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Status of the SuperB Project A major new European particle physics project Fergus Wilson, RAL/STFC On behalf of the SuperB Project Beauty 2011, April 8 th 2011
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Outline Unique Selling Points (USPs) Snapshot of SuperB Physics Project Site Accelerator Design Overview Detector Design Overview Project Funding (€€€€€) Preliminary Schedule Conclusion and Outlook 8th April 2011 Fergus Wilson, STFC/RAL2
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Unique Selling Points (USPs) New European Accelerator Facility to be sited in Italy, ready by 2016 o At Υ(4S), 6.7 GeV positrons on 4.18 GeV electrons, 1.3 km circumference High Luminosity (100 x current records) o ≥ 10 36 cm -2 s -1 15 ab -1 /year rising to 40 ab -1 /year in later years o 1 ab -1 => 1 billion B-meson pairs and 1 billion tau pairs o 75 ab -1 by 2022 Polarization o 60%-85% polarization of electron beam o Improves physics reach by factor of 2 in some regions (e.g. LFV) ψ (3770) to ϒ (5S) and beyond o Can scan a large energy range. o Switching from low-energy to high-energy running very quick (no more than a few weeks if magnets need to be swopped). Charm Threshold Running o 2 months running equivalent to 100 x CLEO-c dataset. Light Source o 30 x brighter than ESRF or Diamond Light Source. Computing o On the scale of a non-upgraded LHC experiment. 8th April 2011 Fergus Wilson, STFC/RAL3
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SuperB Physics Goals – Executive Summary Physics capabilities published in arXiv:1008.1541.arXiv:1008.1541 Identify the flavour structure of New Physics. Different New Physics models predict a different hierarchy of results => multiple measurements needed. Sensitive to New Physics through flavour properties; CP Violation asymmetries in B and D decays; and rare decays. Probe New Physics scales up to 10-100 TeV through indirect measurements. Tests both the quark and lepton sectors. Golden Channels (good SM prediction + good experimental resolution) e.g. inclusive b →sγ, B→Kυυ, B→τυ, τ→μυυ Interplay with Lattice QCD predictions. 8th April 2011 Fergus Wilson, STFC/RAL4
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Physics - What will the CKM look like in 2022? 8th April 2011 Fergus Wilson, STFC/RAL5
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Physics - The Golden Matrix Each mode is a golden signature of New Physics. Overlap with LHC 8th April 2011 6Fergus Wilson, STFC/RAL L=Large,M=Measurable deviation from SM tan β=60 tan β=5 Sensitive region (>3 σ)
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Physics – LHC and SuperB interplay 8th April 2011 Blue = LHC: Can measure m(A) [CP odd Higgs mass] Insensitivity to tanβ [ratio of Higgs vevs] Poor sensitivity to A [coupling] Red=LHC+EW/Low-energy (includes SuperB): Can build on the m(A) measurement to measure tanβ. Current analysis of data prefers tanβ ~10. 7Fergus Wilson, STFC/RAL
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Physics – Charged Higgs (2HDM and MSSM) 8th April 2011 Fergus Wilson, STFC/RAL8 SuperB excludes B-Factories exclude MSSM2HDM-II B →sγ / LEP excludes ATLAS 30fb -1 Higgs-mediated Minimal Flavour Violation Multi-TeV search capability for large tanβ. Includes SM uncertainty ~20% from V ub and f B. B 0 →l + l - and B 0 →l - τ + also sensitive to non-SM Higgs
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Physics - Lepton Flavour Violation ModelBF( τ→μγ) mSUGRA+seesaw10 -7 SUSY+SO(10)10 -8 SM+seesaw, Z’10 -9 SUSY+Higgs10 -10 SM + υ mixing10 -40 8th April 2011 Fergus Wilson, STFC/RAL9 Many models predict LFV at the level that can be detected at SuperB LFV also sensitive to other observable such as μ->eγ (MEG),θ 13 (T2K) and B s mixing phase (LHCb) Polarization doubles sensitivity (not included in numbers below) Example: SU(5) SUSY GUT Theory Predictions: SuperB: Over 50 τ decays can be measured (not to mention spectral functions, second class currents etc...)
