robert haight lansce-ns workshop on statistical nuclear physics and applications in astrophysics and...

38
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 Statistical Neutron-Induced Reactions Studied by Neutron, Proton, and Alpha- Particle Emission

Upload: shana-chase

Post on 05-Jan-2016

215 views

Category:

Documents


1 download

TRANSCRIPT

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

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

Page 2: 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

• Context

• Neutron-induced reactions

• Charged particle emission

• Neutron emission

• (Gamma-ray emission)

• Concentrate around A ~ 56

Outline

Page 3: 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

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.

Page 4: 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

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

Page 5: 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

(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

Page 6: 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

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

Page 7: 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

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

Page 8: 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

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”

Page 9: 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

• 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

Page 10: 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

Light charged-particle emission

p, d, t, 3He, alpha

Page 11: 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

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

Page 12: 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

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)

Page 13: 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

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

Page 14: 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

59Co(n,xalpha) angle-integrated emission spectra are described well by calculations

Ref: S. M. Grimes et al., Nucl. Sci. Eng. 124, 271 (1996)

Page 15: 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

Excitation function for 59Co(n,xalpha) is described well by calculations up to > 20 MeV

Page 16: 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

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

Page 17: 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

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

Page 18: 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

Peter Fu analyzed the differences in the evaluated cross sections for 58Ni(n,alpha) -- 1995

Page 19: 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

Fu’s analysis shows variations in the used level densities

Ra

tio

of

lev

el d

en

sit

ies

Uhl / Fu BSFG / GC

Page 20: 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

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

Page 21: 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

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

Page 22: 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

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

Page 23: 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

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

Page 24: 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

Neutron emission

Page 25: 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

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

Page 26: 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

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)

Page 27: 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

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+

Page 28: 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

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

Page 29: 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

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

Page 30: 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

• 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

Page 31: 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

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

Page 32: 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

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

Page 33: 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

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?

Page 34: 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

• 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

Page 35: 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

Effects of Helium are observed at temperatures above 0.5 Tmelt

Thanks to Stuart Maloy

0.5 TmeltCopper

Page 36: 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

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

Page 37: 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
Page 38: 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

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