Zobrazeno 1 - 10
of 83
pro vyhledávání: '"Pittman, S. T."'
Autor:
Jones, K. L., Bey, A., Burcher, S., Allmond, J. M., Galindo-Uribarri, A., Radford, D. C., Ahn, S., Ayres, A., Bardayan, 1 D. W., Cizewski, J. A., Ruiz, R. F. Garcia, Howard, M. E., Kozub, R. L., Liang, J. F., Manning, B., Matos, M., Nesaraja, C. D., O'Malley, P. D., Padilla-Rodal, E., Pain, S. D., Pittman, S. T., Ratkiewicz, A., Schmitt, K. T., Smith, M. S., Stracener, D. W., Varner, R. L.
The structure of nuclei around the neutron-rich nucleus 132Sn is of particular interest due to the vicinity of the Z = 50 and N = 82 shell closures and the r-process nucleosynthetic path. Four states in 131Sn with a strong single-particle-like compon
Externí odkaz:
http://arxiv.org/abs/2201.08890
Autor:
Jones, K. L., Ahn, S., Allmond, J. M., Ayres, A., Bardayan, D. W., Baugher, T., Bazin, D., Berryman, J. S., Bey, A., Bingham, C., Cartegni, L., Cerizza, G., Chae, K. Y., Cizewski, J. A., Gade, A., Galindo-Uribarri, A., Garcia-Ruiz, R. F., Grzywacz, R., Howard, M. E., Kozub, R. L., Liang, J. F., Manning, B., Matos, M., McDaniel, S., Miller, D., Nesaraja, C. D., O'Malley, P. D., Padgett, S., Padilla-Rodal, E., Pain, S. D., Pittman, S. T., Radford, D. C., Ratkiewicz, A., Schmitt, K. T., Shore, A., Smith, M. S., Stracener, D. W., Stroberg, S. R., Tostevin, J., Varner, R. L., Weisshaar, D., Wimmer, K., Winkler, R.
Publikováno v:
Acta Physica Polonica B, 46(3), 537-546 (2015)
Direct reaction techniques are powerful tools to study the single-particle nature of nuclei. Performing direct reactions on short-lived nuclei requires radioactive ion beams produced either via fragmentation or the Isotope Separation OnLine (ISOL) me
Externí odkaz:
http://arxiv.org/abs/1508.06531
Autor:
Cha, S. M., Chae, K. Y., Kim, A., Lee, E. J., Ahn, S., Bardayan, D. W., Chipps, K. A., Cizewski, J. A., Howard, M. E., Manning, B., O'Malley, P. D., Ratkiewicz, A., Strauss, S., Kozub, R. L., Matos, M., Pain, S. D., Pittman, S. T., Smith, M. S., Peters, W. A.
The $^{24}$Mg($p$, $\alpha$)$^{21}$Na reaction was measured at the Holifield Radioactive Ion Beam Facility at Oak Ridge National Laboratory in order to better constrain spins and parities of energy levels in $^{21}$Na for the astrophysically importan
Externí odkaz:
http://arxiv.org/abs/1508.02128
Autor:
Schmitt, K. T., Jones, K. L., Ahn, S., Bardayan, D. W., Bey, A., Blackmon, J. C., Brown, S. M., Chae, K. Y., Chipps, K. A., Cizewski, J. A., Hahn, K. I., Kolata, J. J., Kozub, R. L., Liang, J. F., Matei, C., Matos, M., Matyas, D., Moazen, B., Nesaraja, C. D., Nunes, F. M., Malley, P. D. O, Pain, S. D., Peters, W. A., Pittman, S. T., Roberts, A., Shapira, D., Shriner Jr, J. F., Smith, M. S., Spassova, I., Stracener, D. W., Upadhyay, N. J., Villano, A. N., Wilson, G. L.
The extraction of detailed nuclear structure information from transfer reactions requires reliable, well-normalized data as well as optical potentials and a theoretical framework demonstrated to work well in the relevant mass and beam energy ranges.
Externí odkaz:
http://arxiv.org/abs/1311.3205
Autor:
Schmitt, K. T., Jones, K. L., Bey, A., Ahn, S. H., Bardayan, D. W., Blackmon, J. C., Brown, S. M., Chae, K. Y., Chipps, K. A., Cizewski, J. A., Hahn, K. I., Kolata, J. J., Kozub, R. L., Liang, J. F., Matei, C., Matoš, M., Matyas, D., Moazen, B., Nesaraja, C., Nunes, F. M., O'Malley, P. D., Pain, S. D., Peters, W. A., Pittman, S. T., Roberts, A., Shapira, D., Shriner Jr, J. F., Smith, M. S., Spassova, I., Stracener, D. W., Villano, A. N., Wilson, G. L.
The best examples of halo nuclei, exotic systems with a diffuse nuclear cloud surrounding a tightly-bound core, are found in the light, neutron-rich region, where the halo neutrons experience only weak binding and a weak, or no, potential barrier. Mo
Externí odkaz:
http://arxiv.org/abs/1203.3081
Autor:
Mountford, D. J., Murphy, A. St J., Achouri, N. L., Angulo, C., Brown, J. R., Davinson, T., Santos, F. de Oliveira, de Séréville, N., Descouvemont, P., Kamalou, O., Laird, A. M., Pittman, S. T., Ujic, P., Woods, P. J.
The most intense gamma-ray line observable from novae is likely to be from positron annihilation associated with the decay of 18F. The uncertainty in the destruction rate of this nucleus through the 18F(p,{\alpha})15O reaction presents a limit to int
Externí odkaz:
http://arxiv.org/abs/1112.4639
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Kuhn, K., Sarazin, F., Nunes, F. M., Alvarez, M. A.G., Andreoiu, C., Bardayan, D. W., Bender, P. C., Blackmon, J. C., García Borge, María José, Braid, R., Brown, B. A., Catford, W. N., Diget, C. Aa., Di Pietro, A., Drake, T. E., Figuera, P., Garnsworthy, A.B., Gómez-Camacho, Joaquín, Hackman, G., Hager, U., Ilyushkin, S. V., Nácher, Enrique, O'Malley, P. D., Perea, Ángel, Pesudo, V., Pittman, S. T., Smalley, D., Svensson, C. E., Tengblad, Olof, Thompson, P., Unsworth, C., Wang, Z. M.
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
10 pags., 8 figs., 4 tabs.
The nature of the and excited states in is studied using the transfer reaction in inverse kinematics at 10A MeV at TRIUMF ISAC-II, in particular to assess whether either of them can be considered as an excited halo sta
The nature of the and excited states in is studied using the transfer reaction in inverse kinematics at 10A MeV at TRIUMF ISAC-II, in particular to assess whether either of them can be considered as an excited halo sta
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::4c2ac174429a96bb1fc8b337848a7fd1
https://api.elsevier.com/content/abstract/scopus_id/85116818453
https://api.elsevier.com/content/abstract/scopus_id/85116818453
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.