Identification of γ rays from Au 172 and α decays of Au 172 , Ir 168 , and Re 164

The very neutron deficient odd-odd nucleus Au-172 was studied in reactions of 342 and 348 MeV Kr-78 beams with an isotopically enriched Ru-96 target. The alpha decays previously reported for Au-172 were confirmed and the decay chain extended down to Tm-152 through the discovery of a new alpha-decayi...

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Veröffentlicht in:Physical review. C, Nuclear physics Nuclear physics, 2009-12, Vol.80 (6), p.064310, Article 064310
Hauptverfasser: Hadinia, B., Cederwall, B., Page, R. D., Sandzelius, M., Scholey, C., Andgren, K., Bäck, T., Ganioğlu, E., Hornillos, M. B. Gómez, Grahn, T., Greenlees, P. T., Ideguchi, E., Jakobsson, U., Johnson, A., Jones, P. M., Julin, R., Juutinen, J., Ketelhut, S., Khaplanov, A., Leino, M., Niikura, M., Nyman, M., Özgür, I., Paul, E. S., Peura, P., Rahkila, P., Sarén, J., Sorri, J., Uusitalo, J., Wyss, R.
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Sprache:eng
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Zusammenfassung:The very neutron deficient odd-odd nucleus Au-172 was studied in reactions of 342 and 348 MeV Kr-78 beams with an isotopically enriched Ru-96 target. The alpha decays previously reported for Au-172 were confirmed and the decay chain extended down to Tm-152 through the discovery of a new alpha-decaying state in Re-164 [E-alpha=5623(10) keV; t(1/2)=864(-110)(+150) ms; b(alpha)=3(1)%]. Fine structure in these alpha decays of Au-172 and Ir-168 were identified. A new alpha-decaying state was also observed and assigned as the ground state in Au-172 [E-alpha=6762(10) keV; t(1/2)=22(-5)(+6) ms]. This decay chain was also correlated down to Tm-152 through previously reported alpha decays. Prompt gamma rays from excited states in Au-172 have been identified using the recoil-decay tagging technique. The partial level scheme constructed for Au-172 indicates that it has an irregular structure. Possible configurations of the alpha-decaying states in Au-172 are discussed in terms of the systematics of nuclei in this region and total Routhian surface calculations.
ISSN:0556-2813
1089-490X
1089-490X
DOI:10.1103/PhysRevC.80.064310