Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Heftrich Michael"'
Autor:
Göbel Kathrin, Beinrucker Clemens, Erbacher Philipp, Fiebiger Stefan, Fonseca Micaela, Heftrich Michael, Heftrich Tanja, Käppeler Franz, Krása Antonin, Lederer-Woods Claudia, Plag Ralf, Plompen Arjan, Reifarth René, Schmidt Stefan, Sonnabend Kerstin, Weigand Mario
Publikováno v:
EPJ Web of Conferences, Vol 146, p 01014 (2017)
We measured the neutron capture cross sections of 69Ga and 71Ga for a quasi-stellar spectrum at kBT = 25 keV and a spectrum with a peak energy at 90 keV by the activation technique at the Joint Research Centre (JRC) in Geel, Belgium. Protons were pro
Externí odkaz:
https://doaj.org/article/823b289a65764369a41ac3d57aeb6683
Autor:
Goebel, Kathrin, Beinrucker, Clemens, Bruckner, Benjamin, Erbacher, Philipp, Fiebiger, Stefan, Fonseca, Micaela, Heftrich, Michael, Heftrich, Tanja, Kaeppeler, Franz, Krasa, Antonin, Kurtulgil, Deniz, Lederer-Woods, Claudia, Plag, Ralf, Plompen, Arjan, Reifarth, Rene, Schmidt, Stefan, Sonnabend, Kerstin, Weigand, Mario
Publikováno v:
Goebel, K, Beinrucker, C, Bruckner, B, Erbacher, P, Fiebiger, S, Fonseca, M, Heftrich, M, Heftrich, T, Kaeppeler, F, Krasa, A, Kurtulgil, D, Lederer-Woods, C, Plag, R, Plompen, A, Reifarth, R, Schmidt, S, Sonnabend, K & Weigand, M 2021, ' Neutron activation of Ga-69 and Ga-71 at k(B)T approximate to 25 keV ', Physical Review C, vol. 103, no. 2, 025802, pp. 1-7 . https://doi.org/10.1103/PhysRevC.103.025802
Background: About 50% of heavy elements are produced by the slow neutron capture process (s process) in stars. The element gallium is mostly produced during the weak s process in massive stars.Purpose: Our activation at kBT ≈ 25 keV is the first ex
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3094::f2b0dde8e7080307fad0693eeecf486a
https://www.pure.ed.ac.uk/ws/files/304584175/PhysRevC.103.025802.pdf
https://www.pure.ed.ac.uk/ws/files/304584175/PhysRevC.103.025802.pdf
Autor:
Göbel, Kathrin, Beinrucker, Clemens, Brückner, Benjamin, Erbacher, Philipp, Fiebiger, Stefan, Fonseca, Micaela, Heftrich, Michael, Heftrich, Tanja, Käppeler, Franz, Krása, Antonin, Kurtulgil, Deniz, Lederer-Woods, Claudia, Plag, Ralf, Plompen, Arjan, Reifarth, René, Schmidt, Stefan, Sonnabend, Kerstin, Weigand, Mario
Publikováno v:
Repositório Científico de Acesso Aberto de Portugal
Repositório Científico de Acesso Aberto de Portugal (RCAAP)
instacron:RCAAP
Repositório Científico de Acesso Aberto de Portugal (RCAAP)
instacron:RCAAP
BMBF (05P15RFFN1) DFG (RE 3461/4-1) Background: About 50% of heavy elements are produced by the slow neutron capture process (s process) in stars. The element gallium is mostly produced during the weak s process in massive stars. Purpose: Our activat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::d2642b3830920ddb5d398dcea575347a
Autor:
Göbel, Kathrin, Beinrucker, Clemens, Erbacher, Philipp, Fiebiger, Stefan, Fonseca, Micaela, Heftrich, Michael, Heftrich, Tanja, Käppeler, Franz, Krása, Antonin, Lederer-Woods, Claudia, Plag, Ralf, Plompen, Arjan, Reifarth, René, Schmidt, Stefan, Sonnabend, Kerstin, Weigand, Mario
Publikováno v:
EPJ Web of Conferences; 2017, Vol. 146, p1-3, 3p