Simulating the RFOFO Ring with Geant Amit Klier University of California, Riverside Muon Collaboration Meeting Riverside, January 2004.

Slides:



Advertisements
Similar presentations
PID Detector Size & Acceptance Chris Rogers Analysis PC
Advertisements

1 Neutrino Factory Front End (IDS) -Chicane & Absorber David Neuffer C. Rogers, P. Snopok, C. Yoshikawa, … January 31, 2012.
Bunched-Beam Phase Rotation David Neuffer Fermilab.
Emittance definition and MICE staging U. Bravar Univ. of Oxford 1 Apr Topics: a) Figure of merit for MICE b) Performance of MICE stages.
FIGURE OF MERIT FOR MUON IONIZATION COOLING Ulisse Bravar University of Oxford 28 July 2004.
FODO-based Quadrupole Cooling Channel M. Berz, D. Errede, C. Johnstone, K. Makino, Dave Neuffer, Andy Van Ginneken.
Bunched-Beam Phase Rotation- Variation and 0ptimization David Neuffer, A. Poklonskiy Fermilab.
1 Emittance Calculation Progress and Plans Chris Rogers MICE CM 24 September 2005.
V.Daniel Elvira Status Report on Cooling Simulations using GEANT4 Motivation: Explore a realistic design of a 44/88 MHz based cooling channel for a -factory.
PID Detector Size & Acceptance Chris Rogers Analysis PC
M.apollonioCM17 -CERN- (22/2 - 25/2 2007)1 Single Particle Amplitude M. Apollonio – University of Oxford.
MICE analysis meeting - (21/09/2006) 1 Transmittance, scraping and maximum radii for MICE STEPVI M. Apollonio – University of Oxford.
V.Daniel Elvira Status Report on Cooling Simulations using GEANT4 Motivation: Explore a realistic design of a 44/88 MHz based cooling channel for a -factory.
Chris Rogers, MICE CM16 Wednesday Plenary Progress in Cooling Channel Simulation.
NF Front End Meeting, April 27, 2010 Initial Cooling with HFOFO Snake Y. Alexahin, FNAL APC.
1 PID Detector Size & Acceptance Chris Rogers Analysis PC
Operated by Brookhaven Science Associates for the U.S. Department of Energy Optimized Parameters for a Mercury Jet Target X. Ding, D. Cline, UCLA, Los.
Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.
Chris Rogers, Analysis Parallel, MICE CM17 Progress in Cooling Channel Simulation.
1 Chris Rogers MICE Collaboration Meeting 11th Feb 2005 Tracking and Cooling performance of G4MICE.
M.apollonio/j.cobbMICE UK meeting- RAL - (9/1/2007) 1 Single Particle Amplitude M. Apollonio – University of Oxford.
FFAG Concepts and Studies David Neuffer Fermilab.
June 21, 2005 S. Kahn -- Small Muon Cooling Ring1 Small Muon Ring for a Cooling Demonstration Steve Kahn For S. Kahn, H. Kirk, A. Garren, F. Mills and.
Emittance measurement: ID muons with time-of-flight Measure x,y and t at TOF0, TOF1 Use momentum-dependent transfer matrices to map  path Assume straight.
Muons within Acceleration Acceptance Cuts at End of Transverse Cooling Channel TOWARDS A GLOBAL OPTIMIZATION OF THE MUON ACCELERATOR FRONT END H. K. Sayed,
MICE pencil beam raster scan simulation study Andreas Jansson.
FFAG-ERIT R&D 06/11/06 Kota Okabe (Kyoto Univ.) for FFAG-DDS group.
FFAG-ERIT Accelerator (NEDO project) 17/04/07 Kota Okabe (Fukui Univ.) for FFAG-DDS group.
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, N.Kazarinov.
Tracking Studies of Phase Rotation Using a Scaling FFAG Ajit Kurup FFAG07 12 th – 17 th April 2007.
2002/7/02 College, London Muon Phase Rotation at PRISM FFAG Akira SATO Osaka University.
2002/7/04 College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University.
Quantitative Optimisation Studies of the Muon Front-End for a Neutrino Factory S. J. Brooks, RAL, Chilton, Oxfordshire, U.K. Tracking Code Non-linearised.
Bunched-Beam Phase Rotation for a Neutrino Factory David Neuffer Fermilab.
Bunched-Beam Phase Rotation and FFAG -Factory Injection David Neuffer Fermilab.
