Charm at : status and prospects
DHEP Seminar February2, 2012
Gagan MohantyTata Institute, Mumbai
Outline of the talk1) Introduction and motivation
2) KEKB SuperKEKB
3) Enter Belle II detector
4) Status of the project
5) Conclusions and prospects
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With a Higgs boson beingdiscovered at the LHC, thestandard model (SM) is onthe verge of completion
What is the fuss about?
Three complementary ways to probe thenew physics (NP) beyond the SM
However, there are many compelling reasons to believe that the SM cannotbe the full story
1) About ten orders of magnitude difference between the matter-antimatterasymmetry in universe and CP violation content of the SM
2) What is the nature of dark matter?
3) and, the list goes onEnergy (ATLAS, CMS)
Luminosity (LHCb, Belle II) Cosmic (neutrino, ray)
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Why a flavor factory in the LHC era?
A flavor factory (FF) studies processes that occur at one-loop level in the SMbut may be of O(1) in NP: FCNC, neutral meson mixing, CP violation. Theseloops probe energy scales that cannot be directly accessed at the LHC.
For instance, if SUSY is found at the LHC, the next question will be: how is itbroken. By studying various flavor-violating couplings the FF can address that.
NP
reac
hin
term
so
fm
ass
NP flavor-violating coupling
Illustration purpose only
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What’s so special about Belle II?
Low background, high trigger efficiency, excellent photon & 0 reconstructioncapability, high flavor-tagging efficiency with low dilution factor
Good kinematic resolution Dalitz-plot analyses are straightforward
Absolute branching fraction can be measured
Ideal for measuring decay channels with large missing energy
Thanks to its pristine e+e environment:
A sample of measurements at Belle II
Belle II TDR, arXiv:1011.0352
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Now, all these sound good. But why charm? Charm provides an interesting test bed for NP as SM footprints in this sector
are tiny owing to a) large GIM/CKM suppression, and b) the lack of a largehierarchy in the down-type quark masses
CP violation is expected (in the SM) to be the order of 103 an excellentNP probe [most promising candidate: singly Cabibbo-suppressed decays]
While talking about percentage effect, one needs a good control on SMpredictions, something that is in general lacking in this sector because oflong-distance effects
PRD 75, 036008 (2007)
An example of “short vs. long”
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Direct CP violation: probe# 1 for Belle II
Luminosities (results) shown on the second (third) column are from Belle
Looking ahead, Belle II has a big advantage over LHCb for the final states withneutral mesons (0, and )
Mode Lint [fb¡1] ACP [%] Belle II with 50 ab¡1 [%]D0 ! K0
S¼0 791 ¡0:28§ 0:19§ 0:10 §0:05D0 ! ¼0¼0 976 ±ACP ¼ 0:6%D0 ! K0
S´ 791 +0:54§ 0:51§ 0:16 §0:10D0 ! K0
S´0 791 +0:98§ 0:67§ 0:14 §0:10D0 ! ¼+¼¡ 976 +0:55§ 0:36§ 0:09 0:07D0 ! K+K¡ 976 ¡0:32§ 0:21§ 0:09 0:05D0 ! ¼+¼¡¼0 532 +0:43§ 1:30D0 ! K+¼¡¼0 281 ¡0:6§ 5:3D0 ! K+¼¡¼+¼¡ 281 ¡1:8§ 4:4D+ ! Á¼+ 955 +0:51§ 0:28§ 0:05 §0:05D+ ! ´¼+ 791 +1:74§ 1:13§ 0:19 §0:20D+ ! ´0¼+ 791 ¡0:12§ 1:12§ 0:17 §0:20D+ ! K0
S¼+ 977 ¡0:363§ 0:094§ 0:067 §0:05D+ ! K0
SK+ 977 +0:08§ 0:28§ 0:14 §0:10
D+s ! K0
S¼+ 673 +5:45§ 2:50§ 0:33 §0:30D+s ! K0
SK+ 673 +0:12§ 0:36§ 0:22 §0:10
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Rare and forbidden decays: probe# 2 for Belle II
(top) FCNC decays and(bottom) lepton flavor(LF), lepton number (L)& baryon-lepton number(BL) violating decays
Shaded regions indicatethe decays with a or 0,where Belle II will havean edge
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Is it all about more data? Any innovation?
