The Zr92(n,γ) reaction and its implications for stellar nucleosynthesis

G. Tagliente; P. M. Milazzo; K. Fujii; U. Abbondanno; G. Aerts; H. Álvarez; F. Alvarez-Velarde; S. Andriamonje; J. Andrzejewski; L. Audouin; G. Badurek; P. Baumann; F. Bečvář; F. Belloni; E. Berthoumieux; S. Bisterzo; F. Calviño; M. Calviani; D. Cano-Ott; R. Capote; C. Carrapiço; P. Cennini; V. Chepel; E. Chiaveri; N. Colonna; G. Cortes; A. Couture; J. Cox; M. Dahlfors; S. David; I. Dillmann; C. Domingo-Pardo; W. Dridi; I. Duran; C. Eleftheriadis; M. Embid-Segura; A. Ferrari; R. Ferreira-Marques; W. Furman; R. Gallino; I. Goncalves; E. Gonzalez-Romero; F. Gramegna; C. Guerrero; F. Gunsing; B. Haas; R. Haight; M. Heil; A. Herrera-Martinez; M. Igashira; E. Jericha; F. Käppeler; Y. Kadi; D. Karadimos; D. Karamanis; M. Kerveno; E. Kossionides; M. Krtička; C. Lamboudis; H. Leeb; A. Lindote; I. Lopes; M. Lozano; S. Lukic; J. Marganiec; S. Marrone; T. Martínez; C. Massimi; P. Mastinu; A. Mengoni; C. Moreau; M. Mosconi; F. Neves; H. Oberhummer; S. O'Brien; J. Pancin; C. Papachristodoulou; C. Papadopoulos; C. Paradela; N. Patronis; A. Pavlik; P. Pavlopoulos; L. Perrot; M. T. Pigni; R. Plag; A. Plompen; A. Plukis; A. Poch; J. Praena; C. Pretel; J. Quesada; T. Rauscher; R. Reifarth; M. Rosetti; C. Rubbia; G. Rudolf; P. Rullhusen; J. Salgado; C. Santos; L. Sarchiapone; I. Savvidis; C. Stephan; J. L. Tain; L. Tassan-Got; L. Tavora; R. Terlizzi; G. Vannini; P. Vaz; A. Ventura; D. Villamarin; M. C. Vincente; V. Vlachoudis; R. Vlastou; F. Voss; S. Walter; H. Wendler; M. Wiescher; K. Wisshak

doi:10.1103/PhysRevC.81.055801

The Zr92(n,γ) reaction and its implications for stellar nucleosynthesis

G. Tagliente, P. M. Milazzo, K. Fujii, U. Abbondanno, G. Aerts, H. Álvarez, F. Alvarez-Velarde, S. Andriamonje, J. Andrzejewski, L. Audouin, G. Badurek, P. Baumann, F. Bečvář, F. Belloni, E. Berthoumieux, S. Bisterzo, F. Calviño, M. Calviani, D. Cano-Ott, R. CapoteC. Carrapiço, P. Cennini, V. Chepel, E. Chiaveri, N. Colonna, G. Cortes, A. Couture, J. Cox, M. Dahlfors, S. David, I. Dillmann, C. Domingo-Pardo, W. Dridi, I. Duran, C. Eleftheriadis, M. Embid-Segura, A. Ferrari, R. Ferreira-Marques, W. Furman, R. Gallino, I. Goncalves, E. Gonzalez-Romero, F. Gramegna, C. Guerrero, F. Gunsing, B. Haas, R. Haight, M. Heil, A. Herrera-Martinez, M. Igashira, E. Jericha, F. Käppeler, Y. Kadi, D. Karadimos, D. Karamanis, M. Kerveno, E. Kossionides, M. Krtička, C. Lamboudis, H. Leeb, A. Lindote, I. Lopes, M. Lozano, S. Lukic, J. Marganiec, S. Marrone, T. Martínez, C. Massimi, P. Mastinu, A. Mengoni, C. Moreau, M. Mosconi, F. Neves, H. Oberhummer, S. O'Brien, J. Pancin, C. Papachristodoulou, C. Papadopoulos, C. Paradela, N. Patronis, A. Pavlik, P. Pavlopoulos, L. Perrot, M. T. Pigni, R. Plag, A. Plompen, A. Plukis, A. Poch, J. Praena, C. Pretel, J. Quesada, T. Rauscher, R. Reifarth, M. Rosetti, C. Rubbia, G. Rudolf, P. Rullhusen, J. Salgado, C. Santos, L. Sarchiapone, I. Savvidis, C. Stephan, J. L. Tain, L. Tassan-Got, L. Tavora, R. Terlizzi, G. Vannini, P. Vaz, A. Ventura, D. Villamarin, M. C. Vincente, V. Vlachoudis, R. Vlastou, F. Voss, S. Walter, H. Wendler, M. Wiescher, K. Wisshak

