David Hitlin DOE Annual Review July 10, 2008 1 SuperB The Super Flavor Factory David Hitlin DOE Annual Review of Caltech July 10, 2008
Dec 20, 2015
David Hitlin DOE Annual Review July 10, 2008 1
SuperB The Super Flavor
Factory
David HitlinDOE Annual Review of Caltech
July 10, 2008
David Hitlin DOE Annual Review July 10, 2008 2
SuperB – the Super Flavor Factory
The Caltech group led the way in recognizing the importance of continuing flavor studies in e+e- substantially beyond the level achievable at BABAR and Belle
The crucial role that flavor physics will play in understanding New Physics found at the LHC is becoming ever more clear to the community
Sensitivity to New Physics at scales accessible to the LHC requires 50-75 ab-1 ⇒ luminosity of 1036
Achieving this luminosity with reasonable power consumption and currents low enough to make the detector background problem tractable is not an easy problem
With SLAC and then Frascati colleagues, several approaches were tried Scale up PEP-II in the existing tunnel– more bunches, more current Revisit old idea of colliding linacs with high disruption- not attractive Use very low emittance rings, like the ILC damping rings, but collide at
an angle with a new final focus scheme – the crabbed waist Several workshops have been held to investigate the physics capabilities
of a Super Flavor Factory Efforts are now centered on SuperB, an international project hosted by
INFN in Italy
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Primary physics objectives of a Super Flavor Factory
Perform measurements in the flavor sector such that: If new particles are discovered at LHC we are able to study the
flavor structure of the New Physics If the New Physics scale is beyond the reach of the LHC,
explore the New Physics scale
More specifically Is there charged lepton flavour violation (LFV) ? Are there new CP-violating phases in b,c or decay ? Are there new right-handed currents ? Are there new loop contributions to flavor-changing neutral currents Are there new Higgs fields ? Is there new flavor symmetry that elucidates the CKM hierarchy ?
We must also understand the requirements for a detector that can address these questions in a 1036 asymmetric e+e- environment ?
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Prospects for a Super Flavor Factory The recent P5 report recommends, in Scenario B and above,
US participation in an overseas Super B factory There are two proposals on the market
SuperKEKB, an upgrade of KEKB, with an initial luminosity of 1-2 x 1035
and an upgrade path to 4-8 x 1035 by 2027, using 83 MW SuperB, a new low emittance collider, with an initial luminosity of
1036 using 17 MW, and an upgrade path to 4 x 1036, to be built atRome II University “Tor Vergata”, using many PEP-II components
This talk will concern SuperB
320 signers80 institutions
INFN has now made aformal request to SLAC for
PEP-II and BABAR Components
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SuperB One Pager SuperB is a Super Flavor Factory with very high initial luminosity,
1036, which can be upgraded to 4x1036 in a straightforward manner It is asymmetric : 4 on 7 GeV Most of the ring magnets can be reused from PEP-II, as can the RF systems,
many vacuum components, linac and injection components – as well as BABAR as the basis for an upgraded detector – the net in-kind value is $270M
The high energy beam can be linearly polarized to ~85% , using the SLC laser gun This is particularly important for confronting New Physics in decays
The primary ECM will be the (4S), but SuperB can run elsewhere in the region, and in the charm &tau threshold regions as well, with a luminosity above 1035
One month at the (3770), for example, yields 10x the total data sample that will be produced by BEPCII
SuperB will be built on the campus of the Rome II University at Tor Vergata There is an FEL already in early stages of construction on the site Tunneling will continue to dig the SuperB tunnel, funded by Regione Lazio
Time scales (Successful) conclusion of the European Roadmap process (INFN, ECFA,
CERN Strategy Group) by the end of 2008, followed by INFNMinistry TDR effort is beginning: construction 5 years : luminosity in 2015-16
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INFN International Review Committee ReportMembers: H. Aihara, J.B. Dainton (chair), R. Heuer (to Nov 07), Y. K. Kim,
J. Lefrançois, A. Masiero, S. Myers (for April 08), T. Nakada (RECFA from April 08), D. Schulte, A. Seiden
Conclusions
● Strongly recommend continuation of work for 1036 cm-2 s-1 asymmetric e+e- collider
● Even more concerted effort to fully evaluate physics potential ↔ machine specifications ● Major design program to establish credibility of machine now critical ← showstoppers ? ● Machine Advisory Committee (MAC) now essential ● Preservation of detector and PEP2 components
