Summary notes of the LCU meeting on 12/02/2008
Present: IA, MA, RB, HB, RC, SF, MG, WH, PL, AM, JN, TR, FR, FS, RT, TW, SW, SY, FZ
Report from meetings
Bunch filling schemes for early running -> WH (pdf)
WH recalled that this is not a new subject and that there is in fact a lot of flexibility, in particular for schemes with a small number of bunches. The minimum spacing considered is 10 rf wavelength or one slot, corresponding to 25 ns or 7.5 meter.
There have been recently discussion with the physics co-ordinator aiming at defining the optimum schemes for early operation with few bunches. There is symmetry between IR1 and IR5, which always see the same bunches colliding and request maximum luminosity.
For IR2 and IR8, several alternatives were presented. IP8 is shifted compared to the LEP-DELPHI IP8 by 3/2 slots or about 11m. LHCb requests
a luminosity of 2-5×1032 cm-2 s-1
, while Alice prefers very low luminosities around 1029 for the
proton runs.
Early operation with 43 bunches can be arranged such that only 4 of these would collide in IP2.
The recent discussions also renewed the interest in operation with 50 ns spacing and 1404 bunches. Potential advantages are fewer long range interactions and the possibility to provide over 1000
bunch collisions per turn in IR1,5,8 and only 2 in IR2. An important advantage
of these new schemes is the intrinsic reduction of luminosity in IP2 without the
need to un-squeeze or separate the bunches at the collision point. It is also
clear that symmetric displacements of bunches in both beams should be preferred
with respect to shifts in one beam, only.
This subject will also be discussed in the LHCCWG / LTC.
IP Coupling/Dispersion Knob by using Sextupole Bumps on LHC optics -> AM (pdf)
Akio Morita described coupling and dispersion knobs used successfully in KEKB and discussed possible applications for the LHC. Simulations at KEK are based on the SAD program. Using orbit bumps and sextupoles, it is in principle possible to correct both dispersion and coupling.
For the LHC, skew quadrupoles will be used for global coupling corrections.
Bumps in sextupoles are proposed to tune dispersion (no means of correcting
vertical dispersion from the crossing schemes are available in the LHC). The
main issue is the amplitude of the bumps, which make it difficult to use them
due to the related aperture reduction. A similar results was obtained when
closed orbit bump were studies to compensate the dispersion mismatch at
injection (in that case the plane concerned was the horizontal one). At that it
was found that tuning capability was very small, i.e., to generate a sizable
dispersion rather large bumps should be introduced.
AOB
None.
Last update: 14-Februar-08
MG & HB
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