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![Page 1: What’s the matter with anti-matter? A short history of CP violation Gabriella Sciolla M.I.T. Outline: The physics of CP violation What is CP and why is.](https://reader033.fdocuments.us/reader033/viewer/2022051717/5a4d1b647f8b9ab0599af62f/html5/thumbnails/1.jpg)
What’s the matter with anti-matter?
A short history of CP violation
Gabriella Sciolla M.I.T.
Outline: The physics of CP violation
What is CP and why is it interesting? CP in particle physics
The “Standard Model”: a crush course Measurements of CP violation
Tests of Standard Model and probe to New Physics
Conclusion Summary & Prospects
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Symmetries and Physics Symmetries are a constant theme in Physics
“For every continuous symmetry of the laws of physics, there must exist a conservation law” Noether’s theorem
Continuous Symmetries Translational symmetry:
All positions in space are physically indistinguishable Consequence: momentum p is conserved
Rotational symmetry: All directions in space are physically indistinguishable Consequence: Angular Momentum L is conserved
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Discrete Symmetries Parity (P)
Flips the space coordinates: Example:
Time Reversal (T) Physics invariant when
Charge Conjugation (C) Transforms matter into corresponding anti-
matter
x xy yz z
( ) ( )P e p e p
t t
( ) ( )C e p e p
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Are C, P and T good symmetries of Nature?
Strong and Electromagnetic Interactions Conserve separately P and C
Weak Interaction Known to maximally violate both C and P
Wu et al. 1957 Only left-handed and right-handed anti- exist
C,P,T: Symmetries of Nature?
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
CPT Theorem and CP conservation
The CPT Theorem “In any relativistic quantum field theory the
product CPT is always conserved”
Consequence Since time reversal T was universally expected
to be conserved CP was expected to be conserved too
What’s the big deal with CP? It has to do with our own existence…
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
The CP symmetry What is CP?
CP = C × PC: Charge ConjugationParticle Anti-particle
P: ParityInverts space coordinates
( ) ( )CP e p e p
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
The importance of CP violation The Big Bang model predicts:
matter and anti-matter produced in equal amounts matter and anti-matter annihilated into energy
This obviously goes against experimental evidence…
e-
e+
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Looking Out, Looking BackThe Universe exists…
Where did all the anti-matter go?
…and it’s made of matter!
8
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
The last echo of the Big Bang
The Cosmic Microwave Background, a result of matter/anti-matter annihilation near the beginning
of time
Image taken by the Wilkinson Microwave Anisotropy Probe (WMAP)
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
The matter dominated Universe
0.3 -10-0.2
Baryonic Asymmetry of the Universe: / ( 6.1 ) 10 Bn n
Only 1/109 particles survived!
What caused this tiny asymmetry?
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.11
Courtesy of Alan Chou (SLAC)
CP violation
Remember CPT theorem: CP expected to be conserved!
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
CP violation in K decaysIn 1964 Fitch and Cronin discovered CP violation in
the decays of KL mesons: KL+-
KL CP=-1} CP=+1}
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
The importance of CP violation discovery Revolutionary result:
Fitch and Cronin awarded the Nobel Prize in 1980
1980 NOBEL PRIZEJ.CroninV. Fitch
symmetry between matter and anti-matter is broken
How could this phenomenon be explained?
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Standard Model of Particle Physics 12 elementary particles
6 leptons 6 quarks
4 forces mediated by various bosons e
e
bt
sc
du
Force Carrier(s) Mass (GeV/c2) Electric Charge
Electromagnetic photon 0 0
Weak W+, Z0 80/90 +1/0Strong gluon 0 0
Gravitational Graviton? 0? 0?
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Standard Model’s minor addition: minor addition: anti-matter
Antiparticle vs. particle Same mass, but opposite quantum numbers
Example: electrical charge flips
e e
Matter Anti matter
e e
Charge=-1 Charge=+1
Charge=+2/3 Charge=-2/3
Charge=+1/3Charge=-1/3
Matter Anti matter
u c t u c td s b d s b
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Photo courtesy of SLAC
SLAC 40-inch bubble chamber, 1971
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
SLAC 40-inch bubble chamber, 1971
Photo courtesy of SLAC
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Standard Model’s recipes: how to make particles
The 6 quarks are the building blocks of matter
Baryons: 3 quarks Proton: (uud) Neutron: (udd) Lambda: (sud)
Mesons: 1 quark (q) + 1 anti-quark (q) Charged pions: + - Neutral Pion 0
u c td s b
uu d
Proton
ud
Charge=+2/3
Charge=-1/3
uu d
Anti-Proton
ud
uu
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Standard Model’s recipes: how particles decay
Most of the particles produced in the lab decay Usually in a tiny fraction of a second!
