Neutrino Factory and Muon Collider Collaboration Introduction MUTAC Review April 2007 Alan Bross.

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Presentation transcript:

Neutrino Factory and Muon Collider Collaboration Introduction MUTAC Review April 2007 Alan Bross

2 Alan Bross NFMCC MUTAC Review April 2007 NFMCC Mission  Extensive experimental program to verify the theoretical and simulation predictions To study and develop the theoretical tools, the software simulation tools, and to carry out R&D on the hardware that is unique to the design of Neutrino Factories and Muon Colliders

3 Alan Bross NFMCC MUTAC Review April 2007 Current Organization R&D Tasks DOE/NSF Laboratories/MCOG P. Bond, S. Holmes, J. Siegrist MUTAC R. Kephart Collaboration Spokespersons A. Bross, H. Kirk Project Manager M. Zisman Simul.  COOL TargetMICE Executive Board Technical Board Collaborating Institutions Neutrino Factory and Muon Collider Collaboration (NFMCC) Other C. Adolphsen J. Byrd D. Finley S. Henderson M. Lindner V. Litvinenko P. McIntosh L. Merminga D. Rubin M. Shaevitz

4 Alan Bross NFMCC MUTAC Review April 2007 Collaborating Institutions National Labs ANL BNL FNAL LBNL ORNL TJNAF Universities Cornell IIT Indiana Michigan State Mississippi Northern Illinois Princeton UC-Berkeley UC-Davis UC-Los Angeles UC-Riverside University of Chicago National Labs Budker CERN DESY INFN JINR, Dubna KEK RAL TRIUMF Universities Karlsruhe Imperial College Lancaster Max Planck Osaka Oxford Pohang Tel Aviv USInternational Corporate Partners Muons Inc. Tech-X Corporation

5 Alan Bross NFMCC MUTAC Review April 2007 Executive Board A. H. A. SesslerLBNLAssociate D. ClineUCLA S. GeerFNAL G. HansonUC Riverside D. KaplanIIT K. McDonaldPrinceton University R. PalmerBNL A. N. SkrinskyBINP D. SummersU. Mississippi A. TollestrupFNAL B. WengBNL J. WurteleLBNL/UC Berkeley M. ZismanLBNL Project J. GallardoBNL Scientific

6 Alan Bross NFMCC MUTAC Review April 2007 Technical Board Alan Rick Fernow Michael Green Don Hartill Dan Kaplan Harold Kirk McDonald Jim Norem Bob Rimmer Mike ZismanProject

7 Alan Bross NFMCC MUTAC Review April 2007 Theory & Simulation Board R. Fernow H. Kirk (BNL) Targetry Simulation D. Neuffer (FNAL) Front-End Systems R. Fernow (BNL) Emittance Exchange/Ring Cooler Coordinator S. Berg/ C. Johnstone (BNL)/(FNAL) Acceleration Simulation A. Sessler (LBNL) Theory M. Berz (MSU) G. Hanson (UCR) E. Keil (FNAL) S. Koscielniak (Triumf) R. Palmer (BNL)

8 Alan Bross NFMCC MUTAC Review April 2007 Scientific Program Targetry R&D: Mercury Intense Target Experiment (MERIT) Co-Spokespersons: Kirk McDonald, Harold Kirk Ionization Cooling R&D: MuCool and MICE MuCool Spokesperson: Alan Bross US MICE Leader: Dan Kaplan Simulations & Theory Coordinator: Rick Fernow Collaborating on Electron Model for Muon Acceleration Project (EMMA) Fermilab Muon Collider Task Force V. Shiltsev, S. Geer

9 Alan Bross NFMCC MUTAC Review April 2007 MERIT –Mercury Intense Target  Test of Hg-Jet target in magnetic field (15T)  Proposal submitted to CERN April, 2004 (approved April 2005)  Located in TT2A tunnel to ISR, in nTOF beam line  First beam ∼ July, 2007

10 Alan Bross NFMCC MUTAC Review April 2007 Muon Cooling: MuCool and MICE Component R&D and Cooling Experiment MuCool 201 MHz RF Testing 50 cm  Be RF window MuCool LH 2 Absorber Body  MuCool u Component testing: RF, Absorbers, Solenoids u Uses (MuCool Test Area –MTA) u Supports Muon Ionization Cooling Experiment (MICE) MuCool Test Area

11 Alan Bross NFMCC MUTAC Review April 2007 Muon Ionization Cooling Experiment (MICE) MICE Measurement of Muon Cooling Emittance First Beam August 2007

12 Alan Bross NFMCC MUTAC Review April 2007 Design Studies  Very Productive Period for the Collaboration u Strong participation in the International Scoping Study of a Future Neutrino Factory and Super- beam facility (ISS) s Super Beams s Beta-Beam Facility s Neutrino Factory u Exciting New developments in Muon Collider Design and Simulation s Complete cooling scenario for a Muon Collider –All cooling components have been simulated s Low-emittance Muon Collider The Collaboration’s Focus was NF

13 Alan Bross NFMCC MUTAC Review April 2007 Neutrino Factory – ISS Preliminary Design  Proton Driver  Target, Capture, Decay (MERIT)     Bunching, Phase Rotation u Reduce  E  Cooling (MICE)  Acceleration (EMMA)  103 MeV  25 & 50 * GeV  Storage/Decay ring * Still under study 10-25

14 Alan Bross NFMCC MUTAC Review April 2007 The Big Neutrino Questions  What is the origin of neutrino mass?  Did neutrinos play a role in our existence? u Galaxy Formation  Did neutrinos play a role in birth of the universe?  Are neutrinos telling us something about unification of matter and/or forces?  Will neutrinos give us more surprises? Big questions  tough questions to answer Is a Neutrino Factory needed in order to answer these questions?

