Space Charge Study Group

Slides:



Advertisements
Similar presentations
Introducing LEP3 zero M. Koratzinos TLEP3 day, 9 January2013.
Advertisements

Benchmark of ACCSIM-ORBIT codes for space charge and e-lens compensation Beam’07, October 2007 Masamitsu AIBA, CERN Thank you to G. Arduini, C. Carli,
Longitudinal motion: The basic synchrotron equations. What is Transition ? RF systems. Motion of low & high energy particles. Acceleration. What are Adiabatic.
Space Charge meeting – CERN – 09/10/2014
E. Benedetto SC meeting 19/3/15 Update on the LIU curve emittance vs. intensity.
Introduction Status of SC simulations at CERN
GRD - Collimation Simulation with SIXTRACK - MIB WG - October 2005 LHC COLLIMATION SYSTEM STUDIES USING SIXTRACK Ralph Assmann, Stefano Redaelli, Guillaume.
Laslett self-field tune spread calculation with momentum dependence (Application to the PSB at 160 MeV) M. Martini.
PTC ½ day – Experience in PS2 and SPS H. Bartosik, Y. Papaphilippou.
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, N.Kazarinov.
First measurements of longitudinal impedance and single-bunch effects in LHC E. Shaposhnikova for BE/RF Thanks: P. Baudrenghien, A. Butterworth, T. Bohl,
H. Bartosik, K. Cornelis, A. Guerrero, B. Mikulek, G. Rumolo, Y. Papaphilippou, B. Salvant, E. Shaposhnikova June 16 th, 2011.
PS Booster Studies with High Intensity Beams Magdalena Kowalska supervised by Elena Benedetto Space Charge Collaboration Meeting May 2014.
Theoretical studies of IBS in the SPS F. Antoniou, H. Bartosik, T. Bohl, Y.Papaphilippou MSWG – LIU meeting, 1/10/2013.
Details of space charge calculations for J-PARC rings.
October 4-5, Electron Lens Beam Physics Overview Yun Luo for RHIC e-lens team October 4-5, 2010 Electron Lens.
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, A.Drozhdin, N.Kazarinov.
1 FFAG Role as Muon Accelerators Shinji Machida ASTeC/STFC/RAL 15 November, /machida/doc/othertalks/machida_ pdf/machida/doc/othertalks/machida_ pdf.
Elias Métral, LHC Beam Commissioning Working Group meeting, 08/06/2010 /191 SINGLE-BUNCH INSTABILITY STUDIES IN THE LHC AT 3.5 TeV/c Elias Métral, N. Mounet.
4 th Order Resonance at the PS R. WASEF, S. Gilardoni, S. Machida Acknowledgements: A. Huschauer, G. Sterbini SC meeting, 05/03/15.
Update on injection studies of LHC beams from Linac4 V. Forte (BE/ABP-HSC) Acknowledgements: J. Abelleira, C. Bracco, E. Benedetto, S. Hancock, M. Kowalska.
1 EMMA Tracking Studies Shinji Machida ASTeC/CCLRC/RAL 4 January, ffag/machida_ ppt & pdf.
H. Bartosik, Y. Papaphilippou. PS2 meant as potential replacement of existing PS PS2 main characteristics given by LHC requirements – Circumference defined.
Elias Métral, SPSU Study Group and Task Force on SPS Upgrade meeting, 25/03/2010 /311 TMCI Intensity Threshold for LHC Bunch(es) in the SPS u Executive.
News on TMCI in the SPS: Injecting high intensity bunches Benoit for the MD team: T. Bohl, K. Cornelis, H. Damerau, W. Hofle, E. Metral, G. Rumolo, B.
Elias Métral, LHC Beam Commissioning Working Group meeting, 30/11/2010 /241 PRELIMINARY FINDINGS FROM INSTABILITY MEASUREMENTS DURING THE 75ns AND 50ns.
