1 STEP III MICE Analysis Workshop RAL – 4/9/2008 m. apollonio, IC.

Slides:



Advertisements
Similar presentations
Space-Charge Instabilities in Linacs. What limits the beam current in ion linacs? This is a very important topics for anyone designing linacs. For example,
Advertisements

1 Acceptance & Scraping Chris Rogers Analysis PC
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.
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.
9/10 solenoid case – a snapshot with Transport m. apollonio IC purpose: understand how the beam envelope changes when operating with a reduced solenoid.
MICE Collaboration meeting May 31 st – June 3 rd 2009 RAL Tim Hayler, Andy Lintern DRAFT SEQUENCE OF EVENTS STEPS
1 Tracker Resolution Malcolm Ellis MICE Analysis Forum Meeting 15 th September 2005.
Cooling channel issues U. Bravar Univ. of Oxford 31-Mar-2004.
SPACE CHARGE EFFECTS IN PHOTO-INJECTORS Massimo Ferrario INFN-LNF Madison, June 28 - July 2.
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.
MICE analysis meeting - (4/5/2006) 1 some reflections on scraping, PID sizes and Transmittance M. Apollonio – University of Oxford.
Alain Blondel MICE: Constraints on the solenoids 2.Field Homogeneity: or ? this will be dictated by the detector requirements. TPG will be.
OPTICS UPDATE Ulisse Bravar University of Oxford 3 August 2004.
1 PID Detectors & Emittance Resolution Chris Rogers Rutherford Appleton Laboratory MICE CM17.
M.apollonioCM17 -CERN- (22/2 - 25/2 2007)1 Single Particle Amplitude M. Apollonio – University of Oxford.
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.
MICE analysis meeting - (26/3/2006) 1 Update on MICE – step III M. Apollonio – University of Oxford.
1 OPTICS OF STAGE III Ulisse Bravar University of Oxford 6 October 2004.
1 Losses in the Cooling Channel Malcolm Ellis PID Meeting 1 st March 2005.
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.
Emittance Calculation Chris Rogers, Imperial College/RAL Septemebr
1. Optical matching in MICE Ulisse Bravar University of Oxford 2 June 2004 Constraints Software MICE proposal mismatch MICE Note 49 (September 2004, Bob.
24 Nov 2009PC Analysis PC Schedule 2009 Tuesdays fortnightly Proposed dates: 13 October  27 October  CM25 4 – 6 November  24 November 8 December.
M.apollonioImperial College - London1 M. Apollonio University of Oxford the MICE diffuser: issues and operation MICE beamline review Nov. 16 th 2007 Imperial.
1 Emittance Calculation Progress and Plans Chris Rogers Analysis PC 18 August 2005.
MICE analysis meeting - (18/5/2006) 1 STEPIII: ICOOL vs G4MICE M. Apollonio – University of Oxford.
1 Effect of staging on module connection and support arrangement Yury Ivanyushenkov RAL.
M.apollonioam M. Apollonio University of Oxford update on STEP III.
RF background simulations MICE collaboration meeting Fermilab Rikard Sandström.
04/01/2006MICE Analysis Meeting1 MICE phase III M. Apollonio, J. Cobb (Univ. of Oxford)
1 Emittance Exchange in MICE ● How would one measure emittance exchange? ● Build a cell of a cooling ring? ● Expensive ● Manpower-consuming ● Nice to demonstrate.
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.
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.
Analysis of MICE Chris Rogers 1 Imperial College/RAL Thursday 28 October, With thanks to John Cobb.
MICE magnetic measurements Sequence of events and MICE hall movements Alain Blondel – 10-April 2012 revision from 13 December 2012.
Emittance measurement: ID muons with time-of-flight Measure x,y and t at TOF0, TOF1 Use momentum-dependent transfer matrices iteratively to determine trace.
