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author Domingo-Pardo, C.
Caballero-Folch, R.
Agramunt, J.
Algora, A.
Arcones, A.
Ameil, F.
Ayyad, Y.
Benlliure, J.
Bowry, M.
Calvino, F.
Cano-Ott, D.
Cortes, G.
Davinson, T.
Dillmann, I.
Estrade, A.
Evdokimov, A.
Faestermann, T.
Farinon, F.
Galaviz, D.
Garcia-Rios, A.
Geissel, H.
Gelletly, W.
Gernhauser, R.
Gomez-Hornillos, M.B.
Guerrero, C.
Heil, M.
Hinke, C.
Knobel, R.
Kojouharov, I.
Kurcewicz, J.
Kurz, N.
Litvinov, Y.
Maier, L.
Marganiec, J.
Marta, M.
Martinez, T.
Martinez-Pinedo, G.
Meyer, B.S.
Montes, F.
Mukha, I.
Napoli, D.R.
Nociforo, Ch.
Paradela, C.
Pietri, S.
Podolyak, Z.
Prochazka, A.
Rice, S.
Riego, A.
Rubio, B.
Schaffner, H.
Scheidenberger, Ch.
Smith, K.
Sokol, E.
Steiger, K.
Sun, B.
Tain, J.L.
Takechi, M.
Testov, D.
Weick, H.
Wilson, E.
Winfield, J.S.
Wood, R.
Woods, P.
Yeremin, A.
author_facet Domingo-Pardo, C.
Caballero-Folch, R.
Agramunt, J.
Algora, A.
Arcones, A.
Ameil, F.
Ayyad, Y.
Benlliure, J.
Bowry, M.
Calvino, F.
Cano-Ott, D.
Cortes, G.
Davinson, T.
Dillmann, I.
Estrade, A.
Evdokimov, A.
Faestermann, T.
Farinon, F.
Galaviz, D.
Garcia-Rios, A.
Geissel, H.
Gelletly, W.
Gernhauser, R.
Gomez-Hornillos, M.B.
Guerrero, C.
Heil, M.
Hinke, C.
Knobel, R.
Kojouharov, I.
Kurcewicz, J.
Kurz, N.
Litvinov, Y.
Maier, L.
Marganiec, J.
Marta, M.
Martinez, T.
Martinez-Pinedo, G.
Meyer, B.S.
Montes, F.
Mukha, I.
Napoli, D.R.
Nociforo, Ch.
Paradela, C.
Pietri, S.
Podolyak, Z.
Prochazka, A.
Rice, S.
Riego, A.
Rubio, B.
Schaffner, H.
Scheidenberger, Ch.
Smith, K.
Sokol, E.
Steiger, K.
Sun, B.
Tain, J.L.
Takechi, M.
Testov, D.
Weick, H.
Wilson, E.
Winfield, J.S.
Wood, R.
Woods, P.
Yeremin, A.
author_sort Domingo-Pardo, C.
collection CERN
description The rapid neutron nucleosynthesis process involves an enormous amount of very exotic neutron-rich nuclei, which represent a theoretical and experimental challenge. Two of the main decay properties that affect the final abundance distribution the most are half-lives and neutron branching ratios. Using fragmentation of a primary 238U beam at GSI we were able to measure such properties for several neutron-rich nuclei from 208Hg to 218Pb. This contribution provides a short update on the status of the data analysis of this experiment, together with a compilation of the latest results published in this mass region, both experimental and theoretical. The impact of the uncertainties connected with the beta-decay rates and with beta-delayed neutron emission is illustrated on the basis of r-process network calculations. In order to obtain a reasonable reproduction of the third r-process peak, it is expected that both half-lives and neutron branching ratios are substantially smaller, than those based on FRDM+QRPA, commonly used in r-process model calculations. Further measurements around N ~ 126 are required for a reliable modelling of the underlying nuclear structure, and for performing more realistic r-process abundance calculations.
