1 Super Beams Takashi Kobayashi IPNS, KEK ’04 June 17, 2004 Paris Contents 1.Introduction 2.“Super beam” experiments 3.Summary Future dream for 10~20years from now
2 Conventional neutrino beam with (Multi-)MW proton beam ( Fact) Pure beam ( ≳ 99%) e ( ≲ 1%) from e chain and K decay(Ke3) can be switched by flipping polarity of focusing device What is (Original) Super Beam? Proton Beam Target Focusing Devices Decay Pipe Beam Dump ,K,K Strongly motivated by high precision LBL osc. exp.
3 Long baseline osc. experiments 1 st phase experiments (Now) 1 st phase experiments (Now) Confirmation of atm. results Confirmation of atm. results K2K(1999~)/MINOS(2005~)/ICARUS/OPERA(2006~) K2K(1999~)/MINOS(2005~)/ICARUS/OPERA(2006~) 2 nd phase experiments (Now~10yrs) 2 nd phase experiments (Now~10yrs) Discovery of e appearance Discovery of e appearance Designed & Optimized aft. SK atm Designed & Optimized aft. SK atm ~MW beam w/ ~50kton detector ~MW beam w/ ~50kton detector T2K-I (approved. 2009~)/NO A (2009?~) / (C2GT) T2K-I (approved. 2009~)/NO A (2009?~) / (C2GT) 3 rd phase experiments(10~20yrs?) 3 rd phase experiments(10~20yrs?) CP violation and mass hierarchy thru e app. CP violation and mass hierarchy thru e app. Typically Multi-MW beam & Mton detector Typically Multi-MW beam & Mton detector 2 nd phase is critical step to go 2 nd phase is critical step to go Classification by “ Super Beam ” Experiments ()() ()()
4 e appearance & CPV e appearance & CPV , a -a for Matter eff.: CP-odd Solar Main Matter # of signal ∝ sin 2 13 (Stat err ∝ sin 13 ), CP-odd term ∝ sin 13 Sensitivity indep. from 13 (if no BG & no syst. err)
5 CPV vs matter effect 295km730km Smaller distance/lower energy small matter effect Pure CPV & Less sensitivity on sign of m 2 Combination of diff. E&L help to solve. e osc. probability w/ 2 2 13 =0.01
6 High intensity narrow band beam -- Off-axis (OA) beam -- (ref.: BNL-E889 Proposal) Target Horns Decay Pipe Far Det. Decay Kinematics Increase osc. max. Decrease background from HE tail 1/~1/~ E (GeV) E (GeV) flux
7 Idea of C2GT (CNGS to Gulf of Taranto) OA-CNGS OA-CNGS Movable underwater Cherenkov det. (r=150m), 2Mt fid vol, L=1,200~1,600km Movable underwater Cherenkov det. (r=150m), 2Mt fid vol, L=1,200~1,600km ~5,000 CC/year ~5,000 CC/year Disappearance & Appearance Disappearance & Appearance sin 2 2 13 sin 2 2 13 Technology to be established (underwater, light collection, LE PID, … ) Technology to be established (underwater, light collection, LE PID, … ) F.Dydak et.al. E GeV) Flux (m -2 ) e 1
8 Kamioka J-PARC (Tokai-mura)T2K-II (0.75MW )4MW 50GeV J-PARC (0.75MW )4MW 50GeV J-PARC OA 2~3deg OA 2~3deg E peak=0.5 ~0.8GeV E peak=0.5 ~0.8GeV L=295km L=295km Hyper Kamiokande Hyper Kamiokande ~360k CC/yr ~360k CC/yr 13, CPV 13, CPV Small matter effect Small matter effect OAB2.0deg OAB2.5deg OAB3.0deg
9 J-PARC (Japan Proton Accelerator Research Complex) Linac 3GeV PS 50GeV PS (0.75MW) N FD Neutrino Beam Line To SK Pacific Ocean (formerly known as JHF) Construction: 2001~2007 Construction: 2001~ MW 50GeV-PS 0.75MW 50GeV-PS Possible upgrade to 4MW Possible upgrade to 4MW Preliminary study done Preliminary study done Rep. rate x 2.5 Rep. rate x 2.5 Double RF cavities (space OK) Double RF cavities (space OK) Eliminate idling time in acc. cycle Eliminate idling time in acc. cycle Double # of circulating protons Double # of circulating protons “ barrier bucket method ” to avoid space charge limit “ barrier bucket method ” to avoid space charge limit Issues Issues Achieve first goal (0.75MW) Achieve first goal (0.75MW) Beam loss Beam loss Target, … Target, … (these apply also for other projects)
