Coulomb breakup of 17Ne from the viewpoint of nuclear astrophysics

J. Marganiec; F. Aksouh; Y. Aksyutina; H. Alvarez Pol; T. Aumann; S. Beceiro; C. Bertulani; K. Boretzky; M. J. Borge; M. Chartier; A. Chatillon; L. Chulkov; D. Cortina-Gil; I. Egorova; H. Emling; O. Ershova; C. Forssén; L. M. Fraile; H. Fynbo; D. Galaviz; H. Geissel; L. Grigorenko; M. Heil; D. H.H. Hoffmann; J. Hoffmann; H. Johansson; B. Jonson; C. Karagiannis; O. Kiselev; J. V. Kratz; R. Kulessa; N. Kurz; C. Langer; M. Lantz; K. Larsson; T. Le Bleis; R. Lemmon; A. Lindahl; Yu A. Litvinov; K. Mahata; C. Müntz; T. Nilsson; C. Nociforo; G. Nyman; W. Ott; V. Panin; Yu Parfenova; S. Paschalis; A. Perea; R. Plag; R. Reifarth; A. Richter; C. Rodríguez Tajes; D. Rossi; G. Schrieder; N. Shulgina; H. Simon; J. Stroth; K. Sümmerer; J. Taylor; O. Tengblad; E. Tengborn; F. Wamers; H. Weick; C. Wimmer; M. Zhukov

Coulomb breakup of ¹⁷Ne from the viewpoint of nuclear astrophysics

J. Marganiec
, F. Aksouh
, Y. Aksyutina
, H. Alvarez Pol
, T. Aumann
, S. Beceiro
, C. Bertulani
, K. Boretzky
, M. J. Borge
, M. Chartier
, A. Chatillon
, L. Chulkov
, D. Cortina-Gil
, I. Egorova
, H. Emling
, O. Ershova
, C. Forssén
, L. M. Fraile
, H. Fynbo
, D. Galaviz

H. Geissel, L. Grigorenko, M. Heil, D. H.H. Hoffmann, J. Hoffmann, H. Johansson, B. Jonson, C. Karagiannis, O. Kiselev, J. V. Kratz, R. Kulessa, N. Kurz, C. Langer, M. Lantz, K. Larsson, T. Le Bleis, R. Lemmon, A. Lindahl, Yu A. Litvinov, K. Mahata, C. Müntz, T. Nilsson, C. Nociforo, G. Nyman, W. Ott, V. Panin, Yu Parfenova, S. Paschalis, A. Perea, R. Plag, R. Reifarth, A. Richter, C. Rodríguez Tajes, D. Rossi, G. Schrieder, N. Shulgina, H. Simon, J. Stroth, K. Sümmerer, J. Taylor, O. Tengblad, E. Tengborn, F. Wamers, H. Weick, C. Wimmer, M. Zhukov

Research output: Contribution to journal › Conference article › peer-review

Abstract

By the Coulomb breakup of ¹⁷Ne, the time-reversed reaction ¹⁵O(2p,γ)¹⁷Ne has been studied. This reaction might play an important role in the rp process, as a break-out reaction of the hot CNO cycle. The secondary ¹⁷Ne ion beam with an energy of 500 MeV/nucleon has been dissociated in a Pb target. The reaction products have been detected with the LAND-R³B experimental setup at GSI. The preliminary differential and integral Coulomb dissociation cross section s_Coul has been determined, which then will be converted into a photo-absorption cross section s_phot _o, and a two-proton radiative capture cross section σ_cap. Additionally, information about the structure of the ¹⁷Ne, a potential two-proton halo nucleus, will be received. The analysis is in progress.

Original language	English
Journal	Proceedings of Science
State	Published - 2012
Externally published	Yes
Event	12th International Symposium on Nuclei in the Cosmos, NIC 2012 - Cairns, QLD, Australia Duration: 5 Aug 2012 → 12 Aug 2012

Cite this

Marganiec, J., Aksouh, F., Aksyutina, Y., Alvarez Pol, H., Aumann, T., Beceiro, S., Bertulani, C., Boretzky, K., Borge, M. J., Chartier, M., Chatillon, A., Chulkov, L., Cortina-Gil, D., Egorova, I., Emling, H., Ershova, O., Forssén, C., Fraile, L. M., Fynbo, H., ... Zhukov, M. (2012). Coulomb breakup of ¹⁷Ne from the viewpoint of nuclear astrophysics. Proceedings of Science.

