Dark current in TESLA linac - PowerPoint PPT Presentation

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Dark current in TESLA linac

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Field emitted particles are accelerated to hundreds of MeV ... Record energy deposition, assume all goes into 2K Helium, disregard generation of secondaries ... – PowerPoint PPT presentation

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Title: Dark current in TESLA linac


1
Dark current in TESLA linac
  • R. Brinkmann
  • TESLA collaboration meeting, Saclay, April 3, 2002

2
Outline of the problem
  • Field emitted particles are accelerated to
    hundreds of MeV before being kicked out by
    quadrupoles
  • Losses into 2K Helium can be much higher than
    indicated by measured Q value on cavity test
    stand
  • Generated secondary electrons (positrons) can be
    re-accelerated ? enhancement of losses, in worst
    case avalanche effect (ongoing study by N.
    Golubeva, V. Balandin)

3
Crude estimate of losses from simple simulation
  • Use phase space distribution of dark current at
    exit of 9-cell cavity from Stolzenburg thesis
  • Transport through downstream lattice (cavities
    and quads) until trajectory hits aperture limit
  • Record energy deposition, assume all goes into 2K
    Helium, disregard generation of secondaries

4
Lost particle energy and average power into 2K
along main linac (1st 50 GeV)
5
Consequence need quality control beyond
measuring Q0
Assume maximum tolerable heat load at 1020 of
RF losses into cavity walls ? dark current per
cavity must be kept below 50nA at TESLA design
gradient If Q0 reduction due to dark current beam
loading, 50nA corresponds to ?(1/Q)
1/(5?1011) This is probably not visible in Q vs.
g curves!
6
Preliminary results on simulation of dark current
losses including e.m. shower (Balandin/Golubeva)
Use EGS4 plus tracking code with e.m. fields in
cavities Realistic geometric setup with all
material, quads, etc. So far, at g20MV/m
additional heat load from re-accelerated
secondary charged particles seems to be small
(order of magnitude lt10 of primary loss), not
enough statistics and linac length simulated
yet Will continue to investigate limit on g from
avalanche effect
7
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8
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