robert haight lansce-ns workshop on statistical nuclear physics and applications in astrophysics and...
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![Page 1: Robert Haight LANSCE-NS Workshop on Statistical Nuclear Physics and Applications in Astrophysics and Technology Ohio University July 8-11, 2008 LA-UR-08-4399](https://reader036.vdocuments.site/reader036/viewer/2022062517/56649f2a5503460f94c4400e/html5/thumbnails/1.jpg)
Robert HaightLANSCE-NS
Workshop on Statistical Nuclear Physics
and Applications in Astrophysics and Technology
Ohio University
July 8-11, 2008
LA-UR-08-4399
Statistical Neutron-Induced Reactions
Studied by Neutron, Proton, and Alpha-Particle Emission
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• Context
• Neutron-induced reactions
• Charged particle emission
• Neutron emission
• (Gamma-ray emission)
• Concentrate around A ~ 56
Outline
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Context – history, data bases, previous works
• Lots of data on charged-particle induced reactions– Protons, 3He, alphas, heavy ions, etc.– Emission spectra, angular distributions, etc. for charged particles and
neutrons – Major experimental efforts in the 1960’s, 1970’s; continuing at lower
intensity through the present time– Major analyses of data
– Gilbert & Cameron– Backshifted Fermi Gas
– E.g. Vonach, Dilg, etc.– Superfluid models
• Neutron-induced reactions – Lots at 14 MeV incident energy– Some at other energies– Evaluated data files – ENDF, JEFF, JENDL, BROND, etc.
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Why then study more neutron-induced reactions?
• Applications– Neutron transport for many applications– Radiation damage in fast fission reactors (AFCI, GNEP) and
fusion reactors of the future from (n,H) and (n,He) reactions– a.k.a. “Gas Production”
– Requirements on accuracy of data
• Basic physics– Learn more about reaction models, level densities– Other data (e.g. total cross sections, known very well) constrain
reaction models– Reactions can be studied over a wide range of incident energies
in the same experiment – use “white” neutron source
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(n,xp) and (n,xalpha) reactions are in competition with neutron emission (n,n’), (n,2n), etc.
Physics:
• Optical model for transmission coefficients
• Nuclear levels
• spectroscopy
• level densities
• We measure as a function of incident neutron energy
•Traces out competition with excitation energy
•Insights into non-statistical reactions, e.g. direct and pre-equilibrium
61Ni
60Ni + n(target)
59Ni + 2n
En
11.388
-7.820
0.000
2+
4+
0+
1.332
2.5062.042
60Co + p
57Fe +
-1.354
(J ,Ex)
(J ,Ex)
(J ,Ex)
n
p
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Visitor center
Isotope production facility
800-MeV proton linac
Proton radiography and UCN
Target-2
Target-4
Proton storage ring
MLNSC -neutron scattering
Visitor center
Isotope production facility
800-MeV proton linac
Proton radiography and UCN
Target-2
Target-4
Proton storage ring
MLNSC -neutron scattering
Los Alamos Neutron Science Center - LANSCE
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LANSCE Neutron Sources cover 16 orders of magnitude in neutron energy
Lujan centerEn < 500 keV
PSR
Target-2“Blue Room”
Target-4(Fast neutrons)
LINAC
• Lujan - ultra-cold to epithermal neutrons up to ~500 keV
• Target 2 - UCN to fast neutrons; also protons
• Target 4 – Fast neutrons from 0.1 to 800 MeV
Proton storage ring
To Areas A, B and C
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We use the 30-degree flight path at Target 4 (WNR)
Proton beam
Charged-particle emission@ 15. 1 meters“NZ”
Neutron emission@ 22.7 meters“FIGARO”
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• Neutron energy range can be studied in one experiment
• Covers energies of statistical reactions – up to ~ 10 MeV
• Covers much higher energies where direct and other pre-equilibrium reactions become important
Our incident neutron energy range is from 1 to 100 MeV
High-energy tailFission spectrum
1.0E-05
1.0E-04
1.0E-03
1.0E-02
1.0E-01
1.0E+00
1.0E-01 1.0E+00 1.0E+01 1.0E+02 1.0E+03
En (MeV)
Y (n
/p/M
eV/S
r)
15 Deg
30 Deg
60 Deg
90 Deg
0.1 1 10 100 1000
100
10 -1
10 -2
10 -3
10 -4
10 -5
Y (
n/p
/sr/
MeV
)
E n (M eV)
1.0E-05
1.0E-04
1.0E-03
1.0E-02
1.0E-01
1.0E+00
1.0E-01 1.0E+00 1.0E+01 1.0E+02 1.0E+03
En (MeV)
Y (n
/p/M
eV/S
r)
15 Deg
30 Deg
60 Deg
90 Deg
0.1 1 10 100 1000
100
10 -1
10 -2
10 -3
10 -4
10 -5
Y (
n/p
/sr/
MeV
)
E n (M eV)
Fast neutron source spectra at LANSCE
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Light charged-particle emission
p, d, t, 3He, alpha
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Many approaches have been used to measure charged-particle emission in reactions induced by fast neutrons
• Gas accumulation: irradiate and then measure by mass spectrometry
• only for Helium (hydrogen contamination is everywhere)• need a monoenergetic neutron source or the result is an average over the spectrum
• Activation: e.g. 56Fe(n,p)56Mn (2.579 hours)• Need monoenergetic source (as above)• Need a radioactive product – e.g. not 56Fe(n,alpha)53Cr(stable)• Not complete when other channels are open, e.g. 56Fe(n,n’p)55Mn (stable); 56Fe(n,n +alpha)52Cr(stable)
• Detect protons, deuterons, tritons, 3He and alpha particles • Monoenergetic source • White source and time-of-flight techniques LANSCE
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Cu & Wshielding
Cu
Mylarwindow
Mo window
Reaction chamber55.9 cm I.D.
