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Measurement of $^{73}$Ge($n,γ$) cross sections and implications for stellar nucleosynthesis

73 Ge( n,γ ) cross sections were measured at the neutron time-of-flight facility n_TOF at CERN up to neutron energies of 300 keV, providing for the first time experimental data above 8 keV. Results indicate that the stellar cross section at kT=30 keV is 1.5 to 1.7 times higher than most theoretical...

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Autores principales: Lederer-Woods, Claudia, Battino, U., Ferreira, P., Gawlik, A., Guerrero, C., Gunsing, F., Heinitz, S., Lerendegui-Marco, J., Mengoni, A., Reifarth, R., Tattersall, A., Valenta, S., Weiss, C., Aberle, O., Andrzejewski, J., Audouin, L., Bécares, V., Bacak, M., Balibrea, J., Barbagallo, M., Barros, S., Bečvář, F., Beinrucker, C., Belloni, F., Berthoumieux, E., Billowes, J., Bosnar, D., Brugger, M., Caamaño, M., Calviño, F., Calviani, M., Cano-Ott, D., Cerutti, F., Chiaveri, E., Colonna, N., Cortés, G., Cortés-Giraldo, M.A., Cosentino, L., Damone, L.A., Deo, K., Diakaki, M., Dietz, M., Domingo-Pardo, C., Dressler, R., Dupont, E., Durán, I., Fernández-Domínguez, B., Ferrari, A., Finocchiaro, P., Frost, R.J.W., Furman, V., Göbel, K., García, A.R., Gheorghe, I., Glodariu, T., Gonçalves, I.F., González-Romero, E., Goverdovski, A., Griesmayer, E., Harada, H., Heftrich, T., Hernández-Prieto, A., Heyse, J., Jenkins, D.G., Jericha, E., Käppeler, F., Kadi, Y., Katabuchi, T., Kavrigin, P., Ketlerov, V., Khryachkov, V., Kimura, A., Kivel, N., Knapova, I., Kokkoris, M., Krtička, M., Leal-Cidoncha, E., Leeb, H., Licata, M., Lo Meo, S., Losito, R., Macina, D., Marganiec, J., Martínez, T., Massimi, C., Mastinu, P., Mastromarco, M., Matteucci, F., Mendoza, E., Milazzo, P.M., Mingrone, F., Mirea, M., Montesano, S., Musumarra, A., Nolte, R., Palomo-Pinto, F.R., Paradela, C., Patronis, N., Pavlik, A., Perkowski, J., Porras, J.I., Praena, J., Quesada, J.M., Rauscher, T., Riego-Perez, A., Robles, M., Rubbia, C., Ryan, J.A., Sabaté-Gilarte, M., Saxena, A., Schillebeeckx, P., Schmidt, S., Schumann, D., Sedyshev, P., Smith, A.G., Stamatopoulos, A., Suryanarayana, S.V., Tagliente, G., Tain, J.L., Tarifeño-Saldivia, A., Tassan-Got, L., Tsinganis, A., Vannini, G., Variale, V., Vaz, P., Ventura, A., Vlachoudis, V., Vlastou, R., Wallner, A., Warren, S., Weigand, M., Wright, T., Žugec, P.
Lenguaje:eng
Publicado: 2019
Materias:
Acceso en línea:https://dx.doi.org/10.1016/j.physletb.2019.01.045
http://cds.cern.ch/record/2655559
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author Lederer-Woods, Claudia
Battino, U.
Ferreira, P.
Gawlik, A.
Guerrero, C.
Gunsing, F.
Heinitz, S.
Lerendegui-Marco, J.
Mengoni, A.
Reifarth, R.
Tattersall, A.
Valenta, S.
Weiss, C.
Aberle, O.
Andrzejewski, J.
Audouin, L.
Bécares, V.
Bacak, M.
Balibrea, J.
Barbagallo, M.
Barros, S.
Bečvář, F.
Beinrucker, C.
Belloni, F.
Berthoumieux, E.
Billowes, J.
Bosnar, D.
Brugger, M.
Caamaño, M.
Calviño, F.
Calviani, M.
Cano-Ott, D.
Cerutti, F.
Chiaveri, E.
Colonna, N.
Cortés, G.
Cortés-Giraldo, M.A.
Cosentino, L.
Damone, L.A.
Deo, K.
Diakaki, M.
Dietz, M.
Domingo-Pardo, C.
Dressler, R.
Dupont, E.
Durán, I.
Fernández-Domínguez, B.
Ferrari, A.
Finocchiaro, P.
Frost, R.J.W.
Furman, V.
Göbel, K.
García, A.R.
Gheorghe, I.
Glodariu, T.
Gonçalves, I.F.
González-Romero, E.
Goverdovski, A.
Griesmayer, E.
Harada, H.
Heftrich, T.
Hernández-Prieto, A.
Heyse, J.