id cern-1600441
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2013
record_format invenio
spelling cern-16004412023-06-20T02:09:09Zdoi:10.1088/1742-6596/665/1/012045http://cds.cern.ch/record/1600441engDomingo-Pardo, C.Caballero-Folch, R.Agramunt, J.Algora, A.Arcones, A.Ameil, F.Ayyad, Y.Benlliure, J.Bowry, M.Calvino, F.Cano-Ott, D.Cortes, G.Davinson, T.Dillmann, I.Estrade, A.Evdokimov, A.Faestermann, T.Farinon, F.Galaviz, D.Garcia-Rios, A.Geissel, H.Gelletly, W.Gernhauser, R.Gomez-Hornillos, M.B.Guerrero, C.Heil, M.Hinke, C.Knobel, R.Kojouharov, I.Kurcewicz, J.Kurz, N.Litvinov, Y.Maier, L.Marganiec, J.Marta, M.Martinez, T.Martinez-Pinedo, G.Meyer, B.S.Montes, F.Mukha, I.Napoli, D.R.Nociforo, Ch.Paradela, C.Pietri, S.Podolyak, Z.Prochazka, A.Rice, S.Riego, A.Rubio, B.Schaffner, H.Scheidenberger, Ch.Smith, K.Sokol, E.Steiger, K.Sun, B.Tain, J.L.Takechi, M.Testov, D.Weick, H.Wilson, E.Winfield, J.S.Wood, R.Woods, P.Yeremin, A.Approaching the precursor nuclei of the third r-process peak with RIBsnucl-exNuclear Physics - ExperimentThe rapid neutron nucleosynthesis process involves an enormous amount of very exotic neutron-rich nuclei, which represent a theoretical and experimental challenge. Two of the main decay properties that affect the final abundance distribution the most are half-lives and neutron branching ratios. Using fragmentation of a primary 238U beam at GSI we were able to measure such properties for several neutron-rich nuclei from 208Hg to 218Pb. This contribution provides a short update on the status of the data analysis of this experiment, together with a compilation of the latest results published in this mass region, both experimental and theoretical. The impact of the uncertainties connected with the beta-decay rates and with beta-delayed neutron emission is illustrated on the basis of r-process network calculations. In order to obtain a reasonable reproduction of the third r-process peak, it is expected that both half-lives and neutron branching ratios are substantially smaller, than those based on FRDM+QRPA, commonly used in r-process model calculations. Further measurements around N ~ 126 are required for a reliable modelling of the underlying nuclear structure, and for performing more realistic r-process abundance calculations.The rapid neutron nucleosynthesis process involves an enormous amount of very exotic neutron-rich nuclei, which represent a theoretical and experimental challenge. Two of the main decay properties that affect the final abundance distribution the most are half-lives and neutron branching ratios. Using fragmentation of a primary $^{238}$U beam at GSI we were able to measure such properties for several neutron-rich nuclei from $^{208}$Hg to $^{218}$Pb. This contribution provides a short update on the status of the data analysis of this experiment, together with a compilation of the latest results published in this mass region, both experimental and theoretical. The impact of the uncertainties connected with the beta-decay rates and with beta-delayed neutron emission is illustrated on the basis of $r$-process network calculations. In order to obtain a reasonable reproduction of the third $r$-process peak, it is expected that both half-lives and neutron branching ratios are substantially smaller, than those based on FRDM+QRPA, commonly used in $r$-process model calculations. Further measurements around $N\sim126$ are required for a reliable modelling of the underlying nuclear structure, and for performing more realistic $r$-process abundance calculations.arXiv:1309.3047oai:cds.cern.ch:16004412013-09-12
spellingShingle nucl-ex
Nuclear Physics - Experiment
Domingo-Pardo, C.
Caballero-Folch, R.
Agramunt, J.
Algora, A.
Arcones, A.
Ameil, F.
Ayyad, Y.
Benlliure, J.
Bowry, M.
Calvino, F.
Cano-Ott, D.
Cortes, G.
Davinson, T.
Dillmann, I.
Estrade, A.
Evdokimov, A.
Faestermann, T.
Farinon, F.
Galaviz, D.
Garcia-Rios, A.
Geissel, H.
Gelletly, W.
Gernhauser, R.
Gomez-Hornillos, M.B.
Guerrero, C.
Heil, M.
Hinke, C.
Knobel, R.
Kojouharov, I.
Kurcewicz, J.
Kurz, N.
Litvinov, Y.
Maier, L.
Marganiec, J.
Marta, M.
Martinez, T.
Martinez-Pinedo, G.
Meyer, B.S.
Montes, F.
Mukha, I.
Napoli, D.R.
Nociforo, Ch.
Paradela, C.
Pietri, S.
Podolyak, Z.
Prochazka, A.
Rice, S.
Riego, A.
Rubio, B.
Schaffner, H.
Scheidenberger, Ch.
Smith, K.
Sokol, E.
Steiger, K.
Sun, B.
Tain, J.L.
Takechi, M.
Testov, D.
Weick, H.
Wilson, E.
Winfield, J.S.
Wood, R.
Woods, P.
Yeremin, A.
Approaching the precursor nuclei of the third r-process peak with RIBs
title Approaching the precursor nuclei of the third r-process peak with RIBs
title_full Approaching the precursor nuclei of the third r-process peak with RIBs
title_fullStr Approaching the precursor nuclei of the third r-process peak with RIBs
title_full_unstemmed Approaching the precursor nuclei of the third r-process peak with RIBs
title_short Approaching the precursor nuclei of the third r-process peak with RIBs
title_sort approaching the precursor nuclei of the third r-process peak with ribs
topic nucl-ex
Nuclear Physics - Experiment
url https://dx.doi.org/10.1088/1742-6596/665/1/012045
http://cds.cern.ch/record/1600441
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