Zobrazeno 1 - 10
of 1 161
pro vyhledávání: '"Langanke K."'
Autor:
Leckenby, G., Sidhu, R. S., Chen, R. J., Mancino, R., Szányi, B., Bai, M., Battino, U., Blaum, K., Brandau, C., Cristallo, S., Dickel, T., Dillmann, I., Dmytriiev, D., Faestermann, T., Forstner, O., Franczak, B., Geissel, H., Gernhäuser, R., Glorius, J., Griffin, C., Gumberidze, A., Haettner, E., Hillenbrand, P. -M., Karakas, A., Kaur, T., Korten, W., Kozhuharov, C., Kuzminchuk, N., Langanke, K., Litvinov, S., Litvinov, Y. A., Lugaro, M., Martínez-Pinedo, G., Menz, E., Meyer, B., Morgenroth, T., Neff, T., Nociforo, C., Petridis, N., Pignatari, M., Popp, U., Purushothaman, S., Reifarth, R., Sanjari, S., Scheidenberger, C., Spillmann, U., Steck, M., Stöhlker, T., Tanaka, Y. K., Trassinelli, M., Trotsenko, S., Varga, L., Vescovi, D., Wang, M., Weick, H., López, A. Yagüe, Yamaguchi, T., Zhang, Y., Zhao, J.
Radioactive nuclei with lifetimes on the order of millions of years can reveal the formation history of the Sun and active nucleosynthesis occurring at the time and place of its birth. Among such nuclei whose decay signatures are found in the oldest
Externí odkaz:
http://arxiv.org/abs/2411.08856
Autor:
Acharya, B., Aliotta, M., Balantekin, A. B., Bemmerer, D., Bertulani, C. A., Best, A., Brune, C. R., Buompane, R., Cavanna, F., Chen, J. W., Colgan, J., Czarnecki, A., Davids, B., deBoer, R. J., Delahaye, F., Depalo, R., García, A., Johnson, M. Gatu, Gazit, D., Gialanella, L., Greife, U., Guffanti, D., Guglielmetti, A., Hambleton, K., Haxton, W. C., Herrera, Y., Huang, M., Iliadis, C., Kravvaris, K., La Cognata, M., Langanke, K., Marcucci, L. E., Nagayama, T., Nollett, K. M., Odell, D., Gann, G. D. Orebi, Piatti, D., Pinsonneault, M., Platter, L., Robertson, R. G. H., Rupak, G., Serenelli, A., Sferrazza, M., Szücs, T., Tang, X., Tumino, A., Villante, F. L., Walker-Loud, A., Zhang, X., Zuber, K.
In stars that lie on the main sequence in the Hertzsprung-Russel diagram, like our sun, hydrogen is fused to helium in a number of nuclear reaction chains and series, such as the proton-proton chain and the carbon-nitrogen-oxygen cycles. Precisely de
Externí odkaz:
http://arxiv.org/abs/2405.06470
Autor:
Tselyaev, V., Lyutorovich, N., Speth, J., Martinez-Pinedo, G., Langanke, K., Reinhard, P. -G.
We present moments and transition probabilities in the neighboring odd-mass nuclei of $^{208}$Pb calculated fully self-consistently from the s.p. properties of $^{208}$Pb with polarization corrections from its excitations, both given from previous Sk
Externí odkaz:
http://arxiv.org/abs/2201.08838
Publikováno v:
EPJ Web of Conferences, Vol 109, p 06004 (2016)
The neutrino-induced nucleosynthesis (ν process) in supernova explosions of massive stars of solar metallicity with initial main sequence masses between 15 and 40 M⊙ has been studied. A new extensive set of neutrino-nucleus cross-sections for all
Externí odkaz:
https://doaj.org/article/6ec71ecc7e2b4311ad3b15f1d62d2367
Autor:
Lyutorovich, N., Tselyaev, V., Speth, J., Martinez-Pinedo, G., Langanke, K., Reinhard, P. -G.
We analyze recent data on a long series of high-spin states in $^{208}$Pb with a self-consistent phonon-coupling model for nuclear excitations based on the Skyrme functionals. The model is the renormalized time-blocking approximation (RenTBA) which t
Externí odkaz:
http://arxiv.org/abs/2111.04602
Publikováno v:
EPJ Web of Conferences, Vol 3, p 01006 (2010)
In the next years the Facility for Antiproton and Ion Research FAIR will be constructed at the GSI Helmholtzzentrum fur Schwerionenforschung in Darmstadt, Germany. This new accelerator complex will allow for unprecedented and pathbreaking research in
Externí odkaz:
https://doaj.org/article/8d3e42c48f45434da814e806a550b446
Publikováno v:
Phys. Rev. C 101, 025805 (2020)
We have calculated electron capture rates for neutron-rich $N=50$ nuclei ($^{78}$Ni, $^{82}$Ge, $^{86}$Kr, $^{88}$Sr) within the Thermal QRPA approach at temperatures $T=0$, corresponding to capture on the ground-state, and at $T=10$ GK (0.86 MeV), w
Externí odkaz:
http://arxiv.org/abs/1910.03335
Autor:
Kirsebom, O. S., Jones, S., Strömberg, D. F., Martínez-Pinedo, G., Langanke, K., Roepke, F. K., Brown, B. A., Eronen, T., Fynbo, H. O. U., Hukkanen, M., Idini, A., Jokinen, A., Kankainen, A., Kostensalo, J., Moore, I., Möller, H., Ohlmann, S. T., Penttilä, H., Riisager, K., Rinta-Antila, S., Srivastava, P. C., Suhonen, J., Trzaska, W. H., Äystö, J.
Publikováno v:
Phys. Rev. Lett. 123, 262701 (2019)
A significant fraction of stars between 7-11 solar masses are thought to become supernovae, but the explosion mechanism is unclear. The answer depends critically on the rate of electron capture on $^{20}$Ne in the degenerate oxygen-neon stellar core.
Externí odkaz:
http://arxiv.org/abs/1905.09407
Autor:
Durante, M., Indelicato, P., Jonson, B., Koch, V., Langanke, K., Meißner, Ulf-G., Nappi, E., Nilsson, T., Stöhlker, Th., Widmann, E., Wiescher, M.
The Facility for Antiproton and Ion Research (FAIR) will be the accelerator-based flagship research facility in many basic sciences and their applications in Europe for the coming decades. FAIR will open up unprecedented research opportunities in had
Externí odkaz:
http://arxiv.org/abs/1903.05693
We study the neutrino-induced production of nuclides in explosive supernova nucleosynthesis for progenitor stars with solar metallicity including neutrino nucleus reactions for all nuclei with charge numbers $Z < 76$ with average neutrino energies in
Externí odkaz:
http://arxiv.org/abs/1805.10231