Zobrazeno 1 - 10
of 60
pro vyhledávání: '"H. Herndl"'
Publikováno v:
Physical Review C. 58:1798-1803
Updated stellar rates for the reaction {sup 23}Mg(p,{gamma}){sup 24}Al are calculated by using all available experimental information on {sup 24}Al excitation energies. Proton and {gamma}-ray partial widths for astrophysically important resonances ar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::eca6a2dc8df7d58563a46efd420f59d5
https://doi.org/10.1103/physrevc.58.1798
https://doi.org/10.1103/physrevc.58.1798
Autor:
Jean Vanhorenbeeck, P. Duhamel, H. Herndl, Michel Gaelens, Freddy Binon, W. Galster, H. Oberhummer, Cs. Sükösd, Alain Ninane, J.S. Graulich, C.R. Bain, Marc Huyse, G. Vancraeynest, Robert Page, Alan Shotter, Michael Wiescher, Philip Woods, E. Liénard, Patrick Decrock, C. Michotte, P. Leleux, R. Coszach, P. Van Duppen, Th. Delbar, Jean Vervier, P. Lipnik, Thomas Davinson
Publikováno v:
Physical Review C. 57:2711-2723
The population of the Na-20 resonances at 448, 661, 797, and 887 keV above the proton threshold has been studied in measurements of the Ne-19(p,gamma)Na-20 reaction with radioactive Ne-19 beams. The data have been analyzed fully in terms of resonance
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f52ac6e43e285079088081f65c9c0b38
https://doi.org/10.1103/physrevc.57.2711
https://doi.org/10.1103/physrevc.57.2711
Autor:
B. A. Brown, H. Herndl
Publikováno v:
Nuclear Physics A. 627:35-52
Extensive shell-model calculations in the mass range A = 86–100 on the neutron-deficient side of the nuclear chart are performed. The complete spectra of all isotopes are computed and compared to experimental excitation energies where available. Be
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::36e55aec8ef73d8398210c51809d7d38
https://doi.org/10.1016/s0375-9474(97)00407-7
https://doi.org/10.1016/s0375-9474(97)00407-7
Autor:
G. P. A. Berg, E. J. Stephenson, T. Black, A.D. Bacher, Edward Stech, Joachim Görres, K. Jiang, H. Herndl, Seonho Choi, N. Kaloskamis, P. Tischhauser, C. C. Foster, Hendrik Schatz, Michael Wiescher
Publikováno v:
Physical Review Letters. 79:3845-3848
The ${}^{28}\mathrm{Si}(\ensuremath{\alpha}{,}^{8}\mathrm{He}{)}^{24}\mathrm{Si}$ reaction has been used to measure the energies of the first two excited states in ${}^{24}$Si. The excitation energies were found to be $1.879\ifmmode\pm\else\textpm\fi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::01de8447b58cf3805d2b15db8d57d13f
https://doi.org/10.1103/physrevlett.79.3845
https://doi.org/10.1103/physrevlett.79.3845
Publikováno v:
Zeitschrift für Physik A: Hadrons and Nuclei. 355:101-105
Recent investigations suggest that the neutrino--heated hot bubble between the nascent neutron star and the overlying stellar mantle of a type--II supernova may be the site of the r--process. In the preceding $\alpha$--process building up the element
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::552a1aa68774bcec9e5c8e9e77a6bf4f
https://doi.org/10.1007/s002180050084
https://doi.org/10.1007/s002180050084
Publikováno v:
Scopus-Elsevier
ResearcherID
ResearcherID
Neutron--induced nucleosynthesis plays an important role in astrophysical scenarios like in primordial nucleosynthesis in the early universe, in the s--process occurring in Red Giants, and in the $\alpha$--rich freeze--out and r--process taking place
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::23df3a8f50a1f32886f7ec5253f455a4
https://doi.org/10.1007/bf01931785
https://doi.org/10.1007/bf01931785
Autor:
C. Coceva, H. Beer, R. Hofinger, Yu. P. Popov, Peter Mohr, P. V. Sedyshev, Heinz Oberhummer, H. Herndl
Publikováno v:
Physical Review C. 54:2014-2022
At the Karlsruhe pulsed 3.75 MV Van de Graaff accelerator the thermonuclear $^{48}\mathrm{Ca}$(n,\ensuremath{\gamma}${)}^{49}$Ca(8.72 min) cross section was measured by the fast cyclic activation technique via the 3084.4 keV \ensuremath{\gamma}-ray l
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d56e782e3083da65021cddde25f8036e
https://doi.org/10.1103/physrevc.54.2014
https://doi.org/10.1103/physrevc.54.2014
Publikováno v:
Physical Review C. 53:977-981
The neutron capture rate on $^{15}\mathrm{N}$ may be of considerable importance for s-process nucleosynthesis in red giants as well as for the nucleosynthesis in inhomogeneous big bang scenarios. We measured the reaction cross section of $^{15}\mathr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2550b04f9c9695ba647e5cf4a172a460
https://doi.org/10.1103/physrevc.53.977
https://doi.org/10.1103/physrevc.53.977
Publikováno v:
Physical Review C. 53:475-496
Existing experimental proton stripping reaction data on {sup 25}Mg leading to threshold states in {sup 26}Al are reinvestigated and reanalyzed in a consistent and improved manner. We use unbound state form factors in the DWBA analysis of the measured
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2a316a214f796b1df1b5b9138ab7478c
https://doi.org/10.1103/physrevc.53.475
https://doi.org/10.1103/physrevc.53.475
Autor:
H. Herndl, Hendrik Schatz, F. Käppeler, H. Beer, Joachim Görres, Michael Wiescher, J. Meissner
Publikováno v:
Physical Review C. 53:459-468
The neutron capture rate on $^{18}\mathrm{O}$ is of considerable interest in the interpretation of nucleosynthesis in inhomogeneous big bang scenarios and for stellar helium burning in massive red giant stars as well as AGB stars. We measured the rea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::daa21a7f9211fd28daf39d35c6f8642d
https://doi.org/10.1103/physrevc.53.459
https://doi.org/10.1103/physrevc.53.459