 1 of 13 Stephen Brooks / RAL / March 2005 Muon Front Ends Providing High-Intensity, Low-Emittance Muon Beams for the Neutrino Factory and Muon Collider.

Slides:



Advertisements
Similar presentations
The US 5 Year Muon Acceleration R&D Program To Boldly Go… MICE Collaboration Meeting Harbin January, 2009.
Advertisements

U.S. Department of Energy Brookhaven Science Associates BNL’s Role in High Energy Physics Thomas B.W. Kirk Associate Director for High Energy and Nuclear.
Proton / Muon Bunch Numbers, Repetition Rate, RF and Kicker Systems and Inductive Wall Fields for the Rings of a Neutrino Factory G H Rees, RAL.
Study of the Luminosity of LHeC, a Lepton Proton Collider in the LHC Tunnel CERN June F. Willeke, DESY.
ISIS Related Issues for MICE Adam Dobbs Proton Accelerator Development Meeting, RAL 24 th March /03/20111A. Dobbs.
Target & Capture for PRISM Koji Yoshimura On behalf of PRISM Target Group Institute of Particle and Nuclear Science High Energy Accelerator Research Organization.
1 M. Popovic NFMC Collaboration Meeting IIT Muon (Pre)Acceleration for 8 GeV Proton Driver Linac Milorad Popovic FNAL 14-March.
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.
WIN'05, June A. Klier - Muon Collider Physics1 Physics at a Future Muon Collider Amit Klier University of California, Riverside WIN’05 – Delphi,
(ISS) Topics Studied at RAL G H Rees, RAL, UK. ISS Work Areas 1. Bunch train patterns for the acceleration and storage of μ ± beams. 2. A 50Hz, 1.2 MW,
FFAG Concepts and Studies David Neuffer Fermilab.
Poster reference: FR5PFP025 Extending the Energy Range of 50Hz Proton FFAGs S.J. Brooks RAL, Chilton, OX11 0QX, UK Magnetic.
Solid Target R&D Programme Colliding the proton beam with a dense target is currently the only known way to produce enough muons for the neutrino factory.
Stephen Brooks / RAL / November 2004  Optimisation of the RAL Muon Front End Design “Progress” from my last BENE talk (May’04) until now.
March 2011Particle and Nuclear Physics,1 Experimental tools accelerators particle interactions with matter detectors.
Future Accelerators at the energy frontier Peter Hansen february 2010 University of Copenhagen.
S.J. Brooks RAL, Chilton, OX11 0QX, UK Options for a Multi-GeV Ring Ramping field synchrotron provides fixed tunes and small.
3 GeV,1.2 MW, Booster for Proton Driver G H Rees, RAL.
Source Group Bethan Dorman Paul Morris Laura Carroll Anthony Green Miriam Dowle Christopher Beach Sazlin Abdul Ghani Nicholas Torr.
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.
The ISIS strong focusing synchrotron also at the Rutherford Appleton Laboratory. Note that ISIS occupies the same hall as NIMROD used to and re- uses some.
Target & Capture for PRISM Koji Yoshimura Institute of Particle and Nuclear Science High Energy Accelerator Research Organization (KEK)
Results from Step I of MICE D Adey 2013 International Workshop on Neutrino Factories, Super-beams and Beta- beams Working Group 3 – Accelerator Topics.
Neutrino Factory International Scoping Study Machine Group Chris Prior RAL/ASTeC and University of Oxford.
Ken Peach Particle Physics Department Neutrino Factory Overview.
Steve Geer OsC RAL 21 June, Muon Accelerator Program MUON COLLIDER & NEUTRINO FACTORY R&D in the U.S.  
Proton Driver: Status and Plans C.R. Prior ASTeC Intense Beams Group, Rutherford Appleton Laboratory.
Quantitative Optimisation Studies of the Muon Front-End for a Neutrino Factory S. J. Brooks, RAL, Chilton, Oxfordshire, U.K. Tracking Code Non-linearised.
, EUROnu Meeting, Strasbourg J. Pasternak Status and recent progress on muon IDS-FFAG J. Pasternak, Imperial College, London / RAL STFC Work.
Front-End Design Overview Diktys Stratakis Brookhaven National Laboratory February 19, 2014 D. Stratakis | DOE Review of MAP (FNAL, February 19-20, 2014)1.
J. Pozimski UKNF WP1 meeting 10 March 2010 UKNF WP1 milestone table status.
Secondary Particle Production and Capture for Muon Accelerator Applications S.J. Brooks, RAL, Oxfordshire, UK Abstract Intense pulsed.
Harold G. Kirk Brookhaven National Laboratory Target Considerations for Nufact and Superbeams ISS Meeting RAL April 26, 2006.
