Zobrazeno 1 - 10
of 15
pro vyhledávání: '"G. Mavilla"'
Publikováno v:
Journal of Power Sources. 247:890-895
Electrocatalyst materials, consisting of Pt or Pt–Ru supported on carbon with and without TiO 2 , are evaluated for their activity towards the methanol oxidation reaction (MOR) in 1.0 M H 2 SO 4 at 25 °C in the presence and absence of visible ligh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::090b9549223736319a6a6b0737af344f
https://doi.org/10.1016/j.jpowsour.2013.08.140
https://doi.org/10.1016/j.jpowsour.2013.08.140
Publikováno v:
ECS Transactions. 53:31-41
Preparation of non-precious metal catalysts (NPMCs) via chemical surface modification of carbon black with 5,6-diamino-1,10-phenanthroline (aphen) was completed. A diazonium coupling reaction was used to covalently attach aphen to the carbon surface
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3cb3042470ac563ee53a99da3f67e334
https://doi.org/10.1149/05312.0031ecst
https://doi.org/10.1149/05312.0031ecst
Autor:
I. Deloncle, G. Mavilla, B. Le Crom, Fairouz Hammache, C. T. Nsangu, P. Roussel, P. Adsley, Alison Laird, Marine Vandebrouck, S. Ancelin, Vincent Tatischeff, J. Guillot, S. P. Fox, C. Hamadache, I. Stefan, N. Oulebsir, M. Assié, C. J. Barton, L. Perrot, G. Marquinez Duran, S. Benamara, D. Suzuki, P. Morfouace, L. Lefebvre, C. A. Diget, N. de Séréville, Jürgen Kiener, A. Lefebfre-Schuhl, A. Coc, A. M. Sánchez-Benítez, A. Mutschler
Publikováno v:
Arias Montano. Repositorio Institucional de la Universidad de Huelva
instname
Journal of Physics: Conference Series
instname
Journal of Physics: Conference Series
26Al was the first cosmic radioactivity ever detected in the galaxy as well as one of the first extinct radioactivity observed in refractory phases of meteorites. Its nucleosynthesis in massive stars is still uncertain mainly due to the lack of nucle
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b60e3c5f47fb3c3d5f64188a808a96f1
https://hdl.handle.net/10272/11678
https://hdl.handle.net/10272/11678
Autor:
L. Lefebvre, Predrag Ujić, J. Kiener, J. Mrazek, André Palma da Cunha Matta, B. Fernández-Domínguez, A. Coc, A. M. Sánchez-Benítez, I. Stefan, P. Morfouace, Didier Beaumel, Daisuke Suzuki, I. Matea, S. Franchoo, B. Le Crom, M. Assié, A. Lefebvre-Schuhl, N. de Sereville, F. Hammache, F. de Oliveira Santos, L. Audouin, G. Mavilla, Vincent Tatischeff, Anuj Parikh, C. Hamadache, Marine Vandebrouck, L. Perrot, Alison Laird, S. P. Fox, P. Roussel
Publikováno v:
J.Phys.Conf.Ser.