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Abstract

Because the relatively small neutron capture cross sections of the zirconium isotopes are difficult to measure, the results of previous measurements are often not adequate for a number of problems in astrophysics and nuclear technology. Therefore, the Zr92(n,γ) cross section has been remeasured at the CERN n-TOF facility, providing a set of improved parameters for 44 resonances in the neutron energy range up to 40 keV. With this information the cross-section uncertainties in the keV region could be reduced to 5% as required for s-process nucleosynthesis studies and technological applications.

Original language	English
Article number	055801
Journal	Physical Review C - Nuclear Physics
Volume	81
Issue number	5
DOIs	https://doi.org/10.1103/PhysRevC.81.055801
State	Published - May 5 2010
Externally published	Yes

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10.1103/PhysRevC.81.055801

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Tagliente, G., Milazzo, P. M., Fujii, K., Abbondanno, U., Aerts, G., Álvarez, H., Alvarez-Velarde, F., Andriamonje, S., Andrzejewski, J., Audouin, L., Badurek, G., Baumann, P., Bečvář, F., Belloni, F., Berthoumieux, E., Bisterzo, S., Calviño, F., Calviani, M., Cano-Ott, D., ... Wisshak, K. (2010). The Zr92(n,γ) reaction and its implications for stellar nucleosynthesis. Physical Review C - Nuclear Physics, 81(5), Article 055801. https://doi.org/10.1103/PhysRevC.81.055801

@article{231d710872dd421592feaf2baa8ef687,

title = "The Zr92(n,γ) reaction and its implications for stellar nucleosynthesis",

abstract = "Because the relatively small neutron capture cross sections of the zirconium isotopes are difficult to measure, the results of previous measurements are often not adequate for a number of problems in astrophysics and nuclear technology. Therefore, the Zr92(n,γ) cross section has been remeasured at the CERN n-TOF facility, providing a set of improved parameters for 44 resonances in the neutron energy range up to 40 keV. With this information the cross-section uncertainties in the keV region could be reduced to 5% as required for s-process nucleosynthesis studies and technological applications.",

author = "G. Tagliente and Milazzo, {P. M.} and K. Fujii and U. Abbondanno and G. Aerts and H. {\'A}lvarez and F. Alvarez-Velarde and S. Andriamonje and J. Andrzejewski and L. Audouin and G. Badurek and P. Baumann and F. Be{\v c}v{\'a}{\v r} and F. Belloni and E. Berthoumieux and S. Bisterzo and F. Calvi{\~n}o and M. Calviani and D. Cano-Ott and R. Capote and C. Carrapi{\c c}o and P. Cennini and V. Chepel and E. Chiaveri and N. Colonna and G. Cortes and A. Couture and J. Cox and M. Dahlfors and S. David and I. Dillmann and C. Domingo-Pardo and W. Dridi and I. Duran and C. Eleftheriadis and M. Embid-Segura and A. Ferrari and R. Ferreira-Marques and W. Furman and R. Gallino and I. Goncalves and E. Gonzalez-Romero and F. Gramegna and C. Guerrero and F. Gunsing and B. Haas and R. Haight and M. Heil and A. Herrera-Martinez and M. Igashira and E. Jericha and F. K{\"a}ppeler and Y. Kadi and D. Karadimos and D. Karamanis and M. Kerveno and E. Kossionides and M. Krti{\v c}ka and C. Lamboudis and H. Leeb and A. Lindote and I. Lopes and M. Lozano and S. Lukic and J. Marganiec and S. Marrone and T. Mart{\'i}nez and C. Massimi and P. Mastinu and A. Mengoni and C. Moreau and M. Mosconi and F. Neves and H. Oberhummer and S. O'Brien and J. Pancin and C. Papachristodoulou and C. Papadopoulos and C. Paradela and N. Patronis and A. Pavlik and P. Pavlopoulos and L. Perrot and Pigni, {M. T.} and R. Plag and A. Plompen and A. Plukis and A. Poch and J. Praena and C. Pretel and J. Quesada and T. Rauscher and R. Reifarth and M. Rosetti and C. Rubbia and G. Rudolf and P. Rullhusen and J. Salgado and C. Santos and L. Sarchiapone and I. Savvidis and C. Stephan and Tain, {J. L.} and L. Tassan-Got and L. Tavora and R. Terlizzi and G. Vannini and P. Vaz and A. Ventura and D. Villamarin and Vincente, {M. C.} and V. Vlachoudis and R. Vlastou and F. Voss and S. Walter and H. Wendler and M. Wiescher and K. Wisshak",