15 Alan Bross NFMCC MUTAC Review April 2007 Neutrino Factory – The Physics Case We Don’t Know – But There is a Natural Decision Point  2012 After NOvA and T2K If  13 not seen or seen at 3  Consider Major Upgrades or New Facility In order to make an informed decision about a New Facility and if the NF plays at role – Will need a TDR ready at this time This defines the R&D Program Double Chooz/Daya Bay

16 Alan Bross NFMCC MUTAC Review April 2007 Neutrino Factory- ISS (3  m 31 2 = eV 2  Best possible reach in   for all performance indicators =Neutrino factory

17 Alan Bross NFMCC MUTAC Review April 2007 Neutrino Factory Detector Design  Totally Active Sampling Calorimeter 25kT  15m  X 15m long -0.5T u Times 10! u Cost estimate s $ M  New Ideas u High T c SC s No Vacuum Insulation u VLHC SC transmission line s Technically proven s Might actually be affordable

18 Alan Bross NFMCC MUTAC Review April 2007 Muon Collider - Motivation Reach Multi-TeV Lepton-Lepton Collisions at High Luminosity Muon Colliders may have special role for precision measurements. Small  E beam spread – Precise energy scans Small Footprint - Could Fit on Existing Laboratory Site

19 Alan Bross NFMCC MUTAC Review April 2007 Evolution of a Physics Program  Intense Low-energy muon physics u Intense K physics, etc  Neutrino Factory  Energy Frontier Muon Collider u TeV PRSTAB 2002

20 Alan Bross NFMCC MUTAC Review April 2007 The Muon Collider Motivation – Elevator Spiel PRSTAB – May 3, 2002 Energy Frontier Physics SMALL Footprint

21 Alan Bross NFMCC MUTAC Review April 2007 Muon Collider at the Energy Frontier  Comparisons with Energy Frontier e + e - Collider u For many processes - Similar cross sections u Advantage in s-channel scalar production  Cross section enhancement of (m  /m e ) 2 –  u Beam Polarization also possible s Polarization likely easier in e + e - machine u More precise energy scan capability s Beam energy spread and Beamstrahlhung limits precision of energy frontier (3TeV) e + e - machines u Muon Decay backgrounds in MC do have Detector implications, however 3 TeV COM Visible E cm

22 Alan Bross NFMCC MUTAC Review April 2007 S-channel Coupling to Higgs

23 Alan Bross NFMCC MUTAC Review April 2007 Higgs 

24 Alan Bross NFMCC MUTAC Review April 2007 MC Physics - Resolving degenerate Higgs Difficult in e + e - machine with equivalent R  1%

25 Alan Bross NFMCC MUTAC Review April 2007 Muon Collider-NF - Synergy Neutrino Factory Muon Collider

26 Alan Bross NFMCC MUTAC Review April 2007 Enabling Technologies for Muon Collider  Although a great deal of R&D has been done (or is ongoing) for a Neutrino Factory, the Technological requirements for a Muon Collider are Much More Aggressive u Bunch Merging is required u MUCH more Cooling is required  1000X in each transverse dimension,  10X in longitudinal u Cooling in 6D (x,x’,y,y’,E,t) is required u Acceleration to much higher energy (20-40 GeV vs TeV) u Storage rings s Colliding beams s Energy loss in magnets from muon decay (electrons) is an issue

27 Alan Bross NFMCC MUTAC Review April 2007 Muon Collider  Ingredients needed in Collider cooling scenario include: u Longitudinal cooling by large factors … u Transverse cooling by very large factors u Final beam compression with reverse emittance exchange u Improvements in bunch manipulations (bunch recombination?) u Reacceleration and bunching from low energy Palmer et al: RFOFO Ring Guggenheim 50-60T Solenoid Channel Muons Inc. High pressure gas-filled cavities Helical Cooling Channel Reverse Emittance Exchange Parametric Resonance Induced Cooling

28 Alan Bross NFMCC MUTAC Review April 2007 A Muon Collider Cooling Scenario

29 Alan Bross NFMCC MUTAC Review April 2007 Low-Emittance Muon Collider (LEMC) Parameter List: E cm = 1.5 TeV Peak L = 7X10 34 #  ’s/bunch = Av Dipole B = 10T  p/p = 1%  * (cm) = 0.5 (!) Proton driver: E = 8 GeV Power  1 MW

30 Alan Bross NFMCC MUTAC Review April 2007 An ILC Upgrade? In this schematic we see the real power of the Muon Collider concept. A 2x2 TeV machine based on a 500 GeV linac.

31 Alan Bross NFMCC MUTAC Review April 2007 Conclusions  Neutrino Factory u Compelling case for a precision neutrino program s With present assumptions Neutrino Factory out-performs other options. However, more is needed before concluding this is the right path –What the on-going Neutrino Physics program tells us –Process must include cost and schedule considerations International Design Study  Muon Collider u New concepts improve the prospects for a multi-TeV Muon Collider  LEMC concept – HCC/REMEX/PIC (Muons Inc.) u Front-end is the same (similar) as for a Neutrino Factory u First complete cooling scenario has emerged s Palmer Scheme The Collaboration has entered a very exciting phase

32 Alan Bross NFMCC MUTAC Review April 2007 The Way Forward  Technical Progress u MERIT and MICE will be taking data in the near future and will address some of the fundamental technical issues in high-power targetry and muon cooling  Expanded Emphasis on MC u New ideas in Muon Cooling have led to a renewed interest in Muon Collider studies with very exciting prospects s Creation of the Fermilab Muon Collider Task Force (MCTF) is a positive step  Resource Limitations u The collaboration is still funding limited and progress in a number of areas is considerably slower than is technically possible u Expansion of our activities into new initiatives is extremely constrained