Jenkins, D.G.
Jericha, E.
Käppeler, F.
Kadi, Y.
Katabuchi, T.
Kavrigin, P.
Ketlerov, V.
Khryachkov, V.
Kimura, A.
Kivel, N.
Knapova, I.
Kokkoris, M.
Krtička, M.
Leal-Cidoncha, E.
Leeb, H.
Licata, M.
Lo Meo, S.
Losito, R.
Macina, D.
Marganiec, J.
Martínez, T.
Massimi, C.
Mastinu, P.
Mastromarco, M.
Matteucci, F.
Mendoza, E.
Milazzo, P.M.
Mingrone, F.
Mirea, M.
Montesano, S.
Musumarra, A.
Nolte, R.
Palomo-Pinto, F.R.
Paradela, C.
Patronis, N.
Pavlik, A.
Perkowski, J.
Porras, J.I.
Praena, J.
Quesada, J.M.
Rauscher, T.
Riego-Perez, A.
Robles, M.
Rubbia, C.
Ryan, J.A.
Sabaté-Gilarte, M.
Saxena, A.
Schillebeeckx, P.
Schmidt, S.
Schumann, D.
Sedyshev, P.
Smith, A.G.
Stamatopoulos, A.
Suryanarayana, S.V.
Tagliente, G.
Tain, J.L.
Tarifeño-Saldivia, A.
Tassan-Got, L.
Tsinganis, A.
Vannini, G.
Variale, V.
Vaz, P.
Ventura, A.
Vlachoudis, V.
Vlastou, R.
Wallner, A.
Warren, S.
Weigand, M.
Wright, T.
Žugec, P.
author_facet Lederer-Woods, Claudia
Battino, U.
Ferreira, P.
Gawlik, A.
Guerrero, C.
Gunsing, F.
Heinitz, S.
Lerendegui-Marco, J.
Mengoni, A.
Reifarth, R.
Tattersall, A.
Valenta, S.
Weiss, C.
Aberle, O.
Andrzejewski, J.
Audouin, L.
Bécares, V.
Bacak, M.
Balibrea, J.
Barbagallo, M.
Barros, S.
Bečvář, F.
Beinrucker, C.
Belloni, F.
Berthoumieux, E.
Billowes, J.
Bosnar, D.
Brugger, M.
Caamaño, M.
Calviño, F.
Calviani, M.
Cano-Ott, D.
Cerutti, F.
Chiaveri, E.
Colonna, N.
Cortés, G.
Cortés-Giraldo, M.A.
Cosentino, L.
Damone, L.A.
Deo, K.
Diakaki, M.
Dietz, M.
Domingo-Pardo, C.
Dressler, R.
Dupont, E.
Durán, I.
Fernández-Domínguez, B.
Ferrari, A.
Finocchiaro, P.
Frost, R.J.W.
Furman, V.
Göbel, K.
García, A.R.
Gheorghe, I.
Glodariu, T.
Gonçalves, I.F.
González-Romero, E.
Goverdovski, A.
Griesmayer, E.
Harada, H.
Heftrich, T.
Hernández-Prieto, A.
Heyse, J.
Jenkins, D.G.
Jericha, E.
Käppeler, F.
Kadi, Y.
Katabuchi, T.
Kavrigin, P.
Ketlerov, V.
Khryachkov, V.
Kimura, A.
Kivel, N.
Knapova, I.
Kokkoris, M.
Krtička, M.
Leal-Cidoncha, E.
Leeb, H.
Licata, M.
Lo Meo, S.
Losito, R.
Macina, D.
Marganiec, J.
Martínez, T.
Massimi, C.
Mastinu, P.
Mastromarco, M.
Matteucci, F.
Mendoza, E.
Milazzo, P.M.
Mingrone, F.
Mirea, M.
Montesano, S.
Musumarra, A.
Nolte, R.
Palomo-Pinto, F.R.
Paradela, C.
Patronis, N.
Pavlik, A.
Perkowski, J.
Porras, J.I.
Praena, J.
Quesada, J.M.
Rauscher, T.
Riego-Perez, A.
Robles, M.
Rubbia, C.
Ryan, J.A.
Sabaté-Gilarte, M.
Saxena, A.
Schillebeeckx, P.
Schmidt, S.
Schumann, D.
Sedyshev, P.
Smith, A.G.
Stamatopoulos, A.
Suryanarayana, S.V.
Tagliente, G.
Tain, J.L.
Tarifeño-Saldivia, A.
Tassan-Got, L.
Tsinganis, A.
Vannini, G.
Variale, V.
Vaz, P.
Ventura, A.
Vlachoudis, V.
Vlastou, R.
Wallner, A.
Warren, S.
Weigand, M.
Wright, T.