Long steelCollimator
15.1 m to neutron source
neutronbeam
0.94 m
Fissionchamber
Sample
CsI(Tl) + photodiode
Silicon surface barrier detector
Low pressure proportionalcounter or thin silicon surfacebarrier detector
2.2 cm diam.
Brass "cleanup"collimator
.
2.7 cm diam.
Charged particles emitted in the reactions are identified by E detectors and their energies are determined by stopping detectors of silicon or CsI(Tl)
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We choose detectors to give information on the complete charged-particle spectra
• Low pressure proportional counters allow identification of helium ions to below 3 MeV
• Silicon detectors stop alpha particles up to 33 MeV
• CsI(Tl) scintillators – 3 cm thick -- stop 100 MeV protons
A large dynamic range of particles is detected. The range is defined by low energy helium ions and high energy protons
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59Co(n,xalpha) angle-integrated emission spectra are described well by calculations
Ref: S. M. Grimes et al., Nucl. Sci. Eng. 124, 271 (1996)
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Excitation function for 59Co(n,xalpha) is described well by calculations up to > 20 MeV
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However, level density parameters needed to be modified to fit the 59Co(n,xalpha) data
Nucleus a ( / MeV ) (MeV)
57Co 4.70 1.2758Co 5.30 0.00
54Mn 5.03 0.0055Mn 5.46 1.2756Mn 6.05 0.00
57Fe 5.72 1.5458Fe 6.19 2.83
Gilbert & Cameron systematics
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Measurements on nickel isotopes show problems with evaluated data libraries
58Ni(n,xalpha)
0
50
100
150
200
0 5 10 15 20
En (MeV)
Cro
ss s
ecti
on
(m
b)
.
LANSCE data
Grimes
Kneff
Graham
Dolya
Haight
Tsabaris
Goverdovski
Qaim84
Fessler
ENDF/B-VI
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Peter Fu analyzed the differences in the evaluated cross sections for 58Ni(n,alpha) -- 1995
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Fu’s analysis shows variations in the used level densities
Ra
tio
of
lev
el d
en
sit
ies
Uhl / Fu BSFG / GC
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Low energy 58Ni(n,alpha) data (Tohoku) could be fit well
• T. Kawano, et al., J. Nucl. Sci. Tech. 36, 256 (1999)
• Baysian analysis (KALMAN)
Parameter Prior Posterior
a(58Ni) (/MeV)
7.994 6.163
a(58Co) (/MeV)
8.942 7.957
a(55Fe) (/MeV)
8.143 8.163
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60Ni(n,xalpha)
0
20
40
60
80
100
120
0 5 10 15 20En (MeV)
Cro
ss S
ecti
on
(m
b)
LANSCE Data
Grimes
Kneff
Graham
Dolya
Fischer
Haight
ENDF/B-VI
The situation with 60Ni is similar with regard to evaluated data libraries
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Recent results for iron also show a problem with the ENDF evaluation
Iron (n,Helium)
0
0.01
0.02
0.03
0.04
0.05
0 2 4 6 8 10 12 14 16 18 20
Neutron Energy (MeV)
Cro
ss S
ecti
on
(b
)
FZK/INPE56Fe
NRG-2003
JENDL-HE56Fe
IEAF-2001
LANSCE data
ENDF/B-VII56Fe
Haight/Kneff + He-accumulation
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Results for hydrogen production are in agreement with ENDF and also confirm LA150 evaluation up to 50 MeV
Fe(n,Hydrogen)
0
200
400
600
800
1000
1200
1400
0 20 40 60 80 100 120 140
En(MeV)
Sig
(m
b)
.
