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Status of the SuperB Project Status of the SuperB Project

Status of the SuperB Project - PowerPoint Presentation

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Status of the SuperB Project - PPT Presentation

A major new European particle physics project Fergus Wilson RALSTFC On behalf of the SuperB Project Beauty 2011 April 8 th 2011 Outline Unique Selling Points USPs Snapshot of SuperB ID: 416113

2011 superb 8th ral superb 2011 ral 8th april physics fergus wilson stfc funding higgs 2010 year lhc tan

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Slide1

Status of the SuperB Project

A major new European particle physics project

Fergus Wilson, RAL/STFCOn behalf of the SuperB ProjectBeauty 2011, April 8th 2011Slide2

Outline

Unique Selling Points (USPs)Snapshot of SuperB Physics

Project SiteAccelerator Design OverviewDetector Design OverviewProject Funding (€€€€€)Preliminary ScheduleConclusion and Outlook8th April 2011Fergus Wilson, STFC/RAL2Slide3

Unique Selling Points (USPs)

New European Accelerator Facility to be sited in Italy, ready by 2016At Υ(4S), 6.7

GeV positrons on 4.18 GeV electrons, 1.3 km circumferenceHigh Luminosity (100 x current records)≥1036 cm-2 s-1 15 ab-1/year rising to 40 ab-1/year in later years1 ab-1 => 1 billion B-meson pairs and 1 billion tau pairs75 ab-1 by 2022Polarization60%-85% polarization of electron beamImproves physics reach by factor of 2 in some regions (e.g. LFV)ψ(3770) to ϒ(5S) and beyondCan scan a large energy range.

Switching from low-energy to high-energy running very quick (no more than a few weeks if magnets need to be swopped).Charm Threshold Running2 months running equivalent to 100 x

CLEO-c dataset.Light Source30 x brighter than ESRF or Diamond Light Source.ComputingOn the scale of a non-upgraded LHC experiment.

8th April 2011

Fergus Wilson, STFC/RAL

3Slide4

SuperB Physics Goals – Executive Summary

Physics capabilities published in 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→K

υυ, B→τυ

, τ→μυυInterplay with

Lattice QCD predictions.8th April 2011

Fergus Wilson, STFC/RAL

4Slide5

Physics - What will the CKM look like in 2022?

8th April 2011Fergus Wilson, STFC/RAL

5Slide6

Physics - The Golden Matrix

Each mode is a golden signature of New Physics.

Overlap with LHC8th April 20116Fergus Wilson, STFC/RALL=Large,M=Measurable deviation from SM

tanβ

=60tan

β=5

Sensitive region

(>3

σ

)Slide7

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

.

7

Fergus Wilson, STFC/RALSlide8

Physics – Charged Higgs (2HDM and MSSM)

8th April 2011

Fergus Wilson, STFC/RAL8SuperB excludesSuperB excludesB-Factories excludeB-Factories excludeMSSM2HDM-II

B

→s

γ

/ LEP excludes

B

→s

γ

/ 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 HiggsSlide9

Physics - Lepton Flavour Violation

Model

BF(τ→μγ)mSUGRA+seesaw10-7SUSY+SO(10)10-8SM+seesaw, Z’10-9SUSY+Higgs10-10

SM + υ mixing

10-40

8th April 2011

Fergus Wilson, STFC/RAL

9

Many models predict LFV at the level that can be detected at SuperB

LFV also sensitive to other observable such as μ->

e

γ

(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...)Slide10

Physics - Charm and Charm CPV

CPV in SM very small => CPV indicates New PhysicsMeasure strong phases8th April 2011

Fergus Wilson, STFC/RAL10xDyD

Now

SuperB

SuperB+BESSuperB+

BES

(3770)

x (x 10

3

)

±3

±0.7

±0.4

±0.2

y (x 10

3

)

±2

±0.2

±0.2

±0.1

δ

k

π

±10

o

±3

o

±2

o

±1

o

δ

k

ππ

±20

o

±5

o

±3

o

±1

oSlide11

Benefits of Polarized Electron Beam

8th April 2011Fergus Wilson, STFC/RAL

111) LFV:Doubles Precision2) τ EDM, τ g-2:Measurement could prove or disprove discrepancy in Δαμ due to New Physics.EDM sensitivity ~ 2 x 10-19

e cmΔατ

(SM) ~ 10-6

Δα

τ

(SUSY) <~ 10

-5

Δ

α

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

SuperB

NuTev

XSlide12

San Vito

dei

Normanni, BrindisiTor VergataNot up to dateSite Decision8th April 2011Fergus Wilson, STFC/RAL

12

Frascati

A number of options – decision by May 2011Slide13

Machine Parameters are stable

8th April 2011

Fergus Wilson, STFC/RAL13Tau/charm threshold runningFlexibility built inModerate power < 20MWNo single critical element

Piwinski angle and crab-waist crossing test at

DaΦne

arXiv:1009.6178Slide14

Detector Design [arXiv:1007.4241]

8th April 2011Fergus Wilson, STFC/RAL

14Double Vertex resolution

Backward EMC

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 optionsSlide15

SuperB – Funding and Developments

SuperB approved through primary law by Italian parliament, December 14th/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 detectorConclusion: solid funding in an uncertain financial world.8th April 2011

Fergus Wilson, STFC/RAL

15Slide16

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 28th 2011 with Italian Science Minister (hopefully).Spokesperson: Marcello.Giorgi@pi.infn.it8th April 2011Fergus Wilson, STFC/RAL16Slide17

INFN Triennal plan (2010-2012)

8th April 2011

Fergus Wilson, STFC/RAL17ConstructionOperationSlide18

Preliminary Schedule

8th April 2011

Fergus Wilson, STFC/RAL18