Zobrazeno 1 - 10
of 214
pro vyhledávání: '"Diget, C A"'
Autor:
Frost-Schenk, J., Adsley, P., Laird, A. M., Longland, R., Angus, C., Barton, C., Choplin, A., Diget, C. Aa., Hirschi, R., Marshall, C., Chaves, F. Portillo, Setoodehnia, K.
Massive stars are crucial to galactic chemical evolution for elements heavier than iron. Their contribution at early times in the evolution of the Universe, however, is unclear due to poorly constrained nuclear reaction rates. The competing $^{17}$O(
Externí odkaz:
http://arxiv.org/abs/2206.04167
Autor:
Girard-Alcindor, V., Mercenne, A., Stefan, I., Santos, F. de Oliveira, Michel, N., Płoszajczak, M., Assié, M., Lemasson, A., Clément, E., Flavigny, F., Matta, A., Ramos, D., Rejmund, M., Dudouet, J., Ackermann, D., Adsley, P., Assunção, M., Bastin, B., Beaumel, D., Benzoni, G., Borcea, R., Boston, A. J., Cáceres, L., Cederwall, B., Celikovic, I., Chudoba, V., Ciemala, M., Collado, J., Crespi, F. C. L., D'Agata, G., De France, G., Delaunay, F., Diget, C., Domingo-Pardo, C., Eberth, J., Fougères, C., Franchoo, S., Galtarossa, F., Georgiadou, A., Gibelin, J., Giraud, S., González, V., Goyal, N., Gottardo, A., Goupil, J., Grévy, S., Guimaraes, V., Hammache, F., Harkness-Brennan, L. J., Hess, H., Oliver, D. S. Judson, Kamalou, O., Kameneyero, A., Kiener, J., Korten, W., Koyama, S., Labiche, M., Lalanne, L., Lapoux, V., Leblond, S., Lefevre, A., Lenain, C., Leoni, S., Li, H., Lopez-Martens, A., Maj, A., Matea, I., Menegazzo, R., Mengoni, D., Meyer, A., Million, B., Monteagudo, B., Morfouace, P., Mrazek, J., Niikura, M., Piot, J., Podolyak, Zs., Portail, C., Pullia, A., Quintana, B., Recchia, F., Reiter, P., Rezynkina, K., Roger, T., Rojo, J. S., Rotaru, F., Salsac, M. D., Benítez, A. M. Sánchez, Sanchis, E., Şenyigit, M., de Séréville, N., Siciliano, M., Simpson, J., Sohler, D., Sorlin, O., Stanoiu, M., Stodel, C., Suzuki, D., Theisen, C., Thomas, J. C., Ujic, P., Valiente-Dobón, J. J., Zielińska, M.
The structure of the unbound $^{15}$F nucleus is investigated using the inverse kinematics resonant scattering of a radioactive $^{14}$O beam impinging on a CH$_2$ target. The analysis of $^{1}$H($^{14}$O,p)$^{14}$O and $^{1}$H($^{14}$O,2p)$^{13}$N r
Externí odkaz:
http://arxiv.org/abs/2111.14412
We introduce two simple online activities to explore the physics of neutron stars. These provide an introduction to the basic properties of compact objects, like their masses and radii, for secondary school students. The first activity explores the i
Externí odkaz:
http://arxiv.org/abs/2104.12449
Autor:
Assié, M., Clément, E., Lemasson, A., Ramos, D., Raggio, A., Zanon, I., Galtarossa, F., Lenain, C., Casal, J., Flavigny, F., Matta, A., Mengoni, D., Beaumel, D., Blumenfeld, Y., Borcea, R., Brugnara, D., Catford, W., de Oliveira, F., De Séréville, N., Didierjean, F., Diget, C. Aa., Dudouet, J., Fernandez-Dominguez, B., Fougères, C., Frémont, G., Girard-Alcindor, V., Giret, A., Goasduff, A., Gottardo, A., Goupil, J., Hammache, F., John, P. R., Korichi, A., Lalanne, L., Leblond, S., Lefevre, A., Legruel, F., Menager, L., Million, B., Nicolle, C., Noury, F., Rauly, E., Rezynkina, K., Rindel, E., Rojo, J. S., Siciliano, M., Stanoiu, M., Stefan, I., Vatrinet, L.
Publikováno v:
Nuclear Inst. and Methods in Physics Research, A 1014 (2021) 165743
The MUGAST-AGATA-VAMOS set-up at GANIL combines the MUGAST highly-segmented silicon array with the state-of-the-art AGATA array and the large acceptance VAMOS spectrometer. The mechanical and electronics integration copes with the constraints of maxi
Externí odkaz:
http://arxiv.org/abs/2104.10707
Autor:
Hubbard, N. J., Diget, C. Aa., Fox, S. P., Fynbo, H. O. U., Howard, A. M., Kirsebom, O. S., Laird, A. M., Munch, M., Parikh, A., Pignatari, M., Tomlinson, J. R.
