1 Neutrino detector test beam requirements 0. Disclaimer 1. News from the neutrino scene 2. Beam requirements for AIDA and others.

Slides:



Advertisements
Similar presentations
ISS meeting UCIrvine 21 August 2006 Alain Blondel 1 Evaluation of « optimal » segmentation for neutrino factory far detectors A. magnetized iron sampling.
Advertisements

Alain Blondel Groupe Neutrino Université de Genève EUROPEAN STRATEGY FOR FUTURE NEUTRINO PHYSICS 1. The questions 2. Question 1: the aims 3. Accelerator.
Sergio Palomares-Ruiz June 22, 2005 Super-NO A Based on O. Mena, SPR and S. Pascoli hep-ph/ a long-baseline neutrino experiment with two off-axis.
Accelerator based Neutrino program around the world 1. Europe: Neutrino platform at CERN ESS second maximum? 2. Japan: T2K and HyperK status 3. USA: LBNF.
ISS-4 22 August IRVINE Alain Blondel NEUtrino DETectors N-EU-DET 4-years working plan for Neutrino Detector R&D to take place in ~ objectives.
Alain Blondel CHIPP Neutrino meeting NEUCHATEL June 2004.
High Energy Neutrino Detectors Deborah Harris Fermilab Nufact’05 Summer Institute June 14-15, 2005.
K.T. McDonald March 18, 2010 LArTPC BNL 1 Magnetizing a Large Liquid Argon Detector Kirk T. McDonald Princeton University (March 18, 2010)
Gary Feldman P5 Meeting 21 February The NO A Experiment P5 Meeting SLAC 21 February 2008 Gary Feldman.
Neutrino physics: experiments and infrastructure Anselmo Cervera Villanueva Université de Genève Orsay, 31/01/06.
Segmented magnetised detectors Anselmo Cervera Villanueva Universidad de Valencia ISS meeting RAL (UK) 25/04/06 RAL (UK) 25/04/06.
How to Build a Neutrino Oscillations Detector - Why MINOS is like it is! Alfons Weber March 2005.
Neutrino detectors for the future Neutrino Facility global numbers : next project ~ 600 M€ (NB NOvA, T2K = 200M$, OPERA=100MCHF, etc...) community between.
K.T. McDonald June 18, 2009 DUSEL FNAL 1 Strategies for Liquid Argon Detectors at DUSEL Kirk T. McDonald Princeton University (June 18, 2009)
Sensitivities (preliminary plots for your eyes only)
Alain Blondel Detectors UNO (400kton Water Cherenkov) Liquid Ar TPC (~100kton)
DoE Review June 26, 2000 A Magnetic Tracking Calorimeter for a Neutrino Factory - Ideas & Issues Jeff Nelson William & Mary Williamsburg, Virginia 1 st.
MICE Project Board Alain Blondel 1 MICE running Preamble ISIS running Step I Step(s) IV Step V (and VI)
Scoping study p-ECFA Alain Blondel ISS-detectors Introduction: working group plans, organization and aims of the meeting.
WP5: Detector Performance and Cost EuroNu Launch Meeting 5 February 2008 Coordinator: Paul Soler, University of Glasgow Deputy: Anselmo Cervera Villanueva,
Report of the SPC panel on Future Neutrino Facilities R.Aleksan, A.Blondel, P.Dornan, K.Meier/T.Nakada, A.Zalewska, F.Zwirner SPC meeting, Report.
27 April ’12 MINER A meeting Alessandro Bravar Université de Genève UniGE Miner a Application Motivation UniGE neutrino group MINER UniGE NA61 / SHI.
Anselmo Cervera Villanueva IFIC (Universidad de Valencia & CSIC) EURODET meeting 7 December 2007 Neutrino Networking activities.
Long Baseline Experiments at Fermilab Maury Goodman.
ISS-detectors report ISS/IDS meeting at CERN Alain Blondel ISS-detectors “--Evaluate the options for the neutrino detection systems -- define a baseline.
Activities relevant to Neutrinos in the UK Alfons Weber Oxford/RAL Durham, 11-Mar-2011.
WP5: Detector Performance and Cost EuroNu Meeting CERN, 26 March 2009 Paul Soler Coordinator: Paul Soler, University of Glasgow Deputy: Anselmo Cervera.
Muon Identification in the MINOS Calibration Detector Anna Holin 05 December 2005 University College London.
Monday, Feb. 19, 2007PHYS 5326, Spring 2007 Jae Yu 1 PHYS 5326 – Lecture #7 Monday, Feb. 19, 2007 Dr. Jae Yu 1.Neutrino Oscillation Experiments 2.Long.
Alain Blondel. AIDA-Neutrino meeting AIDA Neutrino detector studies 1. News from the neutrino scene 2. Beam requirements for AIDA 3. Discuss.
If  13 is large, then what ? Hisakazu Minakata Tokyo Metropolitan University.
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.
Neutrino Physics Opportunities for Fermilab Steering Group 6/12/07 Andy Lankford UC Irvine.