LA150
ENDF/B-VI
New WNR data
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Neutron emission
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With gamma-ray detectors near the sample, we trigger off the prompt gamma-rays to study neutron emission
FIGARO (n,xn+)
n
x
• 20 Neutron detectors
• “Double time-of-flight“ experiment
• Incident neutron energy from TOF from souce
• En’ emitted from TOF ~ 1m
• Neutron emission in coincidence with gamma rays
sample 22 m from WNR source
BaF2
HPGe
BaF2
HPGe
A+1Z
AZ + n(target)
E n
2+
4+
0+
(J,E x) n'
Trigger
A+1Z
AZ + n(target)
E n
2+
4+
0+
(J,E x) n'
Trigger
Neutron emission contingent on one specific -transition
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Nickel data were described well with EMPIRE calculation, with modified level density
58,60Ni(n,n’) (natural elemental isotopes)
Ref: D. Rochman, Nucl. Instr. Meth. in Phys. Res. A523, 102 (2004)
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Iron data are obtained by triggering on the lowest 2+ ground state gamma ray
• Dietrich noted that nearly all of the excited states in 56Fe decay through the 847 keV 2+ state
Fe57
(target)
4 +
(J,E
x)
56Fe + n
2 +
+
0
+
(J,E
x) n'
0.847Trigger
En
2.085
2.6572+
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Iron data are being analyzed
One neutron detector, binned in incident neutron energies
1–1.5 MeV 1.5-2 MeV 2–2.5 MeV
2.5–3 MeV 3–3.5 MeV 3.5-4 MeV
4–4.5 MeV 5–5.5 MeV
6–6.5 MeV
7–7.5 MeV
6.5-7 MeV5.5-6 MeV
7.5-8 MeV 13-15 MeV
4.5–5 MeV
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3-3.5 MeV Iron
0
200
400
600
800
0 1 2 3 4 5
En (MeV)
Ne
utr
on
s/M
eV
(S
cale
d)
5-5.5 MeV Iron
0
50
100
150
200
250
300
0 1 2 3 4 5 6
En (MeV)
Neu
tro
ns/
MeV
(sc
aled
)
4-4.5 MeV Iron
0
100
200
300
0 1 2 3 4 5 6
En (MeV)
Ne
utr
on
s/M
eV (
scal
ed)
13-15 MeV Iron
0
50
100
150
200
0 2 4 6 8 10 12 14 16En (MeV)
Ne
utr
on
s/ M
eV
(sc
ale
d)
Takahashi data (1992)
Examples of preliminary data for 56Fe
0.847
0.8470.847
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• Emission spectra are measured as a function of incident neutron energy
• Only part of data are analyzed so far (one of 3 gamma-ray detectors) and better statistics are on the way
• Energy resolution is good for neutrons of a few MeV
• Gating on other gamma-rays is possible to test angular momentum distribution of states populated by (n,n’)
Preliminary data for 56Fe are encouraging
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Show distribution of “a”
Ref. Dilg et al., Nucl. Phys. A217, 269 (1973)
Systematics give an estimate of accuracy of level density inputs to calculations
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Some observations
• Emission data (p, alpha, n,…) neutron-induced reactions can be described by statistical reactions with suitable parameter selection.
• Can these data be predicted ab initio with confidence from global or other parameters?
• Competition among reaction channels can reduce the errors in the calculated results, but, given “bad” parameters, it is hard to predict the outcome.
• Users need data to some accuracy
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Path forward
• New approach: Measure and model neutron emission spectrum contingent on the following gamma cascade going through a given level (or set of levels)
-- angular momentum selection -- need new reaction model code
(Monte Carlo HF)
A+1Z
AZ + n(target)
E n
2+
4+
0+
(J,E x) n'
Trigger
A+1Z
AZ + n(target)
E n
2+
4+
0+
(J,E x) n'
Trigger
• Increasingly large set of data to test reaction models–Neutron reaction data complement charged-particle data–Will the fits be physics or parameterizations?
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• To provide data for GNEP – “Gas Production” by neutrons on structural and other materials – e.g. Fe, Cr, Ni, Zr, Ta, W etc.
- The cross sections are “source terms” for assessing radiation damage of materials
- Gas production is an important component of radiation damage in materials irradiated to high fluences in advanced fuel concepts.
• Other applications
• Neutron interrogation – transport though containers, etc.
• Shielding
• Fusion
• Criticality safety
• Detector development. For example, neutron output detection same as for fission neutrons
Applications motivate (fund) this work
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Effects of Helium are observed at temperatures above 0.5 Tmelt
Thanks to Stuart Maloy
0.5 TmeltCopper
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Summary
• Increasingly large data set for nucleon-induced reactions on nuclides with A ~ 56 can be used to test reaction model calculations• Charged- particle emission• Neutron emission• Gamma - ray emission
• Model calculations can describe data if suitable parameters are used
• Nuclear level densities are the largest uncertainty in the reaction model calculations
• Some widely used evaluations for helium production are in disagreement with our results … and with others.
• Evaluations for hydrogen production are in somewhat better shape
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An aside -- higher energy data for iron test new evaluations – different physics at higher energies
Iron (n,Helium)
0
0.05
0.1
0.15
0.2
0 20 40 60 80 100
Neutron Energy (MeV)
Cro
ss S
ecti
on
(b
)
FZK/INPE56Fe
NRG-2003
JENDL-HE56Fe
IEAF-2001
LA-15056Fe
LANSCE
TSL-Uppsala