Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of...

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1 Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2 Idaho National Lab, P.O. Box 1625, Idaho Falls ID 83403, 3 Chemical and Materials Engineering and Nuclear Engineering Program, University of Idaho, Idaho Falls ID 83402 August 27, 2012 IPRC Fontana, WI August 2012 Slide 1

Transcript of Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of...

Page 1: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 778432Idaho National Lab, P.O. Box 1625, Idaho Falls ID 83403,

3Chemical and Materials Engineering and Nuclear Engineering Program, University of Idaho, Idaho Falls ID 83402

August 27, 2012IPRC Fontana, WI August 2012

Slide 1

Page 2: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Used Nuclear Fuel (UNF) andThe Fuel Cycle

Slide 2

Reference: Blue Ribbon Commission on America’s Nuclear Future, Jan 2012

• UNF is stored on location in waterponds and dry casks.

• In this form it would remainhazardous for thousands of years.

• The only way to remove thosehazards is to literally destroy themby fission for the transuranics(TRU).

Page 3: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

A Call for Waste Disposal

• U.S. UsedNuclear FuelInventory:

– Currently67,000Metric Tonsof UNF instorage

– Growth Rateof ~2000Metric Tonsper year

Slide 3

Reference: Blue Ribbon Commission on America’s Nuclear Future, Jan 2012

Page 4: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Benefits to ADSMS

• ADSMS can destroy the transuranics (TRU) at a rateequivalent to their production in conventional reactors.

• It is a green and profitable technology.

• The core is sub-critical with all its fuel dissolved in amolten salt matrix; therefore, it cannot melt down in aconventional sense.

• It uses used nuclear fuel as its power source to producehundreds of Megawatts of power.

• It can incinerate the long-lived radioactive waste that isproduced by conventional reactors.

• It can recycle used fuel into fertile fuel for conventionalreactors.

4

Page 5: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Accelerator Driven Systems

• Why an accelerator?– An on-off switch to fission.– Capable of operating subcritical– Can run off of UNF

• Fission Driven by Spallation Neutrons

• Fast neutron source from 800 MeV Proton Beam• Flux Coupled Stack of Isochronous Cyclotrons

– 1 footprint– Redundancy → reliability– Sustainable driver for fission cores

Slide 5

Proton Beam Beam Window Molten Salt Core

Page 6: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Accelerator Complex

• Injector– 2.5 MeV proton beam is fed to the TAMU 100.

• TAMU 100– Produces a 100 MeV proton beam is fed to the TAMU 800.

• TAMU 800– 10 mA beam from each cyclotron is chopped at injection and then

separated into 3 beams after extraction from TAMU 800.– The 4-stack of cyclotrons can produce 12 2.7 MW beams.

• 12 beam lines– Each beam can drive an 65 MWth ADS molten salt core.

Slide 6

Reference: McIntyre, IPAC 2012, Poster Session

Page 7: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Accelerator Technology Advances

• Flux CoupledStack

• Strong FocusingCyclotron– Quadruple

focusing channelsat the magnet polefaces

– Novel Design forSuperconductingRF Cavities

Slide 7

Page 8: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Molten Salt Fission Pot

• 12 Molten Salt Pots– 65 MWTH Each– Produce 300MWE together

• Energy gain of 5.3 taking into account thermal-electric conversion and the efficiency of theaccelerators

– Together they can burn the contents of anAP1000

• NaCl-Based Molten Salt– NaCl – 69%– TRU (0.878) +Lanthanides (0.122) = 31%

• Salt processing and refueling every year

Slide 8

Page 9: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Chloride Molten Salt System

• Why Chlorides?– High actinide solubility– Compatibility with very

fast neutronics– Stable operating

temperature range~500-700 ᵒC

– Low chemicalcorrosiveness

• Why not Chlorides?– Cl36 Production

• Solution: Isotope Separation(USEC)

– Complex chemistry• Multiple oxidation states

– Limited Experimental Data

Slide 9

Fluorides Chlorides

Actinide Solubility atAcceptableTemperature Low High

Vapor Pressure Very Low Low

OperatingTemperature 700 ᵒC+ 500 ᵒC+

Electronegativity(Pauling Scale) 3.98 3.16

Number of OxidationStates 1 8

Number of StableActinide IonizationStates Several 1-2

Page 10: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Chloride Molten Salt Systems