year = "2010",

month = may,

day = "5",

doi = "10.1103/PhysRevC.81.055801",

language = "English",

volume = "81",

journal = "Physical Review C - Nuclear Physics",

issn = "0556-2813",

number = "5",

}

Tagliente, G, Milazzo, PM, Fujii, K, Abbondanno, U, Aerts, G, Álvarez, H, Alvarez-Velarde, F, Andriamonje, S, Andrzejewski, J, Audouin, L, Badurek, G, Baumann, P, Bečvář, F, Belloni, F, Berthoumieux, E, Bisterzo, S, Calviño, F, Calviani, M, Cano-Ott, D, Capote, R, Carrapiço, C, Cennini, P, Chepel, V, Chiaveri, E, Colonna, N, Cortes, G, Couture, A, Cox, J, Dahlfors, M, David, S, Dillmann, I, Domingo-Pardo, C, Dridi, W, Duran, I, Eleftheriadis, C, Embid-Segura, M, Ferrari, A, Ferreira-Marques, R, Furman, W, Gallino, R, Goncalves, I, Gonzalez-Romero, E, Gramegna, F, Guerrero, C, Gunsing, F, Haas, B, Haight, R, Heil, M, Herrera-Martinez, A, Igashira, M, Jericha, E, Käppeler, F, Kadi, Y, Karadimos, D, Karamanis, D, Kerveno, M, Kossionides, E, Krtička, M, Lamboudis, C, Leeb, H, Lindote, A, Lopes, I, Lozano, M, Lukic, S, Marganiec, J, Marrone, S, Martínez, T, Massimi, C, Mastinu, P, Mengoni, A, Moreau, C, Mosconi, M, Neves, F, Oberhummer, H, O'Brien, S, Pancin, J, Papachristodoulou, C, Papadopoulos, C, Paradela, C, Patronis, N, Pavlik, A, Pavlopoulos, P, Perrot, L, Pigni, MT, Plag, R, Plompen, A, Plukis, A, Poch, A, Praena, J, Pretel, C, Quesada, J, Rauscher, T, Reifarth, R, Rosetti, M, Rubbia, C, Rudolf, G, Rullhusen, P, Salgado, J, Santos, C, Sarchiapone, L, Savvidis, I, Stephan, C, Tain, JL, Tassan-Got, L, Tavora, L, Terlizzi, R, Vannini, G, Vaz, P, Ventura, A, Villamarin, D, Vincente, MC, Vlachoudis, V, Vlastou, R, Voss, F, Walter, S, Wendler, H, Wiescher, M & Wisshak, K 2010, 'The Zr92(n,γ) reaction and its implications for stellar nucleosynthesis', Physical Review C - Nuclear Physics, vol. 81, no. 5, 055801. https://doi.org/10.1103/PhysRevC.81.055801

TY - JOUR

T1 - The Zr92(n,γ) reaction and its implications for stellar nucleosynthesis

AU - Tagliente, G.

AU - Milazzo, P. M.

AU - Fujii, K.

AU - Abbondanno, U.

AU - Aerts, G.

AU - Álvarez, H.

AU - Alvarez-Velarde, F.

AU - Andriamonje, S.

AU - Andrzejewski, J.

AU - Audouin, L.

AU - Badurek, G.

AU - Baumann, P.

AU - Bečvář, F.

AU - Belloni, F.

AU - Berthoumieux, E.

AU - Bisterzo, S.

AU - Calviño, F.

AU - Calviani, M.

AU - Cano-Ott, D.

AU - Capote, R.

AU - Carrapiço, C.

AU - Cennini, P.

AU - Chepel, V.

AU - Chiaveri, E.

