Fe 54 E1andM1excitationsin and low ... Schwengner | Institut für Strahlenphysik | γγγγ-ray beam...
Transcript of Fe 54 E1andM1excitationsin and low ... Schwengner | Institut für Strahlenphysik | γγγγ-ray beam...
Text optional: Institutsname � Prof. Dr. Hans Mustermann � www.fzd.de � Mitglied der Leibniz-GemeinschaftRonald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
E1 and M1 excitations in 54Fe
and
low-energy M1 strength in open-shell Fe isotopes
Ronald Schwengner
Helmholtz-Zentrum Dresden-Rossendorf, 01328 Dresden, Germany
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
The bremsstrahlung facility at the electron accelerator ELBE
Accelerator parameters:
• Maximum electron energy:
≈ 18 MeV
• Maximum average current:
≈ 0.8 mA
• Micro-pulse rate:
13 MHz
• Micro-pulse length:
≈ 5 ps
R.S. et al., NIM A 555, 211 (2005)
1 m
Be window
dipole
dipole
dipole
radiator
steerer
quadrupoles
quadrupole
electron-beam dump
quartz windowbeam
hardener
collimator
polarisationmonitor
target
PbPE
door
Pb
photon-beamdump
Pb
HPGe detector
experimentalcave
acceleratorhall
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Detector setup at γELBE
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
3γγγγ-ray beam parameters Values
Energy 1 – 100 MeV
Linear & circular polarization > 95%
Intensity with 5% ∆Eγ/Eγ > 107 γ/s
Electron Accelerator Facility180 MeV Linac pre-injector180 MeV – 1.2 GeV Booster Injector250 MeV – 1.2 GeV Storage RingFELs: planar (linear pol.) and helical (circular pol.)
For more details see:http://www.tunl.duke.edu/higs/
• Highest intensity (γ-rays/s/keV) γ-ray beam in the world
• Produces γ-rays by Compton backscattering inside the optical cavity of a storage-ring FEL
• Produces both linearly and circularly polarized beams
Courtesy of C. Howell (TUNL)
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Flux spectra at γELBE and HIγS
4000 6000 8000 10000Eγ (keV)
0
100
200
300
400
Φγ (
(eV
s)−
1 )
γELBE HIγS
Photon flux
γELBE: bremsstrahlung
HIγS: quasimononergetic,
polarized γ beams
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Measurements at γELBE and HIγS
10000 10500 11000Eγ (keV)
100
101
102
103
Cou
nts
HIγS
Ee = 13.9 MeV
γELBE
Eγ = 10.6 MeV
E1
M1
Identification of multipolarities
from scattering of polarized
γ radiation at HIγS.
E1 radiation in vertical detectors
and M1 radiation in horizontal
detectors.
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Measurement at γELBE
0 2 4 6 8 10 12 14Eγ (MeV)
1
10
100
1000
I s (eV
b)
54Fe28 Energy-integrated scattering
cross sections of levels in 54Fe
(J = 1 assumed)
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Measurements at γELBE and HIγS
6 7 8 9 10 11 12Eγ (MeV)
10−2
10−1
100
B(M
1) (
µ N
2 )
54Fe28
6 7 8 9 10 11 12Eγ (MeV)
10−4
10−3
10−2
B(E
1) (
e2 fm2 )
54Fe28
Transitions with clear M1 or E1 assignments from the experiments at HIγS.
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Experimental and calculated B(M1) values in 54Fe
6 7 8 9 10 11 12 13Eγ (MeV)
10−3
10−2
10−1
100
B(M
1) (
µ N
2 )
54Fe28 1
+ 0
+
5 6 7 8 9 10 11 12 13Eγ (MeV)
10−3
10−2
10−1
100
B(M
1) (
µ N
2 )
54Fe28 1
+ 0
+EXP CALC
Calculations using NuShellX.
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Experimental and calculated B(M1) values in 54Fe
6 7 8 9 10 11 12 13Eγ (MeV)
10−3
10−2
10−1
100
B(M
1) (
µ N
2 )
54Fe28 1
+ 0
+
5 6 7 8 9 10 11 12 13Eγ (MeV)
10−3
10−2
10−1
100
B(M
1) (
µ N
2 )
54Fe28 1
+ 0
+EXP CALC
Calculations by K. Sieja.
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Low-energy enhancement in 54Fe28
0 1 2 3 4 5 6 7 8Eγ (MeV)
0
0.02
0.04
0.06
B(M
1) (
µ N
2 )
π = +
54Fe
56Fe
Values in 56Fe as in
PRL 113, 252502 (2014),
but without lower limits of B(M1)
and without gates in Ex .
