Simulation and Analysis TF

Europe/Berlin
Description
Task force on simulation and analysis activities Join from PC, Mac, Linux, iOS or Android: https://weizmann.zoom.us/j/2651789663?pwd=NWpaMzlLclpmdmtERFpYMS9DQ2gzdz09 Or Telephone: Dial(for higher quality, dial a number based on your current location): US: +1 470 250 9358 or +1 206 337 9723 United Kingdom: +44 203 481 5237 or +44 131 460 1196 Israel: +972 3 978 6688 Meeting ID: 265 178 9663 Password: 946342 International numbers available: https://weizmann.zoom.us/u/aM3jhiGHP Or an H.323/SIP room system: H.323: 162.255.37.11 (US West) 162.255.36.11 (US East) 115.114.131.7 (India Mumbai) 115.114.115.7 (India Hyderabad) 213.19.144.110 (EMEA) 103.122.166.55 (Australia) 209.9.211.110 (Hong Kong SAR) 64.211.144.160 (Brazil) 69.174.57.160 (Canada) 207.226.132.110 (Japan) Meeting ID: 265 178 9663 Password: 946342 SIP: 2651789663@zoomcrc.com Password: 946342 Or Skype for Business (Lync): https://weizmann.zoom.us/skype/2651789663

Intro:

- what do we beam by noise? noise coming from the machine upstream (beam halo, secondaries,… secondary particles accompanying the primary beam)

- beampipe material is copper but we can use whatever we like inside LUXE range (Sasha uses Aluminium)

- Kapton and radiation hardness? (huge photon flux) this is used in similar fluxes in different 

- technologies for the fwd spectrometer could be also Cherenkov

 

Kyle:

- please move to use proper spectrum of the photons (need to see how to implement the fixation)

- backscattering from the collimators —> will be difficult for the IP detectors —> need more distance.

- liso scintillators will be used in SLAC (fast scintillation time) —> please send around documentation

- need to discuss redundancies for the technologies

- distance from dipole to the detector is too large for the particles to travel in air

  - use vacuum all the way with slots? too expensive and a lot of scattering in the slot-window

  - put wires in vacuum is possible (down to the 1 mu scale and even below) but we anyhow need a window at the end of the vacuum

  - can work on the 2 solutions

 

Tony:

- go with 17.2 deg

- Sasha: need to reproduce the bremsstrahlung file again.

  - do we assume foil is in vacuum?

- timing misalignment also implemented? 

- intensity scan:

  - simulate additional ~4 points of lower intensity besides the “best” one for each laser

  - can increase the spot size or the pulse length to play with the intensity rather than playing with the power itself

    - in the gamma+laser setup we can gain a lot by using a larger spot since the Bremss’ photons flux will be bigger than the electron beam.

- misalignments:

  - jitter from XFEL is ~8 fs, but the error would be much larger (driven by the laser jitter)

  - for every point simulated, we’d need another run(s) with “±1sigma” misalignments implemented.

  - in the beginning we can do this only for the “best”

- can launch jobs by early next week

 

Sasha:

- B-field ?

- change distance between the staves from 5.4 to 10 cm (also the overlap is not 7 cm but 4 cm) —> Noam will ask Oz to change that in the drawings

- fwd spectrometer:

  - should use the Cherenkov there for now

  - add the collimators after the end of the pipe (200 um thick window made of Kapton)

  - move setup as much as possible “to the left” but with minimum interference with the IP detectors

- will optimise the processing time (increasing step sizes etc). Now it’d be impossible to simulate ~1e10 electrons (now: 3h per 100k particles on one machine)

- can distribute jobs between the institutions (DESY, UCL, WIS,…) but need a setup which can work out of the box.

- can launch jobs by early next week

There are minutes attached to this event. Show them.
    • 10:00 10:10
      Intro 10m
      Speakers: Dr Anthony Hartin (DESY), Dr Gianluca Sarri (Queen's University Belfast), Dr Noam Tal Hod (Weizmann Institute of Science)
      Slides
    • 10:10 10:25
      Signal simulation status 15m
      Speaker: Dr Anthony Hartin (DESY)
      Slides
    • 10:25 10:40
      GEANT4 simulation status 15m
      Speaker: Oleksandr Borysov (DESY)
      Slides
    • 10:40 10:55
      Rates at the fwd spectrometer 15m
      Speaker: Mr Kyle Fleck (QUB)
      Slides