Zobrazeno 1 - 10
of 488
pro vyhledávání: '"B. R. Fulton"'
Autor:
Alison Laird, B. Davids, D. Connolly, A. Psaltis, B. R. Fulton, M. Williams, Uwe Greife, N. E. Esker, R. Garg, A. Chen, D. A. Hutcheon, Stephanie Lyons, M. Lovely, Chris Ruiz, U. Battino, A. Lennarz, U. Hager, A. Tattersall, J. Riley, Jordi José
Publikováno v:
Physical Review C
Background: Globular clusters are known to exhibit anomalous abundance trends such as the sodium-oxygen anticorrelation. This trend is thought to arise via pollution of the cluster interstellar medium from a previous generation of stars. Intermediate
Autor:
L. Buchmann, B. R. Fulton, N. Galinski, Jennifer Fallis, A. Chen, Jun Chen, B. Davids, C. Akers, S. Sjue, Uwe Greife, D. J. Mountford, S. Reeve, M. Williams, D. A. Hutcheon, C. Davis, L. Erikson, Marco Pignatari, Götz Ruprecht, Raphael Hirschi, Kelly Chipps, D. Howell, L. Martin, Chris Ruiz, D.F. Ottewell, M. Taggart, Urs Frischknecht, Laurelle Veloce, J. R. Brown, C. Aa. Diget, U. Hager, Arthur Choplin, Alison Laird, John D'Auria, S. P. Fox, M. A. Bentley, A. St. J. Murphy
Publikováno v:
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 A, 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 S J, Ottewell, D, Pignatari, M, Reeve, S, Ruprecht, G, Sjue, S, Veloce, L & Williams, M 2019, ' A direct measurement of the 17O(a,g)21Ne reaction in inverse kinematics and its impact on heavy element production ', Physics Letters B, vol. 798 . https://doi.org/10.1016/j.physletb.2019.134894, https://doi.org/10.1016/j.physletb.2019.134894
Physics Letters B, Vol 798, Iss, Pp-(2019)
Physics Letters B, Vol 798, Iss, Pp-(2019)
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c1c47f576749b9c6a3ad52b1f28477d4
http://arxiv.org/abs/1910.00870
http://arxiv.org/abs/1910.00870
Autor:
B. Davids, Martín Alcorta, P. Machule, B. R. Fulton, K. Hudson, M. Williams, Nadeem A. Khan, N. E. Esker, J.C. Lighthall, D. Connolly, Oliver S. Kirsebom
The Electromagnetic Mass Analyser (EMMA) is a new vacuum-mode recoil mass spectrometer currently undergoing the final stages of commissioning at the ISAC-II facility of TRIUMF. EMMA employs a symmetric configuration of electrostatic and magnetic defl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::13e036a028affd311540c813367f5daa
Autor:
Adam Mahl, D. A. Hutcheon, Jennifer Fallis, Alison Laird, G. Christian, Chris Ruiz, Luke E. Erikson, S. V. Ilyushkin, Barry Davids, Uwe Greife, C. Akers, U. Hager, D. Connolly, Patrick O'Malley, B. R. Fulton, A. Chen
Publikováno v:
Physical Review C. 97
Background: Nucleosynthesis of mid-mass elements is thought to occur under hot and explosive astrophysical conditions. Radiative α capture on S34 has been shown to impact nucleosynthesis in several such conditions, including core and shell oxygen bu
Autor:
U. Hager, Gloria Marquínez-Durán, V. Pesudo, Oliver S. Kirsebom, Mustafa Rajabali, D.W. Miller, Olof Tengblad, Valentina Scuderi, Enrique Nácher, C. Unsworth, Maria Fisichella, B. R. Fulton, M. Lattuada, Frederique Sarazin, María José García Borge, A. M. Moro, Joaquín Gómez-Camacho, A. B. Garnsworthy, Ángel Perea, P. C. Bender, Mario Cubero., Martín Alcorta, P. Figuera, J. P. Fernández-García, R. Braid, A. Di Prieto, G. Hackman, K. Kuhn, Patrick O'Malley, Mirta Alvarez, Josè A. Lay, A. M. Sánchez-Benítez, M. Moukaddam, Z. M. Wang, C. E. Svensson, Ismael Martel
Publikováno v:
Proceedings of The 26th International Nuclear Physics Conference — PoS(INPC2016).
The angular distributions of the elastic, inelastic scattering and break-up cross sections of the one neutron halo $^{11}$Be on a heavy-mass target ($^{197}$Au) have been measured at laboratory energies below (31.9 MeV) and around (39.6 MeV) the Coul
Autor:
B. R. Fulton, K. Kuhn, Corina Andreoiu, Joaquín Gómez-Camacho, R. Braid, M. M. Rajabali, A. B. Garnsworthy, Ismael Martel, P. C. Bender, Luis Acosta, M. Lattuada, G. Marquínez-Durán, Valentina Scuderi, G. Hackman, V. Pesudo, A. M. Sánchez-Benítez, U. Hager, Oliver S. Kirsebom, Martín Alcorta, M. Moukaddam, Ángel Perea, J. A. Lay, Z. Wang, M. Cubero, M. A. G. Alvarez, C. Unsworth, P. Figuera, M. J. G. Borge, D. Miller, Enrique Nácher, C. E. Svensson, J. P. Fernández-García, A. M. Moro, Maria Fisichella, A. Di Pietro, P. D. O'Malley, Olof Tengblad, F. Sarazin
Publikováno v:
Physical Review Letters
Angular distributions of the elastic, inelastic, and breakup cross sections of the halo nucleus ^{11}Be on ^{197}Au were measured at energies below (E_{lab}=31.9 MeV) and around (39.6 MeV) the Coulomb barrier. These three channels were unambiguously
Autor:
Simpson, E. C.1 edward.simpson@anu.edu.au, Cook, K. J.1, Bezzina, L. T.1, Carter, I. P.1, Dasgupta, M.1, Hinde, D. J.1
Publikováno v:
EPJ Web of Conferences. 10/18/2024, Vol. 306, p1-6. 6p.
Autor:
Huang, Z. J.1, Lin, C. J.1,2 cjlin@ciae.ac.cn, Yang, L.1, Jia, H. M.1, Yang, F.1, Ma, N. R.1, Wen, P. W.1, Luo, T. P.1, Chang, C.1, Duan, H. R.1, Zhu, S. X.1, Yin, C.1, Yang, J. H.1,2
Publikováno v:
EPJ Web of Conferences. 10/18/2024, Vol. 306, p1-4. 4p.
Autor:
Huang, Z. J.1, Lin, C. J.1,2 cjlin@ciae.ac.cn, Yang, L.1, Jia, H. M.1, Yang, F.1, Ma, N. R.1, Wen, P. W.1, Luo, T. P.1, Chang, C.1, Duan, H. R.1, Zhu, S. X.1, Yin, C.1
Publikováno v:
EPJ Web of Conferences. 10/8/2024, Vol. 304, p1-5. 5p.
Autor:
L. Buchmann, Alison Laird, U. Hager, Chris Ruiz, Luke E. Erikson, Jennifer Fallis, D. W. Bardayan, Barry Davids, A. Spyrou, C. Akers, L. Martin, D.F. Ottewell, B. R. Fulton, G. Christian, D. A. Hutcheon, A. St. J. Murphy, K. J. Nelson, A. Rojas
Publikováno v:
Physical Review C. 94
Background: The rate of the F18(p,γ)Ne19 reaction affects the final abundance of the radioisotope F18 ejected from novae. This nucleus is important as its abundance is thought to significantly influence the first-stage 511-keV and continuum γ-ray e