Bands and Coulomb effects in
50
Cr
F. Brandolini,
1
J. Sanchez-Solano,
2
S. M. Lenzi,
1
N. H. Medina,
3
A. Poves,
2
C. A. Ur,
1,
* D. Bazzacco,
1
G. De Angelis,
4
M. De Poli,
4
E. Farnea,
4
A. Gadea,
4
D. R. Napoli,
4
and C. Rossi-Alvarez
1
1
Dipartimento di Fisica and INFN, Padova, Italy
2
Departamento de Fisica Teorica, Universidad Autonoma, Cantablanco, Madrid, Spain
3
Instituto de Fı ´sica, Universidade de Sa ˜ o Paulo, Sa ˜ o Paulo, Brazil
4
INFN, Laboratori Nazionali di Legnaro, Legnaro, Italy
~Received 11 December 2001; published 2 August 2002!
Experimental evidence for the coexistence of states with different K
p
value was found in
50
Cr. The band-
crossing of the K 50
1
ground state band with a K 510
1
one is confirmed. Large scale shell model calculations
could explain all of the observed experimental features and in particular the known experimental Coulomb
energy differences in the mirror pair
50
Fe-
50
Cr.
DOI: 10.1103/PhysRevC.66.021302 PACS number~s!: 21.10.Tg, 23.20.Lv, 27.40.1z
A wealth of experimental information on the structure of
nuclei in the middle of the 1 f
7/2
shell has been recently col-
lected at LNL @1–6#. The attention was mainly focused on
the yrast sequence of states of both natural and unnatural
parities up to the band termination in the 1 f
7/2
n
and 1 d
3/2
21
^ 1 f
7/2
n 11
configuration space, respectively. In order to inves-
tigate rotational collectivity and single particle properties
through experimental electromagnetic moments, lifetimes
were deduced with the Doppler shift attenuation method
~DSAM! for many levels. Large prolate deformation is pro-
duced in most ground state ~g.s.! bands, which decreases
approaching band termination. Large scale shell model
~LSSM! calculations for natural parity states were systemati-
cally made in the full pf configuration space, getting in gen-
eral an excellent agreement with the experimental findings
@7–9#. The unnatural parity sidebands were described by ex-
tending the pf space to include a nucleon-hole in the 1 d
3/2
orbital.
In the present work
50
Cr is further investigated @2,3#, be-
cause of the peculiarity in this region, that the g.s. band
shows evidence of bandcrossing, which is mainly based on
the presence of two close-lying 10
1
levels. Different inter-
pretations were given for the side band: in Ref. @9# it was
suggested to be oblate, while in Ref. @10# to be a high-K
prolate one. This question gained more interest recently, be-
cause the backbending was shown to be correlated with a
discontinuity of Coulomb energy difference ~CED! in the
mirror pair
50
Fe-
50
Cr @11#. In this context, rotational align-
ment ~RAL!, described by the cranked shell model ~CSM!,
was recently proposed @12# as a further explanation of the
observed backbending in
50
Fe-
50
Cr, following a previous
suggestion @13#. It will be shown that prolate strongly-
coupled Nilsson configurations, i.e., deformation alignment
~DAL!, can explain most of the observed features and that
the yrast 10
1
level can be approximately described as a K
510
1
state, due to the simultaneous excitation of a proton
and a neutron from the @ 321# 3/2
2
to the @ 312# 5/2
2
orbital
and from the @ 312# 5/2
2
to the @ 303# 7/2
2
one, respectively.
This was already suggested by the authors in Ref. @14#, but
additional arguments will be given here.
The reaction
28
Si(
28
Si, a 2 p )
50
Cr was performed at the
GASP spectrometer of LNL, using a target of 0.8 mg/cm
2
backed with 15 mg/cm
2
of Au, at the bombarding energy of
115 MeV. Experimental data for
50
Cr, obtained from the
same experiment @3#, are now extended to some nonyrast
states. In Fig. 1 the level scheme shows the up-to-date infor-
mation for the low-lying levels up to the 14
1
band terminat-
ing state in the 1 f
7/2
space. Only transitions from levels rel-
evant for the present discussion are shown. The levels shown
on the leftmost part of the figure were taken from Ref. @15#.
The K quantum number is assigned on the basis of arguments
presented in the following. The experimental properties of
positive parity levels of interest are summarized in Table I.
The level at 3324 keV was known to have I
p
54
1
and to
decay mostly to the yrast 4
1
state, with a lifetime of t
50.14(3) ps @15#.
The level at 3825 keV was reported in Ref. @15# as
(4,5,6)
1
. In the present work an upper limit of 1 ps for its
lifetime is estimated by a broad gating on the 541 keV feed-
ing transition from the 5
2
level at 4366 keV, whose lifetime
is determined to be 2.0~5! ps. Both values have been ob-
tained in the present work with a DSAM analysis of the 662
and 541 keV lines, with the procedure described in greater
detail in Ref. @3#. From the quoted limit, the squared mixing
ratio d
2
is estimated to be smaller than a few percent. The
angular distribution of the 662 keV transition to the 6
1
state,
when gated by the feeding 541 keV one, is forward-peaked
as expected for a pure D I 50 M 1 transition, so that the final
assignment to the level at 3286 keV is I
p
56
1
.
The 4
1
level at 3324 keV is fed by the 3875 keV one with
a 551 keV line. The 3875 keV level resulted to have a life-
time of 0.9~3! ps from the analysis of the 712 keV branch so
that its decay scheme allows to assign I
p
55
1
.
The level at 3792 keV, having a lifetime of 13~2! ps, has
been previously suggested to be 4
2
@3#. This is in analogy to
46
Ti, where the yrast 3
2
level is interpreted as the band head
of a K
p
53
2
band due to the parallel coupling of a proton in
the @ 202# 3/2
1
Nilsson orbital with one in the @ 321# 3/2
2
. In
the present case the first available orbital is the @ 312# 5/2
2
*On leave from NIPNE Bucharest, Romania.
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