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.
MICE pencil beam raster scan simulation study Andreas Jansson.
M.apollonioCM17 -CERN- (22/2-25/2/2007)1 M. Apollonio – University of Oxford sizes for PID & shields.
Goals and Status of MICE The International Muon Ionization Cooling Experiment J.S. Graulich.
The status of the construction of MICE Step IV K. Long, on behalf of the MICE collaboration.
Some Thoughts on Magnetic Measurements for MICE Michael A. Green Lawrence Berkeley Laboratory Berkeley CA 94720, USA.
MICE magnetic measurements: AFC considerations Alain Blondel see a previous discussion for reference in CM35 (Feb 2013 slides by V. Blackmore, A. Blondel.
1 Forces Yury Ivanyushenkov RAL. 2 Goal: find maximal (static and dynamical) possible forces in MICE magnetic system. Method: calculation of axial magnetic.
Harold G. Kirk Brookhaven National Laboratory Progress in Quad Ring Coolers Ring Cooler Workshop UCLA March 7-8, 2002.
Marco apollonio/J.CobbMICE coll. meeting 16- RAL - (10/10/2006) 1 Transmittance, scraping and maximum radii for MICE STEPVI M. Apollonio – University of.
1 Search for Worst-Case Forces MICE Video Conference, September 8, 2004 Yury Ivanyushenkov Applied Science Division, Engineering and Instrumentation Department,
MICE Detector Integration A. Bross Mice Video Meeting August 27, 2003.
17 Sept 2007 Analysis PC 18 Sept Analysis PC Schedule 2007 Tuesdays alternate weeks, 15:30 – 17:00 GMT, with ad hoc exceptions Tue 3 April Tue 17.
Measuring Multiple Scattering in Step IV Timothy Carlisle Oxford See MICE Note 374 for updated results.
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
MICE S TEP IV P HYSICS ‘D ELIVERABLES ’ V. Blackmore MAP 2014 Spring Meeting 30 th May, /15 AKA “What will we learn from Step IV?”
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.
MICE. Outline Experimental methods and goals Beam line Diagnostics – In HEP parlance – the detectors Magnet system 2MICE Optics Review January 14, 2016.
Marco apollonioAnalysis Meeting (9/12/2006)1 transmission vs amplitude with a finite size diffuser M. Apollonio – University of Oxford.
1May, IPPP- Imperial College, London1 NF activities at IC (part II) m. apollonio.
Step IV Physics Paper Readiness
MICE at Step IV without SSD
Beam-beam effects in eRHIC and MeRHIC
BEAM DISTRIBUTION FLATTENING TECHNIQUES
C. Rogers, ASTeC Intense Beams Group Rutherford Appleton Laboratory
Impact of Magnet Performance on the Physics Program of MICE
Beam-beam R&D for eRHIC Linac-Ring Option
The Detector System of the MICE Experiment
Presentation transcript:

1 STEP III MICE Analysis Workshop RAL – 4/9/2008 m. apollonio, IC

2 def: two tracker solenoids & no RFs & LiH absorber inserted in between a) STEP III was thought as an intermediate stage to calibrate the trackers, the main assumption being  upstream =  downstream b) a possibility is using STEPIII to show a first effect of cooling [MA, JC CM14, Osaka 2006] however first studies showed that assumption (a) is naïve and cooling in (b) is not exactly how you would expect

3  i =0.1 cm rad  i =0.2 cm rad  i =0.3 cm rad  i =0.6 cm rad  i =1.0 cm rad emittance growth in vacuum: NO ABSORBERS

4 Non Flip Mode Flip Mode +2.8 % +2.3 % in vacuum

5 how can it be? there is no reason to violate Liouville’s theorem (Hamiltonian System), however: a)little mismatch due to non-paraxial beams (at higher emittances) b)non-linear forces  phase space does not transform linearly

6 xx linear transformation NON-linear transformation effective EMITTANCE

7 phase space density for low SPA regions  much less sensitive to tails equilibrium vacuum growth subtracted emi. % variation