Effect of shell closure N=50,82. Measurements of neutron emission
probability with high efficiency3He neutron detector TETRA
Dmitry Testov
09 November 2011
Introduction
78NiN/Z1,79
132Sn N/Z=1,64
Ni
Sn
Nuclei of interest
Qβ = 5-25 MeVSn = 0–5 MeV
For nuclei with N > Z, the neutron drip line islocated where the neutron separation energyequals zero
The blue areas indicate the nuclei which couldpotentially be produced and accelerated intobeams by SPIRAL2
One- and two-β-delayed neutronemission scheme of strongly neutronrich nucleus Az. In a daughter nucleusAz+1 the strength function of β—decay Sβ(E) depending on excitation energy Exis shown.
Introduction
Precursor
Emitter
Yu.Lyutostansky and I.Panov, Z.Phys.A, 313,235 (1983)
Known β-2n emitters
Nuclides T1/2,ms xn Pxn,%11Li 8.5 2n 4.1(4)
3n 1.9(2)14Be 14.5 2n 0.80(8)
3n 0.2(2)15B 10.4 2n 0.4(2) 17B 5.1 2n 11(7)
3n 3.5(7)4n 0.4(3)
30Na 48 2n 1.17(16)32Na 13.5 2n 8(2)34Na 5.5 2n ~ 5098Rb 110 2n 0.38(6)100Rb 51 2n 2.7(7)
Predicted β-2n emitters
Nuclides T1/2,ms Qb-B2nPxn,%
(MeV)86As 0.9 1.33 0.02 94Br 0.07 3.78 3.12112Nb 0.10 3.79 1.28134In 0.1 5.54 99136Sb 0.8 2.25 10.6/0.28142J 0.2 2.28 0.76150Cs 0.15 2.97 1.48
(a) Total β-decay half-lives for Ga/Cu isotopescalculated from the 1) DF3+CQRPA including the allowed and first-forbidden transitions, 2) FRDM+RPAfor the allowedtransitions in comparison with the experimental data. (b) Delayed neutron emission probabilities for Ga isotopes calculatedfrom DF3+ CQRPA: 1) including allowed and first-forbidden transitions, 2) for allowed transitions.
Gamow-Teller and first-forbidden decays near the r-process paths at N = 50, 82 (1)
78Ni
____ 1f7/2
-------- μ(n)____ 2d5/2
____ 1g9/2
____ 1f5/2
____1p3/2
____1f7/2
____ 1p1/2
____ 1g7/2
____ 2d5/2
neutrons
____ 1g9/2
____ 2p1/2
____ 1f5/2
-------- μ(p)
____ 2p3/2
protons
FF , L=1
GT, L=0
N=50
____ 1f7/2
-------- μ(n)____ 2d5/2
____ 1g9/2
____ 1f5/2
____1p3/2
____1f7/2
____ 1p1/2
____ 1g7/2
____ 2d5/2
neutrons
____ 1g9/2
____ 2p1/2
____ 1f5/2
-------- μ(p)
____ 2p3/2
protons
FF , L=1
GT, L=0
N=50
N<50 GT transitions dominate N>50 FF transitions 2d5/2 → 1f5/2 dominates
The experimental β-decay half-lives for the Cd/Snisotopes(1) DF3 + CQRPA for allowed and first-forbiddentransitions, (2) experimental data (see text).Comparison between DF3 + CQRPA calculations of thedelayed neutron emission probabilities and experimentaldata:(1) DF3 + CQRPA for allowed and first-forbiddentransitions, (2) experimental data).
Gamow-Teller and first-forbidden decays near the r-process paths at N = 50, 82 (2)
N ≈ 82; Z < 50
N ≈ 82; Z ≥ 50
Nuclei at r-process path produced at ALTO (78Ni region)
85Ga≥150ns
86Ge≥150ns
87As0.57s
86Ga≥150ns
87Ge≈0.14s
88As≥300ns
84Ge
83Ga
85As
82Zn>150ns
84Ga
85Ge
86As
83Zn>150ns
74Co>150ns
75Co>150ns
81As
76Ni
80Ge
79Ga
77Cu
78Zn
82As
77Ni>150ns
81Ge
80Ga
79Zn
78Cu
82Ge
81Ga
83As
80Zn
79Cu
83Ge
82Ga
84As
81Zn
80Cu>300ns
88Ge≥300ns
89As≥300ns
90As≥150ns
91As≥150ns
76Co 77Co
78Ni>150ns
75Fe 76Fe
r-process path
N = 50; Z = 28N = 82; Z = 50
Mechanisms of detecting neutrons
3He (n,p) cross-section as a function of neutron energy
Energy, MeV
3He gasmoderator
a neutron source
nn
n
As can be seen, the cross-section is much larger for thermal neutrons (~ 0.0253eV) than for fast neutrons (~ 1 MeV). Fission neutrons are born fast. Thus, tomaximize the efficiency of the 3He tubes, the neutrons must be slowed (ormoderated) to thermal energies. Neutron moderation is most often achieved viaelastic scattering collisions with hydrogenous material. For this reason, 3He tubesare often embedded in high-density polyethylene (C6H12).