A new underground laboratory at Frejus Jacques Bouchez CEA-SACLAY NNN05-Aussois April 7, 2005 Historical overview Latest developments Outlook.
NuMI Off-Axis Experiment Alfons Weber University of Oxford & Rutherford Appleton Laboratory EPS2003, Aachen July 19, 2003.
MICE CC visit at CERN Alain Blondel 1   MICE The International Muon Ionization Cooling Experiment.
Alain Blondel -- After the ISS -- What did ISS achieve? 1. Established a « baseline » for the accelerator study 2. Rejuvenated simulation and study of.
EUROnu WP5 Detector Costing EuroNu Annual General Meeting, Strasbourg 3 June 2010 Paul Soler.
NUFACT’06 Summary of working group 1 Neutrino Oscillations Experiments Mark Messier Indiana University August 30, 2006.
Detector possibilities: scintillator based detectors EUCARD 1 st Annual Meeting, RAL, 13 April 2010 Paul Soler.
CHIPP Aug 2010J.S. GraulichSlide 1 MICE and the Neutrino Factory Jean-Sebastien Graulich, Geneva.
MICE RF review Alain Blondel 1   MICE The International Muon Ionization Cooling Experiment.
Accelerator-based Long-Baseline Neutrino Oscillation Experiments Kam-Biu Luk University of California, Berkeley and Lawrence Berkeley National Laboratory.
Alain Blondel 4 March 2011 NEU2012 summary NEU2012: towards a concrete proposal by the neutrino community (emphasis on long baseline accelerator expts)
Answers to the referees questions to the baby MIND proposal submitted to the SPSC on October, 6, 2015 Baby MIND at WAGASCI: There is no run mentioned behind.
2 July 2002 S. Kahn BNL Homestake Long Baseline1 A Super-Neutrino Beam from BNL to Homestake Steve Kahn For the BNL-Homestake Collaboration Presented at.
1 Performance of a Magnetised Scintillating Detector for a Neutrino Factory Scoping Study Meeting U.C. Irvine Monday 21 st August 2006 M. Ellis & A. Bross.
10/20/2015 TASD and MIND prototype and tests at CERN SPSC Oct Tests of TASD and MIND prototypes at CERN.
Neutrino detector IA request Lines of thought first meeting on 24 August 2007 on- the fly notes by AB present: Alain Blondel, André Rubbia, Anselmo Cervera,
EURO EURO A High Intensity Neutrino Oscillation Facility in Europe Introduction Aims Structure Tasks Link to other activities Future dates.
2008 European School of High-Energy Physics - Trest, Czech Republic - 19 August - 1st September Target Tracker Data Analysis In OPERA Experiment S. Dmitrievsky,
MIND Systematic Errors EuroNu Meeting, RAL 18 January 2010 Paul Soler.
Monte Carlo simulation of the particle identification (PID) system of the Muon Ionization Cooling Experiment (MICE) Mice is mainly an accelerator physics.
Detector: Status and Plans 6 th IDS-NF Meeting, RAL, 22 September 2010 Paul Soler.
A. Blondel WP 4.7 LAGUNA_LBNO LARG+ND meeting Near detector for CN2PY -- discussion What is needed? What does it take? Ideas…
LBNO Near detector task force LAGUNA-LBNO FP7 WP 4.7 Plenary meeting Hamburg
EUROnu Review: 14 th April 2011 EUROnu Introduction and Objectives Neutrino oscillations: much interest since 1 st paper in extension required to.
G. Sullivan – Quarknet, July 2003 Calorimeters in Particle Physics What do they do? –Measure the ENERGY of particles Electromagnetic Energy –Electrons,
Epiphany06 Alain Blondel A revealing comparison: A detailed comparison of the capability of observing CP violation was performed by P. Huber (+M. Mezzetto.
LBNO Near detector task force LAGUNA-LBNO FP7 WP 4.7 Plenary meeting Hamburg
SPSC recommendations [Installation at PS-T9] Baby MIND weekly meeting 28 th October 2015.
Alain Blondel. LAGUNA meeting CERN 3-5 March 2011
An Experimental EXERCISE
Wrong sign muons detection in a
Alain Blondel 11 October 2010 GDR NEU2012 summary
Alain Blondel. EUCARD meeting NEU April 2010
Gary Feldman P5 Meeting 21 February
XVth International Workshop on Neutrino Factories, Betabeams and Superbeams LAGUNA-LBNO Many thanks to D. Duchesneau, F. Di Lodovico, T. Patzak, A. Rubbia.
Alain Blondel Neutrino Experiments
Based on material presented at various meetings
Presentation transcript:

1 Neutrino detector test beam requirements 0. Disclaimer 1. News from the neutrino scene 2. Beam requirements for AIDA and others