@article{ea028af26c824c81b09b5ccc328ca135,

title = "Coulomb breakup of 17Ne from the viewpoint of nuclear astrophysics",

abstract = "By the Coulomb breakup of 17Ne, the time-reversed reaction 15O(2p,γ)17Ne has been studied. This reaction might play an important role in the rp process, as a break-out reaction of the hot CNO cycle. The secondary 17Ne ion beam with an energy of 500 MeV/nucleon has been dissociated in a Pb target. The reaction products have been detected with the LAND-R3B experimental setup at GSI. The preliminary differential and integral Coulomb dissociation cross section sCoul has been determined, which then will be converted into a photo-absorption cross section sphot o, and a two-proton radiative capture cross section σcap. Additionally, information about the structure of the 17Ne, a potential two-proton halo nucleus, will be received. The analysis is in progress.",

author = "J. Marganiec and F. Aksouh and Y. Aksyutina and \{Alvarez Pol\}, H. and T. Aumann and S. Beceiro and C. Bertulani and K. Boretzky and Borge, \{M. J.\} and M. Chartier and A. Chatillon and L. Chulkov and D. Cortina-Gil and I. Egorova and H. Emling and O. Ershova and C. Forss{\'e}n and Fraile, \{L. M.\} and H. Fynbo and D. Galaviz and H. Geissel and L. Grigorenko and M. Heil and Hoffmann, \{D. H.H.\} and J. Hoffmann and H. Johansson and B. Jonson and C. Karagiannis and O. Kiselev and Kratz, \{J. V.\} and R. Kulessa and N. Kurz and C. Langer and M. Lantz and K. Larsson and \{Le Bleis\}, T. and R. Lemmon and A. Lindahl and Litvinov, \{Yu A.\} and K. Mahata and C. M{\"u}ntz and T. Nilsson and C. Nociforo and G. Nyman and W. Ott and V. Panin and Yu Parfenova and S. Paschalis and A. Perea and R. Plag and R. Reifarth and A. Richter and \{Rodr{\'i}guez Tajes\}, C. and D. Rossi and G. Schrieder and N. Shulgina and H. Simon and J. Stroth and K. S{\"u}mmerer and J. Taylor and O. Tengblad and E. Tengborn and F. Wamers and H. Weick and C. Wimmer and M. Zhukov",

year = "2012",

language = "英语",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

note = "12th International Symposium on Nuclei in the Cosmos, NIC 2012 ; Conference date: 05-08-2012 Through 12-08-2012",

}

Marganiec, J, Aksouh, F, Aksyutina, Y, Alvarez Pol, H, Aumann, T, Beceiro, S, Bertulani, C, Boretzky, K, Borge, MJ, Chartier, M, Chatillon, A, Chulkov, L, Cortina-Gil, D, Egorova, I, Emling, H, Ershova, O, Forssén, C, Fraile, LM, Fynbo, H, Galaviz, D, Geissel, H, Grigorenko, L, Heil, M, Hoffmann, DHH, Hoffmann, J, Johansson, H, Jonson, B, Karagiannis, C, Kiselev, O, Kratz, JV, Kulessa, R, Kurz, N, Langer, C, Lantz, M, Larsson, K, Le Bleis, T, Lemmon, R, Lindahl, A, Litvinov, YA, Mahata, K, Müntz, C, Nilsson, T, Nociforo, C, Nyman, G, Ott, W, Panin, V, Parfenova, Y, Paschalis, S, Perea, A, Plag, R, Reifarth, R, Richter, A, Rodríguez Tajes, C, Rossi, D, Schrieder, G, Shulgina, N, Simon, H, Stroth, J, Sümmerer, K, Taylor, J, Tengblad, O, Tengborn, E, Wamers, F, Weick, H, Wimmer, C & Zhukov, M 2012, 'Coulomb breakup of ¹⁷Ne from the viewpoint of nuclear astrophysics', Proceedings of Science.