10 J-PARC December, 2003 Tokai-village December, 2003
11 2 detectors×48m × 50m ×250m, Total mass = 1 Mton Far Detector: Hyper-Kamiokande
T.Kobayashi (KEK) 12 Sensitivity for 13 sin 2 2 13 ~0.006 (90%) sin 2 2 13 < can be searched if syst err ~ few % 0.5xsin 2 2 13 sin 2 2 13 ~0.018 (3 )
13 / CC interaction spectrum for CPV meas. / CC interaction spectrum for CPV meas. Wrong sign BG (x10 case) cross section difference N CC (/100MeV/22.5kt/year) : 2 years : 6.8 years
14 sin 2 2 13 =0.02 Very Preliminary Expected signal and BG (SK full sim) signalbackground =0 = /2 total e e e e m 21 2 =6.9x10 -5 eV 2 m 32 2 =2.8x10 -3 eV 2 12 =0.594 23 = /4 13 =0.05 (sin 2 2 13 =0.01) :2yr, :6.8yr 4MW 0.54Mt
T.Kobayashi (KEK) 15 Sensitivity for CPV in T2K-II no BG signal stat only (signal+BG) stat only stat+2%syst. stat+5%syst. stat+10%syst. CHOOZ excluded sin 2 2 13 m 31 2 ~3x10 -3 eV 2 T2K 3 discovery 3 CP sensitivity : | |>20 o for sin 2 2 13 >0.01 with 2% syst. 4MW, 540kt 2yr for 6~7yr for m 21 2 =6.9x10 -5 eV 2 m 32 2 =2.8x10 -3 eV 2 12 =0.594 23 = /4 T2K-I 90%
16 Europe: SPL Frejus Geneve Italy 130km 40kt 400kt 4MW 2.2GeV Superconducting Proton Linac CERN 4MW 2.2GeV Superconducting Proton Linac CERN Low energy wide band (E ~0.3GeV) Low energy wide band (E ~0.3GeV) L=130km L=130km Water Cherenkov 40 400kt (UNO) Water Cherenkov 40 400kt (UNO) ~18,000 CC/year/400kt ~18,000 CC/year/400kt 13, CPV 13, CPV Small matter effect Small matter effect SPL in R&D, UNO in conceptual design SPL in R&D, UNO in conceptual design
17 Mezzetto Fluxes for SPL beam Low energy wide band beam Low energy wide band beam Less NC 0 BG for e search Less NC 0 BG for e search
18 13 Sensitivity for CPV sin 2 2 13 =0.03 13 (deg) 2 5 (deg)
19BNL-Homestake 28GeV AGS upgrade to 1MW (2MW) cf current 0.1MW 28GeV AGS upgrade to 1MW (2MW) cf current 0.1MW Wide band beam (0.5~6GeV) Wide band beam (0.5~6GeV) L=2,540km L=2,540km Mton UNO (alternative option: Liq. Ar.) Mton UNO (alternative option: Liq. Ar.) ~13,000 CC/year/500kt ~13,000 CC/year/500kt Cover higher osc. maxima Cover higher osc. maximaGoals e appearance e appearance Sign of m 23 Sign of m 23 CPV CPV 12, m 12 12, m 12 Possible w/ only run at certain parameter region (Ref: Diwan et al., PRD68, , 2003) 2540 km Homestake BNL
Page 20 S. Holmes, Mulit-MW Workshop, May 2004 Brookhaven AGS Upgrade Direct injection of ~ 1 protons via a 1.2 GeV sc linac extension –low beam loss at injection; high repetition rate possible –further upgrade to 1.5 GeV and 2 protons per pulse possible (x 2) 2.5 Hz AGS repetition rate –triple existing main magnet power supply and magnet current feeds –double rf power and accelerating gradient –further upgrade to 5 Hz possible (x 2)
21 Detector options: UNO (or Liq. Ar?) Highway tunnel Detector Perlite insulation h =20 m ≈70 m Electronic crates A. Rubbia C.K.Jung 440kton fiducial mass A.Rubbia ~100kton
22 Mass Hierarchy Resolution w/ only running, reversed hierarchy rejected >2.5 level w/ only running, reversed hierarchy rejected >2.5 level with w/ / running, then >10 with w/ / running, then >10 Diwan, Mar.2004
23 Sensitivity on CPV Diwan, Mar.2004