2 Disclaimer -- I was asked to give this presentation just before Xmas, and before a long stretch of funding requests and other critical deadlines  I present these slides as ‘best information available’  I have no particular mandate to do so (except from AIDA group)

3 The Neutrino Scene – activities at CERN 1.Present neutrino oscillation experiments in which European groups are involved MINOS Iron calorimeter / T2K (TPC, ECAL) had test beams for detector development in East area Completed. 2. Experiment at CERN running now: NA61/SHINE T2K data at 30GeV beam energy is probably completed -- but may need T2K data at 40 or 50 GeV if T2K proton energy changes Fermilab Groups preparing requests: -- will request 120 GeV beam for NUMI beams and other energies (40 60…) for their DUSEL future project -- will request low energy (8 GeV+ Berylium) for the BooNE beam likely to need a dedicated Cherenkov request to DPE and SPSC in preparation 3. Future experiments in which Europeans will be involved or are studying -- AIDA project -- Liquid Argon projects -- Water Cherenkov projects

4 There are several neutrino projects proposed: Long baseline (‘Active neutrino’ oscillations) L = 500km * E (GeV) (x0.2 – 2 ) -- low energy superbeam to Frejus  Water Cherenkov detector -- beta beam to Frejus 130 km (0.26 GeV  0.5 GeV) -- neutrino factory to detector ~ km -- higher energy ‘CNGS like’ beam to Pyhasalmi (2300 km)  4.6 GeV -- keep CNGS itself (but no near detector!) to Umbria or Golf of Taranto Short Baseline L ~ 1 km * E (GeV) (‘sterile neutrinos’) -- revive PS neutrino beam 1 GeV OR try to combine all neutrino beams in the north area this is presently the favored scenario: CN2PY as backbone to future neutrino program at CERN OR accept that all neutrino activities go to overseas projects -- T2HK in Japan (Water Cherenkov at 300km)  0.7 GeV or Liquid Argon detector at 650 km -- DUSEL in the US (new neutrino beam) 1300km  2.6 GeV No matter what happens, involvment of European groups in future neutrino projects will require test beams E  GeV

Long distance: 2300km Pyhasalmi Fine grain detector e.g. 20kton fid. Larg + Magnetized detector Long distance allows rapid sensitivity to sign(  m 2 13 ) 1st step easier: SPS C2PY  consortium 1st priority Nextsteps HP 50 GeV PS … …or neutrino factory Getting our feet on (under) the ground: LAGUNA –LBNO new FP7 design study Alain Blondel HIF Workshop main options Short distance: 130km Memphys at Frejus SPL+beta beam CP and T violation Medium term plans include long term plans! A. Rubbia

Sensitivity plot from the SPC panel report (2009): work from EUROnu, Laguna, IDS-NF, DUSEL, T2KK etc… Alain Blondel HIF Workshop km 2300km Limitation due to matter effect sytematics

Alain Blondel HIF Workshop Will also study short baseline + sterile neutrino expts

8 -- Stopping properties of pions and muons in fine grain detector This will be studied in the MICE EMR at RAL (or Larg at KEK) using stopping e/mu/pi of both signs in May 2012  MICE/KEK BEAMS -- Charge separation for electrons in Minerva – like detector (with lower density?) in magnetic field This can be studied in the MORPURGO magnet at CERN beam requirement : electron beam from GeV (perhaps 10 GeV) -- Charge separation in MIND-like detector This can be studied in a baby-MIND detector at CERN beam requirement : muons from 0.8 – 2 GeV (perhaps 10 GeV?) -- hadronic shower angular and transverse momentum resolution in TASD and MIND or LArg (tau detection in superbeam or high energy neutrino factory) this requires about 2m deep MIND (that is CDHS shower box) and 2x2x5m deep TASD or LArg in hadron test beam e.g. at CERN or Fermilab beam requirement protons pions of 0.5 to 10 GeV. Beam Requirements -- Physics issues:

9 Fast detectors for magnetized near detectors in Superbeam, beta-beam, neutrino factory Accurate position resolution (mm)  triangular shaped scintillator bars Magnetic field  si-PMT readout MICE calorimeter = 1m 3 Next step: test at CERN in Dipole magnet in H8  1.6m diameter. Variable density by spacing planes -- reconstruction of showering electrons -- stopping properties of pions and muons First test in T9 beam at CERN – position resolution few mm

10

11 neutrino event in ND m Liquid KEK

12

13

14

15 CONCLUSIONS 1.Neutrino experiments will develop and require test beams 2.Typical energies required are more akin to East area 3.Size of test detectors can be quite large (2x2x5 or more) 4.A large 1x1x2m, B=1.5 T magnet is requested for some of the studies 5.Beam energies in the range GeV (Frejus, T2HK, WCherenkov) 0.5 – 10 GeV (CN2PY) consistent with East Area beams for several tests but large magnet and large detector size prefer North Area 6. Request = a Neutrino Test Beam area at CERN! 7. Time scale is …