What’s the matter with anti-matter? A short history of CP violation Gabriella Sciolla M.I.T....

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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

description

November 13, 2003What 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

Transcript of What’s the matter with anti-matter? A short history of CP violation Gabriella Sciolla M.I.T....

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.

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

Page 2: 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.

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

Page 3: 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.

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

Page 4: 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.

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?

Page 5: 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.

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…

Page 6: 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.

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

Page 7: 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.

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+

Page 8: 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.

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!

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Page 9: 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.

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)

Page 10: 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.

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?

Page 11: 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.

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!

Page 12: 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.

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}

Page 13: 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.

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?

Page 14: 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.

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?

Page 15: 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.

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

Page 16: 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.

November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.

Photo courtesy of SLAC

SLAC 40-inch bubble chamber, 1971

Page 17: 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.

November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.

SLAC 40-inch bubble chamber, 1971

Photo courtesy of SLAC

Page 18: 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.

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

Page 19: 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.

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

Page 20: 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.

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

Page 21: 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.

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

Page 22: 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.

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

Page 23: 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.

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

Page 24: 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.

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

Page 25: 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.

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…

Page 26: 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.

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

Page 27: 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.

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

Page 28: 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.

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

Page 29: 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.

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!!!

Page 30: 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.

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

Page 31: 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.

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

Page 32: 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.

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

Page 33: 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.

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

+

-

Page 34: 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.

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!

Page 35: 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.

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…

Page 36: 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.

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

Page 37: 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.

November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.

The SLAC accelerators

BaBar Detector

Page 38: 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.

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)

Page 39: 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.

November 13, 2003 What can we learn from CPV? G. Sciolla – M.I.T.

The BaBar experiment at SLAC

MIT people at work!

Page 40: 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.

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

Page 41: 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.

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

Page 42: 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.

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:

Page 43: 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.

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

Page 44: 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.

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

Page 45: 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.

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

Page 46: 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.

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!

Page 47: 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.

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

Page 48: 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.

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…

Page 49: 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.

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!

Page 50: 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.

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…