1 EPIC SIMULATIONS V.S. Morozov, Y.S. Derbenev Thomas Jefferson National Accelerator Facility A. Afanasev Hampton University R.P. Johnson Muons, Inc. Operated.
Muon cooling with Li lenses and high field solenoids V. Balbekov, MAP Winter Meeting 02/28-03/04, 2011 OUTLINE  Introduction: why the combination of Li.
V.Balbekov, 12/09/08 HCC simulation with wedge absorbers V. Balbekov, Fermilab Muon Collider Design Workshop December 8-12, 2008 JeffersonLab, Newport.
1 Advances for a Solenoid/Dipole 6D Cooling Ring X. Ding, UCLA Muon Accelerator Program-Winter Meeting Jefferson Lab 3/1/11.
Harold G. Kirk Brookhaven National Laboratory Progress in Quad Ring Coolers Ring Cooler Workshop UCLA March 7-8, 2002.
S. Kahn 5 June 2003NuFact03 Tetra Cooling RingPage 1 Tetra Cooling Ring Steve Kahn For V. Balbekov, R. Fernow, S. Kahn, R. Raja, Z. Usubov.
RAL Muon Beam Line Properties. ISIS 70 MeV H- injection Ring accelerates up to 800 MeV in about 10 ms 50 Hz cycle - Dual Harmonic System ~ 2 x 1.5 MHz;
MICE at STFC-RAL The International Muon Ionization Cooling Experiment -- Design, engineer and build a section of cooling channel capable of giving the.
FRONTEND DESIGN & OPTIMIZATION STUDIES HISHAM KAMAL SAYED BROOKHAVEN NATIONAL LABORATORY June 26, 2014 Collaboration: J. S. Berg - X. Ding - V.B. Graves.
Marco apollonio/J.CobbMICE coll. meeting 16- RAL - (10/10/2006) 1 Transmittance, scraping and maximum radii for MICE STEPVI M. Apollonio – University of.
Stephen Brooks / RAL / May 2004  Optimisation of the RAL Muon Front End Design.
1 PID Detector Size & Acceptance Chris Rogers Analysis PC
1 EMMA Tracking Studies Shinji Machida ASTeC/CCLRC/RAL 4 January, ffag/machida_ ppt & pdf.
2 July 2002Realistic Fields for a Ring Cooler Magnet System -- S.Kahn Page 1 Realistic Fields for a Ring Cooler Steve Kahn 2 July 2002 NuFact’02 Meeting.
Context of the Neutrino Factory Neutrino factory (2018) –4MW proton driver –p +   +   +  e + e  Linear e + e − collider (2014/5) –Leptons at 0.4.
Harold G. Kirk Brookhaven National Laboratory Quad/dipole Ring Coolers * Nufact’03 Columbia University June 6, 2003 * With contributions from A. Garren.
Nufact02, London, July 1-6, 2002K.Hanke Muon Phase Rotation and Cooling: Simulation Work at CERN new 88 MHz front-end update on cooling experiment simulations.
28-Aug-2003 Steve Kahn Standardized MucGeant I/O Front End to MucGeant Standardize the input files for MucGeant: –The input should be in the ICOOL for003/4.
Bunched-Beam Phase Rotation - Ring Coolers? - FFAGs? David Neuffer Fermilab.
Adiabatic buncher and (  ) Rotator Exploration & Optimization David Neuffer(FNAL), Alexey Poklonskiy (FNAL, MSU, SPSU)
1 Tracking study of muon acceleration with FFAGs S. Machida RAL/ASTeC 6 December, ffag/machida_ ppt.
1 Front End – gas-filled cavities David Neuffer May 19, 2015.
MICE Step IV Lattice Design Based on Genetic Algorithm Optimizations Ao Liu on behalf of the MICE collaboration Fermilab Ao Liu on behalf of the MICE collaboration.
1 Front End – present status David Neuffer December 4, 2014.
August 8, 2007 AAC'07 K. Yonehara 1 Cooling simulations for Muon Collider and 6DMANX Katsuya Yonehara Fermilab APC MCTF.
Muons, Inc. Feb Yonehara-AAC AAC Meeting Design of the MANX experiment Katsuya Yonehara Fermilab APC February 4, 2009.
Research and development toward a future Muon Collider Katsuya Yonehara Accelerator Physics Center, Fermilab On behalf of Muon Accelerator Program Draft.
1 6D Cooling Chris Rogers, ASTeC-STFC Topical Workshop 23 Oct 2007.
+-- Collider Front end- Balbekov version
MICE Step IV Lattice Design Based on Genetic Algorithm Optimizations
Parametric Resonance Ionization Cooling of Muons
M. Migliorati, C. Vaccarezza INFN - LNF
Using MICE to verify simulation codes?
Design of the MANX experiment
Geant Simulation of Muon Cooling Rings
Presentation transcript:

Simulating the RFOFO Ring with Geant Amit Klier University of California, Riverside Muon Collaboration Meeting Riverside, January 2004

Jan. 28, 2004Simulating RFOFO with GEANT 2 OUTLINE Basics - geometry and magnetic field Setting the parameters Reference orbit and the clock Single particles in the ring “ Cooling ” with an Ideal Absorber Acceptance and RF parameters Cooling of a beam With/without muon decay Comparing to other results

Jan. 28, 2004Simulating RFOFO with GEANT 3 Basic ingredients Simulation software data-driven Geant v3.21 (R. Raja) Geometry from B. Palmer, R. Fernow, V. Balbekov (MC-Note 264) Realistic magnetic field maps – external (R. Godang, S. Bracker: MC-Note 271)

Jan. 28, 2004Simulating RFOFO with GEANT 4 The ring geometry 33 m circumference 12 cells (2.75m): LH 2 wedge absorber – opening angle 110°, pointing upwards no windows 6 RF cavities – cm long, acceptance radius 25 cm 2 tilted solenoids inner/outer r = 77/88 cm tilt angle ±3° (only for display here)

Jan. 28, 2004Simulating RFOFO with GEANT 5 A view of a single cell

Jan. 28, 2004Simulating RFOFO with GEANT 6 3-D view of the RFOFO ring

Jan. 28, 2004Simulating RFOFO with GEANT 7 Setting the ring parameters The reference orbit Run without RF acceleration or absorbers Find a closed orbit (periodic in cells) Start at the middle of the wedge absorber – symmetry plane  One of 2 point in which p T vanishes (with no RF and absorber)

Jan. 28, 2004Simulating RFOFO with GEANT 8 With only magnetic field turned on The ring shows stability for initial p z ’ s in the range ~165 – 260 MeV/c The strategy: Find closed orbits for various initial P z x and y dependence  dispersion functions Set the clock – determine RF cavity entry times (the clock ’ s rotation frequency should be an integer  RF frequency)  Then RF cavities and absorbers can be turned on

Jan. 28, 2004Simulating RFOFO with GEANT 9 Closed orbits in a single cell Solid line – the reference orbit 270 MeV 250 MeV 227 MeV E = 200 MeV 200 MeV 227 MeV 250 MeV E = 270 MeV

Jan. 28, 2004Simulating RFOFO with GEANT 10 Dispersion functions at the center of the wedge

Jan. 28, 2004Simulating RFOFO with GEANT 11 Setting the clock RF frequency: f = MHz Set the entry times of the RF cavities p z = MeV/c (E  227 MeV)  the 25 th harmonic (actually, ~ MHz was the closest I could get)

Jan. 28, 2004Simulating RFOFO with GEANT 12 Turn on RF and LH 2 absorber Use an “ ideal ” absorber no multiple scattering, straggling Simplified RF acceleration field: In the cavity volume (cavity coordinates): E x =E y =0, E z =G · sin[  (t-t ent )+  ent ] (G=13.5 MV/m,  ent =-13° for the single-particle simulation) Inject muons at 5 initial points in each phase space coordinate central value, ±1,2  (Gaussian beam from MC-264)

Jan. 28, 2004Simulating RFOFO with GEANT 13 Perfect absorber – perfect cooling

Jan. 28, 2004Simulating RFOFO with GEANT 14

Jan. 28, 2004Simulating RFOFO with GEANT 15 Introducing “ realistic ” absorbers.. Turn on all processes (except muon decay) Looks like a big mess! But only a few particles are shown here! High statistics are needed to simulate cooling – a beam

Jan. 28, 2004Simulating RFOFO with GEANT 16 The beam Gaussian distributions (from MC-264):  x =  y = 4.25 cm  p x =  p y = 30 MeV/c  z = 7 cm (  cT = 8 cm in the Note)  p z = 22.5 MeV/c (   E = 20 MeV in the Note) To find the best acceptance: 400 muons, no decay, ideal absorber Count the number of muons after 6 ring turns ( “ stable ” ) For cooling simulation: 1600 muons, w/ & w/o decay, “ realistic ” absorber

Jan. 28, 2004Simulating RFOFO with GEANT 17 Finding the best acceptance using ideal absorber  ent ~ -2 o ~14 MV/m

Jan. 28, 2004Simulating RFOFO with GEANT 18 Simulating beam cooling with a “ realistic ” absorber A Gaussian beam of 1600 muons was generated with all physics processes on The same beam without muon decay – performance cross-check Emittance calculation (similar to ECALC9) Slightly different cuts; No transverse amplitude – momentum correlation (  L calculated only from E-t covariance matrix)

Jan. 28, 2004Simulating RFOFO with GEANT 19 The beam in 15 turns (no muon decay)

Jan. 28, 2004Simulating RFOFO with GEANT 20 Cooling performance: transmission, 2-D emittances

Jan. 28, 2004Simulating RFOFO with GEANT 21 Cooling performance: 6-D emittance, merit factor

Jan. 28, 2004Simulating RFOFO with GEANT 22 Performance after 10 turns – comparison to other simulations ICOOL (MC-239) Balbekov (MC-264) Geant (current) Transmission, no decay (%) Transmission with decay (%) Merit factor5055~40 Possible reason for lower merit factor: smaller initial beam (longitudinal)

Jan. 28, 2004Simulating RFOFO with GEANT 23 Why do we see the jump in longitudinal emittance? (first few turns)

Jan. 28, 2004Simulating RFOFO with GEANT 24 Conclusions Geant performance shows good agreement with other simulations (ICOOL, Balbekov) lower merit factor maybe due to different initial beam To be done: Use “ standard ” ECALC9 to calculate emittance More realistic ring – absorber windows, injection, etc. Geant-Simulate other cooling rings (e.g. Kirk-Garren) – with R. Godang, S. Kahn, EE working group MC-Note in preparation, to be published soon …