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Physics - Charm and Charm CPV CPV in SM very small => CPV indicates New Physics Measure strong phases 8th April 2011 Fergus Wilson, STFC/RAL10 xDxD yDyD
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Benefits of Polarized Electron Beam 8th April 2011 Fergus Wilson, STFC/RAL11 1) LFV: Doubles Precision 1) LFV: Doubles Precision 2) τ EDM, τ g-2: Measurement could prove or disprove discrepancy in Δα μ due to New Physics. EDM sensitivity ~ 2 x 10 -19 e cm Δα τ (SM) ~ 10 -6 Δα τ (SUSY) <~ 10 -5 Δα τ (SuperB) precision~ 10 -6 2) τ EDM, τ g-2: Measurement could prove or disprove discrepancy in Δα μ due to New Physics. EDM sensitivity ~ 2 x 10 -19 e cm Δα τ (SM) ~ 10 -6 Δα τ (SUSY) <~ 10 -5 Δα τ (SuperB) precision~ 10 -6 3) Electroweak: Investigate LEP A FB v. SLD A LR discrepancy. Investigate NuTev discrepancy. Constrain Higgs mass Sin 2 θ w resolution ±0.00018 3) Electroweak: Investigate LEP A FB v. SLD A LR discrepancy. Investigate NuTev discrepancy. Constrain Higgs mass Sin 2 θ w resolution ±0.00018 SuperB NuTev X
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San Vito dei Normanni, Brindisi Tor Vergata Not up to date Site Decision 8th April 2011 Fergus Wilson, STFC/RAL12 Frascati A number of options – decision by May 2011
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Machine Parameters are stable 8th April 2011 Fergus Wilson, STFC/RAL13 Tau/charm threshold running Flexibility built in Moderate power < 20MW No single critical element Piwinski angle and crab-waist crossing test at Da Φ ne arXiv:1009.6178
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Detector Design [arXiv:1007.4241]arXiv:1007.4241 8th April 2011 Fergus Wilson, STFC/RAL14 Double Vertex resolution Backward EMC Logging rate: 1.9 Gbytes/sec Logging rate: 1.9 Gbytes/sec Optimized IFR (muons) TOF Forward PID Cluster counting in drift chamber (improves dE/dx) Reuses much of BaBar e.g. CsI crystals Improved hermiticity SuperB baseline SuperB with options
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SuperB – Funding and Developments SuperB approved through primary law by Italian parliament, December 14 th /15 th 2010. Parliament also approved INFN “Piano Triennale” 2010-2012 funding profile which includes SuperB. SuperB is a “Progetti Bandiera” national flagship project. 8% of national research budget allocated to flagship projects. 19M€ in 2010, 50M€ per year thereafter until EOY 2015. SuperB is the only project receiving multi-year funding so far. ~120M$ in-kind contribution from US through use of PEP-II machine components and BaBar detector. 50M€ allocated for Tier 2 Grid computing centres in Southern Italy. ~100M€ via Italian Institute of Technology (IIT) for beam-lines. Only ~25M€ needed from international collaborators for detector Conclusion: solid funding in an uncertain financial world. 8th April 2011 Fergus Wilson, STFC/RAL15
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Conclusion and Outlook August 2010: Physics, Accelerator, Detector reports published. SuperB has been approved by the Italian Government, December 2010, as a “Flagship” project. A unique opportunity for Europe and International Collaboration. The necessary funding is in place. First beams in 2016. 15 ab -1 /year rising to 40 ab -1 /year. Site selection to be announced May 2011. Present participation in preparation by Italy, Canada, France, Germany, Poland, Russia, Spain, UK, US. Collaboration is still growing. Working towards TDR. Opportunities in detector, accelerator, computing and physics. First formal meeting Elba, May 28 th 2011 with Italian Science Minister (hopefully). Spokesperson: Marcello.Giorgi@pi.infn.it 8th April 2011 Fergus Wilson, STFC/RAL16
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INFN Triennal plan (2010-2012) 8th April 2011 Fergus Wilson, STFC/RAL17 Construction Operation
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Preliminary Schedule 8th April 2011 Fergus Wilson, STFC/RAL18
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