Already have some good working examples from Belle and BaBarSee the talk of A. Zupanc
Charm tagging at B factory
Great prospects for Belle II especially for channels with missing neutrinosviz. D(s) l l and D0 K/ l l
arXiv:1307.6240
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The list can go on, let’s move to the project
Need 50 more data Enter SuperKEKB
40 times higherluminosity
81035
SuperKEKB
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(cm
2s
1)
(1) Smaller y*
(2) Increase beam currents
(3) Increase y
How to increase the luminosity?
Collision with very small spot-size beams
Invented by P. Raimondi at Frascati
“Nano-Beam” scheme
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-
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Machine design parameters of two machines
parametersKEKB SuperKEKB
unitsLER HER LER HER
Beam energy Eb 3.5 8 4 7 GeV
Half crossing angle φ 11 41.5 mrad
Horizontal emittance εx 18 24 3.2 4.6 nm
Emittance ratio κ 0.88 0.66 0.37 0.40 %
Beta functions at IP βx*/βy
* 1200/5.9 32/0.27 25/0.30 mm
Beam currents Ib 1.64 1.19 3.60 2.60 A
Beam-beam parameter ξy 0.129 0.090 0.0881 0.0807
Luminosity L 2.1 x 1034 8 x 1035 cm-2s-1
• Nano-beams and a factor of two more beam current to increase L• Large crossing angle• Change beam energies to solve the problem of short lifetime for the LER
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e 2.6 A
e+ 3.6 A
To obtain 40 higher luminosity
Colliding bunches
Damping ring
Low emittance gun
Positron source
New beam pipe& bellows
Belle II
New IR
TiN-coated beam pipewith antechambers
Redesign the lattices of HER &LER to squeeze the emittance
Add / modify RF systemsfor higher beam current
New positron target /capture section
New superconducting/permanent final focusingquads near the IP
Low emittanceelectrons to inject
Low emittancepositrons to inject
Replace short dipoleswith longer ones (LER)
KEKB to SuperKEKB
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Need to build a new detector
- low p m identification f smm efficiency- hermeticity f n “reconstruction”
- radiation damage and occupancy- fake hits and pile-up noise in the EM
- higher rate trigger, DAQ and computing
Critical issues at L= 8 1035 cm2s1
4 Higher background ( 10-20)
4 Higher event rate ( 10)
4 Require special features
Belle II
Have to employ and develop newtechnologies to make such anapparatus work!
Belle II TDR, arXiv:1011.0352 14
Enter Belle II
electrons (7 GeV)
positrons (4 GeV)
KL and muon detector:Resistive Plate Counter (barrel outer layers)Scintillator + WLS Fiber + SiPM (end-caps,inner 2 barrel layers)
Particle IdentificationTime-of-Propagation counter (barrel)Prox. focusing Aerogel RICH (forward)
Central Drift ChamberHe(50%):C2H6(50%), small cells, longlever arm, fast electronics
EM Calorimeter:CsI(Tl), waveform sampling (barrel)Pure CsI + waveform sampling (end-caps)
Vertex Detector2 layers DEPFET + 4 layers DSSD
Beryllium beam pipe2 cm diameter
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Belle II compared with Belle
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SVD: 4 DSSD layersg 2 DEPFET + 4 DSSD layersCDC: small cell, long lever armPID: ACC+TOFgTOP+A-RICHECL: waveform sampling (+pure CsI for endcaps)KLM: RPCg Scintillator+SiPM (endcaps, barrel inner 2 lyrs) 16
Vertex Detector (PXD+SVD)2 layers DEPFET + 4 layers DSSD
A close-up view of the vertex region
Beryllium beam pipe2cm diameter
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SVD
PXD
Beam Pipe r = 10mmPXD (2 layers DEPFET)
Layer 1 r = 14mmLayer 2 r = 22mm
SVD (4 layers DSSD)Layer 3 r = 38mmLayer 4 r = 80mmLayer 5 r = 104mmLayer 6 r = 135mm
Few words on PXD
DEPFET sensor: very good S/N
Mechanical mockup of the pixel detector
DEPFET pixel sensor
DEPFET:http://aldebaran.hll.mpg.de/twiki/bin/view/DEPFET/WebHome
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SVD: high-point and current status
Gearing up for ladder production!