Example of a weak decay: -
Feynman Diagram Solid lines: quarks or leptons Dashed lines: carriers of forces Each vertex carries a coupling constant gW
Its strength determines the probability of the decay
d
u
W
time
gW gW
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Weak Interactions: Quark-Lepton Symmetry? Experimental observation in weak interactions:
Leptons always and only couple inside the same family Quarks instead violate this rule in -
How to preserve lepton-quark symmetry? Introducing “Quark Mixing” mechanism…
s
u
W
time u c
d s e
e
d
u
W
time u c
d s e
e
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Standard Model: Quark Mixing Mechanism “Weak eigenstates” are linear combinations of
“Flavor eigenstates” Flavor eigenstates: quarks as we defined them so far Weak eigenstates: linear combinations of ordinary quarks
The matrix that transforms flavor eigenstates (d,s) into weak eigenstates (d’, s’) is called mixing matrix Just a 2x2 rotation 1 parameter: Cabibbo angle C
C C
C C
d'= d cos + s sin with s'= -d sin + s cos' 'u cd s
C C
C C
cos sin' -sin cos'd ds s
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
CP violation in the Standard Model What if extend this mechanism to 3 families of quarks?
Kobayashi and Maskawa, 1973 Parameterization of the 3x3 rotation in complex space:
3 angles (Euler angles) and a complex phase
This complex phase elegantly introduces CP violation in the Model explaining Fitch and Cronin’s results
It also predicted the existence of third quark family
)(
1)1(211
)(211
6
23
22
32
O
AiA
A
iA
VVVVVVVVV
V
tbtstd
cbcscd
ubusud
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Success of the CKM predictions The third families of quark and leptons were soon
discovered
L. LedermanNobel Prize 88
Upsilon (bb) – Fermilab ‘77 Tau lepton – SLAC ‘75
M. PerlNobel Prize 95
Top quark – Fermilab ‘95
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
CKM and CP violation
Why we love CKM Elegant and simple mechanism Good success record The CKM is predictive
CKMMeasure CP violation in channels theoretically very well understood and look for deviations
w.r.t. Standard Model prediction
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
How to test CKM?
Kaons known for 40 years but… Experimental results very hard to interpret
theoretically: Loose constraints from K measurement No constraints from ’ yet…
…or clear theory but very hard to reach experimentally: BF(KL)~10-11!
Is there a way out? Yes, using B mesons…
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Unitarity of CKM implies: V†V = 1 6 unitarity conditions Of particular interest:
All sides are ~ O(1) possible to measure both sides and angles! Angles from CP asymmetries in B meson decays Sides from measurement of decay rates and mixing of B mesons
The Unitarity Triangle
0VVVVVV *tbtd
*cbcd
*ubud
*
*| |ub ud
cd cb
V VV V || *
*
cbcd
tdtb
VVVV
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Testing the Standard Model Measuring directly and independently the
angles tests the Standard Model in the CP violation
sector
B oscillationsB decays
CP violation in B decays
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Testing the Standard ModelIn practice:
Measure sides first (easier) and identify allowed area for apex of the triangle
Measure one angle and check for consistency
Confirmation of Standard Model
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Testing the Standard ModelIn practice:
Measure sides first (easier) and identify allowed area for apex of the triangle
Measure one angle and check for consistency
Discovery of New Physics!!!
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
The Bs
What are neutral B mesons? Bound states of b and d quarks:
B characteristics: B0 and B0 look identical from outside
Flavor can only be inferred by their decay products B0 and B0 decay after 1.6 ps in other lighter particles
Some of these decays are especially interesting…
Particle Quarks Mass Charg
e Spin
B0 bd 5.28 GeV/c2 0 0B0 bd 5.28 GeV/c2 0 0
bt
sc
du
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
CP violation in B0 decays If CP is conserved, B0 and B0 will behave exactly the same
Different types of CP violation: “Direct CP violation”:
Decay rates for B0 and B0 to certain final states are not the same
“Time-dependent CP violation”: The decay rate of B0 and B0 to some final states is not the
same over time This kind of CP violation is especially interesting because
the theory can make specific predictions…
0 0( ) ( )Rate B K Rate B K
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Time dependent CP asymmetry Consider the B0 decays B0J/KS
Eigenstate of CP Clean experimental signature
Time Dependent CP asymmetry
It can be calculated that for this decay, the ACP(t) has a sinusoidal shape and its amplitude is related to angle
0 0
0 0( ( ) ) ( ( ) )( ) ( ( ) ) ( ( ) )
CP CPCP
CP CP
N B t f N B t fA tN B t f N B t f
0Kb
c
sc
d0B
/J
d
ACP(t) = sin2 sinmt
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
How to measure CPV at B factories
.
