Zobrazeno 1 - 10
of 157
pro vyhledávání: '"Thibaud, J. P."'
Autor:
Belhout, A., Ouichaoui, S., Beaumevieille, H., Bouchemha, A., Bogaert, G., Fortier, S., Kiener, J., Lefebvre-Schuhl, A., Maison, J. M., Rosier, L., Rotbard, J., Tatischeff, V., Thibaud, J. P., Vernotte, J.
The angular distributions of $^{8}$Be states in the excitation energy region, E$_{x}$ $\ \sim$($16.5-18.2$) MeV, produced in the $^{7}$Li($^{3}% $He,d)$^{8}$Be proton transfer reaction have been measured at the Orsay 14.8$-$MV tandem accelerator for
Externí odkaz:
http://arxiv.org/abs/1709.05482
Autor:
Thibaud J. C. Richard, Laura K. Herzog, Julia Vornberger, Aldwin Suryo Rahmanto, Olle Sangfelt, Florian A. Salomons, Nico P. Dantuma
Publikováno v:
Scientific Reports, Vol 10, Iss 1, Pp 1-12 (2020)
Abstract Even though K63-linked polyubiquitin chains do not target proteins for proteasomal degradation, they play nevertheless a complementary protective role in maintaining protein homeostasis by directing malfunctioning proteins and organelles to
Externí odkaz:
https://doaj.org/article/c16e088089de40dbade83e4e69e958b1
Autor:
Hammache, F., Heil, M., Typel, S., Galaviz, D., Sümmerer, K., Coc, A., Uhlig, F., Attallah, F., Caamano, M., Cortina, D., Geissel, H., Hellström, M., Iwasa, N., Kiener, J., Koczon, P., Kohlmeyer, B., Mohr, P., Schwab, E., Schwarz, K., Schümann, F., Senger, P., Sorlin, O., Tatischeff, V., Thibaud, J. P., Vangioni, E., Wagner, A., Walus, W.
Publikováno v:
Phys.Rev.C82:065803,2010
The recently claimed observations of non-negligible amounts of 6Li in old halo stars have renewed interest in the Big-Bang Nucleosynthesis (BBN) of 6Li. One important ingredient in the predicted BBN abundance of 6Li is the low-energy 2H(alpha,gamma)6
Externí odkaz:
http://arxiv.org/abs/1011.6179
Autor:
Benhabiles-Mezhoud, H., Kiener, J., Thibaud, J. -P., Tatischeff, V., Deloncle, I., Coc, A., Duprat, J., Hamadache, C., Lefebvre-Schuhl, A., Dalouzy, J. -C., De Grancey, F., De Oliveira, F., Dayras, F., De Séréville, N., Pellegriti, M. -G., Lamia, L., Ouichaoui, S.
Publikováno v:
Phys.Rev.C83:024603,2011
$\gamma$-ray production cross sections have been measured in proton irradiations of N, Ne and Si and $\alpha$-particle irradiations of N and Ne. In the same experiment we extracted also line shapes for strong $\gamma$-ray lines of $^{16}$O produced i
Externí odkaz:
http://arxiv.org/abs/1011.2561
Nuclear interactions of ions accelerated at the surface of flaring stars can produce fresh isotopes in stellar atmospheres. Although this nucleosynthesis is not significant for the chemical evolution of the Galaxy, it can be important for a number of
Externí odkaz:
http://arxiv.org/abs/0801.1777
Autor:
Tatischeff, V., Thibaud, J. -P.
The high 6-Li abundances recently measured in metal-poor halo stars are far above the value predicted by Big Bang nucleosynthesis. They cannot be explained by galactic cosmic-ray interactions in the interstellar medium either. Various pre-galactic so
Externí odkaz:
http://arxiv.org/abs/astro-ph/0610756
Autor:
Chafa, A., Tatischeff, V., Aguer, P., Barhoumi, S., Coc, A., Garrido, F., Hernanz, M., Jose, J., Kiener, J., Lefebvre-Schuhl, A., Ouichaoui, S., de Sereville, N., Thibaud, J. -P.
Publikováno v:
Phys.Rev.Lett.95:031101,2005; Erratum-ibid.96:019902,2006
We report on the observation of a previously unknown resonance at E=194.1+/-0.6 keV (lab) in the 17-O(p,alpha)14-N reaction, with a measured resonance strength omega_gamma(p,alpha)=1.6+/-0.2 meV. We studied in the same experiment the 17-O(p,gamma)18-
Externí odkaz:
http://arxiv.org/abs/astro-ph/0506500
Autor:
Tatischeff, V., Duprat, J., Kiener, J., Assuncao, M., Coc, A., Engrand, C., Gounelle, M., Lefebvre, A., Porquet, M. -G., De Sereville, N., Thibaud, J. -P., Bourgeois, C., Chabot, M., Hammache, F., Scarpaci, J. -A.
Publikováno v:
Phys.Rev. C68 (2003) 025804
Gamma-ray production cross sections have been measured for gamma-ray lines copiously emitted in the $^3$He bombardment of $^{16}$O nuclei: the 937, 1042 and 1081 keV lines of $^{18}$F and the 1887 keV line of $^{18}$Ne. Four Ge detectors with BGO shi
Externí odkaz:
http://arxiv.org/abs/nucl-ex/0308024
Autor:
de Sereville, N., Coc, A., Angulo, C., Assuncao, M., Beaumel, D., Bouzid, B., Cherubini, S., Couder, M., Demaret, P., Santos, F. de Oliveira, Figuera, P., Fortier, S., Gaelens, M., Hammache, F., Kiener, J., Labar, D., Lefebvre, A., Leleux, P., Loiselet, M., Ninane, A., Ouichaoui, S., Ryckewaert, G., Smirnova, N., Tatischeff, V., Thibaud, J. -P.
Publikováno v:
Phys.Rev.C67:052801,2003
The 18F(p,alpha)15O reaction is recognized to be one of the most important reactions for nova gamma-ray astronomy as it governs the early E <= 511keV gamma emission. However in the nova temperature regime, its rate remains largely uncertain due to un
Externí odkaz:
http://arxiv.org/abs/nucl-ex/0304014
Autor:
de Sereville, N., Coc, A., Angulo, C., Assuncao, M., Beaumel, D., Bouzid, B., Cherubini, S., Couder, M., Demaret, P., Santos, F. de Oliveira, Figuera, P., Fortier, S., Gaelens, M., Hammache, F., Kiener, J., Labar, D., Lefebvre, A., Leleux, P., Loiselet, M., Ninane, A., Ouichaoui, S., Ryckewaert, G., Smirnova, N., Tatischeff, V., Thibaud, J. -P.
Publikováno v:
Nucl.Phys. A718 (2003) 259-262
The ^18F(p, alpha)^15O reaction is recognized as one of the most important reaction for nova gamma-ray astronomy as it governs the early =< 511 keV emission. However, its rate remains largely uncertain at nova temperatures due to unknown low-energy r
Externí odkaz:
http://arxiv.org/abs/nucl-ex/0209017