• LiCl-KCl– Pyroprocessing advantages– Wealth of available data– Secondary Salt– Not suitable for primary salt

• KCl– n,α reaction, 36Cl production

• MgCl2• NaCl

– High actinide solubility– Well modeled– Primary Salt Choice

Slide 10

0

100

200

300

400

500

600

700

800

900

0 20 40 60 80 100

T (ᵒ

C)

Mole % PuCl3

Binary Phase Diagram: NaCl-PuCl3

with ADSMS Operating Range

NaCl PuCl3

Reference: Bjorklund, et al, 1959.

Page 11: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Fuel Salt Preparation

• Preparation of Oxide Spent Nuclear fuel:– Electrolytic Oxide Reduction– Rare Earth and

Actinide Oxidation– Uranium Reduction

• Avoids typical proliferation hazards– Non-aqueous– 1 Pot Process– No segregation of Pu– Radioactive lanthanides remain with

the minor actinides throughout the process

Slide 11

90%

1%2%

2%

5%238U235UTRUOther

Lanthanides

Page 12: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Electrolytic Reduction

• Developed at ANL and INL– LiCl-1wt% Li2O– Uranium, TRU, Noble Metals,

and Rare Earth Reduction inCathode Basket

– >90% Reduction of TRU

Slide 12

Sintered Oxide

Fuel

Post

Electrolytic

Reduction of

Oxide Fuel

Oxide Fuel before and after

Voloxidation

Page 13: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Heavy Metal Oxidation

• CdCl2 Oxidation• Lanthanides Oxidize first• Uranium oxidizes last of the Actinides• Noble Metals are left as waste product• UCl3 can provide lower melt temp for

operation.

Slide 13

Page 14: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Molten Salt Reconditioning

• Similar steps as Salt Preparation• Potassium reduction helps to keep lower operating

temperature and avoid salt freezing• Criticality concerns mitigated via batch processing

Slide 14

Page 15: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Criticality Concerns DuringReconditioning

• During reconditioning, TRU is reduced into metal form from themolten salt.

• Criticality calculations were performed with the Monte Carlocode MCNPX for several vessel designs and depositionscenarios.

• Critical mass calculations are sensitive to:– Deposition Geometry

• Dendrite formation or preferred TRU deposition decreases the critical mass

– Vessel Design• Bucket Shape• Infinite lattice geometry- series of individual cells can be modeled and share

neutrons

– Absorber width and placement• Hafnium wall thickness has an exponential on criticality- diminishing returns

Slide 15

Cone half-angle 75°Critical mass: 35.1 kg

Cone half-angle 15°Critical mass: 14.4 kg

Uniform depositionCritical mass: 168.3 kg

Page 16: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Conclusions

• Proposing a power producing solution tothe nuclear waste problem.

• Making innovative advances inaccelerator technology.

• Actively seeking– Experimental and modeling support,

suggestions, and lessons learned and

– Collaborations to assist with actinide saltexperiments, corrosion, and radiationdamage testing.

Slide 16

Page 17: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

The ADSMS Collaboration

[email protected]

Texas A&M University: Nuclear Engineering:Physics: Saeed Assadi Marvin Adams

Karie Badgley Pavel TsvetkovWilliam Baker Idaho National Lab:Austin Baty Michael SimpsonJustin Comeaux Prabhat TripathyTim ElliottJames Gerity University of Idaho:Ray Garrison Supathorn PhongikaroonJoshua KellamsAl McInturff Brookhaven National Lab:Peter McIntyre Ilan Ben-ZviNate Pogue Bill HorakAkhdiyor Sattarov Hans LudewigElizabeth Sooby Francois Meot

Mechanical Engineering: Deepak RapariaTed Hartwig Nick SimosDavid Foley Mike TodosowShreyas Balachandran Bill Weng

Chemistry:Abraham Clearfield

Page 18: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Questions?

Slide 18

Thank youfor yourattention!