Origami chip-on-sensor
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Mechanical mockup
+KS
IP profile
B vertex
B decay point reconstructionusing the KS trajectory
Larger radial coverageof SVD
Performance comparison
sin
ba
p
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Less Coulombscattering
Pixel detector closeto the beam pipe
CDC: Main tracking device
Much bigger than in Belle
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Wire stringing in a clean room Exceeding the expectation
Aerogel radiatorHamamatsu HAPD + readout
Barrel PID: Time of Propagation Counter (TOP)
Aerogel radiator
Hamamatsu HAPD+ new ASIC
200mm
n~1.05
Endcap PID: Aerogel RICH (ARICH)
200
PID devices
Quartz radiatorFocusing mirror
Small expansion blockHamamatsu MCP-PMT (measure t, x and y)
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Cherenkov ring imaging with precisetime measurement
Device uses the internal reflection ofCerenkov ring images from quartzsimilar to the BaBar DIRC
Reconstruct Cherenkov angle fromtwo hit coordinates and the time ofpropagation of the photon
Quartz radiator (2cm)
Photon detector (MCP-PMT)
Excellent time resolution ~40 ps
Single photon sensitivity in 1.5 T
Fast read-out electronics
Barrel PID: TOP counter
Hamamatsu SL10 MCP PMT 8 PMTs with read-out electronics
quartz bar
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TOP performance
LikelihoodFunctions:
pK
tim
e
B0gK+p- fullsimulation results:
Ng (signal) = 22Ng (bkg) = 15
ep = 92 % (Belle: 89%)eK = 7.4 % (Belle: 12%)
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Aerogel
Hamamatsu HAPD
Clear Cherenkov image observed
Endcap PID: Aerogel RICH
Test Beam setup
Cherenkov angle distribution
6.6 σ p/K at 4GeV/c !
RICH with a novel “focusing”radiator – a two-layer radiator
Employ multiple layers withdifferent refractive indicesCherenkov images from theindividual layers overlap onthe photon detector.
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Event size and rate: Belle II vs. LHC expts
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A snapshot of the Belle II computing model
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Belle II: a truly global collaboration
Recently several new additions from Italy and USA
A very strong group of over 500 highly motivated scientists!
SuperKEKB and Belle II ScheduleCommissioning in three phases:
Phase 1: w/o final quads and Belle II
basic machine tuning
low emittance beam tuning
vacuum scrubbing (at least a month at beamcurrents of 0.5-1 A)
Damping ring commissioning
Phase 2: with final quads and Belle II,but no vertex detector
low * beam tuning
small x-y coupling tuning
collision tuning
study beam background (carefully check thebeam background before VXD installation)
Phase 3: with QCS and full Belle II
physics run
luminosity increase
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SuperKEKB luminosity projection
Goal of Belle II/SuperKEKB
9 months/year20 days/month
Commissioning startsin early 2015
Shutdownfor upgrade
Inte
gra
ted
lum
ino
sit
y(a
b1)
Pe
ak
lum
ino
sit
y(c
m-2
s-1
)
Calendar Year
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Same size data as Belle
Aim to reach 50 ab1 by the end of 2022
Conclusions and future prospect
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e+e B factories have proven to be an excellent tool for flavor physics, producinga wealth of physics results, the most celebrated one being the confirmation of theKobayashi-Maskawa mechanism for CP violation in the SM
Thanks for your kind attention
Major upgrade of KEKB factory to SuperKEKB (50 data) will take this legacyforward by providing a suitable probe for NP complementary to LHC
Belle II at SuperKEKB should resolve current flavor puzzles from the presentgeneration B factory, e.g., difference in the UT angle 1 between b c tree andb s loop diagrams, possible enhanced loop contribution in B K decays
It will also have a prolific charm physics program: should greatly improve theprecision of mixing/CPV parameters (together with LHCb) and should probe NPby diligently searching for direct CP asymmetries and rare and forbidden decays
2008