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Shell-model calculations of M1 strength functions
0 2 4 6 8 10 12 14 16Eγ (MeV)
10−1
100
101
102
103
f 1 (1
0−9 M
eV−
3 )
94Mo
(3He,
3He’) data
shell modelM1
E1 + M1(γ,n) data
E1
)-3
(M
eV
M1
f
-910
-810
-710
Fe, Voinov et al. (2004) 56
)γαHe,3
(
Fe, Larsen et al. (2013) 56
)γ (p,p'
SM calc
Fe56
(a)
(MeV)γE0 1 2 3 4 5 6 7
)-3
(M
eV
M1
f-9
10
-810
-710
Fe57
(b)Fe, Voinov et al. (2004)
57)γHe'
3He,
3 (
Fe, Larsen et al. (2013/2014) 57
)γ (p,p'
SM calc
RITSSCHIL NuShellX
R.S., S. Frauendorf, A.C. Larsen
PRL 111, 232504 (2013)
B.A. Brown, A.C. Larsen
PRL 113, 252502 (2014)
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Shell-model calculations for 60Fe34,64Fe38,
68Fe42
Code: NuShellX@MSU[B.A. Brown and W.D.M. Rae, Nucl. Data Sheets 120, 115 (2014)]
Model space: CA48PN with CA48MH1 Hamiltonian (48Ca core)[M. Hjorth-Jensen, T.T.S. Kuo, and E. Osnes, Phys. Rep. 261, 125 (1995)]
Orbits: π(0f(6−t)7/2 , 0ft
5/2, 1pt3/2, 1p
t1/2) ν(0ff 5
5/2, 1pp3
3/2, 1pp1
1/2, 0gg9
9/2)
Limitations of occupation numbers:
- t = 0 to 2.- f 5 = 2 to 6.- p3 = 0 to 4 for 60Fe and 2 to 4 for 64,68Fe.- p1 = 0 to 2 for all.- g9 = 0 to 2, 4, 6 for 60,64,68Fe, respectively.
Calculations: 40 levels of each spin from 0 to 10 and of each parity.
Transition strengths: eπ = 1.5 e, eν = 0.5 e; gs = 0.9 g frees
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
B(E2) values in Fe isotopes
Experimental and calculated reduced E2 transition strengthsof the 2+
1→ 0+
1transitions in 60,62,64,66,68Fe.
E (2+1) B(E2, 2+
1→ 0+
1) β2
(keV) (W.u.)EXP CALC EXP GLOB CALC CALC
60Fe34 824 772 13.6(14) 19.6 26.2 0.3162Fe36 877 544 14.7(18) 17.3 27.8 0.32
13.6(17)64Fe38 746 595 30.9+13.8
−7.2 19.1 26.8 0.3222.6(22)
66Fe40 574 568 21.0(21) 23.4 27.8 0.3268Fe42 522 616 24.2 25.4 0.31
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Average M1 strengths in Fe isotopes
0 1 2 3 4 5 6Eγ (MeV)
0
0.02
0.04
0.06
B(M
1) (
µ N
2 )
π = +
64Fe
68Fe
60Fe
0 1 2 3 4 5 6Eγ (MeV)
0
0.02
0.04
0.06
0.08
B(M
1) (
µ N
2 )
π = −
64Fe
68Fe
60Fe
⇒ Enhancement of M1 strength toward very low transition energy.
⇒ Development of a bump around 3 MeV with increasing neutron number.
PRL 118, 092502 (2017)
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Dipole strength functions in 151Sm and 153Sm
) -
3 S
F (
Me
Vγ
8−10
7−10
6−10
Sm, present exp.151
(p,d)
, n ), FilipescuγSm(150
, n ), FilipescuγSm(152
), Kopecky, E1γSm(n,149
GDR
M1
nS
(MeV)γ
-ray energy Eγ0 2 4 6 8 10
) -
3 S
F (
MeV
γ
8−10
7−10
6−10
Sm, present exp.153
(p,d)
, n ), FilipescuγSm(152
, n ), FilipescuγSm(154
), Kopecky, E1γSm(n,149
GDR
M1
nS
(p,d) data:
A. Simon et al.
PRC 93, 034303 (2016)
⇒ First observation of upbend
and scissors resonance
in one nuclide
⇒ Strength in the scissors region
about twice of that found in
(γ, γ) experiments
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Strength functions in 60Fe and 68Fe
0 1 2 3 4 5 6Eγ (MeV)
0
10
20
30
40
50
60
70f 1
(10−
9 MeV
−3 )
M1−60
Fe
M1−68
Fe
E1−RIPL
f 2 E
γ2 (10
−9 M
eV−
3 )
E2−60
Fe (x10)
E2−68
Fe (x10)
Dipole strength function
f1 = 16π/9 (hc)−3B(M1) ρ(Ex , J)
ρ(Ex , J) - level density
of the shell-model states,
includes π = +, π = −,
all spins from 0 to 10.
