Zobrazeno 1 - 10
of 307
pro vyhledávání: '"Hutcheon D.A."'
Autor:
Psaltis, A., Chen, A.A., Connolly, D.S., Davids, B., Gilardy, G., Giri, R., Greife, U., Huang, W., Hutcheon, D.A., Karpesky, J., Lennarz, A., Liang, J., Lovely, M., Paneru, S.N., Ruiz, C., Tenkila, G., Williams, M.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 21 January 2021 987
Autor:
Vockenhuber, C., Erikson, L.E., Buchmann, L., Greife, U., Hager, U., Hutcheon, D.A., Lamey, M., Machule, P., Ottewell, D., Ruiz, C., Ruprecht, G.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 2009 603(3):372-378
Autor:
Psaltis, A., Chen, A.A., Connolly, D.S., Davids, B., Gilardy, G., Giri, R., Greife, U., Huang, W., Hutcheon, D.A., Karpesky, J., Lennarz, A., Liang, J., Lovely, M., Paneru, S.N., Ruiz, C., Tenkila, G., Williams, M.
Publikováno v:
Nucl.Instrum.Meth.A
Nucl.Instrum.Meth.A, 2021, 987, pp.164828. ⟨10.1016/j.nima.2020.164828⟩
Nucl.Instrum.Meth.A, 2021, 987, pp.164828. ⟨10.1016/j.nima.2020.164828⟩
Radiative capture reactions play a pivotal role for our understanding of the origin of the elements in the cosmos. Recoil separators provide an effective way to study these reactions, in inverse kinematics, and take advantage of the use of radioactiv
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=arXiv_dedup_::935d89658f8d858b6c003dce141e68f0
https://hal.archives-ouvertes.fr/hal-03022681
https://hal.archives-ouvertes.fr/hal-03022681
Autor:
Fallis, J., Akers, C., Laird, A.M., Simon, A., Spyrou, A., Christian, G., Connolly, D., Hager, U., Hutcheon, D.A., Lennarz, A., O'Malley, P., Quinn, S.J., Riley, J., Rojas, A., Ruiz, C., Williams, M.
Publikováno v:
In Physics Letters B 10 August 2020 807
Autor:
Fallis, J., Akers, C., Laird, A.M., Simon, A., Spyrou, A., Christian, G., Connolly, D., Hager, U., Hutcheon, D.A., Lennarz, A., O'Malley, P., Quinn, S.J., Riley, J., Rojas, A., Ruiz, C., Williams, M.
Publikováno v:
Physics Letters
The p-nuclei are the few stable nuclei heavier than iron on the neutron-deficient side of the valley of stability that cannot be produced through astrophysical neutron-capture reactions. The limited experimental data on reactions through which the p-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3000::3b327f78013707bbf47c93e29cd7ffbb
http://repo.scoap3.org/api
http://repo.scoap3.org/api
Autor:
Vockenhuber, C., Ouellet, C.O., Buchmann, L., Caggiano, J., Chen, A.A., D’Auria, J.M., Frekers, D., Hussein, A., Hutcheon, D.A., Kutschera, W., Jayamanna, K., Ottewell, D., Paul, M., Pearson, J., Ruiz, C., Ruprecht, G., Trinczek, M., Wallner, A.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, B June 2007 259(1):688-693
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:
In Physics Letters B 10 November 2019 798
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
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 inh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3000::b495214da762c4048d7ca56db0c48b18
http://repo.scoap3.org/api
http://repo.scoap3.org/api
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.
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 16O can inhibit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______305::f2aa409493484bcd4c0eb5680007f48c
https://surrey.eprints-hosting.org/853009/
https://surrey.eprints-hosting.org/853009/