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RIS citation export for THBP16: Emittance Growth From Electron Clouds Forming in the LHC Arc Quadrupoles

TY  - CONF
AU  - Paraschou, K.
AU  - Bartosik, H.
AU  - Deniau, L.
AU  - Iadarola, G.
AU  - Maclean, E.H.
AU  - Mether, L.
AU  - Papaphilippou, Y.
AU  - Pieloni, T.
AU  - Potdevin, J.M.B.
AU  - Rumolo, G.
AU  - Tomás García, R.
ED  - Cai, Yunhai
ED  - Nagaitsev, Sergei
ED  - Kim, Dong Eon
ED  - Marx, Michaela
ED  - Schaa, Volker R. W.
TI  - Emittance Growth From Electron Clouds Forming in the LHC Arc Quadrupoles
J2  - Proc. of HB2023, Geneva, Switzerland, 09-13 October 2023
CY  - Geneva, Switzerland
T2  - ICFA Advanced Beam Dynamics Workshop on High-Intensity and High-Brightness Hadron Beams
T3  - 68
LA  - english
AB  - Operation of the Large Hadron Collider with proton bunches spaced 25 ns apart favours the formation of electron clouds. In fact, a slow emittance growth is observed in proton bunches at injection energy (450 GeV), showing a bunch-by-bunch signature that is compatible with electron cloud effects. The study of these effects is particularly relevant in view of the planned HL-LHC upgrade, which relies on significantly increased beam intensity and brightness. Particle tracking simulations that take into account both electron cloud effects and the non-linear magnetic fields of the lattice suggest that the electron clouds forming in the arc quadrupoles are responsible for the observed degradation. In this work, the simulation results are studied to gain insight into the mechanism which drives the slow emittance growth. Finally, it is discussed how optimising the optics of the lattice can allow the mitigation of such effects.
PB  - JACoW Publishing
CP  - Geneva, Switzerland
SP  - 487
EP  - 490
KW  - simulation
KW  - emittance
KW  - resonance
KW  - optics
KW  - electron
DA  - 2024/04
PY  - 2024
SN  - 2673-5571
SN  - 978-3-95450-253-0
DO  - doi:10.18429/JACoW-HB2023-THBP16
UR  - https://jacow.org/hb2023/papers/thbp16.pdf
ER  -