● Increasing global involvement if timescale for a TDR is to be met
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SuperB Experimental Hall & Transfer Line
-+
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SuperB arameters
Beam-beamtransparencyconditions inred
SuperKEKB
3.5 80.8 (0.4)
5000 12 | 5
9.4 | 4.1 3 200
9 (24) 0.36742
330
83
0.2090.405
45
IP beam distributions
for KEKB
IP beam distributions for
SuperB(without
transparency conditions)
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Crabbed waist beam distribution at the IP
Crab sextupoles
OFF
Crab sextupoles
ON
waist is orthogonal to the axis of bunch
waist moves to the axis of other beam
All particles from both beams collide in the minimum y region, with a net luminosity gain
E. Paoloni
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Charm FCNC
Charm mixing and CPVB Physics: (4S)
PhysicsBs Physics: (5S)
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polarized e- beam: reduced background
Very important order of magnitude 10-8 10-9
Complimentarity with e
A Super Flavor Factory is also a factory Lepton Flavor Violation
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LFV in decays: SuperB capability
SuperB sensitivity directly confronts many New Physics models BABAR
SuperBsensitivityFor 75 ab-1
We expect to see LFV events, not just improve limits
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Why do we need a very large sample ~75ab-1 ?
Im (
13) L
L
Im (
13) L
L
Re (13)LL Re (13)LL
SM SM
Example: CPV in loop B decays
Determination of coupling [in this case : (13)LL] with 10 ab-1 and 75 ab-1
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Caltech’s role in SuperB and US the collaboration We are clearly to engine behind US SuperB activities
Member of Steering Committee Leading and actively working in the R&D group on EMC upgrade for the
revised BABAR detector Contributing to development of Monte Carlo and reconstruction
software to optimize the EMC in particular, and the overall detector Working towards formation of a US contingent of the SuperB
Collaboration Expect 100-150 US collaborators
A meeting to inform potential US participants is scheduled for July 25
The proto-Collaboration has already produced an impressive CDR The group is now entering the TDR phase
For the US to be well-positioned as TDR responsibilities are worked out over the next year or so, some actual resources will soon be needed INFN is beginning to provide R&D funding for Italian groups On the appropriate time scale and in the appropriate way, the US
groups need support of this kind
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Ren-yuan Zhu, with ADR funds, has been for several years, workingon the development of LYSO crystals for HEPVery attractive for the SuperB endcap EMC and the CMS upgrade
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5x5 Projective LYSO array with CsI(Tl) surround
A 7x7 array is best, but it can beapproximated by a 5x5 arraysurrounded by CsI(Tl) to catchthe outer few percent of shower
CMS APD readout module2 @ 5mmx5mm APD(10x10mm APDs are now available)
16 spare BABAR CsI(Tl)crystals may be available
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High statistics flavor physics (50-75 ab-1) at an e+e- collider will likely provide information crucial to the understanding of new physics found at LHC SuperB, with an initial luminosity of 1036 cm-2s-1 can provide such a
sample in the canonical five years The achievable levels of sensitivity in rare b, c and decays allow
substantial coverage in the parameter space of new physics SuperB presents a strong physics opportunity for the US community
US participation in SuperB would leverage $270M of PEP-II and BABAR components through an in-kind contribution
New funding of $10-20M/year over the TDR and construction period would also be needed to allow US participation in design and construction of the collider and detector upgrade
Such participation in encouraged by P5 in Scenario B and above We are working towards a turn-on date of 2015/16
The Caltech group will, as it did in PEP-II and BABAR, play a central role in SuperB, should it go forward
We propose to begin by transitioning from the current intense analysis phase of BABAR into the TDR phase of SuperB
Conclusions
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From the SuperKEKB web page
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Q&A Is there a motivation to continue e+e- flavor physics studies with a
Super B factory beyond the BABAR/Belle/(LHCb) era ? Yes – provided that new measurements have sensitivity to New
Physics in b, c and decay What size data sample is required to provide this sensitivity ?