Tunes modulation in a space charge dominated beam: The particles behavior in the “necktie” Space charge meeting – CERN - 21/11/2013 Vincenzo Forte Thanks.
Beam Physics Issue in BEPCII Commisionning Xu Gang Accelerator physics group.
Space charge studies at the CERN PS A. Huschauer, Raymond Wasef H. Damerau, S. Gilardoni, S.Hancock, D. Schoerling, R. Steerenberg Acknowledgements: All.
Beam-beam Simulation at eRHIC Yue Hao Collider-Accelerator Department Brookhaven National Laboratory July 29, 2010 EIC Meeting at The Catholic University.
Pushing the space charge limit in the CERN LHC injectors H. Bartosik for the CERN space charge team with contributions from S. Gilardoni, A. Huschauer,
Lecture 4 Longitudinal Dynamics I Professor Emmanuel Tsesmelis Directorate Office, CERN Department of Physics, University of Oxford ACAS School for Accelerator.
MTE commissioning status S. Gilardoni, BE/ABP With C. Hernalsteens and M. Giovannozzi.
CLIC Frequency Multiplication System aka Combiner Rings Piotr Skowronski Caterina Biscari Javier Barranco 21 Oct IWLC 2010.
Toward an Improved Model of the Fermilab Booster Synchrotron A. Drozhdin, J.-F. Ostiguy and W. Chou Beam Physics Department Introduction The Booster is.
LIU Day 2014 – M.Bodendorfer - LEIR model. LEIR model A plan for understanding/upgrading the LEIR performance limitations M.Bodendorfer BE/ABP & LEIR.
First evaluation of Dynamic Aperture at injection for FCC-hh
Weiming Guo Accelerator Physics Group / ASD Advanced Photon Source
LIU-PS Beam Dynamics Working Group Introduction and objectives
Parameters of ejected beam
ICE SECTION The coolest place to be! Elias Métral
Transverse Damping Requirements
People who attended the meeting:
CERN Space Charge Studies 2012/2013
Cryo Problem MD Planning Tue (1.11.) C B Day Time MD MP Tue 01:00
CERN Space Charge Studies 2012/2013
Space charge studies at the SPS
Multi-Turn Extraction studies and PTC
Beam-beam effects in eRHIC and MeRHIC
Summary of the dedicated MD on July 4th 50ns in SPS with nominal and low γt optics – transverse aspects T. Argyropoulos, H. Bartosik, T. Bohl, A. Burov,
Longitudinal beam parameters and stability
Impact of remanent fields on SPS chromaticity
Jeffrey Eldred, Sasha Valishev
Multiturn extraction for PS2
Summary of Space-Charge Measurements, 2011
SC Overview 2013 White & Rouge The Codes in Comparison The Noise Issue
R. Bartolini Diamond Light Source Ltd
E. Métral, G. Rumolo, R. Tomás (CERN Switzerland), B
Update on PTC/ORBIT space charge studies in the PSB
Beam-Beam Interaction in Linac-Ring Colliders
Preliminary results of the PTC/ORBIT convergence studies in the PSB
LHC impedance: Comparison between phase 1 and IR3MBC – follow-up
News on TMCI in the SPS: Injecting high intensity bunches
A Design Study of a Compressor ring for
Beam dynamics requirements after LS2
SPS collective effects Hannes, Gianni, Giovanni, Benoit, Yannis
Simulation of Multiturn Injection into SIS-18
PSB magnetic cycle 900 ms MeV to 2 GeV
Another Immortal Fill….
Presentation transcript:

Space Charge Study Group Mandate Webpage Kick-off Meetings concerning PTCORBIT First impressions about PTCORBIT (PS, SPS)

Mandate Revisiting the space charge limits for PSB, PS & SPS in the context of the LHC Injection Upgrade (LIU) which is part of the High Luminosity project of the LHC (HL-LHC). This mandate might be reformulated as: "Finding the limits of the machine performance of the 3 machines due to space charge in presence of a full nonlinear model of these machines.“ ==> PTCORBIT? This task will require reviewing the theory with the help of space charge experts around the world. Equally relevant will be to compare the theoretical predictions with machine experiments.

Webpage Web address: cern.ch/frs/Source/space_charge Mandate Core Team and collaborators Literature Meetings In fact we have had a kick off meeting on 13th of May when Etienne & Sasha have been discussing their plans for the advancement of PTCORBIT. Christian and Elias have introduced the PSB and PS/SPS respectively in terms of space charge issues. And on the 30th of May Sasha gave a presentation about what has been achieved during this period.

Do we need PTCORBIT for our space charge Studies? My personal View… I have asked the following questions to the PSB, PS & SPS collaborators: A) Do you consider PTCORBIT relevant for the analysis of your machine? B) I know that for the PSB the demands on the features of PTCORBIT are most relevant and it seems that there is still a need for more development that we should ask Etienne for, if we decide to go for PTCORBIT. Personally, I think we should continue this development even if it is not easy to communicate with Etienne nor with Sasha. Etienne is properly the one to fix the remaining problems with PTCORBIT. C) My general feeling has been that one might need a closer look at the optics models of all 3 machines. Please excuse me, since I am coming from the LHC and we had the luxury to measure everything and have very sophisticated models. This will be difficult to do for these reliable but old machines nevertheless we should make our best effort to come up with the best we can know about those machines. Of course, we need sufficient manpower to do so! Do you agree with this analysis? D) Most exciting is the fact that apparently Hannes has found issues with the results of his space charge calculations in ORBIT itself. It would be great if Hannes could elaborate on this a little bit. After all, the PTC part is only single particle part to serve ORBIT.

PTC-ORBIT @ PS (Simone) Needs: Simulate eventual emittance blow-up of high-intensity LHC beams (for PS upgrade or not…) Help in determining the maximum acceptable Laslett tune spread, i.e., maximum intensity per bunch and/or minimum emittance Identify, if possible, an eventual cure (resonance compensation, change of working point?) Understand continuous losses observed during the injection process of the high intensity non-LHC beams

Code status for PS PTC-Orbit running for single particle case able to reproduce the collapsing of the injection bump with time-varying fields Tune and chromaticity correct as in the standard PTC standalone simulation Space charge simulation Only one run done so far Technically the code works but the physical parameters have to be optimized Missing: Lattice optimization to speed-up the simulation

Space charge simulations for SPS (Hannes) Motivation High intensity single bunches are produced since 2010 and injected into SPS A series of parallel MD sessions were dedicated to finding intensity limitations first with the nominal LHC optics and later with the new low γt optics (which should provide higher beam stability) Space charge tune spread of ΔQ~0.05 for nominal LHC beams (1.3e11 p/b, εn,xy=2.5 μm) Recent studies with up to 3.3e11 p/b and injected emittances of εn,xy~1.2-1.5 μm ==> significantly increased space charge tune spread (ΔQ~0.15 and higher) MD sessions are currently devoted to studies of emittance preservation for high intensity and working point optimization Working point optimization should/could be accompanied by space charge simulations with PTC-ORBIT Benefit/relevance of PTC-ORBIT for SPS space charge simulations Ultimate goal is to develop an “effective” machine model including the nonlinear (multipole) components of the machine (presently ongoing) and use this model for optimizing the working point in the presence of space charge tune shift For this purpose, PTC-ORBIT seems to be a suitable tool … TMCI threshold can be increased by increasing chromaticity or longitudinal emittance

Present status of PTC-ORBIT simulations for SPS Ideal lattice used for beginning Nominal and low γt optics – ideal lattice without field errors or misalignment Static magnetic fields and RF-voltage ==> very simple case, no acceleration Actual configuration of travelling wave RF-cavities is modeled (thanks to a modification in PTC) “2.5D” space charge model is used Around 2500 transverse space charge nodes around the lattice 1 longitudinal space charge kick 2.5D simulation is good approximation for “long bunches”: longitudinal size much bigger than transverse size (should be satisfied in SPS for LHC beams, full bunch length around 1.1m and transverse beam sizes on the order of a few cm) For now, beam pipe is not included in simulations Beam size much smaller than vacuum chamber ==> only small contribution to tune spread expected from wall effects Taking wall effects into account requires huge grid size compared to beam size and therefore long computation time Full 3D simulation would require vacuum chamber definition Again the problem of the small beam size compared to chamber size Unpractical due to the different kind of vacuum chambers in the SPS TMCI threshold can be increased by increasing chromaticity or longitudinal emittance

First simulations - Observations Simulated one set of parameters for both optics cases to gain confidence in code Intensity 2e11 p/b, emittances εn,xy~2.5 μm Phase space distributions matched to the corresponding optics functions and bucket sizes of the respective optics: Transverse: Gaussian cut at 3σ Longitudinal: parabolic with a cut around 2.2σ Nominal working points for the 2 optics (ξx,y=0.1) Low γt: (Qx, Qy)=(20.13, 20.18) Nominal optics: (Qx, Qy)=(26.13, 26.18) Simulation of 3000 turns (~60ms) Low γt opics: Minimal emittance blow-up (<1%) in both planes Nominal optics: Significant emittance growth in horizontal plane: initially exponential growth by a factor of 1.5 and beam halo formation!?? Minimal emittance blow-up (<1%) in vertical plane!! The exponential emittance growth disappears for increased RF-voltages (twice the RF-voltage, but still matched bucket by increasing longitudinal emittance) or by switching off longitudinal space charge calculations!!