UKNF OsC RAL – 31 st January 2011 UKNF - Status, high lights, plans J. Pozimski.
Road Map of Future Neutrino Physics A personal view Ken Peach Round Table discussion at the 6 th NuFACT Workshop Osaka, Japan 26 th July – 1 st August.
1 of 12 Stephen Brooks JAI Advisory Board, February 2006  Neutrino Factory Muon Beam Production Studies.
Scaling VFFAG eRHIC Design Progress Report 4 July 15, 2013Stephen Brooks, eRHIC FFAG meeting1.
1 FFAG Role as Muon Accelerators Shinji Machida ASTeC/STFC/RAL 15 November, /machida/doc/othertalks/machida_ pdf/machida/doc/othertalks/machida_ pdf.
J. Pasternak First Ideas on the Design of the Beam Transport and the Final Focus for the NF Target J. Pasternak, Imperial College London / RAL STFC ,
Electron Model for a 3-10 GeV, NFFAG Proton Driver G H Rees, RAL.
MICE at STFC-RAL The International Muon Ionization Cooling Experiment -- Design, engineer and build a section of cooling channel capable of giving the.
John Womersley Welcome Director of Particle Physics, CCLRC International Scoping Study Meeting, RAL April 2006.
 Stephen Brooks / RAL / April 2004 Muon Front Ends Providing High-Intensity, Low-Emittance Muon Beams for the Neutrino Factory and Muon Collider.
NEUTRINO DETECTORS Cutting-Edge Accelerator Research for a Neutrino Factory and Other Applications Ajit Kurup for the FETS and UKNF Collaborations Cutting-Edge.
FFAG Studies at RAL G H Rees. FFAG Designs at RAL Hz, 4 MW, 3-10 GeV, Proton Driver (NFFAGI) Hz,1 MW, GeV, ISIS Upgrade (NFFAG) 3.
Stephen Brooks / RAL / May 2004  Optimisation of the RAL Muon Front End Design.
Muon Colliders: Progress and Plans Steve Geer 1.Introduction 2.Muon Collider Ingredients 3.Comaparison with Neutrino Factories 4.Cooling Channel Design.
Proton Source & Site Layout Keith Gollwitzer Accelerator Division Fermi National Accelerator Laboratory Muon Accelerator Program Review Fermilab, August.
IDS-NF Accelerator Baseline The Neutrino Factory [1, 2] based on the muon storage ring will be a precision tool to study the neutrino oscillations.It may.
Muon Collider R&D Plans & New Initiative 1.Introduction 2.Muon Collider Schematic 3.Conceptual Breakthrough 4.Ongoing R&D 5.Muon Collider Task Force 6.Muon.
Acceleration Overview J. Scott Berg Brookhaven National Laboratory January 8, 2014.
Progress in the construction of the MICE cooling channel and first measurements Adam Dobbs, EPS-HEP, 23 rd July 2011.
Frictional Cooling A.Caldwell MPI f. Physik, Munich FNAL
H. Haseroth Friday, August 31, 2001 MUG Meeting 1 Overview of the CERN Neutrino Factory Machine Studies H. Haseroth for the Neutrino Factory Working Group.
Context of the Neutrino Factory Neutrino factory (2018) –4MW proton driver –p +   +   +  e + e  Linear e + e − collider (2014/5) –Leptons at 0.4.
FFAG’ J. Pasternak, IC London/RAL Proton acceleration using FFAGs J. Pasternak, Imperial College, London / RAL.
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.
Bunched-Beam Phase Rotation - Ring Coolers? - FFAGs? David Neuffer Fermilab.
ICHEP Conference Amsterdam 31st International Conference on High Energy Physics 24  31 July 2002 Gail G. Hanson University of California, Riverside For.
MCS meeting 20/11/2015 S. Guiducci. Introduction Yesterday meeting has shown an interest in a large physics community to incremental development of muon.
Ionization Cooling for Muon Accelerators Prepared by Robert Ryne Presented by Jean-Pierre Delahaye MICE Optics Review Jan, 2016 RAL.
, UKNF Meetin, Imperial College J. Pasternak Status and Recent Progress in the Muon FFAG Designs J. Pasternak, Imperial College, London / RAL.
PSI, Zurich February 29 – March Session classification : Accelerator Concepts Tuesday, March 1, 2016 Summary Vyacheslav Yakovlev Fermilab, USA.
UK Neutrino Factory Conceptual Design
The Accelerator Complex from the International Design Study
Muon Front End Status Chris Rogers,
Accelerator R&D for Future Neutrino Projects
Meson Production Efficiencies
K. Tilley, ISIS, Rutherford Appleton Laboratory, UK Introduction
Presentation transcript:

 1 of 13 Stephen Brooks / RAL / March 2005 Muon Front Ends Providing High-Intensity, Low-Emittance Muon Beams for the Neutrino Factory and Muon Collider

 2 of 13 Stephen Brooks / RAL / March 2005 Contents Future Accelerator Projects Requiring Muon Front Ends –Neutrino Factory –Muon Collider Choice of Particle – why Muons? Front End Components and Options Context: National R&D Programme –UK Neutrino Factory (UKNF) group

 3 of 13 Stephen Brooks / RAL / March 2005 The Neutrino Factory Goal: To fire a focussed beam of neutrinos through the interior of the Earth –What’s the point? Constrains post-Standard Model physics –But why does this involve muons? Neutrinos appear only as decay products Decaying an intense, high-speed beam of muons produces collimated neutrinos

 4 of 13 Stephen Brooks / RAL / March 2005 The Neutrino Factory p +   +   +  e + e  Uses 4-5MW proton driver –Could be based on ISIS

 5 of 13 Stephen Brooks / RAL / March 2005 The Neutrino Factory “Front end” is the muon capture system

 6 of 13 Stephen Brooks / RAL / March 2005 The Muon Collider Goal: to push the energy frontier in the lepton sector after the linear collider p +   +,  −   +,  −  +-+- 3+3TeV Muon Collider Ring

 7 of 13 Stephen Brooks / RAL / March 2005 Why Collide Muons? ParticleProtonElectronMuon Mass938 MeV0.511 MeV106 MeV Synchrotron radiation limit (LEP-II RF) 28.5 TeV0.102 TeV5.55 TeV Machine issues B-field limit at 7 TeV (LHC) Linear 1 TeV collider more cost-effective Half-life of 2.2  s Physics problems Messy collisions None

 8 of 13 Stephen Brooks / RAL / March 2005 Design Challenges Must accelerate muons quickly, before they decay –Conventional synchrotrons cycle too slow –Once  is high, you have a little more time High emittance of pions from the target –Use an accelerator with a really big aperture? –Or try beam cooling (emittance reduction) –In reality, do some of both

 9 of 13 Stephen Brooks / RAL / March 2005 Muon Front End Components Targetry, produces pions (  ± ) Pion to muon decay channel –Uses a series of wide-bore solenoids “Phase rotation” systems –Outside scope of this talk Muon ionisation cooling (as in “MICE”) –Expensive components, re-use in cooling ring Muon acceleration (RLAs vs. FFAGs)

 10 of 13 Stephen Brooks / RAL / March 2005 The Decay Channel Has to deal with the “beam” coming from the pion source Evolution of pions from 2.2GeV proton beam on tantalum rod target

 11 of 13 Stephen Brooks / RAL / March 2005 The Decay Channel Has to deal with the “beam” coming from the pion source Pion half-life is 18ns or 12m at 200MeV –So make the decay channel about 30m long Grahame Rees designed an initial version –Used S/C solenoids to get a large aperture and high field (3T mostly, 20T around target) Needed a better tracking code…

 12 of 13 Stephen Brooks / RAL / March 2005 The Decay Channel (ctd.) Developed a more accurate code, Muon1 Used it to validate Grahame’s design… –3.1% of the pions/muons were captured …and parameter search for the optimum –Within constraints: 0.5m drifts, etc. –Increased transmission to 9.6% Increased in the older code (PARMILA) too –Fixed a problem in the original design!