Ingredient #1:Exclusivereconstruction
Ingredient #2:Flavor tagging(coherent state)
Ingredient #3: t determination
e- 4S
B0
B0
e-
+
-
Breco
Btag
e+
z~ c t
+
-
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
The experimental challenge Rare events:
Experimental accessible BF: ~ 10-6 -10-5
Millions of Bs needed!
Time dependent analysis: Bs produced with a boost
Asymmetric B factory!
Full B reconstruction and flavor tag State of the art detector with excellent
tracking and particle identification: BaBar Detector!
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
The solution: asymmetric B factories
Asymmetric e+e- B factories First proposed in 1987 by P. Oddone (LBL) Elegant and conceptually simple Challenging for accelerator builders!
2 beam pipes, 2 sets of magnets, difficult interaction region…
Many proposals, only 2 survived: PEP-II at SLAC (California) KEK-B at KEK (Japan)
Similar in design and achievements Will discuss PEP-II and BaBar as an example…
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
The PEP-II accelerator
Asymmetric B factory 9.0 GeV e- beam 3.1 GeV e+ beam
Very high luminosity 9 BB pairs/second > 500 M B mesons
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
The SLAC accelerators
BaBar Detector
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
The BABAR Detector
DIRC (PID))
1.5 T solenoid
CsI(Tl) EMC
Drift Chamber
Instrumented Flux Return
Silicon Vertex Tracker
e+ (3.1GeV)
e- (9GeV)
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
The BaBar experiment at SLAC
MIT people at work!
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Ingredient #1: Reconstruct the B0 decay
Accelerator and detector were completed in 1999
First goal: measure CP violation in the “golden channel” B0J/KS
Experimental challenge: Very rare decays BF (~10-4) It took 2 years to accumulate
enough data to measure CPV
Today’s sample: >4,000 clean B decays
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Gold plated event at BaBar
B0 J/ KS B0 K-X
Zoom on interaction region
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Distinguish B0 from B0 We are measuring the asymmetry:
B0 and B0 look identical from outside Flavor can only be inferred by their decay products
Strategy: Combine the many sources of flavor tagging information using Artificial
Neural Networks to optimize performance Very tricky business: the measurement is very sensitive to this
ingredient!!!
B0 D*- D0
l +(soft)
K +
B0D*-
(hard)
W+
Ingredient #2:
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Ingredient #3:t measurement
Time dependent analysis:
The technique: e- 4S
B0
B0
e+
z~ c t ~ 250 m
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
The CP fit: sin2 from 88M B0B0
sin(2) = 0.722 ± 0.040stat ± 0.023syst
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
What did we learn?
Compare measurement of angle with
measurement of sides:
sin2 from BaBar vs. indirect constraints
Excellent agreement with Standard Model expectation
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
CKM
CKM and CPV: end of the story?
Why we love CKM Elegant and simple mechanism The CMK is predictive
Measurements in B and K sector confirm predictions
Good News: new sources of CP violation must exist besides CKM (New Physics!)
Deviations from CKM expected in some channels
Just one (major) problem:X It fails to explain the matter-antimatter
asymmetry observed in the Universe by several orders of magnitude!
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
New Physics in penguin decays?
Standard Model predicts ACP(t)
New Physics can modify ACP(t): look for deviations >2.5 effect observed: more data needed…
0
S
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
sin2charmonium vs penguins
Fluctuation or first signs New
Physics?
…more data will tell…
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
Other sources of CP violations The explanation of the matter-antimatter
asymmetry doesn’t necessarily reside in the quark sector
Other possible sources of CP violation: CP violation in strong interactions
Search for neutron EDM (electric dipole moment) CP violation in neutrinos
Especially promising: Recent discovery of neutrino mixing: neutrinos have masses! 3x3 mixing matrix as in the quark sector CP violation term as in the CKM mechanism
Interesting experiments planned in the near future Stay tuned!
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November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.
ConclusionThe mysteries of CP violation are being uncovered
thanks to new studies of B meson decays
Standard Model is still holding well, but…
First unambiguous evidence of CPV in B system First quantitative test of CP side of Standard Model
New Physics must be hiding somewhere: Penguins? Neutrinos? The quest continues…