Table of Nuclides, http://atom.kaeri.re.kr/, Nuclear Data Evaluation Laboratory, Korea Atomic Energy Research Institute (2007).
th = 5320 barns
3He + n = 3H + p + 780 keV
CELL
Zero energy threshold
Zero cross-talk
Low gamma sensitivity
Free geometry
Easy in use
High efficiency
Low internal background
Preprint JINR P13-2007-154
Neutron detectors TETRA with 3He filled counters
Pressure of 3He 7 atm90 counters (d=32 mm; L = 50 cm)Eff. 60% (0.4 – 1.5 MeV)
3He-detector Scintillator
Neutron energy ? VThreshold 0 ~30÷300 keVCross talk no yesEfficiency 30-60% 10-30%
Multiplicity Yes ?
Angle correlation Yes (<200) ?
Time scale 10 µs ns
Chemistry of 112 Fobos
Vassilissa Shin
Uses of 3He detectors in different setups
Neutron-Neutron coincidence
Neutron-Fragments coincidence
Efficiency of TETRA as a function of 3He gas pressure (MCNP-simulations)
2 4 6 8 10 12 14 16 18 20 220
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
Efficiency of TETRA as a function of 3He-pressure for different neutron energies
0.5 MeV 1 MeV 2 MeV 5 MeV 8 MeV
3He pressure, atm
Eff
7 atm
0.5 MeV1 MeV2 MeV
5 MeV
8 MeV
0 0,01 0,02 0,03 0,04 0,05 0,06 0,07
Efficiency Difference between 7 atm & 20 atm
0.5 MeV 1 MeV 2 MeV 5 MeV 8 MeV
4 atm 7 atm 10 atm 20 atm
0,130,08 0,06 0,03
0,520,57 0,59 0,63
Efficiency/atm; Efficiency/$ (En=1MeV)
Eff/atm (%)Eff, %
3He pressure
Eff
ration = efficiency / pressure% per atm
1.0300%
Nucl. Instr. and Meth. A540 (2005) 430-436
Van de Graaff Accelerator, Charles University, Prague
Calibration for average delayed neutron energy measurementsEn=400-1500 keV
moderatorcounters
Neutron flux
Neutron flux
Neutron efficiency depends on neutron energy
2n/1n = 3.10-4
Probably the observed two neutronactivity belong to 136Sb, then
Pβ-2n(136Sb)~ (1.4±0.2)%
Predictions: Pβ-2n(136Sb)= (10.6 - 0.28) %*
Delayed neutron emitters in the 136Sb region
Intensity: calculation [1], primary electron beam, 50MeV, 10μA[1] Nucl. Instrum. and Mety. in Phys. Res. B 204 (2003) 246–250
136Sb0.923 s
β- : 100.00 %β-n : 16.30 % 8,85•103 [1/s]
136Te17.63 s
β- : 100.00 %β-n : 1.31 % 9,8•106 [1/s]
135Te134Te
136In
135Sb1.679 s
β- : 100.00 %β-n : 22.00 %
134Te
136Cd
135I134I 136I
136Sn0.25 s
β- : 100.00 %β-n : 30.00 %
9•101 [1/s]
133Te
2n 1n β
1n β
Z
N
84 85 86
52
51
50
1n β
JINR proposal at IPN Orsay: approved
e-LINAC
ECS bunker
PARRNe mass separator
ISOL installation at ALTO
Secondary beam lines
Laser, located one level up
Laser arrives here
Experiment 2009 = upgrade needed
paraffin + polyethylene shielding (very bulky)
The efficiency measured for the neutron detector is up to 35%
Neutron lifetime in the detector is 35 μs
BEAM
Germanium Detectors
Tape axis
Collection Chamber
3He counters
Detection chamber is inside
(0.47 ≤ Pn(136Te) ≤ 4.89)%
Pn(136Te) 1.31 %
beta
Neutron detector TETRA installation at ALTO
0,1 1 100
0,1
0,2
0,3
0,4
0,5
0,6
0,7
Internal Layer 1 Layer 2 Layer 3 Outer Layer 4Overall efficiency
En, MeV
Effi
cien
cybeam
Efficiency of the TETRA (MCNP simulations)
* For neutron energy 0.144 – 1.5 MeV** For gamma energy 1 MeV
0.1 1 100
0.1
0.2
0.3
0.4
0.5
0.6
0.7
Efficiency of TETRA in respect to different schielding
