Zobrazeno 1 - 10
of 3 012
pro vyhledávání: '"Rapp W"'
Autor:
Hirsch L; Department of Neuroscience, Albert-Ludwigs Universität, Institute of Sports and Sports Science, Freiburg, Germany., Barioudi H; Faculty of Information Technology, Dortmund University of Applied Sciences and Arts Dortmund, Dortmund, Germany., Wintergerst D; Department of Neuroscience, Albert-Ludwigs Universität, Institute of Sports and Sports Science, Freiburg, Germany., Rombach R; Deutscher Behindertensportverband und Nationales Paralympisches Komitee (DBS) e.V., Frechen, Germany., Rapp W; Olympic Training Center Freiburg-Hochschwarzwald, Freiburg, Germany., Felderhoff T; Faculty of Information Technology, Dortmund University of Applied Sciences and Arts Dortmund, Dortmund, Germany., Mrachacz-Kersting N; Department of Neuroscience, Albert-Ludwigs Universität, Institute of Sports and Sports Science, Freiburg, Germany.; BrainLinks-BrainTools Center, IMBIT, Albert-Ludwigs University of Freiburg, Freiburg, Germany.
Publikováno v:
Frontiers in sports and active living [Front Sports Act Living] 2024 Sep 11; Vol. 6, pp. 1441586. Date of Electronic Publication: 2024 Sep 11 (Print Publication: 2024).
Autor:
Rapp, W., Dillmann, I., Käppeler, F., Giesen, U., Klein, H., Rauscher, T., Hentschel, D., Hilpp, S.
Publikováno v:
Phys.Rev.C78:025804,2008
The $^{92}$Mo($\alpha,n$)$^{95}$Ru, $^{94}$Mo($\alpha,n$)$^{97}$Ru, and $^{112}$Sn($\alpha,\gamma$)$^{116}$Te cross sections were measured at the upper end of the $p$-process Gamow window between 8.2 MeV and 11.1 MeV. Our results are slightly lower t
Externí odkaz:
http://arxiv.org/abs/0809.0234
Publikováno v:
J.Phys.G35:014029,2008
We have performed $p$-process simulations with the most recent stellar $(n,\gamma)$ cross sections from the "Karlsruhe Astrophysical Database of Nucleosynthesis in Stars" project (version v0.2, http://nuclear-astrophysics.fzk.de/kadonis). The simulat
Externí odkaz:
http://arxiv.org/abs/0805.4756
Publikováno v:
Astrophys.J.653:474-489,2006
The astrophysical p process, which is responsible for the origin of the proton rich stable nuclei heavier than iron, was investigated using a full nuclear reaction network for a type II supernova explosion when the shock front passes through the O/Ne
Externí odkaz:
http://arxiv.org/abs/astro-ph/0608341
Autor:
Gyurky, Gy., Kiss, G. G., Elekes, Z., Fulop, Zs., Somorjai, E., Palumbo, A., Gorres, J., Lee, H. Y., Rapp, W., Wiescher, M., Ozkan, N., Guray, R. T., Efe, G., Rauscher, T
Publikováno v:
Phys.Rev. C74 (2006) 025805
The 106Cd(alpha,gamma)110Sn reaction cross section has been measured in the energy range of the Gamow window for the astrophysical p-process scenario. The cross sections for 106Cd(alpha,n)109Sn and for 106Cd(alpha,p)109In below the (alpha,n) threshol
Externí odkaz:
http://arxiv.org/abs/nucl-ex/0605034
The astrophysical p-process is responsible for the origin of the proton rich nuclei,which are heavier than iron. A huge network involving thousands of reaction rates is necessary to calculate the final p-abundances. But not all rates included in the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0408060
Publikováno v:
In Journal of Electromyography and Kinesiology February 2017 32:15-21
Autor:
Pfennig, Norbert
Elemente der Naturwissenschaft 28, p. 48-48.