7th Nuclear Physics in Astrophysics and 28th International Nuclear Physics Divisional Conference of the European Physical Society
7th Nuclear Physics in Astrophysics and 28th International Nuclear Physics Divisional Conference of the European Physical Society, May 2015, York, United Kingdom. pp.012016, ⟨10.1088/1742-6596/940/1/012016⟩
Journal of Physics: Conference Series
Arias Montano. Repositorio Institucional de la Universidad de Huelva
instname
7th Nuclear Physics in Astrophysics and 28th International Nuclear Physics Divisional Conference of the European Physical Society
7th Nuclear Physics in Astrophysics and 28th International Nuclear Physics Divisional Conference of the European Physical Society, May 2015, York, United Kingdom. pp.012016, ⟨10.1088/1742-6596/940/1/012016⟩
Journal of Physics: Conference Series
Arias Montano. Repositorio Institucional de la Universidad de Huelva
instname
The cosmological 7Li problem arises from the signi cant discrepancy of about a factor 3 between the predicted primordial 7Li abundance and the observed one. The main process for the production of 7Li during Big-Bang nucleosynthesis is the decay of 7B
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f20afeaa9dbb583a0f9073e20bace46a
https://hal.archives-ouvertes.fr/hal-01703777
https://hal.archives-ouvertes.fr/hal-01703777
Autor:
P. Roussel, N. de Séréville, Jürgen Kiener, Vincent Tatischeff, L. Lefebvre, A. M. Sánchez-Benítez, I. Deloncle, Mandira Sinha, M. Assié, Marine Vandebrouck, Alison Laird, A. Coc, A. Lefebvre-Schuhl, I. Stefan, S. Ancelin, G. Mavilla, Fairouz Hammache, L. Perrot, S. Benamara, P. Morfouace, S. P. Fox
Publikováno v:
Physical Review C. 89
The ${}^{26}\mathrm{Al}$ radioisotope is of great importance for understanding the chemical and dynamical evolution of our galaxy. Among the possible stellar sources, massive stars are believed to be the main producer of this radioisotope. Understand
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::04fe18362d6d34325caedf8d4bfb3b93
https://doi.org/10.1103/physrevc.89.065805
https://doi.org/10.1103/physrevc.89.065805
Autor:
Daisuke Suzuki, P. Morfouace, B. Fernández-Domínguez, A. M. Sánchez-Benítez, I. Matea, S. Franchoo, A. Lefebvre-Schuhl, N. de Sereville, J. Kiener, P. Roussel, Marine Vandebrouck, I. Stefan, B. Le Crom, Predrag Ujić, A. Coc, S. P. Fox, J. Mrazek, Alison Laird, C. Hamadache, L. Audouin, S. Ancelin, F. Hammache, G. Mavilla, Anuj Parikh, L. Lefebvre, M. Assié, Fdo Santos, André Palma da Cunha Matta, L. Perrot, Didier Beaumel, Tatischeff
Publikováno v:
Physical Review C. 88
The observed primordial ${}^{7}$Li abundance in metal-poor halo stars is found to be lower than its Big-Bang nucleosynthesis (BBN) calculated value by a factor of approximately three. Some recent works suggested the possibility that this discrepancy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a1466b5960b1ddc5aadd67212f52d5cf
https://doi.org/10.1103/physrevc.88.062802
https://doi.org/10.1103/physrevc.88.062802
Autor:
Megumi Niikura, E. A. Sokol, G. Mavilla, K. Kolos, J. Bettane, E. A. Kuznetsova, V. Smirnov, J. N. Wilson, S. Ancelin, Yu. Penionzhkevich, D. Verney, F. Ibrahim, D. A. Testov
Publikováno v:
ResearcherID
Beta decay properties are among the easiest and therefore, the first ones to be measured to study new neutron rich isotopes. Eventually it could be sufficient just a few number of nuclei to estimate its lifetime and neutron emission probability. With
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f944c7b713be2ef13af96fc6046a0f7a
https://doi.org/10.1142/9789814508865_0047
https://doi.org/10.1142/9789814508865_0047
Publikováno v:
ECS Meeting Abstracts. :1023-1023
not Available.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b1b729499534b9e9f62e3d40ce1743c2
https://doi.org/10.1149/ma2013-01/26/1023
https://doi.org/10.1149/ma2013-01/26/1023
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Autor:
F Hammache, A Coc, N de Séréville, I Stefan, P Roussel, M Assié, L Audouin, D Beaumel, S Franchoo, B Fernandez-Dominguez, S Fox, C Hamadache, J Kiener, A Laird, B Le Crom, A. Lefebvre-Schuhl, L Lefebvre, I Matea, A Matta, G Mavilla
Publikováno v:
Journal of Physics: Conference Series; 2018, Vol. 940 Issue 1, p1-1, 1p