Final Results from IDS-NF Study NUFACT14 Workshop, Glasgow on behalf of the IDS-NF Collaboration Paul Soler, 26 August 2014.

Slides:



Advertisements
Similar presentations
1 Neutrino Factory Front End (IDS) -Chicane & Absorber David Neuffer C. Rogers, P. Snopok, C. Yoshikawa, … January 31, 2012.
Advertisements

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.
Participants WP3total Imperial College CERN STFC University Warwick CRNS University Oxford6 6 Total Euro  - WP3.
1 Optimization of baseline front end for a neutrino factory David Neuffer FNAL (August 19, 2009)
1 Neutrino Factory Front End (IDS) and Variations David Neuffer G. Prior, C. Rogers, P. Snopok, C. Yoshikawa, … August 2011 NuFACT99 -Lyon.
1 Muon Bunching for a Muon Collider David Neuffer FNAL August 3, 2010.
1 RAL + Front End Studies International Design Study David Neuffer FNAL (January 5, 2009)
1 Front End Studies and Plans David Neuffer FNAL (November 10, 2009)
Catalina Island Meeting May, Proton Drivers for Neutrino Factories: The CERN Approach Presented by B. Autin, CERN.
Thomas Roser Snowmass 2001 June 30 - July 21, MW AGS proton driver (M.J. Brennan, I. Marneris, T. Roser, A.G. Ruggiero, D. Trbojevic, N. Tsoupas,
The Front End MAP Review Fermi National Accelerator Lab August 24-26, 2010 Harold G. Kirk Brookhaven National Laboratory.
-Factory Front End Phase Rotation Optimization David Neuffer Fermilab Muons, Inc.
(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,
Summary Near Detector at IDS Meeting in FNAL EuroNu Annual General Meeting, Strasbourg 3 June 2010 Paul Soler.
Ajit Kurup, Imperial College London. Neil Bliss, Norbert Collomb, Alan Grant, STFC/DL, Daresbury. Costing Methodology and Status of the Neutrino Factory.
Alain Blondel Neutrino Factory scenarios I will endeavour to address some principle design issues related to the physics use of high intensity muon beams.
WP5: Detector Performance and Cost EuroNu Launch Meeting 5 February 2008 Coordinator: Paul Soler, University of Glasgow Deputy: Anselmo Cervera Villanueva,
Institutional Logo Here Harold G. Kirk DOE Review of MAP (FNAL August 29-31, 2012)1 The Front End Harold Kirk Brookhaven National Lab August 30, 2012.
Storage Ring : Status, Issues and Plans C Johnstone, FNAL and G H Rees, RAL.
3 GeV,1.2 MW, Booster for Proton Driver G H Rees, RAL.
Proton Driver Status ISIS Accelerator Division John Thomason.
Source Group Bethan Dorman Paul Morris Laura Carroll Anthony Green Miriam Dowle Christopher Beach Sazlin Abdul Ghani Nicholas Torr.
Fermilab, Proton Driver, Muon Beams, Recycler David Neuffer Fermilab NufACT05.
Related poster [1] TPAG022: Slow Wave Electrode Structures for the ESS 2.5 MeV Chopper – Michael A. Clarke-Gayther Status Funding bids have been prepared.
Proton Driver: Status and Plans C.R. Prior ASTeC Intense Beams Group, Rutherford Appleton Laboratory.
ICHEP 2012 Melbourne, 7 July 2012 Paul Soler on behalf of the MICE Collaboration The MICE Beam Line Instrumentation (Trackers and PID) for precise Emittance.
EDM2001 Workshop May 14-15, 2001 AGS Intensity Upgrade (J.M. Brennan, I. Marneris, T. Roser, A.G. Ruggiero, D. Trbojevic, N. Tsoupas, S.Y. Zhang) Proton.