24 Fermilab Proton Driver (PD) 8 GeV synchrotron option Original concept (May 2002, Fermilab-TM-2169) Original concept (May 2002, Fermilab-TM-2169) Large aparture (100x150mm) magnets Large aparture (100x150mm) magnets LINAC 400MeV 600MeV LINAC 400MeV 600MeV MI cycle time 1.87s 1.53s MI cycle time 1.87s 1.53s Net results : MI power of 1.9MW 8 GeV superconducting linac Recent study Recent study Direct injection Direct injection 8GeV & 40~120GeV(MI) 8GeV & 40~120GeV(MI) Future flexibility Future flexibility Issue: Cost? Issue: Cost? Replace injector for Main Injector Increase MI power by x5~6 (2MW) Improve MINOS & NO A sensitivities
25 ~ 700m Active Length 2 MW 8 GeV Linac X-RAY FEL LAB Slow-Pulse Spallation Source & Neutrino Target Neutrino “Super- Beams” Main MW 8 GeV NUMI Anti- Proton SY-120 Fixed- Target Off- Axis Also includes upgrades to Main Injector for current and cycle To Homestake 120 GeV and 8 Gev Potential Flexibility of LINAC B.Foster and D.Michael, BNL-APS SB WS Mar.04
26 NO A + PD : Mass hierarchy G.Feldman Jun.04
27 Homestake BNL Henderson Mine Fermilab ~8m ~200M ~4m 30 mR maximum off axis 120 GeV protaons 8 GeV protons Another possibility with PD 1290km A case study for future experiment with PD A case study for future experiment with PD 2MW 8/120GeV PD “ 4MW ” 2MW 8/120GeV PD “ 4MW ” WB/OA to (or Henderson) WB/OA to (or Henderson) E =0.5~3GeV E =0.5~3GeV Cover higher osc max Cover higher osc max 500kt WC or 100kt Liq.Ar 500kt WC or 100kt Liq.Ar ~50k CC/year/500kt ~50k CC/year/500kt Studies of physics potential started Studies of physics potential started FeHo (Fermilab-Homestake) Beam Line D.Michael 5yrs
28 Sensitivities with 500kt Water C D.Michael May 04, FNAL ( m 2 )<1% (sin 2 2 )~4% (90%) Disappearance Appearance 100kt Liq Ar could be better thanks to det. resolution Studies in progress. 5yrs running
29 Summary of ( “ super-beam ” ) LBL experiments E p (GeV)Power(MW) Bea m 〈 E 〉 (GeV)L(km) M det (kt) CC CC(/yr) K2K WB ~50~1% MINOS(LE)1200.4WB ~2,5001.2% CNGS4000.3WB18732~2~5,0000.8% T2K-I500.75OA ~3,0000.2% NO A OA~2810?50~4,6000.3% C2GT4000.3OA0.8~12001,000?~5,0000.2% T2K-II504OA0.7295~500~360,0000.2% NO A+PD 1202OA~2810?50?~23,0000.3% BNL-Hs281WB/OA~12540~500~13,000 SPL-Frejus2.24WB ~500~18,0000.4% FeHo8/120 “4”“4”“4”“4”WB/OA1~31290~500~50,000 Running, constructing or approved experiments I II III
x m 2 (L/E) [ /2] T2K-II K2K MINOS CNGS NO A T2K-I C2GT NO A+PD BNL-Hs (<5 ) SPL-Frejus 13 5 osc. maxima BNL-Hs C2GT NO A MINOS CNGS T2K K2K SPL-Frejus “ Graphical ” Summary of experiments m 2 =2.5x10 -3 eV 2 <30GeV FeHo FeHo <10yrs 10~20yrs <5yrs
31Summary Next generation “ Super Beam ” experiments will provide chances to clarify whole view of mixing Next generation “ Super Beam ” experiments will provide chances to clarify whole view of mixing 13 13 CPV, sign of m 2,.. CPV, sign of m 2,.. High precision measurements of parameters High precision measurements of parameters Several experiments are under consideration Several experiments are under consideration (Multi-)MW beam + Mton detector (or Liq.Ar) (Multi-)MW beam + Mton detector (or Liq.Ar) Japan: 4MW J-PARC Mt Hyper-Kamiokande Japan: 4MW J-PARC Mt Hyper-Kamiokande Europe: 4MW 2.2GeV SPL Mt UNO Europe: 4MW 2.2GeV SPL Mt UNO US-BNL: 1(2)MW AGS US-BNL: 1(2)MW AGS US-FNAL: 2MW PD/MI NO A/ US-FNAL: 2MW PD/MI NO A/ Future direction much depend on results from “ 2 nd phase ” experiments Future direction much depend on results from “ 2 nd phase ” experiments T2K-I(2009~) and NO A(if approved) T2K-I(2009~) and NO A(if approved) Let ’ s do experiments to know 13 (2 nd phase) ASAP!!, Let ’ s do experiments to know 13 (2 nd phase) ASAP!!, While keeping R&D efforts for future projects While keeping R&D efforts for future projects (while reducing too many meeting!) (while reducing too many meeting!)