| Article | |
| Title | Use of the $^{18}O(^{18}O,^{14}O)^{22}O$ reaction to measure the mass of $^{22}O$ |
| Author(s) | Hickey, G T (Australian Natl. U., Canberra) ; Weisser, D C (Australian Natl. U., Canberra) ; Cerny, J (Australian Natl. U., Canberra) ; Crawley, G M (Australian Natl. U., Canberra) ; Zeller, A F (Australian Natl. U., Canberra) ; Ophel, T R (Australian Natl. U., Canberra) ; Hebbard, D F (Australian Natl. U., Canberra) |
| Publication | CERN, 1976 |
| In: | 3rd International Conference on Nuclei Far from Stability, pp.251-253 |
| DOI | 10.5170/CERN-1976-013.251 |
| Subject category | Nuclear Physics |
| Abstract | Counter-telescopes and recoil-coincidence techniques were used to observe the /sup 18/O(/sup 18/O,/sup 14/O)/sup 22/O reaction at 100 Me V. These data establish a mass excess for /sup 22/O of 9.48+or-0.10 Me V, which differs by approximately 2.0 MeV from the previous value, but is in excellent agreement with several theoretical predictions. (8 refs). |
Záznam vytvorený 2005-08-18, zmenený 2016-11-22