Man darf dem Verlag für die Initiative dankbar sein, mit dem vorliegenden Buch eine Reihe von Aufsätzen einem grösseren Leserkreis zugänglich gemacht zu haben, welche eigens für dieses Buch gesch
Man darf dem Verlag für die Initiative dankbar sein, mit dem vorliegenden Buch eine Reihe von Aufsätzen einem grösseren Leserkreis zugänglich gemacht zu haben, welche eigens für dieses Buch gesch
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e761bc0ce22c83609e6059377cccd00b
Autor:
Abbondanno, U., Aerts, G., Álvarez, F., Álvarez, H., Andriamonje, S., Andrzejewski, J., Badurek, G., Baumann, P., Bečvář, F., Benlliure, J., Berthomieux, E., Betev, B., Calviño, F., Cano-Ott, D., Capote, R., Cennini, P., Chepel, V., Chiaveri, E., Colonna, N., Cortes, G., Cortina, D., Couture, A., Cox, J., Dababneh, S., David, S., Dolfini, R., Domingo-Pardo, C., Duran, I., Embid-Segura, M., Ferrant, L., Ferrari, A., Ferreira-Marques, R., Frais-Koelbl, H., Furman, W., Goncalves, I., Gonzalez-Romero, E., Goverdovski, A., Gramegna, F., Griesmayer, E., Gunsing, F., Haas, B., Haight, R., Heil, M., Herrera-Martinez, A., Isaev, S., Jericha, E., Kadi, Y., Käppeler, F., Kerveno, M., Ketlerov, V., Koehler, P.E., Konovalov, V., Krtička, M., Leeb, H., Lindote, A., Lopes, M.I., Lozano, M., Lukic, S., Marganiec, J., Marrone, S., Martinez-Val, J., Mastinu, P., Mengoni, A., Milazzo, P.M., Molina-Coballes, A., Moreau, C., Mosconi, M., Neves, F., Oberhummer, H., O'Brien, S., Pancin, J., Papaevangelou, T., Paradela, C., Pavlik, A., Pavlopoulos, P., Perlado, J.M., Perrot, L., Peskov, V., Plag, R. *, Plompen, A., Plukis, A., Poch, A., Policarpo, A., Pretel, C., Quesada, J.M., Rapp, W., Rauscher, T., Reifarth, R., Rosetti, M., Rubbia, C., Rudolf, G., Rullhusen, P., Salgado, J., Schäfer, E., Soares, J.C., Stephan, C., Tagliente, G., Tain, J.L., Tassan-Got, L., Tavora, L.M.N., Terlizzi, R., Vannini, G., Vaz, P., Ventura, A., Villamarin-Fernandez, D., Vincente-Vincente, M., Vlachoudis, V., Voss, F., Wendler, H., Wiescher, M., Wisshak, K.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 2005 538(1):692-702
Autor:
Lorusso, G., Colonna, N. *, Marrone, S., Tagliente, G., Heil, M., Cano-Ott, D., Mosconi, M., Moreau, C., Mengoni, A., Abbondanno, U., Aerts, G., Alvarez-Pol, H., Alvarez-Velarde, F., Andriamonje, S., Andrzejewski, J., Angelopoulos, A., Assimakopoulos, P., Badurek, G., Baumann, P., Bečvář, F., Benlliure, J., Berthomieux, E., Bisceglie, E., Calviño, P., Capote, R., Cennini, P., Chepel, V., Chiaveri, E., Coceva, C., Cortes, G., Cortina, D., Couture, A., Cox, J., Dababneh, S., Dahlfors, M., David, S., Dolfini, R., Domingo-Pardo, C., Duran, I., Eleftheriadis, C., Embid-Segura, M., Ferrant, L., Ferrari, A., Ferreira-Marques, R., Frais-Koelbl, H., Furman, W.I., Goncalves, I.F., Gonzalez-Romero, E., Goverdovski, A., Gramegna, F., Griesmayer, E., Gunsing, F., Haas, B., Haight, R., Herrera-Martinez, A., Ioannides, K.G., Isaev, S., Jericha, E., Käppeler, F., Kadi, Y., Karamanis, D., Ketlerov, V., Kitis, G., Koehler, P.E., Konovalov, V., Kossionides, E., Krticka, M., Leeb, H., Lindote, A., Lopes, M.I., Lozano, M., Lukic, S., Marganiec, J., Mastinu, P.F., Milazzo, P.M., Molina-Coballes, A., Neves, F., Oberhummer, H., O’Brien, S., Pancin, J., Paradela, C., Pavlik, A., Pavlopoulos, P., Perrot, L., Peskov, V., Plag, R., Plompen, A., Plukis, A., Poch, A., Policarpo, A., Pretel, C., Quesada, J.M., Rapp, W., Rauscher, T., Reifarth, R., Rosetti, M., Rubbia, C., Rudolf, G., Rullhusen, P., Salgado, J., Savvidis, E., Soares, J.C., Stephan, C., Tain, J.L., Tassan-Got, L., Tavora, L.M.N., Terlizzi, R., Tsangas, N., Vannini, G., Vaz, P., Ventura, A., Villamarin, D., Vincente, M.C., Vlachoudis, V., Vlastou, R., Voss, F., Wendler, H., Wiescher, M., Wisshak, K.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 21 October 2004 532(3):622-630