Zobrazeno 1 - 10
of 200
pro vyhledávání: '"Knie, K."'
Autor:
Wallner, A., Faestermann, T., Feige, J., Feldstein, C., Knie, K., Korschinek, G., Kutschera, W., Ofan, A., Paul, M., Quinto, F., Rugel, G., Steier, P.
Publikováno v:
Nature Communications 6:5956, 2015
Half of the heavy elements including all actinides are produced in r-process nucleosynthesis whose sites and history still remain a mystery. If continuously produced, the Interstellar Medium (ISM) is expected to build up a quasi-steady state of abund
Externí odkaz:
http://arxiv.org/abs/1509.08054
Autor:
Dillmann, I., Heil, M., Käppeler, F., Faestermann, T., Knie, K., Korschinek, G., Poutivtsev, M., Rugel, G., Wallner, A., Rauscher, T.
Although $^{79}$Se represents an important branching in the weak s process, the stellar neutron capture cross sections to this isotope have not yet been measured experimentally. In this case, experimental data is essential for evaluating the importan
Externí odkaz:
http://arxiv.org/abs/0806.2063
Autor:
Fitoussi, C., Raisbeck, G. M., Knie, K., Korschinek, G., Faestermann, T., Goriely, S., Lunney, D., Poutivtsev, M., Rugel, G., Waelbroeck, C., Wallner, A.
Publikováno v:
Phys.Rev.Lett.101:121101,2008
An 60Fe peak in a deep-sea FeMn crust has been interpreted as due to the signature left by the ejecta of a supernova explosion close to the solar system 2.8 +/- 0.4 Myr ago [Knie et al., Phys. Rev. Lett. 93, 171103 (2004)]. To confirm this interpreta
Externí odkaz:
http://arxiv.org/abs/0709.4197
Autor:
Wallner, A., Rühm, W., Rugel, G., Nakamura, N., Arazi, A., Faestermann, T., Knie, K., Maier, H. J., Korschinek, G.
Publikováno v:
Radiation Research, 2010 Aug 01. 174(2), 137-145.
Externí odkaz:
https://www.jstor.org/stable/40785305
Autor:
Rühm, W., Wanner, A., Cullings, H., Egbert, S. D., El-Faramawy, N., Faestermann, T., Kaul, D., Knie, K., Korschinek, G., Nakamura, N., Roberts, J., Rugel, G.
Publikováno v:
Radiation Research, 2010 Aug 01. 174(2), 146-154.
Externí odkaz:
https://www.jstor.org/stable/40785306
Autor:
Marchetti, A. A., McAninch, J. E., Rugel, G., Rühm, W., Korschinek, G., Martinelli, R. E., Faestermann, T., Knie, K., Egbert, S. D., Wallner, A., Wallner, C., Tanaka, K., Endo, S., Hoshi, M., Shizuma, K., Fujita, S., Hasai, H., Imanaka, T., Straume, T.
Publikováno v:
Radiation Research, 2009 Jan 01. 171(1), 118-122.
Externí odkaz:
https://www.jstor.org/stable/25167853
Autor:
Dolinskii, A., Knie, K., Dimopoulou, C., Gostishchev, V., Litvinov, S., Nolden, F., Steck, M.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 2011 629(1):16-24
Publikováno v:
GMS Journal for Medical Education; VOL: 37; DOC83 /20201203/
Since October 2018, a longitudinal communication curriculum for medical students has been implemented at Witten/Herdecke University. In the summer semester 2020, the concept for the 4th preclinical semester included a practical training on "sharing i
Publikováno v:
Physical Review Letters 125(2020)13, 031101
For the time period from 1.5 to 4 Myr before present we found in deep ocean ferromanganese crusts a 53Mn excess concentration in terms of 53Mn/Mn of about 4 x 10^-14 over that expected for cosmogenic production. We conclude that this 53Mn is of super
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4577::b5d02b46c4aa966628e982c5e4350eb4
https://www.hzdr.de/publications/Publ-31232-1
https://www.hzdr.de/publications/Publ-31232-1
Publikováno v:
eingereichtes Abstract für abgesagte DPG-Frühjahrstagung: https://www.dpg-verhandlungen.de/year/2020/conference/hannover/part/ms/session/12/contribution/4
For the age range from 1.5 to 4 Myr ago we found in deep ocean ferromanganese crusts an excess concentration in terms of 53Mn/Mn of about 4 · 10−14 over that expected for cosmogenic production. We conclude that this 53Mn is of supernova origin bec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4577::7133f08eac287511b0865dcec975b316
https://www.hzdr.de/publications/Publ-30214-2
https://www.hzdr.de/publications/Publ-30214-2