Revealing new structures in odd–odd 54Mn nucleus
The excited states of odd–odd 54 Mn ( Z = 25 , N = 29 ) nucleus have been investigated using the fusion evaporation reaction 55 Mn( α , α n) 54 Mn at the beam energy of 34 MeV. A new and improved level scheme of 54 Mn has been proposed in this work with the placement of 22 new γ -ray transitions. Sp...
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Published in | The European physical journal. A, Hadrons and nuclei Vol. 59; no. 10 |
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Main Authors | , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
Berlin/Heidelberg
Springer Berlin Heidelberg
16.10.2023
|
Subjects | |
Online Access | Get full text |
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Summary: | The excited states of odd–odd
54
Mn (
Z
=
25
,
N
=
29
) nucleus have been investigated using the fusion evaporation reaction
55
Mn(
α
,
α
n)
54
Mn at the beam energy of 34 MeV. A new and improved level scheme of
54
Mn has been proposed in this work with the placement of 22 new
γ
-ray transitions. Spin and parity (J
π
) of most of the levels in the revised level scheme have been firmly assigned. The placement of some of the already known
γ
rays in the level scheme and J
π
assignments of some of the levels reported earlier have also been revised. The new level scheme, which has been extended up to
∼
6 MeV, provides new insight and interesting structural aspects of the generation of high angular momentum in this odd–odd Mn isotope with neutron number (
N
=
29
) just above the
N
=
28
shell gap. Three octupole-phonon-coupled negative parity states have been identified for the first time in this nucleus.
E
3 transitions have also been observed to decay from these states. Shell model calculations with two different interactions i.e. kb3gpn and gx1pn have been performed which well reproduced the low-lying, few-particle states but fail to reproduce the higher-lying multi-particle states. These higher-lying states have been understood as resulting from collective excitations. An oblate minimum obtained from the Total Routhian Surface calculations provides support to this conjecture. |
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ISSN: | 1434-601X |
DOI: | 10.1140/epja/s10050-023-01147-9 |