Source Group Bethan Dorman Paul Morris Laura Carroll Anthony Green Miriam Dowle Christopher Beach Sazlin Abdul Ghani Nicholas Torr.
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.
UKNF OsC RAL – 31 st January 2011 UKNF - Status, high lights, plans J. Pozimski.
WP5: Detector Performance and Cost EuroNu Meeting CERN, 26 March 2009 Paul Soler Coordinator: Paul Soler, University of Glasgow Deputy: Anselmo Cervera.
R.G. 7/09/20101 Options for neutrinos. R.G. 7/09/20102 Conventional beam from the SPS (1/3) Neutrinos using the SPS Nominal CNGS 732 km baseline from.
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 ,
-Factory Front End Phase Rotation Gas-filled rf David Neuffer Fermilab Muons, Inc.
Staging of a Neutrino Factory (and beyond…) Mark Palmer Director, US Muon Accelerator Program NuFACT 2014, Glasgow, August 25-30, 2014 NUFACT2014 XVIth.
 Stephen Brooks / RAL / April 2004 Muon Front Ends Providing High-Intensity, Low-Emittance Muon Beams for the Neutrino Factory and Muon Collider.
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.
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.
Institutional Logo Here July 11, 2012 Muon Accelerator Program Advisory Committee Review (FNAL July 11-13, 2012)1 The Front End.
CHIPP Aug 2010J.S. GraulichSlide 1 MICE and the Neutrino Factory Jean-Sebastien Graulich, Geneva.
 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.
Proton Driver / Project X Keith Gollwitzer Fermilab August 30, 2012.
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.
Proton Driver Design Keith Gollwitzer Fermilab February 19, 2014.
WP3: The Neutrino Factory Costing Status Ajit Kurup CERN Costing Workshop 8 th December 2011.
1 Muon Capture for a Muon Collider David Neuffer July 2009.
Proton Driver Keith Gollwitzer Accelerator Division Fermilab MAP Collaboration Meeting June 20, 2013.
MIND Systematic Errors EuroNu Meeting, RAL 18 January 2010 Paul Soler.
Detector: Status and Plans 6 th IDS-NF Meeting, RAL, 22 September 2010 Paul Soler.
1 Front End – present status David Neuffer December 4, 2014.
Near Detector Tasks EuroNu Meeting, CERN 26 March 2009 Paul Soler.
Research and development toward a future Muon Collider Katsuya Yonehara Accelerator Physics Center, Fermilab On behalf of Muon Accelerator Program Draft.
Proton Driver Developments and the Neutrino Factory Christopher R Prior ASTeC Intense Beams Group STFC Rutherford Appleton Laboratory, U.K.
PSI, Zurich February 29 – March Session classification : Accelerator Concepts Tuesday, March 1, 2016 Introduction Vyacheslav Yakovlev Fermilab,
UK Neutrino Factory Conceptual Design
Towards a Common Proton Driver for a Neutrino Factory
EURONu Collaboration Board,
The Accelerator Complex from the International Design Study
Neutrino beams from the decay of muons
Detector Baseline EuroNu Meeting, RAL 20 January 2010 Paul Soler.
nuSTORM at Fermilab D Adey
The COMET Experiment Ajit Kurup, Imperial College London, on behalf of the COMET Collaboration. ABSTRACT The COherent Muon to Electron Transition (COMET)
Muon Front End Status Chris Rogers,
Neutrino Oscillation Physics with a Neutrino Factory
Superbeams with SPL at CERN
Progress towards Pulsed Multi-MW CERN Proton Drivers
LHC (SSC) Byung Yunn CASA.
Presentation transcript:

Final Results from IDS-NF Study NUFACT14 Workshop, Glasgow on behalf of the IDS-NF Collaboration Paul Soler, 26 August 2014

2 International Design Study o International Design Study for a Neutrino Factory (IDS-NF) ― Principal objective: deliver Reference Design Report by 2013  Physics performance of the Neutrino Factory  Specification of each of the accelerator, diagnostic and detector systems that make up the facility  Schedule and cost of the Neutrino Factory accelerator, diagnostics, and detector systems. ― Co-sponsored by EU through EUROnu ― Web site: o Interim Design Report: IDS-NF-020 delivered 2011 o EUROnu reports: o Reference Design Report that itemises facility, accelerator and detector performance and physics reach will be published by the end of the year arXiv: NUFACT14, Glasgow 26 August 2014

3 Optimisation of Neutrino Factory  Optimisation for high  13 : only one baseline For large  13 : Energy 10 GeV, Baseline ~2000 km For small  13 : Energy ~25 GeV, Baseline ~4000 km Contours of CP coverage 100 kton MIND NUFACT14, Glasgow 26 August 2014

4 Neutrino Factory Baseline Neutrino Factory Baseline o Magnetised Iron Neutrino Detector (MIND): –100 kton at ~2000 km Baseline reviewed 2012: from 25 GeV to 10 GeV muons (v4.0), one storage ring with detector at 2000 km, due to large  13 results 562 m NUFACT14, Glasgow 26 August 2014

5 Neutrino Factory Baseline o Proton driver –Proton beam ~8 GeV on target o Target, capture and decay –Create , decay into  (MERIT) o Bunching and phase rotation –Reduce  E of bunch o Ionization Cooling –Reduce transverse emittance (MICE) o Acceleration –120 MeV  10 GeV with RLAs –FFAG option now not favoured o Decay ring –Store for ~100 turns –Long straight sections Neutrino spectra calculable to high accuracy 562 m NUFACT14, Glasgow 26 August 2014

6 Optimum energy proton driver o Optimum beam energy –Depends on choice of target –Optimum energy for high-Z targets around 8 GeV –Results validated by HARP hadron production experiment MARS+FLUKA Adopted 10 ± 5 GeV arXiv: NUFACT14, Glasgow 26 August 2014

7 Proton Driver o Requirements: o Choice is regional decision LINAC based (SPL) proton driver at CERN Synchrotron(s)/FFAG based proton driver (green field solution) – studied at RAL. PIP based solution at Fermilab. arXiv: NUFACT14, Glasgow 26 August 2014

8 Proton Driver (SPL) o Superconducting Proton LINAC, SPL, at CERN: 5 GeV Accumulation Duration = 400  s Compression t = 0  s t = 12  s t = 24  s t = 36  s etc. until t = 96  s Accumulator [120 ns pulses - 60 ns gaps] SPL beam [42 bunches - 21 gaps] Compressor [120 ns bunch - V(h=3) = 4 MV] Target [2 ns bunches – 6 times] NUFACT14, Glasgow 26 August 2014

9 Proton Driver (RCS) o Hardware options: 4 MW operation Option with a Rapid Cycling Synchrotron (RCS) Rees, Prior (RAL) 10 GeV RCS Achromatic Hˉ collimation line 3 GeV RCS booster mean radius = m 10 GeV RCS 180 MeV H ˉ linac NUFACT14, Glasgow 26 August 2014

10 Proton Driver (RCS) o Solution found around ISIS upgrade at RAL Based on MW ISIS upgrade with 800 MeV Linac and 3.2 (≈ 3.3) GeV RCS Assumes a sharing of the beam power at 3.2 GeV between the two facilities Both facilities can have the same ion source, RFQ, chopper, linac, H − injection, accumulation and acceleration to 3.2 GeV Requires additional RCS machine in order to meet the power and energy needs of the Neutrino Factory Options for the bunch compression to 1 – 3 ns RMS bunch length: - adiabatic compression in the RCS - ‘fast phase rotation’ in the RCS - ‘fast phase rotation’ in a dedicated compressor ring NUFACT14, Glasgow 26 August 2014

11 Proton Improvement Plan (PIP) o Fermilab option: 1-4 MW operation from 3-8 GeV Proton Improvement Plan (PIP): staging Linac facility at Fermilab PIPII: GeV PIPIII: ~1 3 GeV? PIPIV: GeV? NUFACT14, Glasgow 26 August 2014

12 Target o Had to increase radiation shielding in solenoid surrounding new design for target station Target station and start of decay channel NUFACT14, Glasgow 26 August 2014 Proof-of-principle: MERIT

13 Muon Front End o Adiabatic B-field taper from Hg target to longitudinal drift o Added chicane to remove protons o Drift in ~1.5 T, ~60 m solenoid o Adiabatically bring on RF voltage to bunch beam o Phase rotation using variable frequencies –High energy front sees -ve E-field –Low energy tail sees +ve E-field –End up with smaller energy spread o Ionisation Cooling –Try to reduce transverse beam size –Prototyped by MICE NUFACT14, Glasgow 26 August 2014

14 Muon Front End o Buncher: –33 normal conducting RF cavities –RF frequency: MHz –Gradient: MV/m 18.9 m~60.7 m FE Targ et Solenoid DriftBuncherRotatorCooler ~33m42 m ~80 m p π→μ NUFACT14, Glasgow 26 August 2014

