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MCNP and capabilities at UofC Grayson C. Rich Enrico Fermi Institute and Kavli Institute for Cosmological Physics University of Chicago DAMIC-M kickoff meeting Paris 2018 Jun 12
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Page 1: Enrico Fermi Institute and Kavli Institute for ... · 2018-06-12  · MCNP and capabilities at UofC Grayson C. Rich Enrico Fermi Institute and Kavli Institute for Cosmological Physics

MCNP and capabilities at UofC

Grayson C. Rich Enrico Fermi Institute and Kavli Institute for Cosmological Physics

University of Chicago

DAMIC-M kickoff meeting Paris

2018 Jun 12

Page 2: Enrico Fermi Institute and Kavli Institute for ... · 2018-06-12  · MCNP and capabilities at UofC Grayson C. Rich Enrico Fermi Institute and Kavli Institute for Cosmological Physics

Monte Carlo N-Particle transport code• Developed by Los Alamos National Lab

- These folks need to know how neutrons move

- Development dates back 50+ years

• Export controlled - distribution is restricted by US government, users must apply for license

• Some people consider it the unassailable standard for simulation of low-energy neutron transport

• Can use MPI to take advantage of many-core architectures (i.e., supercomputers or university clusters)

- Mildly complicated by export control

• Features “variance reduction” techniques intended to speed up simulation (weighting of particles, roulette, biasing of sources)

2G.C. Rich - DAMIC-M kickoff - 2018 Jun 12 [1] D.Z. Freedman, Phys Rev D 9 (1974) [2] A. Drukier, L. Stodolsky, Phys Rev D 30 (1984)

Page 3: Enrico Fermi Institute and Kavli Institute for ... · 2018-06-12  · MCNP and capabilities at UofC Grayson C. Rich Enrico Fermi Institute and Kavli Institute for Cosmological Physics

Example inputc CsI crystal 99 99 -4.51 -1 -2 3 IMP:N=1 IMP:P=1 $ central scatterer (CsI) c PTFE reflector around crystal 700 21 -2.25 (1 -711 700 -2) : (2 -710 -711 ) IMP:N=1 IMP:P=1 c Al housing around crystal 701 20 -2.7 (700 -701 711 -704):(701 -702 711 -705): & (702 -710 711 -704):(710 -703 -704) IMP:N=1 IMP:P=1 c borosilicate glass window 702 22 -2.23 700 -3 -1 IMP:N=1 IMP:P=1 c Deuterium gas cell 100 2 -0.0005 -100 101 -102 IMP:N=1 IMP:P=1 $ D cell … c CSI ASSEMBLY c Target Detector 1 1 cx 0.95 $ cylinder bounding sides of scatterer 2 px 2.55 $ plane bounding top of scatterer 3 px -2.55 $ plane bounding bottom of scatterer c surfaces related to outer (aluminum) boundary 700 px -2.7 $ bottom of assembly 701 px -2.5 $ lip near bottom 702 px 1.71 $ top lip 703 px 2.8 $ top of assembly 704 1 cx 1.27 $ outer of Al assembly, thickest parts, 1inch dia. 705 1 cx 1.17 $ out of Al assembly, axial midsection, 23.4mm dia. c interior surfaces of assembly 710 px 2.7 $ bdry of top layer of Al with reflector, Al 1mm thick 711 1 cx 1.09 $ outer edge of PTFE reflector, 1.4mm thickness … c tally counting neutrons entering/exiting CsI f91:n 1 2 3 *c91 90 0 fq91 d f c fc91 Neutron current across boundaries of CsI crystal. Neutrons entering in 90-180 bin of surf 1 and 3, 0-90 surf 2

3G.C. Rich - DAMIC-M kickoff - 2018 Jun 12

Page 4: Enrico Fermi Institute and Kavli Institute for ... · 2018-06-12  · MCNP and capabilities at UofC Grayson C. Rich Enrico Fermi Institute and Kavli Institute for Cosmological Physics

Simulation geometries• Complicated geometries are realizable (see image of CCD

test chamber geometry, made in part by Karthik Ramanathan, UofC grad student)

4G.C. Rich - DAMIC-M kickoff - 2018 Jun 12

Page 5: Enrico Fermi Institute and Kavli Institute for ... · 2018-06-12  · MCNP and capabilities at UofC Grayson C. Rich Enrico Fermi Institute and Kavli Institute for Cosmological Physics

Np

Np Np Am

Cs Ka1 esc. I Ka1 esc.

