Summary notes of the LCU meeting on 17/09/2013
Present: RA, FB, RB, HB, RdM, LD, OD, SF, MHF, MF, MG, JJ, ALat, LL, GR, BS, MS, RT, RV, FZ
Report from meetings
Optics aspect of PIC and US1 scenarios for HL-LHC -> MF (slides)
In addition to the full upgrade, which is referred to as US2, we were asked for the upcoming workshop RLIUP to also look at two reduced scenarios, namely:
PIC (performance improvement and consolidation) and US1 (upgrade scenario 1). The triplets in IP1 and IP5 will be replaced in any
of the three scenarios under consideration. A long discussion took place about
whether the three scenarios should be considered as part of a staged approach or
as independent alternatives...
Crab cavities are only included in the full upgrade scenario. Miriam looked at the round and flat beam optics at injection, pre-squeeze and squeezed, for these scenarios. Going to a larger triplet but not changing most of the straight section as considered for the PIC would lead to a situation in which the TAN would be the main aperture limit unless it is also modified.
The aperture could be optimized slightly just by centering beams in the TAN using the MCBX correctors. Modifying also the TAN and beam screen would be beneficial for the reduced upgrade scenarios.
Massimo suggested to always specify which emittance and crossing angles and tolerances were assumed for any discussion of available and required aperture in terms of n1.
HL-LHC TAN aperture with reduced tolerances -> RA (slides)
Reyes looked at the upgrade scenarios with flat and round beams assuming a new TAN with
RECTELLIPSE shaped geometry of 41mm/37mm RECTELLIPSE opening. As also observed in energy deposition studies by L. Esposito and F. Cerutti, the new TAN would be much less effective in absorbing the neutral particles generated in the collisions than the present TAN. Using the reduced tolerances presented by Roderik in the last meeting and both 2.5 and 3.5 murad normalized emittances, she calculated the apertures in terms of n1 for the new geometry and what would happen if the aperture would be reduced by 10, 20 or 30%. She finds that a 30% reduction would result in a TAN aperture which is tighter than the Q2. Flat beams (beta*=7.5 cm) are more restrictive than round beams (beta*=15 cm).
It is worth stressing that changing the emittance and using expected values is
not correct as not all components included in the aperture estimates scale with
emittance, e.g., the orbit contribution. Stefano suggests to present the views
of Helmut at the collimation WG and/or MPP for feedback. Massimo approves this
proposal.
Overall, the results show that the original specification of the
TAN aperture is optimal and there is no margin for reduction.
Stephane
proposes to check what would be the gain in the efficiency of the TAN in case it
would be located just next to the IP-side of the D2 separation dipole. Riccardo
replies that some new configurations are under consideration by the FLUKA team.
AOB
None
Last update: 23-September-2013
MG & HB
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