50-75 ab-1 (BABAR+Belle total sample is <2 ab-1) What luminosity is required to gather a sample of this size in five
years ? At least 1036 cm-2s-1
Can an asymmetric collider with this luminosity be built ? Yes, using an innovative new approach: a low emittance collider,
based on concepts developed for the ILC damping rings, and employing a new type of final focus – a “crabbed waist”. The machine is called SuperB
Can a detector be built that can withstand the machine backgrounds ? Yes. The beam currents are less than those at PEP-II and KEKB
In this era of increasing energy prices, can you pay the power bill ? Yes. The wallplug power, 17MW, is less than half that of KEKB
(40mw)
David Hitlin DOE Annual Review July 10, 2008 25
SuperB+Lattice improvements
Interplay between metrology and New Physics sensitivity
Today
= ± 0.0028 = ± 0.0024
= 0.163 ± 0.028 = 0.344± 0.016
Improving the precision of Unitarity Triangle measurements, along with reducing theoretical uncertainties, can provide evidence
for New Physics
David Hitlin DOE Annual Review July 10, 2008 26
CMSSM : e vanishes at all SPS points MVF-NP extensions : e vanishes as s130is independent of s13
1 1 7510ab : 75ab for ( ), 7.5 for ( )
10 B B
LFV
2
5 disc
B B
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107 B
(
M 1
/2
SuperB
SO(10) MSSMLFV from PMNS
LFV from CKMBeyond MFV
SUSY GUTnow
SuperB
Recent work :J.K.Parry, H.-H. Zhanghep-ph/0710.5443
Allowed by ms
From Bs phase
now
SuperB
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t -¬
t -¬
t -¬ t -
¬
Flipping the helicity of the polarizedelectron beam allows us todetermine the chiral structureof dimension 6 four fermionlepton flavor-violating interactions
t -¬ t -
¬
Polarized ’s can probe the chiral structure of LFV
Dassinger, Feldmann, Mannel, and TurczykJHEP 0710:039,2007;
[See also Matsuzaki and SandaarXiv:0711.0792 [hep-ph]
t -¬t-¬
t -¬ -
¬ -
¬
-¬ -
¬
-¬
David Hitlin DOE Annual Review July 10, 2008 29
SPS4 is ruled out by exp value of (Bs)
SPS1a is the least favorable for flavor effects, but SuperB and only SuperBcan observe 2 deviations in several observables
Minimal Flavor Violation : SNOWMASS points
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Many channels can show effects in the range S~(0.01-0.04)
New Physics in CPV: sin2 from “s Penguins”…
SuperB
(*) theory limited
d d
sb
W-
B0d
t ss
K0
g
sb b s
~
~ ~
23d
LR
X
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1 10
1
10-1
10-2 (TeV)gluinom
is measured with a significance >3 away
from zero
23| |LR
23| |LR
Arg(23)LR=(44.5± 2.6)o
= (0.026 ± 0.005)
1 10
g
sb b s
~
~ ~
New Physics contribution (2-3 transitions)
23d
LR
MSSM + generic soft SUSY breaking terms
Flavor-changing NP effects in the squark propagator NP scale SUSY mass
flavor-violating coupling X
0.01
0.1
2
, ,
2, ,
( )qij LR RR LLq
ij LR RR LL
M
m
~ gm m
David Hitlin DOE Annual Review July 10, 2008 32
KB
Exhibit B: SM Branching fractions: Current 10ab-1 75ab-1 * , ( )SB K K K
Actual limit
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CP Violation in charmNOW
SuperB