Page 19: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

0.8

0.9

1.0

1.1

1.2

1.3

1.4

0 20 40 60 80 100

ton

s

years

239Pu and TRU' inventories 1 core

0

10

20

30

40

50

60

70

80

90

0 5 10 15 20

MW

years

Wth one core

Wth from 12 core ADSMS

Page 20: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

Neutrons are born in thisregion. All Actinides canfission at ratesproportional to theirfraction in the fuel

0.00

0.10

0.20

0.30

0.40

1.E-04 1.E-02 1.E+00

Me

V-1

En MeV

Fission NeutronSpectrum from 239Pu

If they do give any fission (no capture), they scattering in the medium they loosetheir energy, move this way on the plot. Only 239Pu can fission !!!

Outside second region capture becomes also important and as a result one starts tobreed back minor actinides. We need ultra fast neutrons in the core, smaller core!!!!

Page 21: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Main vessel dimensions

Inner radius 0.32 m

Height 1.5 m

Outer radius of downflow

tube

0.27 m

Thickness of downflow tube 0.0254 m

Manifold plate thickness 0.01 m

Wall material/Thickness

Ni 0.00635 m

Hastelloy-N 0.0127 m

HT-9 0.0254 m

Ni Beam line and beam “windows”

OD 0.26 m

Beam window shape half sphere

Thickness 0.003 m

Absorber/Reflector

B4C 0.48 m radius, 0.1 m thick

Lead 0.65 m radius, 0.3 m thick

Wth, MW 800

Proton Beam 4, 800MeV, 10mA

Total flux, 1015cm-2s-1 1.3

Fast fraction, nf 28%

keff 0.96

Burn Up (GWd/tHM) 500 (100y)

Tmelt,oC 515

Composition 31%(TRU+La)Cl3 69%NaCl

Density, g/cc 3.142

Total load, t 22.2 (56 in 100y) Actinide

Power density, W/cc 165W

Tin/Tout,oC 565/575

Page 22: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Objectives of Corrosion Testing

• Identify corrosion resistantmaterials in chloride molten salts

• Quantify the effect of variousoxygen concentrations in the salt– Mimic realistic operating

conditions– Simulate worst-case scenarios

• Control the environment andsuppress corrosion– Monitor and stabilize redox

potential in the salt– Cathodic Protection: Naval Ships

and your Hot Water Heater

• Combine molten salt corrosionwith neutron damage effects– Swelling– He Embrittlement

Centrifugal pump operatedcontinuously for one year inmolten salt at 500 C

Slide 22

Page 23: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Initial Mass Spectroscopy Data

A clear trend was seen in the refractory material:

0

0.000005

0.00001

0.000015

0.00002

0.000025

0.00003

0.000035

0 5 10 15 20 25 30

Wt%

inS

alt

Sam

ple

Time (hours)

Wt% Metal in the salt through the Chloride Salt

Corrosion Test

Nb Wt %

ECAE Nb

Wt%

Ta Wt %

Evaporation?

Passivation?

Slide 23

Page 24: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

2) Blue salt: Zircaloy Exposure inChloride Salt, t=2hr

Slide 24

Page 25: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

3) Stainless Steel Exposure in ChlorideSalt, t=6hrs

Slide 25

Page 26: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Initial Testing at the Center forAdvanced Energy Studies

• Baseline corrosion test:– LiCl-KCl and LiBr-KBr– 11 different materials– Inert, argon glove box– 24 hour experiments– Each experiment run at 700 C

• Samples:– 6 samples per metal

• 3 samples per salt compound– 1 Control– 2 Exposed to salt

– All samples were etched and prepared in the same manner

• Salt and Materials Characterization– Inductively Coupled Plasma Mass Spectrometry– Scanning Electron Microscopy– Tension Test

Slide 26

Page 27: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Sample Prep and ExperimentalControls

• Etched according to ASM Handbook recommendations• Rinsed with nano-pure water then dried using isopropyl

alcohol and baked at 150 ᵒC• Exposed to salt for 24 hours• Salt samples taken at 2, 4, 6, 12, 18, and 24 hours• Same operating temperature for each experiment• Eutectic salt cations remained consistent, i.e. LiBr-KBr

and LiCl-KClZircaloy Samples before and after

corrosion test

Page 28: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Future Corrosion Work

