SPS collective effects Hannes, Gianni, Giovanni, Benoit, Yannis

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Presentation transcript:

SPS collective effects Hannes, Gianni, Giovanni, Benoit, Yannis Space charge Electron cloud TMCI longitudinal limitations  covered by Elena

Space charge Space charge is not a limitation for nominal and ultimate LHC parameters For LIU : 25 ns (2.2E11p/b at LHC injection with 2.5 mm.mrad) 50 ns (3.5E11 p/b at LHC injection with 3 mm.mrad) Note that the achievable density at SPS extraction is expected to strongly depend on the injected density

Electron cloud 25 ns, nominal intensity there is electron cloud in the SPS (pressure rise and instability with low vertical chromaticity) With typical chromaticity, acceptable beam quality 25 ns, high intensity (ultimate and LIU) baseline: coat large parts of SPS with aC in LS2 machine studies in 2012 to identify (1) current intensity limit without coating (2) possible intermediate solutions (coating only MBB chambers)

TMCI Nominal Q26 optics Threshold found at 1.6E11 p/b in Q26 with very low positive chromaticity and optimized settings to minimize damping mechanisms Above the threshold, need to increase chromaticity, leading to transverse emittance degradation  TMCI is a limitation for LIU in Q26 for both LHC25 and LHC50 New Q20 optics Threshold for Q20 not clearly found yet, despite very high intensities sent into the SPS (~5E11 p/b). However, many other effects can prevent the instability from appearing at such high intensities (e.g. space charge in combination with non linearities)  TMCI is not a limitation for LIU in Q20