15 Muon Front End o Phase rotation: –56 cells of 0.75 m length –Total length: 42 m –56 normal conducting RF cavities with SC coils –RF frequency MHz –Gradient 12 MV/m 18.9 m~60.7 m FE Targ et Solenoid DriftBuncherRotatorCooler ~33m42 m ~80 m p π→μ NUFACT14, Glasgow 26 August 2014

16 Muon Front End o Cooling channel: MICE demonstration –100 cells of 0.75 m length –Total length: ~80 m –100 normal conducting RF cavities with SC coils –RF frequency MHz –Gradient 15 MV/m –LiH absorbers (1.1 cm)  0.86 m 18.9 m~60.7 m FE Targ et Solenoid DriftBuncherRotatorCooler ~33m42 m ~80 m p π→μ NUFACT14, Glasgow 26 August 2014

17 Muon Front End o Front end performance: –0.066  /proton –Cooling increases muon yield by a factor of ~2.2 –Cooling channel is most cost-effective way to increase yield of muons ~ m~60.7 m FE Targ et Solenoid DriftBuncherRotatorCooler ~33m42 m ~80 m p π→μ NUFACT14, Glasgow 26 August 2014

18 Acceleration o Redefined baseline after moving to 10 GeV (IDR: 25 GeV) –Baseline: two “dog-bone” Recirculating Linear Accelerators (RLA) –First RLA up to 2.8 GeV –Second RLA up to 10 GeV Side view NUFACT14, Glasgow 26 August 2014

19 Decay Ring Geometry o Racetrack geometry for decay ring with insertion −Straight: 562 m −Upper arc: 121 m −Lower arc: 113 m −Insertion: 46 m −Matching: 105 m (total)  Circumference = 1556 m 562 m Divergence < 0.1/  Three  + and three  - bunches NUFACT14, Glasgow 26 August 2014

20 o Magnetised Iron neutrino Detector (MIND) o Octagonal plates and toroidal field o Magnetic field T from 8x15 kA current delivered by Superconducting Transmission Line (STL): ~10cm hole o Extruded scintillator with WLS fibre and SiPMT MIND Far Detector Bross, Wands (FNAL) 100 kton 14mx14mx3cm plates STL NUFACT14, Glasgow 26 August 2014

21 Near Detector NUFACT13, Beijing: 24 August 2013 o Two near detectors required, one at each straight: –Neutrino flux (<1% precision) and extrapolation to far detector –Charm production (main background) and taus for Non Standard Interactions (NSI) searches –Cross-sections and other measurements (ie PDFs, sin 2  W ) 9th IDS-NF, Fermilab: 8th October 2012 beam 3 m B>1 T ~20 m High Res Detector Mini-MIND VertexDetector Two options Scintillating fibre tracker HiResMuNu: straw tube tracker NUFACT14, Glasgow 26 August 2014

22 o Full simulation and reconstruction of neutrino interactions  Multi-variate analysis (MVA) with five variables, tuned for sin 2 2  13 ~0.1: Boosted Decision Tree (BDT) adopted Golden Channel e   analysis R. Bayes Momentum resolution Migration matrix Wrong-sign muon signal and background separation NUFACT14, Glasgow 26 August 2014

23 MIND efficiencies and background R. Bayes BDT efficiency, focussing  + BDT background (stored  -, focussing  + ) BDT background (stored  +, focussing  + ) BDT efficiency, focussing  - Tau signal NUFACT14, Glasgow 26 August 2014

24 Performance 10 GeV Neutrino Factory o Systematic errors: 1% signal and 20% background  Results 10 GeV Neutrino Factory,  /year for 10 years with 100 kton MIND at 2000 km gives best sensitivity to CP violation o This provides best sensitivity out of all future proposed facilities CP violation 5  coverage is 85% (ie. 85% probability of CPV discovery!) arXiv: NUFACT14, Glasgow 26 August 2014

25 Conclusions o International Design Study for a Neutrino Factory (IDS-NF) has concluded its study –Interim Design Report delivered March 2011 –Reference Design Report should be published by end of 2014 (it should have come out already but delayed by a number of “crises” that everyone in this room is aware of –It defines benchmark 10 GeV Neutrino Factory –Concepts for accelerator systems have been defined –100 kton Magnetised Iron Neutrino Detectors (MIND) –Best sensitivity for CP violation of all possible future neutrino facilities o We need to continue with international programme to have unified voice NUFACT14, Glasgow 26 August 2014