AU - Colonna, N.

AU - Cortes, G.

AU - Couture, A.

AU - Cox, J.

AU - Dahlfors, M.

AU - David, S.

AU - Dillmann, I.

AU - Domingo-Pardo, C.

AU - Dridi, W.

AU - Duran, I.

AU - Eleftheriadis, C.

AU - Embid-Segura, M.

AU - Ferrari, A.

AU - Ferreira-Marques, R.

AU - Furman, W.

AU - Gallino, R.

AU - Goncalves, I.

AU - Gonzalez-Romero, E.

AU - Gramegna, F.

AU - Guerrero, C.

AU - Gunsing, F.

AU - Haas, B.

AU - Haight, R.

AU - Heil, M.

AU - Herrera-Martinez, A.

AU - Igashira, M.

AU - Jericha, E.

AU - Käppeler, F.

AU - Kadi, Y.

AU - Karadimos, D.

AU - Karamanis, D.

AU - Kerveno, M.

AU - Kossionides, E.

AU - Krtička, M.

AU - Lamboudis, C.

AU - Leeb, H.

AU - Lindote, A.

AU - Lopes, I.

AU - Lozano, M.

AU - Lukic, S.

AU - Marganiec, J.

AU - Marrone, S.

AU - Martínez, T.

AU - Massimi, C.

AU - Mastinu, P.

AU - Mengoni, A.

AU - Moreau, C.

AU - Mosconi, M.

AU - Neves, F.

AU - Oberhummer, H.

AU - O'Brien, S.

AU - Pancin, J.

AU - Papachristodoulou, C.

AU - Papadopoulos, C.

AU - Paradela, C.

AU - Patronis, N.

AU - Pavlik, A.

AU - Pavlopoulos, P.

AU - Perrot, L.

AU - Pigni, M. T.

AU - Plag, R.

AU - Plompen, A.

AU - Plukis, A.

AU - Poch, A.

AU - Praena, J.

AU - Pretel, C.

AU - Quesada, J.

AU - Rauscher, T.

AU - Reifarth, R.

AU - Rosetti, M.

AU - Rubbia, C.

AU - Rudolf, G.

AU - Rullhusen, P.

AU - Salgado, J.

AU - Santos, C.

AU - Sarchiapone, L.

AU - Savvidis, I.

AU - Stephan, C.

AU - Tain, J. L.

AU - Tassan-Got, L.

AU - Tavora, L.

AU - Terlizzi, R.

AU - Vannini, G.

AU - Vaz, P.

AU - Ventura, A.

AU - Villamarin, D.

AU - Vincente, M. C.

AU - Vlachoudis, V.

AU - Vlastou, R.

AU - Voss, F.

AU - Walter, S.

AU - Wendler, H.

AU - Wiescher, M.

AU - Wisshak, K.

PY - 2010/5/5

Y1 - 2010/5/5

N2 - Because the relatively small neutron capture cross sections of the zirconium isotopes are difficult to measure, the results of previous measurements are often not adequate for a number of problems in astrophysics and nuclear technology. Therefore, the Zr92(n,γ) cross section has been remeasured at the CERN n-TOF facility, providing a set of improved parameters for 44 resonances in the neutron energy range up to 40 keV. With this information the cross-section uncertainties in the keV region could be reduced to 5% as required for s-process nucleosynthesis studies and technological applications.

AB - Because the relatively small neutron capture cross sections of the zirconium isotopes are difficult to measure, the results of previous measurements are often not adequate for a number of problems in astrophysics and nuclear technology. Therefore, the Zr92(n,γ) cross section has been remeasured at the CERN n-TOF facility, providing a set of improved parameters for 44 resonances in the neutron energy range up to 40 keV. With this information the cross-section uncertainties in the keV region could be reduced to 5% as required for s-process nucleosynthesis studies and technological applications.

UR - http://www.scopus.com/inward/record.url?scp=77952469452&partnerID=8YFLogxK

U2 - 10.1103/PhysRevC.81.055801

DO - 10.1103/PhysRevC.81.055801

M3 - Article

AN - SCOPUS:77952469452

SN - 0556-2813

VL - 81

JO - Physical Review C - Nuclear Physics

JF - Physical Review C - Nuclear Physics

IS - 5

M1 - 055801

ER -

The Zr92(n,γ) reaction and its implications for stellar nucleosynthesis

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