TY - JOUR

T1 - Coulomb breakup of 17Ne from the viewpoint of nuclear astrophysics

AU - Marganiec, J.

AU - Aksouh, F.

AU - Aksyutina, Y.

AU - Alvarez Pol, H.

AU - Aumann, T.

AU - Beceiro, S.

AU - Bertulani, C.

AU - Boretzky, K.

AU - Borge, M. J.

AU - Chartier, M.

AU - Chatillon, A.

AU - Chulkov, L.

AU - Cortina-Gil, D.

AU - Egorova, I.

AU - Emling, H.

AU - Ershova, O.

AU - Forssén, C.

AU - Fraile, L. M.

AU - Fynbo, H.

AU - Galaviz, D.

AU - Geissel, H.

AU - Grigorenko, L.

AU - Heil, M.

AU - Hoffmann, D. H.H.

AU - Hoffmann, J.

AU - Johansson, H.

AU - Jonson, B.

AU - Karagiannis, C.

AU - Kiselev, O.

AU - Kratz, J. V.

AU - Kulessa, R.

AU - Kurz, N.

AU - Langer, C.

AU - Lantz, M.

AU - Larsson, K.

AU - Le Bleis, T.

AU - Lemmon, R.

AU - Lindahl, A.

AU - Litvinov, Yu A.

AU - Mahata, K.

AU - Müntz, C.

AU - Nilsson, T.

AU - Nociforo, C.

AU - Nyman, G.

AU - Ott, W.

AU - Panin, V.

AU - Parfenova, Yu

AU - Paschalis, S.

AU - Perea, A.

AU - Plag, R.

AU - Reifarth, R.

AU - Richter, A.

AU - Rodríguez Tajes, C.

AU - Rossi, D.

AU - Schrieder, G.

AU - Shulgina, N.

AU - Simon, H.

AU - Stroth, J.

AU - Sümmerer, K.

AU - Taylor, J.

AU - Tengblad, O.

AU - Tengborn, E.

AU - Wamers, F.

AU - Weick, H.

AU - Wimmer, C.

AU - Zhukov, M.

PY - 2012

Y1 - 2012

N2 - By the Coulomb breakup of 17Ne, the time-reversed reaction 15O(2p,γ)17Ne has been studied. This reaction might play an important role in the rp process, as a break-out reaction of the hot CNO cycle. The secondary 17Ne ion beam with an energy of 500 MeV/nucleon has been dissociated in a Pb target. The reaction products have been detected with the LAND-R3B experimental setup at GSI. The preliminary differential and integral Coulomb dissociation cross section sCoul has been determined, which then will be converted into a photo-absorption cross section sphot o, and a two-proton radiative capture cross section σcap. Additionally, information about the structure of the 17Ne, a potential two-proton halo nucleus, will be received. The analysis is in progress.

AB - By the Coulomb breakup of 17Ne, the time-reversed reaction 15O(2p,γ)17Ne has been studied. This reaction might play an important role in the rp process, as a break-out reaction of the hot CNO cycle. The secondary 17Ne ion beam with an energy of 500 MeV/nucleon has been dissociated in a Pb target. The reaction products have been detected with the LAND-R3B experimental setup at GSI. The preliminary differential and integral Coulomb dissociation cross section sCoul has been determined, which then will be converted into a photo-absorption cross section sphot o, and a two-proton radiative capture cross section σcap. Additionally, information about the structure of the 17Ne, a potential two-proton halo nucleus, will be received. The analysis is in progress.

UR - https://www.scopus.com/pages/publications/84887450744

M3 - 会议文章

AN - SCOPUS:84887450744

SN - 1824-8039

JO - Proceedings of Science

JF - Proceedings of Science

T2 - 12th International Symposium on Nuclei in the Cosmos, NIC 2012

Y2 - 5 August 2012 through 12 August 2012

ER -

Coulomb breakup of ¹⁷Ne from the viewpoint of nuclear astrophysics

Abstract

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