no schielding
En, MeV
Effi
cien
cyEffect of background shielding on efficiency (MCNP simulations)
No shielding at all (00 cm)Green line
A layer of 5 cm of polyethylenegives an advantage to anefficiency of neutron registrationfrom a neutron source placed atthe center of the detector up to 5 –10 % at neutron energy more than2 MeV0.1 1 10
00.050.1
0.150.2
0.250.3
0.35Efficiency of the inner layer
no schieldingCH2, 20 cm15 borated +5 CH2Borated, 20 cm
En, MeV
Effi
cien
cy
0.1 1 100
0.02
0.040.060.08
0.10.120.14
Efficiency of the outer layer
no schieldingCH2, 20 cm15 borated +5 CH2Borated, 20 cm
En, MeV
Effi
cien
cy
ONLY polyethylene (20 cm)Orange line
0.1 1 100
0.1
0.2
0.3
0.4
0.5
0.6
0.7
Efficiency of TETRA in respect to different schielding
no schielding CH2, 20 cm
En, MeV
Effi
cien
cy
ONLY Boron polyethylene 20cmBlue line0.1 1 10
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
Efficiency of TETRA in respect to different schielding
no schielding CH2, 20 cm Borated, 20 cm
En, MeV
Effi
cien
cy
Mixed shielding piepolyethylene (5 cm) +
Boron polyethylene (15 cm)Yellow Line
0.1 1 100
0.1
0.2
0.3
0.4
0.5
0.6
0.7
Efficiency of TETRA in respect to different schielding
no schielding CH2, 20 cm 15 borated +5 CH2 Borated, 20 cm
En, MeV
Effi
cien
cy
82,83,84,85 Gallium precursors
84Ga 84Ge 84As
83Ge 83As
n n
Ф1 Ф2 Ф3
A general scheme presenting the relevantnuclei participating in the decay chain of aneutron reach Ga isotope
0 2 4 6 8 10 1270
75
80
85
90
95
100
105
9293
9495
969798
99100
101102
7980
8182
8384
8586
Ga Rb
Emax(neutron), MeV
Isto
pes
Plasma ion source,Ф1, Ф2, Ф3 are ON
Laser ion source,Ф1 is ON; Ф2=0, Ф3=0
First experiment is scheduled on march 2012
Maximum En of neutrons
624 keV2+→0+84Ge nouvelle scientifique
Red: ionisation laser, aftera few hours of beamtimerouge
Blue: total statistic (surfaceionisation) from the thesis ofM. Lebois (previousexperiment on the samemass)
84Ga→84GeT1/2= 0.085 s
Laser beam of 84Ga at ALTO October 2011
136Sb
84Ga
TETRA Neutron Detector Setup: prototype for DESIR
Moderator: polyethylene, distance between parallel faces - 5 cm.
Efficiency: 30-60% (depends on geometry)
Life time: 15-30 µs (depends on geometry)
close to 4-π geometry
Geometry: Ø 3 cm, 3He at 7 atm Ø 3 cm, 3He at 7 atmlength 50 cm length 25 cm
Total numberof counters: 90 342
TETRA Detector
Why does it call TETRA ????
Greek prefixes (Cardinal) – “4”:- 4Pi-geometry
- Study multiple neutron emission (4 neutrons ?!) …. and more
Kingdom: Animalia Phylum: ChordataClass: ActinoptervaiiOrder: Characiformes Family: - Alestiidae- Characidae- Lebiasinidae
Tetra species (from biology, some):Pygmy tetra, Odontostilbe dialepturaCopper tetra, Hasemania melanuraBlack neon tetra, Hyphessobrycon herbertaxelrodiCoffe-bean-tetra, Hyphessobrycon takasei……..New tetra species to be added (from nuclear physics):
Antimony tetra, Stibium duplicemGallium tetra, Dives Insolens
Tetra are species of small freshwaterfish from Africa, Central America andSouth America belonging to thebiological family Characidae and to itsformer subfamilies Alestiidae (the"African tetras") and Lebiasinidae.
Fish “TETRA”
TETRA