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Neutronics Analysis of Fusion Systems
Presentation slides for the fusion energy neutronics workshop
Jonathan Shimwell
fusion,neutronics,neutron,photon,radiation,simulation,openmc,dagmc
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Nuclear data

  • Reactions
  • Isotope chart
  • Transmutation reactions
  • Q values
  • Threshold reactions
  • Fusion fuels (DT,DD ...)
  • Energy distribution from DT
  • Microscopic cross sections
  • Experimental data
  • Libraries (ENDF, TENDL, FENDL ...)
  • Cross section regions
  • Multigroup / continuous energy
  • Group structures
  • Reaction rate equation
  • Macroscopic cross sections
  • Scattering / thermalisation
  • Decay data
  • Photons
  • Energy distribution from radioactive material

Reactions

Nuclear reactions notation

Target nuclei (incident projectile, resulting fragments) resulting nuclei

Be9(n,2n)2He4 Target Projectile Product Product

Neutron induced reactions

  • 999 reactions channels with unique reaction IDs (MT numbers)
  • MT 3 is elastic scattering (n,'n)
  • MT 16 is neutron multiplication (n,2n)
  • MT 18 is neutron multiplication (n,f)
  • MT 205 is tritium production (n,Xt) where X is a wild card
  • MT 444 is damage energy

πŸ”— ENDF reaction numbers


Transmutation reactions

Reactions that result in a change of the isotope

No transmutation

(n, elastic) (n, inelastic) (n, heating)

Element transmutation

(n,p) (n,alpha) (n,fission) Be9(n,2n)2He4

Isotope transmutation

(n, gamma) Pb208(n,2n)Pb207


Transmutation of lead to gold

  • 1 stable isotope of gold Au$_{79}^{197}$
  • 3 natural isotopes of lead
    • Pb$_{82}^{204}$ βš› -3 protons, -4 neutrons
    • Pb$_{82}^{206}$ βš› -3 protons, -6 neutrons
    • Pb$_{82}^{207}$ βš› -3 protons, -7 neutrons
    • Pb$_{82}^{208}$ βš› -3 protons, -8 neutrons
  • 2 reactions for converting gold to lead
    • Pb204 (n,3npa) Au197
    • Pb204 (n,nta) Au197
  • No cross section data found in ENDF

Q values

Amount of energy absorbed (-ve) or release (+ve) during the nuclear reaction

Reaction Energy release [MeV] Threshold reaction
Be9(n,2n) -1.6 Yes
Pb208(n,2n) -7.3 Yes
Li6(n,t) 4.8 No
Li7(n,nt) -2.4 Yes

Mass and Binding energy converted to kinetic energy

Online Q value calculator at NNDC


Fusion fuels

Q values of fusion fuel reactions

Reaction Energy release (MeV)
D + T -> He$^{4}$ + n 17.6
D + D -> He$^{3}$+n 3.3
D + D -> T + p 4.0
D + He$^{3}$->He$^{4}$+p 18.3 *
  • No neutron emitted

Aneutronic Fusion fuels

  • Neutrons are not emitted in the primary fuel reaction
  • Neutrons can be emitted by reactions with the products
  • Energy capture via direct conversion or divertor?
Reaction Energy release
[MeV]
D + Li$^{6}$ -> 2He$^{4}$ 22.4
P + Li$^{6}$ -> He$^{4}$ + He$^{3}$ 4.0
He$^{3}$ + Li$^{6}$ -> He$^{4}$ + p 16.9
He$^{3}$ + He$^{3}$ -> He$^{4}$ + 2p 12.86
p + Li$^{7}$ -> 2He$^{4}$ 17.2
p -> B$^{11}$ -> 3He$^{4}$ 8.7
p -> N$^{15}$ -> C$^{12}$ + He$^{4}$ 5.0

Energy of neutrons from DT fuel

  • A DT plasma has several fusion reactions.
  • DT is the most likely reaction.
  • DD and TT reactions also occur with lower probabilities.
  • All reactions and emit different energy neutrons.