Žugec, P.
author_sort Lederer-Woods, Claudia
collection CERN
description 73 Ge( n,γ ) cross sections were measured at the neutron time-of-flight facility n_TOF at CERN up to neutron energies of 300 keV, providing for the first time experimental data above 8 keV. Results indicate that the stellar cross section at kT=30 keV is 1.5 to 1.7 times higher than most theoretical predictions. The new cross sections result in a substantial decrease of 73 Ge produced in stars, which would explain the low isotopic abundance of 73 Ge in the solar system.
id cern-2655559
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2019
record_format invenio
spelling cern-26555592023-03-14T19:20:14Zdoi:10.1016/j.physletb.2019.01.045http://cds.cern.ch/record/2655559engLederer-Woods, ClaudiaBattino, U.Ferreira, P.Gawlik, A.Guerrero, C.Gunsing, F.Heinitz, S.Lerendegui-Marco, J.Mengoni, A.Reifarth, R.Tattersall, A.Valenta, S.Weiss, C.Aberle, O.Andrzejewski, J.Audouin, L.Bécares, V.Bacak, M.Balibrea, J.Barbagallo, M.Barros, S.Bečvář, F.Beinrucker, C.Belloni, F.Berthoumieux, E.Billowes, J.Bosnar, D.Brugger, M.Caamaño, M.Calviño, F.Calviani, M.Cano-Ott, D.Cerutti, F.Chiaveri, E.Colonna, N.Cortés, G.Cortés-Giraldo, M.A.Cosentino, L.Damone, L.A.Deo, K.Diakaki, M.Dietz, M.Domingo-Pardo, C.Dressler, R.Dupont, E.Durán, I.Fernández-Domínguez, B.Ferrari, A.Finocchiaro, P.Frost, R.J.W.Furman, V.Göbel, K.García, A.R.Gheorghe, I.Glodariu, T.Gonçalves, I.F.González-Romero, E.Goverdovski, A.Griesmayer, E.Harada, H.Heftrich, T.Hernández-Prieto, A.Heyse, J.Jenkins, D.G.Jericha, E.Käppeler, F.Kadi, Y.Katabuchi, T.Kavrigin, P.Ketlerov, V.Khryachkov, V.Kimura, A.Kivel, N.Knapova, I.Kokkoris, M.Krtička, M.Leal-Cidoncha, E.Leeb, H.Licata, M.Lo Meo, S.Losito, R.Macina, D.Marganiec, J.Martínez, T.Massimi, C.Mastinu, P.Mastromarco, M.Matteucci, F.Mendoza, E.Milazzo, P.M.Mingrone, F.Mirea, M.Montesano, S.Musumarra, A.Nolte, R.Palomo-Pinto, F.R.Paradela, C.Patronis, N.Pavlik, A.Perkowski, J.Porras, J.I.Praena, J.Quesada, J.M.Rauscher, T.Riego-Perez, A.Robles, M.Rubbia, C.Ryan, J.A.Sabaté-Gilarte, M.Saxena, A.Schillebeeckx, P.Schmidt, S.Schumann, D.Sedyshev, P.Smith, A.G.Stamatopoulos, A.Suryanarayana, S.V.Tagliente, G.Tain, J.L.Tarifeño-Saldivia, A.Tassan-Got, L.Tsinganis, A.Vannini, G.Variale, V.Vaz, P.Ventura, A.Vlachoudis, V.Vlastou, R.Wallner, A.Warren, S.Weigand, M.Wright, T.Žugec, P.Measurement of $^{73}$Ge($n,γ$) cross sections and implications for stellar nucleosynthesisnucl-exNuclear Physics - Experiment73 Ge( n,γ ) cross sections were measured at the neutron time-of-flight facility n_TOF at CERN up to neutron energies of 300 keV, providing for the first time experimental data above 8 keV. Results indicate that the stellar cross section at kT=30 keV is 1.5 to 1.7 times higher than most theoretical predictions. The new cross sections result in a substantial decrease of 73 Ge produced in stars, which would explain the low isotopic abundance of 73 Ge in the solar system.$^{73}$Ge($n,γ$) cross sections were measured at the neutron time-of-flight facility n_TOF at CERN up to neutron energies of 300 keV, providing for the first time experimental data above 8 keV. Results indicate that the stellar cross section at kT = 30 keV is 1.5 to 1.7 times higher than most theoretical predictions. The new cross sections result in a substantial decrease of 73Ge produced in stars, which would explain the low isotopic abundance of 73Ge in the solar system.arXiv:1901.10207oai:cds.cern.ch:26555592019-01-29
spellingShingle nucl-ex
Nuclear Physics - Experiment
Lederer-Woods, Claudia
Battino, U.
Ferreira, P.
Gawlik, A.
Guerrero, C.
Gunsing, F.
Heinitz, S.
Lerendegui-Marco, J.
Mengoni, A.
Reifarth, R.
Tattersall, A.
Valenta, S.
Weiss, C.
Aberle, O.
