$$uBucharest, IFIN-HH
002689800 700__ $$aPatel, Z$$uSurrey U.
002689800 700__ $$aPerea, A$$uMadrid, Inst. Estructura Materia
002689800 700__ $$aPucknell, V$$uDaresbury
002689800 700__ $$aRahkila, P$$uJyvaskyla U.
002689800 700__ $$aRapisarda, E$$uCERN
002689800 700__ $$aRegan, P H$$jORCID:0000-0002-9870-182X$$uSurrey U.$$uTeddington, Natl. Phys. Lab$$vNational Physical Laboratory, Teddington, Middlesex, TW11 0LW, United Kingdom
002689800 700__ $$aRotaru, F$$uBucharest, IFIN-HH
002689800 700__ $$aShand, C M$$uSurrey U.
002689800 700__ $$aSimpson, E C$$uAustralian Natl. U., Canberra
002689800 700__ $$aSotty, Ch$$uBucharest, IFIN-HH$$uKU Leuven, Dept. Phys. Astron.$$vKU Leuven, Instituut voor Kern- en Stralingsfysica, Celestijnenlaan 200D, Leuven, 3001, Belgium
002689800 700__ $$aStegemann, S$$uCologne U.
002689800 700__ $$aStora, T$$uCERN
002689800 700__ $$aTengblad, O$$uMadrid, Inst. Estructura Materia
002689800 700__ $$aTurturica, A$$uBucharest, IFIN-HH
002689800 700__ $$aVan Duppen, P$$uKU Leuven, Dept. Phys. Astron.
002689800 700__ $$aVedia, V$$uUCM, Madrid, Dept. Phys.
002689800 700__ $$aWadsworth, R$$uYork U., England
002689800 700__ $$aWalker, P M$$uSurrey U.
002689800 700__ $$aWarr, N$$uCologne U.
002689800 700__ $$aWearing, F$$uLiverpool U.
002689800 700__ $$aDe Witte, H$$uKU Leuven, Dept. Phys. Astron.
002689800 773__ $$c271-275$$pPhys. Lett. B$$v793$$y2019
002689800 8564_ $$81517538$$s356326$$uhttp://cds.cern.ch/record/2689800/files/scoap3-fulltext.pdf$$yArticle from SCOAP3
002689800 960__ $$a13
002689800 980__ $$aARTICLE
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