Cs Ka2 esc.

I Ka2 esc.

I Kb1 esc.

Cs Kb1 esc.

10 20 30 40 50 60

E [KeV]

100

101

102

103

104

Count

241AMMCNP

Neutral- and charged-particle transport possible• Can simulate not only neutral particles (neutrons, photons), but can also transport charged particles

• Can track recoiling ions, electrons generated by interactions

- Tracking of electrons can add lots of computation time

- Has techniques for efficiently approximating net result of photon interaction without tracking resulting electrons

5G.C. Rich - DAMIC-M kickoff - 2018 Jun 12

Page 6: Enrico Fermi Institute and Kavli Institute for ... · 2018-06-12  · MCNP and capabilities at UofC Grayson C. Rich Enrico Fermi Institute and Kavli Institute for Cosmological Physics

Particle-tracking output: MCNPX-PoliMi• By default, MCNP does not produce step information (e.g., can’t see if particle X scattered off of

nucleus of type Y at time Z)

• Default outputs are in the form of tallies

- Tallies are flexible but time coincidences can be especially difficult if not impossible

• PoliMi is an official “hack” of MCNP’s internal tracking information

- Also accessible via “PTRAC” output built into MCNP

- Learning curve for PTRAC use is much more steep, however…

• Utilities for PTRAC use also exist

- Can allow certain explorations that PoliMi makes difficult

- Flexibility generally makes this the way you would want to approach tracking

- Opens up use of MCNP6, the newest version of the code which brings all the features of parallel versions 5 and X plus some new low-energy electron improvements (among other things)

6G.C. Rich - DAMIC-M kickoff - 2018 Jun 12

Page 7: Enrico Fermi Institute and Kavli Institute for ... · 2018-06-12  · MCNP and capabilities at UofC Grayson C. Rich Enrico Fermi Institute and Kavli Institute for Cosmological Physics

Quick comparisons with GEANT4• Input

- Do not have to define a physics list

- “Variance reduction” techniques can be turned off, reverting to “analog transport” (necessary for tracking)

• Output

7G.C. Rich - DAMIC-M kickoff - 2018 Jun 12 [1] S.D. Monk et al., Nucl. Instrum. Meth. B 399 (2017) [2] C. Guardiola et al., J. Inst. 6 (2011)

- Some studies have found serious discrepancies (e.g., figure from [1])

- Exact source is not clear

‣ Possibly related to interpolation of cross sections [2]

‣ Possibly related to simplified treatment of materials by GEANT4 [2]

- You can also find studies that show very good agreement, or good agreement in certain situations

Page 8: Enrico Fermi Institute and Kavli Institute for ... · 2018-06-12  · MCNP and capabilities at UofC Grayson C. Rich Enrico Fermi Institute and Kavli Institute for Cosmological Physics

Expertise at UofC• Experience using MCNPX/5/6 in myriad use cases

- In-beam neutron scattering experiments (quenching factor measurements)

‣ These involve time coincidences, quenching in liquid scintillator detectors, energy cuts, location-dependent beam-neutron production, etc…

- Neutron source experiments (e.g., 252Cf, AmBe), including photo-neutron source QF measurements

- Various gamma-focused simulations (e.g., 241Am, 137Cs, 55Fe) including Compton calibration

- Background simulations (cosmic-induced neutrons, neutrons from U/Th in surroundings)

• Familiarity with tally-based output as well as tracking

- Utilization of both PoliMi and PTRAC (allowing use of MCNP6)

8G.C. Rich - DAMIC-M kickoff - 2018 Jun 12


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