Andrzejewski, J.
Audouin, L.
Bécares, V.
Bacak, M.
Balibrea, J.
Barbagallo, M.
Barros, S.
Bečvář, F.
Beinrucker, C.
Belloni, F.
Berthoumieux, E.
Billowes, J.
Bosnar, D.
Brugger, M.
Caamaño, M.
Calviño, F.
Calviani, M.
Cano-Ott, D.
Cerutti, F.
Chiaveri, E.
Colonna, N.
Cortés, G.
Cortés-Giraldo, M.A.
Cosentino, L.
Damone, L.A.
Deo, K.
Diakaki, M.
Dietz, M.
Domingo-Pardo, C.
Dressler, R.
Dupont, E.
Durán, I.
Fernández-Domínguez, B.
Ferrari, A.
Finocchiaro, P.
Frost, R.J.W.
Furman, V.
Göbel, K.
García, A.R.
Gheorghe, I.
Glodariu, T.
Gonçalves, I.F.
González-Romero, E.
Goverdovski, A.
Griesmayer, E.
Harada, H.
Heftrich, T.
Hernández-Prieto, A.
Heyse, J.
Jenkins, D.G.
Jericha, E.
Käppeler, F.
Kadi, Y.
Katabuchi, T.
Kavrigin, P.
Ketlerov, V.
Khryachkov, V.
Kimura, A.
Kivel, N.
Knapova, I.
Kokkoris, M.
Krtička, M.
Leal-Cidoncha, E.
Leeb, H.
Licata, M.
Lo Meo, S.
Losito, R.
Macina, D.
Marganiec, J.
Martínez, T.
Massimi, C.
Mastinu, P.
Mastromarco, M.
Matteucci, F.
Mendoza, E.
Milazzo, P.M.
Mingrone, F.
Mirea, M.
Montesano, S.
Musumarra, A.
Nolte, R.
Palomo-Pinto, F.R.
Paradela, C.
Patronis, N.
Pavlik, A.
Perkowski, J.
Porras, J.I.
Praena, J.
Quesada, J.M.
Rauscher, T.
Riego-Perez, A.
Robles, M.
Rubbia, C.
Ryan, J.A.
Sabaté-Gilarte, M.
Saxena, A.
Schillebeeckx, P.
Schmidt, S.
Schumann, D.
Sedyshev, P.
Smith, A.G.
Stamatopoulos, A.
Suryanarayana, S.V.
Tagliente, G.
Tain, J.L.
Tarifeño-Saldivia, A.
Tassan-Got, L.
Tsinganis, A.
Vannini, G.
Variale, V.
Vaz, P.
Ventura, A.
Vlachoudis, V.
Vlastou, R.
Wallner, A.
Warren, S.
Weigand, M.
Wright, T.
Žugec, P.
Measurement of $^{73}$Ge($n,γ$) cross sections and implications for stellar nucleosynthesis
title Measurement of $^{73}$Ge($n,γ$) cross sections and implications for stellar nucleosynthesis
title_full Measurement of $^{73}$Ge($n,γ$) cross sections and implications for stellar nucleosynthesis
title_fullStr Measurement of $^{73}$Ge($n,γ$) cross sections and implications for stellar nucleosynthesis
title_full_unstemmed Measurement of $^{73}$Ge($n,γ$) cross sections and implications for stellar nucleosynthesis
title_short Measurement of $^{73}$Ge($n,γ$) cross sections and implications for stellar nucleosynthesis
title_sort measurement of $^{73}$ge($n,γ$) cross sections and implications for stellar nucleosynthesis
topic nucl-ex
Nuclear Physics - Experiment
url https://dx.doi.org/10.1016/j.physletb.2019.01.045
http://cds.cern.ch/record/2655559
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AT mastinup measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT mastromarcom measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT matteuccif measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT mendozae measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT milazzopm measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT mingronef measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT miream measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT montesanos measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT musumarraa measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT nolter measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT palomopintofr measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT paradelac measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT patronisn measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT pavlika measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT perkowskij measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT porrasji measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT praenaj measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT quesadajm measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT rauschert measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT riegopereza measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT roblesm measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT rubbiac measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT ryanja measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT sabategilartem measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT saxenaa measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT schillebeeckxp measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT schmidts measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT schumannd measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT sedyshevp measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT smithag measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT stamatopoulosa measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT suryanarayanasv measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT taglienteg measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT tainjl measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT tarifenosaldiviaa measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT tassangotl measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT tsinganisa measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT vanninig measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT varialev measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT vazp measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT venturaa measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT vlachoudisv measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT vlastour measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT wallnera measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT warrens measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT weigandm measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT wrightt measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis
AT zugecp measurementof73gengcrosssectionsandimplicationsforstellarnucleosynthesis