• Continue salt analysis and evaluate precisionof results

• Experiment with sample preparationtechniques

• Next round of corrosion tests:– 500 hours– Like materials for corrosion crucible and coupons– Nickel and Nickel Alloys in comparison with

Stainless Steel– Gas monitoring of a closed system

• Radiation damage of testing of Nickel andNickel Alloys– Simulate He embrittlement– Assess possibility to use Hastelloy-N or Pure

Nickel for both vessel and heat exchanger tubingSlide 28

Page 29: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Initial Mass Spectroscopy Data

0

50

100

150

200

250

300

350

-5 0 5 10 15 20 25 30

Concentr

ati

on

of

Meta

l(m

icro

gra

ms/lit

er)

Time (hours)

Raw Mass Spec Data from 316 Stainless Steel Salt

Sample

Chromium / 53 [#2]

Manganese / 55 [#1]

Manganese / 55 [#3]

Iron / 56 [#1]

Cobalt / 59 [#3]

Nickel / 60 [#2]

Nickel / 60 [#3]

Copper / 63 [#2]

Copper / 63 [#3]

Slide 29

Page 30: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

We are seeking collaborators!

• Neutronics

• Molten salt chemistry /corrosion

• High-power spallation targetry

• Beam dynamics – strong-focusing cyclotron

• Superconducting magnetics

• Superconducting RF

• Fuel cycle simulation/optimization

• Counter-flow heat exchanger

• Safety analysis, what-if scenarios

Please contact us - [email protected]

Slide 30

Page 31: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Metal SamplesTested:

• Niobium• ECAE Niobium

(Equal ChannelAngular Extrusion)

• Tantalum• Nickel• Zircaloy (two types)• 316 Stainless Steel• Tungsten• Hastelloy-N• HT-9 Steel• T91 Steel

Initial ObservationsMade

• Salt changed colors ina number ofexperiments

• Often times a metallicfilm appeared to coverthe bottom of thecrucible

• Vapor formed throughthe duration of thebromide studies

• Any wire used in earlyiterations of theexperimental set uphad clear vaporeffects-color changeand hardening

Tungsten Salt Column after Test (LiBr-KBr)

Slide 31

Page 32: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Modeling and Experimentation: Bridgingthe gap in data

• Molecular Dynamics Modeling:– Ionic structure of a molten salt

• Interaction Potentials: forces describe the salt’s behavior

– Intermolecular Bonds, Repulsive Forces,Dispersion, Electrostatics, and PolarizationEffects

– Solves the equations of motion at every time step

• With this program, we can calculate:– Density: We have already implemented this in our

neutronics calculations– Heat Capacity– Diffusion Coefficients– Viscosity– Thermal Conductivity– Electrical Conductivity

Reference:: 1. N. Ohtori, M. Salanne, and P. Madden. J. Chem. Phys. 130, 104507(2009).2. M. Salanne, C. Simon, P. Turq, and P. Madden, Journal of Fluorine Chemistry 130(2009) 38-44.

Slide 32

1

1.5

2

2.5

3

3.5

4

4.5

0 20 40 60 80 100D

ensi

ty(g

/cc)

Mol % UCl3

Density vs molar concentration in NaCl-UCl3

melt

Calculated

Experimental

Page 33: Department of Physics and Astronomy, Texas A&M University, … · 2016-08-12 · 1Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station TX 77843 2Idaho

August 27, 2012

Density Calculations

Slide 33

2.9

3

3.1

3.2

3.3

3.4

3.5

3.6

650 700 750 800 850 900 950 1000 1050 1100 1150

Den

sity

(g/c

c)

Temperature (K)

Density Map of NaCl-PuCl3 System with and withoutLanthanide Additions

66-34 mol% (No Lanthanides)

67-33 mol% (No Lanthanides)

68-32 (No Lanthanides)

69-31 mol% (No Lanthanides)

67-33 mol% ( 87.8% PuCl3 and 12.2% La)

68-32 mol% ( 87.8% PuCl3 and 12.2% La)

69-31 mol% ( 87.8% PuCl3 and 12.2% La)