Microscopic Cross Section

  • Measured in Barns (1 barn = $10^{-28}m^{2}$)
  • Energy dependant
  • Cross section evaluations exist for:
    • different incident particles
    • different nuclides
    • different interactions.
  • Important neutron reactions plotted
    • Tritium breeding
    • Neutron multiplication


Reaction rate equation

  • The reaction rate ($RR$) can be found by knowing the number of neutrons per unit volume ($n$), the velocity of neutrons ($v$), the material density ($p$), Avogadro's number ($N_{a}$), the microscopic cross section at the neutron energy ($\sigma_{e}$) and the atomic weight of the material ($M$).
  • This reduces down to the neutron flux ($\phi$), nuclide number density ($N_{d}$) and microscopic cross section $\sigma_{e}$.
  • This can be reduced one more stage by making use of the Macroscopic cross section ($\Sigma_{e}$).

$$ RR = \frac{nv\rho N_{a}\sigma_{e} }{M} = \phi N_{d} \sigma_{e} = \phi \Sigma_{e} $$


Macroscopic cross section

  • Lithium metatitanate has a material density of 3.4 g/cm3
  • When plotting materials the Macroscopic cross section accounts for number density of the different isotopes
  • Units for Macroscopic cross section are cm$^{-1}$


Multigroup cross sections

  • Discretize a continuous distribution
  • Histogram of average cross section in each energy bin
  • Continuous cross section has rules for interpolation that can be accounted for.
  • Groups are not equally spaced.
  • Structures are optimized for different energy ranges (fission, fast fission, fusion etc)


Cross section regions

Reactions have characteristics

  • 1/v section
  • resolved resonance
  • unresolved resonance
  • thresholds
  • scattering


Angular distribution

  • The scattering angle varies depending on the energy of the incident neutron
  • Low energy neutrons have isotropic scattering (even probability in all directions)
  • High energy neutrons are more likely to have a low deflection angle and are forwards bias.


Energy distribution

  • There is also data on neutrons released in reactions such as (n,2n).
  • The (n,2n) reaction is a threshold reaction and requires energy.
  • No run away chain reaction possible.


Experimental data

  • Availability of experimental data varies for different reactions and different isotopes.

  • Typically the experimental data is then interpreted to create evaluation libraries, such as ENDF, JEFF, JENDL, CENDL.


Nuclear data libraries

There are several groups that produce and distribute nuclear data

  • TENDL 2023 πŸ‡ͺπŸ‡Ί 2850 neutron
  • JENDL 5 πŸ‡―πŸ‡΅ 795 neutron
  • ENDF/B-VIII.0 πŸ‡ΊπŸ‡Έ 557 neutron
  • JEFF 3.3 πŸ‡ͺπŸ‡Ί 562 neutrons
  • BROND 3.1 πŸ‡·πŸ‡Ί 372 neutrons
  • FENDL 3.2b 🌐 191 neutron
  • CENDL 3.2 πŸ‡¨πŸ‡³ 272 neutron

Path length

  • Path length = 1 / $\Sigma_{T}$
  • A 14MeV neutron will lose energy via scattering interactions
  • As the neutron energy decreases the path length also decreases
  • Path length at thermal energy is more constant


Energy loss

The average logarithmic energy decrement (or loss) per collision ($\xi$) is related to the atomic mass ($A$) of the nucleus

$\xi = 1+ \frac{(A-1)^2}{2A} ln \frac{(A-1)}{(A+1)}$

Hydrogen Deuterium Beryllium Carbon Uranium
Mass of nucleus 1 2 9 12 238
Energy decrement 1 0.7261 0.2078 0.1589 0.0084

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Why lithium

  • Lithium has a particularly high cross section for tritium production
  • Li6 has a very high cross section at low neutron energies
  • Li7 has a reasonable cross section at high neutron energies
  • Other reaction channels are relativity low
  • Often alloyed with Si or other elements to improve material properties (e.g. flammability)

  • Elements up to Iron plotted

Why beryllium

  • Beryllium has the lowest threshold energy for any isotope with a n,2n reaction.
  • This means even low energy 3MeV neutrons can undergo (n,2n) reactions.
  • Often alloyed with Ti or other elements to improve material properties (e.g. swelling due to retention)
  • Lead is also a popular choice for a neutron multiplier

  • Elements up to Iron plotted

Other materials

Tungsten

  • High atomic number = good gamma attenuation

  • High neutron capture resonances = good neutron attenuation

Water

  • High hydrogen content = excellent neutron moderator

Helium 4

  • Low interaction cross sections and low density = transparent to neutrons and gammas

Neutron spectra through materials

By knowing the materials present can you identify which blanket results in which spectrum

  • FLiBe, Molten salt, typically 90% enriched Li6
  • HCPB, helium cooled pebble bed, typically 60% enriched Li6
  • HCLL, helium cooled lithium lead, typically 90% enriched Li6
  • WCCB, Water cooled ceramic breeder, typically 60% enriched Li6
  • WCLL, water cooled lithium lead, typically 90% enriched Li6
  • Liquid Lithium, typically natural enrichment

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