MICE analysis meeting - (26/3/2006) 1 Update on MICE – step III M. Apollonio – University of Oxford.

Slides:



Advertisements
Similar presentations
1 Acceptance & Scraping Chris Rogers Analysis PC
Advertisements

PID Detector Size & Acceptance Chris Rogers Analysis PC
1 Simulation Status/Plans Malcolm Ellis Sci Fi Tracker Meeting Imperial College, 10 th September 2004.
1 Progress report on Calorimeter design comparison simulations MICE detector phone conference Rikard Sandström.
CM31: Multiple Scattering in GEANT4 Timothy Carlisle University of Oxford.
Emittance definition and MICE staging U. Bravar Univ. of Oxford 1 Apr Topics: a) Figure of merit for MICE b) Performance of MICE stages.
1 Angular Momentum from diffuser Beam picks up kinetic angular momentum (L kin ) when it sits in a field –Canonical angular momentum (L can ) is conserved.
“Amplitude Cooling” in Step III & IV Timothy Carlisle.
MICE analysis meeting - (01/06/2006) 1 few words on emittance growth in step III M. Apollonio – University of Oxford.
1 PID, emittance and cooling measurement Rikard Sandström University of Geneva MICE Analysis phone conference.
Changing the absorbers: how does it fit in the MICE experimental programme? Besides the requirement that the amount of multiple scattering material be.
MICE analysis meeting - (4/5/2006) 1 some reflections on scraping, PID sizes and Transmittance M. Apollonio – University of Oxford.
OPTICS UPDATE Ulisse Bravar University of Oxford 3 August 2004.
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.
1 Muon Yield Comparisons for Different ICOOL Versions and Lattices X. Ding Front End, Nov. 23, 2010.
MICE analysis meeting - (6/4/2006) 1 Update on MICE – step III 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.
1 G4MICE downstream distributions G4MICE plans Rikard Sandström Universite de Geneve MICE collaboration meeting 27/6-05.
1 Statistics Toy Monte Carlo David Forrest University of Glasgow.
Chris Rogers, MICE CM16 Wednesday Plenary Progress in Cooling Channel Simulation.
1 OPTICS OF STAGE III Ulisse Bravar University of Oxford 6 October 2004.
M.apollonioAM STEPIII – sizes and positioning m.apollonio, Oxford.
MICE CM - Fermilab, Chicago - (11/06/2006) 1 A (short) history of MICE – step III M. Apollonio – University of Oxford.
Beamline-to-MICE Matching Ulisse Bravar University of Oxford 2 August 2004 MICE performance with ideal Gaussian beam JUNE04 beam from ISIS beamline (Kevin.
1. Optical matching in MICE Ulisse Bravar University of Oxford 2 June 2004 Constraints Software MICE proposal mismatch MICE Note 49 (September 2004, Bob.
1 Downstream PID update - How cooling section affects TOF measurement Rikard Sandström PID phone conference
30 June 2004MICE VC1 MICE  functions Since last VC report: –New Mike Green configurations for decreased spacing between focus and matching coils of 400mm,
NF Front End Meeting, April 27, 2010 Initial Cooling with HFOFO Snake Y. Alexahin, FNAL APC.
M.apollonioImperial College - London1 M. Apollonio University of Oxford the MICE diffuser: issues and operation MICE beamline review Nov. 16 th 2007 Imperial.
Beam Parameter Study - preliminary findings Tim Carlisle.
MICE Experiments Introduction Introduction Disclaimers Disclaimers Assumptions Assumptions Baseline programme Baseline programme Full programme Full programme.
MICE analysis meeting - (18/5/2006) 1 STEPIII: ICOOL vs G4MICE M. Apollonio – University of Oxford.
M.apollonioam M. Apollonio University of Oxford update on STEP III.
Overview of Experiment and Parameter Choices presented by Giles Barr.
RF background simulations MICE collaboration meeting Fermilab Rikard Sandström.
04/01/2006MICE Analysis Meeting1 MICE phase III M. Apollonio, J. Cobb (Univ. of Oxford)
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.
M.apollonioam M. Apollonio reviving STEPIII S-III: shown 1 st time at CM14 leading idea: use solid absorber(s) and show cooling without mom. recovery.
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.
Diffuser Studies Chris Rogers, IC/RAL MICE VC 09 March 2005.
13 Nov 2007 Analysis PC 13 Nov Analysis PC Schedule 2007/ 08 Tuesdays alternate weeks, 16:30 – 18:00 GMT, with ad hoc exceptions 30 October  13.
1 STEP III MICE Analysis Workshop RAL – 4/9/2008 m. apollonio, IC.
Analysis of MICE Chris Rogers 1 Imperial College/RAL Thursday 28 October, With thanks to John Cobb.
Timothy Carlisle, Oxford CM 28. Step 3 Matching Step 3  Step 3 rematched for 830 mm spool piece  Calc. B(z) & BetaFn with the following:  Minimize.
1 Front End – present status David Neuffer March 31, 2015.
M.apollonioCM17 -CERN- (22/2-25/2/2007)1 M. Apollonio – University of Oxford sizes for PID & shields.
Results from Step I of MICE D Adey 2013 International Workshop on Neutrino Factories, Super-beams and Beta- beams Working Group 3 – Accelerator Topics.
Multiple Scattering (MSC) in Geant4 Timothy Carlisle Oxford.
1 Front End for MAP Neutrino Factory/Collider rf considerations David Neuffer May 29, 2014.
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.
1 Front End – present status David Neuffer March 17, 2015.
Marco apollonio/J.CobbMICE coll. meeting 16- RAL - (10/10/2006) 1 Transmittance, scraping and maximum radii for MICE STEPVI M. Apollonio – University of.
M.apollonioMICE UK- RAL- 2/5/20071 MICE beam diffuser M. Apollonio,P. Lau, W. Lau, J. Tacon, S. Yang – Univ. Oxford.
MCS: Multiple Coulomb Scattering Sophie Middleton.
Step IV Studies Timothy Carlisle Oxford. Intro. CM28 – Step III vs Step IV Cooling formula & G4MICE disagree on – Also observed in ICOOL (note #199 –
Re-tuning MICE June 1 st 2010 Tim Carlisle. Intro At the moment MICE coil currents optimized for: central Pz = 0 RF No LH2 want to rematch M1 & M2 in.
Measuring Multiple Scattering in Step IV Timothy Carlisle Oxford See MICE Note 374 for updated results.
2 nd Muon Collider Design workshop, JLab, Newport News VA December 8-12, 2008 Helical FOFO Snake Simulations Y. Alexahin (FNAL)
M. Ellis - MICE Collaboration Meeting - Wednesday 27th October Sci-Fi Tracker Performance Software Status –RF background simulation –Beam simulation.
Final Cooling Options For a High- Luminosity High-Energy Lepton Collider David Neuffer FNAL Don Summers, T. Hart, … U. Miss.
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.
(one of the) Request from MPB
CM Nov 2009 DOES MICE NEED STEP III ? Somewhat hard to understand MICE Schedule… –If the gods are (un)kind it’s possible that SS1, SS2 & FC1 are.
Marco apollonioAnalysis Meeting (9/12/2006)1 transmission vs amplitude with a finite size diffuser M. Apollonio – University of Oxford.
Step IV Physics Paper Readiness
MICE Step IV Lattice Design Based on Genetic Algorithm Optimizations
Presentation transcript:

MICE analysis meeting - (26/3/2006) 1 Update on MICE – step III M. Apollonio – University of Oxford

MICE analysis meeting - (26/3/2006) 2 Investigate emittance growth Optmize thickness for absorbers tested emittance growth for LiH (2 absorbers) with thinner absorbers

MICE analysis meeting - (26/3/2006) 3  parameters used in simulation  Pz=207 MeV/c with a spread of 10%  initial emittances ranging from 0.1 to 1.0 (cm rad)  generated muons per point (i.e. initial emittance)  lost muons: worse cases at high initial  (=1.0 cm rad)  4% (LiH, C, non flip mode)  3% (C, flip mode)

MICE analysis meeting - (26/3/2006) 4 Flip mode: 2 absorbers LiH, Li, Be, CH, C 2x7cm absorbers = 13% pz reduction 0.22, 0.26, 0.39, 0.4, 0.57 (cm rad)

MICE analysis meeting - (26/3/2006) 5 net d  /  after the absorbers current optimization schemes: evbeta+MINUIT ICOOL+MINUIT with 2 absorbers equilibrium asymptotic cooling

MICE analysis meeting - (26/3/2006) 6 Flip mode: 2 absorbers of LiH Variable thickness (2x3cm, 2x4cm, … ) 2x4 cm 2x3 cm

MICE analysis meeting - (26/3/2006) 7 Flip mode: 2 absorbers of LiH Variable thickness (… 2x5cm, 2x6cm ) 2x3 cm 2x5 cm

MICE analysis meeting - (26/3/2006) 8 Flip mode: 2 absorbers of LiH Variable thickness (2x3cm, 2x4cm, 2x5cm, 2x6cm) EMI=1.0 2x3cm2x4 cm

MICE analysis meeting - (26/3/2006) 9 Flip mode: 2 absorbers of LiH Variable thickness (2x3cm, 2x4cm, 2x5cm, 2x6cm) EMI=0.5 2x3cm2x4 cm

MICE analysis meeting - (26/3/2006) 10 2x7cm =-13% 2x6cm =-11% 2x5cm =-9.2% 2x4cm=-7.2% 2x3cm=-5.4% Summary Plot

MICE analysis meeting - (26/3/2006) 11 Summary tried to reduce the thickness of the absorbers confirmed the behaviour already shown at dp/p=-13% great discrepancy with the simple model (see slide 5) emittance re-growth in the central region Side communication  started working on the G4MICE for stepIII thanks to Chris for his modifications of the code  The stepIII channel is available but currents are to be changed to the values I found in ICOOL optimization  Work in progress

MICE analysis meeting - (26/3/2006) 12 (%)  (cm rad) new set of data: more points (see next slides) Non Flip Mode +2.8 % +2.3 % Flip Mode