 13 of 13 Stephen Brooks / RAL / March 2005 UKNF Research Efforts MICE at RAL (phase I ~2007; II ~ ) FFAG electron model at Daresbury –Under definition! Target shock studies program Beamline design and optimisation work –Myself, Grahame (+ new recruit soon) –Network with European “BENE” collaboration

 14 of 13 Stephen Brooks / RAL / March 2005 BACKUP! In case the time is longer than my slides. Web report

 15 of 13 Stephen Brooks / RAL / March 2005 Muon Acceleration Options Accelerators must have a large aperture Few turns (or linear) in low energy part, so muons don’t decay Recirculating Linacs (RLAs, studied first) FFAGs (cyclotron-like devices) –Grahame is playing with isochronous ones

 16 of 13 Stephen Brooks / RAL / March 2005 NuFact Intensity Goals “Success” is   /yr in the storage ring Proton Energy/GeVIntensity/MWTarget eff (pi/p)MuEnd eff (mu/pi)Operationalmu/year in storage ringCurrent/uA 8420%1.0%30% E "Not great" scenario 8160%2.0%35% E ISIS MW only to reach 10^ %3.5%40% E "Quite good" 5MW scenario (gets 10^21) %55% E Required to reach 10^ = PtO2 target inclined at 200mrad, see Mokhov FNAL PiTargets paper20% = 2.2GeV dataset from Paul Drumm

 17 of 13 Stephen Brooks / RAL / March 2005 Tracking & Optimisation System Distributed Computing –~450GHz of processing power –Can test millions of designs Genetic Algorithms –Optimisation good up to 137 parameters… Accelerator design-range specification language –Includes “C” interpreter

 18 of 13 Stephen Brooks / RAL / March 2005 Decay Channel Lattice Drifts Length (m) D [0.5,1] D2+0.5 [0.5,1] Solenoids Field (T)Radius (m)Length (m) S1 20 [0,20] 0.1 [fixed] [0.2,0.45] S2-4 −3.3, 4, −3.3 [-5,5] 0.3 [0.1,0.4] 0.4 [0.2,0.6] S5-S24 ±3.3 (alternating) [-4,4] S [0.1,0.4] Final (S34)0.15 [fixed] 12 parameters –Solenoids alternated in field strength and narrowed according to a pattern 137 parameters –Varied everything individually Tantalum Rod Length (m)0.2 [fixed] Radius (m)0.01 [fixed] Angle (radians)0.1 [0,0.5] Z displacement (m) from S1 start (S1 centred) [0,0.45] Original parameters / Optimisation ranges

 19 of 13 Stephen Brooks / RAL / March 2005 Improved Transmission Decay channel: –Original design: 3.1%  + out per  + from rod –12-parameter optimisation  6.5%  + /  % through chicane –137 parameters  9.6%  + /  % through chicane Re-optimised for chicane transmission: –Original design got 1.13% –12 parameters  1.93% –137 parameters  2.41% 3`700`000 runs so far 1`900`000 runs 330`000 runs

 20 of 13 Stephen Brooks / RAL / March 2005 Optimised Design for the Decay Channel (137 parameters) Maximum Length Minimum Drift Maximum Aperture Maximum Field (not before S6) (mostly) (except near ends) (except S4, S6)

 21 of 13 Stephen Brooks / RAL / March 2005 Why did it make all the solenoid fields have the same sign? Original design had alternating (FODO) solenoids Optimiser independently chose a FOFO lattice Has to do with the stability of off-energy particles FODO lattice FOFO lattice

 22 of 13 Stephen Brooks / RAL / March 2005 Design Optimised for Transmission Through Chicane Nontrivial optimum found Preferred length? Narrowing can only be due to nonlinear end-fields