Publikováno v:
ApJ 912 59 (2021)
The $^{23}$Na($\alpha,p$)$^{26}$Mg reaction has been identified as having a significant impact on the nucleosynthesis of several nuclei between Ne and Ti in type-Ia supernovae, and of $^{23}$Na and $^{26}$Al in massive stars. The reaction has been su
Externí odkaz:
http://arxiv.org/abs/2103.09315
Autor:
Cruz, S., Wimmer, K., Bhattacharjee, S. S., Bender, P. C., Hackman, G., Krücken, R., Ames, F., Andreoiu, C., Austin, R. A. E., Bancroft, C. S., Braid, R., Bruhn, T., Catford, W. N., Cheeseman, A., Chester, A., Cross, D. S., Diget, C. Aa., Drake, T., Garnsworthy, A. B., Kanungo, R., Knapton, A., Korten, W., Kuhn, K., Lassen, J., Laxdal, R., Marchetto, M., Matta, A., Miller, D., Moukaddam, M., Orr, N. A., Sachmpazidi, N., Sanetullaev, A., Svensson, C. E., Terpstra, N., Unsworth, C., Voss, P. J.
Background: Neutron-rich nuclei around neutron number N = 60 show a dramatic shape transition from spherical ground states to prolate deformation in 98Sr and heavier nuclei. Purpose: The purpose of this study is to investigate the single-particle str
Externí odkaz:
http://arxiv.org/abs/2008.07634
We present a simple activity based on the liquid-drop model which allows secondary school students to explore the uses of mathematical models and gain an intuitive understanding of the concept of binding energy, and in particular the significance of
Externí odkaz:
http://arxiv.org/abs/2007.06872
Autor:
Spieker, M., Weisshaar, D., Gade, A., Brown, B. A., Adrich, P., Bazin, D., Bentley, M. A., Brown, J. R., Campbell, C. M., Diget, C. Aa., Elman, B., Glasmacher, T., Hill, M., Longfellow, B., Pritychenko, B., Ratkiewicz, A., Rhodes, D., Tostevin, J. A.
Publikováno v:
Phys. Rev. C 100, 061303(R) (2019)
New experimental data obtained from $\gamma$-ray tagged one-neutron and one-proton knockout from $^{55}$Co is presented. A candidate for the sought-after $T=1, T_z = 0, J^{\pi} = 6^+$ state in $^{54}$Co is proposed based on a comparison to the new da
Externí odkaz:
http://arxiv.org/abs/2003.10363
Autor:
Cruz, S., Wimmer, K., Bender, P. C., Krücken, R., Hackman, G., Ames, F., Andreoiu, C., Austin, R. A. E., Bancroft, C. S., Braid, R., Bruhn, T., Catford, W. N., Cheeseman, A., Chester, A., Cross, D. S., Diget, C. Aa., Drake, T., Garnsworthy, A. B., Kanungo, R., Knapton, A., Korten, W., Kuhn, K., Lassen, J., Laxdal, R., Marchetto, M., Matta, A., Miller, D., Moukaddam, M., Orr, N. A., Sachmpazidi, N., Sanetullaev, A., Svensson, C. E., Terpstra, N., Unsworth, C., Voss, P. J.
The region around neutron number N = 60 in the neutron-rich Sr and Zr nuclei is one of the most dramatic examples of a ground state shape transition from (near) spherical below N = 60 to strongly deformed shapes in the heavier isotopes. The single-pa
Externí odkaz:
http://arxiv.org/abs/1911.00670
Autor:
Taggart, M. P., Akers, C., Laird, A. M., Hager, U., Ruiz, C., Hutcheon, D. A., Bentley, M. A., Brown, J. R., Buchmann, L., Chen, A. A., Chen, J., Chipps, K. A., Choplin, A., D'Auria, J. M., Davids, B., Davis, C., Diget, C. Aa., Erikson, L., Fallis, J., Fox, S. P., Frischknecht, U., Fulton, B. R., Galinski, N., Greife, U., Hirschi, R., Howell, D., Martin, L., Mountford, D., Murphy, A. St. J., Ottewell, D., Pignatari, M., Reeve, S., Ruprecht, G., Sjue, S., Veloce, L., Williams, M.
Publikováno v:
Physics Letters B 798 (2019) 134894
During the slow neutron capture process in massive stars, reactions on light elements can both produce and absorb neutrons thereby influencing the final heavy element abundances. At low metallicities, the high neutron capture rate of 16-O can inhibit
Externí odkaz:
http://arxiv.org/abs/1910.00870