Zobrazeno 1 - 10
of 99
pro vyhledávání: '"Galinski, N"'
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
Autor:
Kirsebom, O. S., Bender, P., Cheeseman, A., Christian, G., Churchman, R., Cross, D. S., Davids, B., Evitts, L. J., Fallis, J., Galinski, N., Garnsworthy, A. B., Hackman, G., Lighthall, J., Ketelhut, S., Machule, P., Miller, D., Nobs, C. R., Pearson, C. J., Rajabali, M. M., Radich, A. J., Rojas, A., Ruiz, C., Sanetullaev, A., Unsworth, C. D., Wrede, C.
Publikováno v:
Phys. Rev. C 93, 025802 (2016)
Several lifetimes in 23Mg have been determined for the first time using the Doppler-shift attenuation method. A Monte Carlo simulation code has been written to model the gamma-ray line shape. An upper limit of 12 fs at the 95% C.L. has been obtained
Externí odkaz:
http://arxiv.org/abs/1508.07188
Autor:
Wilson, G. L., Catford, W. N., Orr, N. A., Diget, C. Aa., Matta, A., Hackman, G., Williams, S. J., Celik, I. C., Achouri, N. L., Falou, H. Al, Ashley, R., Austin, R. A. E., Ball, G. C., Blackmon, J. C., Boston, A. J., Boston, H. C., Brown, S. M., Cross, D. S., Djongolov, M., Drake, T. E., Hager, U., Fox, S. P., Fulton, B. R., Galinski, N., Garnsworthy, A. B., Jamieson, D., Kanungo, R., Leach, K. G., Orce, J. N., Pearson, C. J., Porter-Peden, M., Sarazin, F., Simpson, E. C., Sjue, S., Smalley, D., Sumithrarachchi, C., Svensson, C. E., Triambak, S., Unsworth, C., Wadsworth, R.
The levels in 26Na with single particle character have been observed for the first time using the d(25Na,p gamma) reaction at 5 MeV/nucleon. The measured excitation energies and the deduced spectroscopic factors are in good overall agreement with (0+
Externí odkaz:
http://arxiv.org/abs/1508.01757
Autor:
Salter, P. J. C., Aliotta, M., Davinson, T., Falou, H. Al, Chen, A., Davids, B., Fulton, B. R., Galinski, N., Howell, D., Lotay, G., Machule, P., Murphy, A. StJ., Ruiz, C., Sjue, S., Taggart, M., Walden, P., Woods, P. J.
The 18Ne(a,p)21Na reaction provides one of the main HCNO-breakout routes into the rp-process in X-ray bursts. The 18Ne(a,p_0)21Na reaction cross section has been determined for the first time in the Gamow energy region for peak temperatures T=2GK by
Externí odkaz:
http://arxiv.org/abs/1202.6650
Autor:
Tanihata, I., Alcorta, M., Bandyopadhyay, D., Bieri, R., Buchmann, L., Davids, B., Galinski, N., Howell, D., Mills, W., Openshaw, R., Padilla-Rodal, E., Ruprecht, G., Sheffer, G., Shotter, A. C., Mythili, S., Trinczek, M., Walden, P., Savajols, H., Roger, T., Caamano, M., Mittig, W., Roussel-Chomaz, P., Kanungo, R., Gallant, A., Savard, G., Thompson, I. J.
Publikováno v:
Physical Review Letters 100 (2008) 192502
The p(\nuc{11}{Li},\nuc{9}{Li})t reaction has been studied for the first time at an incident energy of 3$A$ MeV delivered by the new ISAC-2 facility at TRIUMF. An active target detector MAYA, build at GANIL, was used for the measurement. The differen
Externí odkaz:
http://arxiv.org/abs/0802.1778
Autor:
Cavallaro M., De Napoli M., Cappuzzello F., Agodi C., Bondí M., Carbone D., Cunsolo A., Davids B., Davinson T., Foti A., Galinski N., Kanungo R., Lenske H., Orrigo S.E.A., Ruiz C., Sanetullaev A.
Publikováno v:
EPJ Web of Conferences, Vol 117, p 06009 (2016)
The structure of the 10Li unbound nucleus is a subject of large interest and its description is nowadays a matter of debate. We have investigated this system using the d(9Li,p)10 Li one-neutron transfer reaction at 100 MeV in inverse kinematics. The
Externí odkaz:
https://doaj.org/article/ebe0d1102e9f4455aab9845957030936
Autor:
Taggart, Matthew Paul, Akers, C., Laird, Alison Monica, Hager, U, Ruiz, C, Hutcheon, D, Bentley, Michael Anthony, Brown, James Robert, Buchmann, L, Chen, Jie, Chipps, Kelly Anne, Choplin, A., D'Auria, J.M., Davids, B, Davis, C, Diget, Christian Aaen, Erikson, L., Fallis, J., Fox, Simon Paul, Frischknecht, U., Fulton, Brian Robert, Galinski, N., Greife, U, Hirschi, R., Howell, D., Martin, L., Mountford, D. J., Murphy, A, Ottewell, D., Pignatari, M., Reeve, Scott, Ruprecht, G, Sjue, S. K. L., Veloce, L., Williams, M.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::867c2c0e3100e2a3045a4ae6740fe962
https://eprints.whiterose.ac.uk/151440/8/1_s2.0_S0370269319306082_main.pdf
https://eprints.whiterose.ac.uk/151440/8/1_s2.0_S0370269319306082_main.pdf
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/
Autor:
Sanetullaev, A., Kanungo, R., Tanaka, J., Alcorta, M., Andreoiu, C., Bender, P., Chen, A.A., Christian, G., Davids, B., Fallis, J., Fortin, J.P., Galinski, N., Gallant, A.T., Garrett, P.E., Hackman, G., Hadinia, B., Ishimoto, S., Keefe, M., Krücken, R., Lighthall, J., McNeice, E., Miller, D., Purcell, J., Randhawa, J.S., Roger, T., Rojas, A., Savajols, H., Shotter, A., Tanihata, I., Thompson, I.J., Unsworth, C., Voss, P., Wang, Z.
Publikováno v:
Physics Letters B. 755:481-485
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=base_oa_____::c02d711a9a60e9c0553d9a14697295d1