Experimental observation of the M1 scissors mode in 254No
Abstract
We present the first experimental evidence of the scissors mode in the superheavy nucleus 254No produced in the 208Pb(48Ca, 2$$\mathcal{n}\gamma$$))254No reaction. The spectrum of γ rays emitted by the excited 254No nuclei shows an enhanced γ-ray yield for transition energies of ≈2.5 MeV. By measuring the linear polarization properties of the emitted γ rays, we confirm that the transitions in the enhancement region are predominantly of magnetic-dipole character, characteristic for the scissors mode. To further characterize the enhanced γ-ray yield, simulations of the electromagnetic decay of 254No were performed. The observed enhancement is reproduced by including an M1 component in the γ strength function with total strength $$B(M1\uparrow) = 11.8(19) \mu^{2}_{N}$$. This is in good agreement with the integrated M1 strength from sum-rule estimates and new calculations within the quasi-particle random-phase approximation presented here. Our results provide a stringent test of phenomenological formulae for the scissors mode currently used in stellar nucleosynthesis calculations. We find that those formulae are not satisfactory, and we recommend using sum-rule estimates assuming a rigid-body moment of inertia instead for describing the scissors mode in superheavy nuclei.
- Authors:
- more »
- Publication Date:
- Research Org.:
- Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
- Sponsoring Org.:
- USDOE National Nuclear Security Administration (NNSA); European Research Council (ERC); Academy of Finland; Science and Technology Facilities Council (STFC)
- OSTI Identifier:
- 1891679
- Alternate Identifier(s):
- OSTI ID: 1891724
- Report Number(s):
- LLNL-JRNL-826474
Journal ID: ISSN 0370-2693; S037026932200613X; 137479; PII: S037026932200613X
- Grant/Contract Number:
- AC52-07NA27344; 637686
- Resource Type:
- Published Article
- Journal Name:
- Physics Letters. B
- Additional Journal Information:
- Journal Name: Physics Letters. B Journal Volume: 834 Journal Issue: C; Journal ID: ISSN 0370-2693
- Publisher:
- Elsevier
- Country of Publication:
- Netherlands
- Language:
- English
- Subject:
- 73 NUCLEAR PHYSICS AND RADIATION PHYSICS; scissors mode; y-strength function; transfermium nuclides
Citation Formats
Bello Garrote, F. L., Lopez-Martens, A., Larsen, A. C., Deloncle, I., Péru, S., Zeiser, F., Greenlees, P. T., Kheswa, B. V., Auranen, K., Bleuel, D. L., Cox, D. M., Crespo Campo, L., Giacoppo, F., Görgen, A., Grahn, T., Guttormsen, M., Hagen, T. W., Harkness-Brennan, L., Hauschild, K., Henning, G., Herzberg, R. -D., Julin, R., Juutinen, S., Laplace, T. A., Leino, M., Midtbø, J. E., Modamio, V., Pakarinen, J., Papadakis, P., Partanen, J., Renstrøm, T., Rezynkina, K., Sandzelius, M., Sarén, J., Scholey, C., Siem, S., Sorri, J., Stolze, S., and Uusitalo, J. Experimental observation of the M1 scissors mode in 254No. Netherlands: N. p., 2022.
Web. doi:10.1016/j.physletb.2022.137479.
Bello Garrote, F. L., Lopez-Martens, A., Larsen, A. C., Deloncle, I., Péru, S., Zeiser, F., Greenlees, P. T., Kheswa, B. V., Auranen, K., Bleuel, D. L., Cox, D. M., Crespo Campo, L., Giacoppo, F., Görgen, A., Grahn, T., Guttormsen, M., Hagen, T. W., Harkness-Brennan, L., Hauschild, K., Henning, G., Herzberg, R. -D., Julin, R., Juutinen, S., Laplace, T. A., Leino, M., Midtbø, J. E., Modamio, V., Pakarinen, J., Papadakis, P., Partanen, J., Renstrøm, T., Rezynkina, K., Sandzelius, M., Sarén, J., Scholey, C., Siem, S., Sorri, J., Stolze, S., & Uusitalo, J. Experimental observation of the M1 scissors mode in 254No. Netherlands. https://doi.org/10.1016/j.physletb.2022.137479
Bello Garrote, F. L., Lopez-Martens, A., Larsen, A. C., Deloncle, I., Péru, S., Zeiser, F., Greenlees, P. T., Kheswa, B. V., Auranen, K., Bleuel, D. L., Cox, D. M., Crespo Campo, L., Giacoppo, F., Görgen, A., Grahn, T., Guttormsen, M., Hagen, T. W., Harkness-Brennan, L., Hauschild, K., Henning, G., Herzberg, R. -D., Julin, R., Juutinen, S., Laplace, T. A., Leino, M., Midtbø, J. E., Modamio, V., Pakarinen, J., Papadakis, P., Partanen, J., Renstrøm, T., Rezynkina, K., Sandzelius, M., Sarén, J., Scholey, C., Siem, S., Sorri, J., Stolze, S., and Uusitalo, J. Tue .
"Experimental observation of the M1 scissors mode in 254No". Netherlands. https://doi.org/10.1016/j.physletb.2022.137479.
@article{osti_1891679,
title = {Experimental observation of the M1 scissors mode in 254No},
author = {Bello Garrote, F. L. and Lopez-Martens, A. and Larsen, A. C. and Deloncle, I. and Péru, S. and Zeiser, F. and Greenlees, P. T. and Kheswa, B. V. and Auranen, K. and Bleuel, D. L. and Cox, D. M. and Crespo Campo, L. and Giacoppo, F. and Görgen, A. and Grahn, T. and Guttormsen, M. and Hagen, T. W. and Harkness-Brennan, L. and Hauschild, K. and Henning, G. and Herzberg, R. -D. and Julin, R. and Juutinen, S. and Laplace, T. A. and Leino, M. and Midtbø, J. E. and Modamio, V. and Pakarinen, J. and Papadakis, P. and Partanen, J. and Renstrøm, T. and Rezynkina, K. and Sandzelius, M. and Sarén, J. and Scholey, C. and Siem, S. and Sorri, J. and Stolze, S. and Uusitalo, J.},
abstractNote = {We present the first experimental evidence of the scissors mode in the superheavy nucleus 254No produced in the 208Pb(48Ca, 2$\mathcal{n}\gamma$))254No reaction. The spectrum of γ rays emitted by the excited 254No nuclei shows an enhanced γ-ray yield for transition energies of ≈2.5 MeV. By measuring the linear polarization properties of the emitted γ rays, we confirm that the transitions in the enhancement region are predominantly of magnetic-dipole character, characteristic for the scissors mode. To further characterize the enhanced γ-ray yield, simulations of the electromagnetic decay of 254No were performed. The observed enhancement is reproduced by including an M1 component in the γ strength function with total strength $B(M1\uparrow) = 11.8(19) \mu^{2}_{N}$. This is in good agreement with the integrated M1 strength from sum-rule estimates and new calculations within the quasi-particle random-phase approximation presented here. Our results provide a stringent test of phenomenological formulae for the scissors mode currently used in stellar nucleosynthesis calculations. We find that those formulae are not satisfactory, and we recommend using sum-rule estimates assuming a rigid-body moment of inertia instead for describing the scissors mode in superheavy nuclei.},
doi = {10.1016/j.physletb.2022.137479},
journal = {Physics Letters. B},
number = C,
volume = 834,
place = {Netherlands},
year = {Tue Nov 01 00:00:00 EDT 2022},
month = {Tue Nov 01 00:00:00 EDT 2022}
}
https://doi.org/10.1016/j.physletb.2022.137479
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