Neutrino Factory and Muon Collider Collaboration Meeting UCLA January, 2007 Alan Bross.

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Presentation transcript:

Neutrino Factory and Muon Collider Collaboration Meeting UCLA January, 2007 Alan Bross

2 Alan Bross NFMCC Meeting January 2007 Welcome  It has been a very productive year with a great deal of progress u MuCool u MERIT u MICE u Simulations – International Scoping Study  And the upcoming year is shaping up to be exciting u MERIT and MICE taking data u Neutrino Factory International Design Study u Renewed attention to the energy frontier s Muon Collider Collaboration Meeting XI You are not getting older You are getting Better

3 Alan Bross NFMCC Meeting January 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

4 Alan Bross NFMCC Meeting January 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

5 Alan Bross NFMCC Meeting January 2007 Collaborating Institutions National Labs ANL BNL FNAL LBNL ORNL TJNAF Universities Cornell IIT Indiana Michigan State Northern Illinois Princeton UC-Berkeley UC-Davis UC-Los Angeles UC-Riverside University of Chicago National Labs Budker 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

6 Alan Bross NFMCC Meeting January 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

7 Alan Bross NFMCC Meeting January 2007 Technical Board Alan Rick Fernow Michael Green Don Hartill Dan Kaplan Harold Kirk McDonald Jim Norem Bob Rimmer Mike ZismanProject

8 Alan Bross NFMCC Meeting January 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)

9 Alan Bross NFMCC Meeting January 2007 Core 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 Fermilab Muon Collider Task Force

10 Alan Bross NFMCC Meeting January 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 End-to-End Cooling simulation for a Muon Collider s Low-emittance Muon Collider The Collaboration’s Focus was NF

11 Alan Bross NFMCC Meeting January 2007 Neutrino Factory – ISS Preliminary Design  Proton Driver  Target, Capture, Decay     Bunching, Phase Rotation u Reduce  E  Cooling  Acceleration  103 MeV  * GeV  Storage/Decay ring * Still under study

12 Alan Bross NFMCC Meeting January 2007 The Big Neutrino Questions  What is the origin of neutrino mass?  Did neutrinos play a role in our existence?  Did neutrinos play a role in forming galaxies?  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?

13 Alan Bross NFMCC Meeting January 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 New Facility In order to make an informed decision wheter or not a NF is this new facitily – Will need a TDR ready at this time This defines the R&D Program

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

15 Alan Bross NFMCC Meeting January 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

Muon Collider Back To The Future NFMCCMCNFCNFMCCMCNFCNFMCC

17 Alan Bross NFMCC Meeting January 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

18 Alan Bross NFMCC Meeting January 2007 Muon Collider-NF - Synergy Neutrino Factory Muon Collider

19 Alan Bross NFMCC Meeting January 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

20 Alan Bross NFMCC Meeting January 2007 First End to End MC Cooling Simulation

21 Alan Bross NFMCC Meeting January 2007 Muon Collider Parameters

22 Alan Bross NFMCC Meeting January 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 s Many new ideas emerging u Front-end is the same as for a Neutrino Factory u First full simulation of required cooling has been competed The Collaboration has entered a very exciting phase

23 Alan Bross NFMCC Meeting January 2007 Outlook  As you are all aware, our funding situation has been very tight and remains so. u Has certainly limited what we can do  However, given our recent MUTAC reviews and the recommendations of the Advanced Accelerator R&D Panel u We are on solid ground in asking for increased funding  And at our DOE briefing meeting in March we will make a strong case to the Office of High Energy Physics to follow the AARD Panel’s recommendation

24 Alan Bross NFMCC Meeting January 2007 Lets Begin Governor Swartzenegger helping operator improve the luminosity at PEP-II