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Phys. Rev. Lett. 79, 4100–4103 (1997)

Spins, Parity, Excitation Energies, and Octupole Structure of an Excited Superdeformed Band in 194Hg and Implications for Identical Bands

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G. Hackman1, T. L. Khoo1, M. P. Carpenter1, T. Lauritsen1, A. Lopez-Martens2, I. J. Calderin1, R. V. F. Janssens1, D. Ackermann1, I. Ahmad1, S. Agarwala1, D. J. Blumenthal1, S. M. Fischer1, D. Nisius1, P. Reiter1, J. Young1, H. Amro1,3, E. F. Moore3, F. Hannachi2, A. Korichi2, I. Y. Lee4, A. O. Macchiavelli4, T. Døssing5, and T. Nakatsukasa6
1Argonne National Laboratory, Argonne, Illinois 60439
2Centre de Spectrometrie Nucleaire et de Spectrometrie de Masse, IN2P3-CNRS, F-91405 Orsay, France
3North Carolina State University, Raleigh, North Carolina 27695 and TUNL, Durham, North Carolina 27708
4Lawrence Berkeley National Laboratory, Berkeley, California 94720
5Niels Bohr Institute, DK-2100 Copenhagen 0, Denmark
6UMIST, Manchester M60 1QD, United Kingdom

Received 8 July 1997; published in the issue dated 24 November 1997

An excited superdeformed band in 194Hg, observed to decay directly to both normal-deformed and superdeformed yrast states, is proposed to be a Kπ = 2- octupole vibrational band, based on its excitation energies, spins, and likely parity. The transition energies are identical to those of the yrast superdeformed band in 192Hg, but originate from levels with different spins and parities. The evolution of transition energies with spin suggests that cancellations between pairing and particle alignment are partly responsible for the identical transition energies.

© 1997 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.79.4100
DOI:
10.1103/PhysRevLett.79.4100
PACS:
21.10.Re, 21.10.Hw, 23.20.Lv, 27.80.+w

See Also

Comment: R. R. Chasman, Comment on “Spins, Parity, Excitation Energies, and Octupole Structure of an Excited Superdeformed Band in 194Hg and Implications for Identical Bands”, Phys. Rev. Lett. 80, 4610 (1998).

Reply: G. Hackman, T. L. Khoo, M. P. Carpenter, T. Lauritsen, A. Lopez-Martens, I. J. Calderin, R. V. Janssens, D. Ackermann, I. Ahmad, S. Agarwala, D. J. Blumenthal, S. M. Fischer, D. Nisius, P. Reiter, J. Young, H. Amro, E. F. Moore, F. Hannachi, A. Korichi, I. Y. Lee, A. O. Macchiavelli, T. Døssing, and T. Nakatsukasa, Hackman et al. Reply:, Phys. Rev. Lett. 80, 4611 (1998).