⇒ Strength in the scissors region
about three times that found in
(γ, γ) experiments.
PRL 118, 092502 (2017)
Eγ < 2 MeV 2 ≤ Eγ ≤ 5 MeV Sum60Fe34 5.67 3.52 9.1964Fe42 4.46 5.13 9.5968Fe42 3.98 6.63 10.61
B(M1)tot(µ2
N)
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Absorption strength in 68Fe
0
0.2
0.4
0.6
0.8
1
B(M
1) (
µ N
2 )
68Fe
0+
gs 1+
0 1 2 3 4 5 6 7 8Eγ (MeV)
0
0.2
0.4
0.6
0.8
1
B(M
1) (
µ N
2 )
68Fe
0+
2 1+
0+
15
∑B(M1) (µ2
N) (2≤ Eγ ≤ 5 MeV)
0+1→ 1+ 0+
2→ 1+
60Fe34 0.66 1.9864Fe42 1.65 2.5968Fe42 1.74 3.45
⇒ Strength from excited statesabout two times that found in(γ, γ) experiments because ofmore strong M1 transitionsin the scissors region.
PRL 118, 092502 (2017)
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
M1 transitions in 68Fe
0
1
2
3
4
5
6
0 1 2 3 4 5 6 7 8 9 10
Ex (
MeV
)
J
68Fe π = +
Transitions with B(M1) > 0.1µ2
N.
Line widths ∼ B(M1) values.
Ji = Jf , Jf ± 1, Eγ < 2 MeV:low-energy upbend
Ji = Jf ± 1, Eγ ≈ 3 MeV:scissors region
Ji = Jf + 1, Ex ∼ J(J + 1):shears bands
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Nuclear rotation
electric (collective) rotation magnetic rotation
J
z
x
E2
M1
M1
M1
M1
M1
M1
M1
E2
E2
E2
E2
E2
M1
M1
M1
M1
M1
M1
E2
E2
E2
E2
B(E2) ∼ Q20 B(M1) ∼ µ2
⊥
E x =h2
2ΘJ(J + 1); E γ ∼ J
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Predicted Appearance of magnetic rotation
0 20 40 60 80 100 120 140 160
0
20
40
60
80
100
120
140
Neutron Number N
ProtonNumberZ
j"
2
j
0.25
0.15
28 50
82
126
28
50
82
64
64
20
20
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Magnetic rotation - “Shears bands”
S. Frauendorf, Rev. Mod. Phys. 73, 463 (2001).
Examples at A ≈ 80:
H. Schnare et al., PRL 82, 4408 (1999).
R.S. et al., PRC 65, 044326 (2002).
R.S. et al., PRC 66, 024310 (2002).
R.S. et al., PRC 80, 044305 (2009).
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
E2 transitions in 68Fe
0
5
10
0 1 2 3 4 5 6 7 8 9 10
Ex (
MeV
)
J
68Fe π = +
Line widths ∼ B(E2) values.
Ji = Jf , Jf ± 1:admixtures to dipole transitions
Ji = Jf + 2, Ex ≈ J(J + 1)/(2J ):collective bands
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Average E2 strengths in 68Fe
0 1 2Eγ (MeV)
0
20
40
60
80
B(E
2) (
e2 fm4 )
68Fe, π = +
Ji = Jf + 2Ji = 2
34
5 6
7
810
9
Largest B(E2) valuesin rotational-like sequences:
Ex ≈ J(J + 1)/(2J )
Eγ ≈ (2J − 1)/J
J ≈ 12 MeV−1
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Summary
◦ Photon-scattering experiments on 54Fe28 carried out at γELBE and HIγS. 30 prominent
E1 and 16 M1 transitions observed up to 11.5 MeV.
◦ Strength in the quasicontinuum in analysis. Additional experiment with bremsstrahlung
up to 7.5 MeV needed.
◦ Large-scale shell-model calculations performed for 60Fe34,64Fe38,
68Fe42.
Collective properties of yrast states are reproduced in the used model space.
◦ The low-energy M1 strength decreases with increasing neutron number and a bump in
the scissors region develops while the sum of the two stays nearly constant.
◦ The strength in the scissors region includes many transitions between excited states.
This explains the different strengths found in experiments using photoexcitation and
light-ion induced reactions.
⇒
Ronald Schwengner | Institut für Strahlenphysik | http://www.hzdr.de
Collaborators
Experiments at γELBE (HZDR): D. Bemmerer, R. Beyer, A.R. Junghans, T. Kogler,A. Wagner et al.
Experiments at HIγS (TUNL): M. Bhike, Krishichayan, W. Tornow,U. Gayer, H. Pai (U Darmstadt),V. Derya (U Koln)
Calculations: B.A. Brown (NSCL/MSU)S. Frauendorf (U Notre Dame)K. Sieja (IPHC/CNRS)