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LArSoft Coordination Meeting

US/Central
FNAL

FNAL

Erica Snider (Fermilab)
Description

To connect via Zoom:  Meeting ID 831-443-820

(See instructions for setting Zoom default to join a meeting with audio and video off: https://larsoft.org/zoom-info)

PC, Mac, Linux, iOS, Android:  https://fnal.zoom.us/j/831443820

Phone:

H.323:

162.255.37.11 (US West)
162.255.36.11 (US East)
213.19.144.110 (EMEA)
See https://fnal.zoom.us/ for more information
 

At Fermilab:  WH13SW (Disappearance Room)

Support

Minutes for LArSoft coordination meeting on Mar 12, 2019

Present | Lynn Garren, Robert Hatcher, Alex Himmel, Kyle Knoepfel, Saba Sehrish, Erica Snider|

Remote | Patrick Green, Diego Garcia-Gamez, Andrzej Szelc, Katherine Lato |

Release and Project status report [Erica Snider]

  • v08_12_00 released on march 6
  • this week updates to nutools, and no meerge requests so far
  • Neext week:
    • migration to root v6.16/00 - to fix an iorule problem
    • will combine with migration to art 3.02
  • Genie v3
    • validation testing by MicroBooNE, once done will get sign off from other experiments
  • LArTPC data overlay workshop
  • LArSoft workshop 2019
    • 1.5 days, dates TBD
    • Tentative program - LArSoft introduction, Advanced computing techniques, dnd Long-term vision
    • [Lynn] suggested to add a session patch releases

Conclusion:

A semi-analytic way of Simulating light [Andrzej Szelc]

  • Introduces analytic model for light propagation
  • Optical libraries size are very large (for DUNE and SBND, > 1 GB)
    • problem for cvmfs, so moved to StashCache
  • Does not provide timing information (though this is solved in LArSoft)
  • Need to run a campaign of grid jobs every time a detector parameter changes
  • For DUNE 1x2x6, segmenting the bars into sub-detectors makes it impossible to generate the library due to memory issues. Needed for the TDR
  • DUNE needs realistic X-Arapuca supercell geometry for physics studies. SBND libraries also becoming cumbersome
  • An alternate method for simulation of light to make things work
    • Improved parameterization of photon arrival times for both VUV and visible light
    • A semi-analytic model for predicting N hits based on position in the detector for direct VUV and reflected light coming off cathode
  • Simulation of the VUV arrival times
    • this work provides optimzation and extension of existing feature in LArSoft for the photon arrival time
    • VUV arrival times change as function of distance due to Rayleigh scattering
    • Index of refraction also changing rapidly across emission spectrum
    • This needs to be taken into account
      • Landau + exponential for short distances (< 300 cm)
      • Landau for longer distances (> 300 cm(
    • Visible arrival calculated as distance / velocity
    • Smearing in times approximated as exponential (w cutoff)
  • Semi-analytic modelling of light (direct)
    • Calculate solid angle
      • Functions for square and circular detectors
      • No library needed, so avoid memory issues
      • No issue from segmentation of bars into X-Arapuca supercells or windows
      • Can scale to full size of DUNE
    • Need correction due to Rayleigh scattering + reflections
    • Detailed study of border effects on-going
  • Corrections to direct light due to scattering
    • Gaisser-Hillas functions fit well
      • Based on ratio of solid angle calculation to full simulation as a function of angle from photo-detector
      • Parameterize as function of angle and distance to photo-detector
  • Show agreement with full simulation is better than for libraries
  • Reflected light (visible)
    • Created by TPB coated foils on cathode
    • Calc cathode solid angle for VUV
    • Correct for scattering using Gaisser-Hillas curves
    • Detected photons from solid angle to optical detector (from foils)
    • Parameterize corrections as function of angle, distance from cathode
  • VU direct light results:
    • there is no bias and performs better the photon librarries
  • Performance for DUNE 1x2x6: also better than the optical libraries
  • Should not be looking outside the range ( for range -500 < y < 500 cm)
  • Most of the changes in larsim
    • bulk of code is in LArG4/OpFastScintillatiton
  • Improvement in the PhotonVisibility Serevice
    • use pre-calculated values result in huge efficiency improvement
    • discrepency introdiced by this is negligible ~0.1 ns
  • the use of feature is off by default
  • fcl configuration provided to enable optical library and time correction and also to enable nhits and time correction
  • More improvements to the code: remove duplicated code
  • Future improvements:
    • is it worth splitting the photon counter module into two since it does too many things
  • based on old LArG4 - for DUNE
  • Testing
    • DUNE CI tests
    • ArgoNeuT and LArIAT ok
    • ICARUS and MicroBooNE have some problem
    • SBND failed. Wrong tag. Will re-check
  • Almost ready to go (modulo the failing CI tests)
  • Thread safety?
    • Not
    • Should be able to make it not a service (Photon visibility)
  • Kyle raised some issues related to multi-threading
    • Will address with the move to the new LArG4.

Conclusion

  • This feature request was approved.
    • larsim: feature/lightprop_ugr_mcr
    • larana: feature/lightprop_ugr_mcr
There are minutes attached to this event. Show them.
    • 1
      Release and project report
      Speaker: Dr Erica Snider (Fermilab)
      Slides
    • 2
      Updates to light simulation
      Speakers: Dr Andrzej Szelc (University of Manchester), Dr Diego Garcia-Gamez (University of Manchester)
      Slides