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An introduction to Flavour Physics
!
Part 4 !
Thomas Blake Warwick Week 2015
1
An introduction to Flavour Physics
• What’s covered in these lectures:
1. An introduction to flavour in the SM.!
2.Neutral meson mixing and sources of CP violation.
3.CP violation in the SM.
4.Flavour changing neutral current processes.!
➡Neutral meson mixing, rare decays, lepton flavour violation and constraints on new particles.
2
The flavour problem• If there is TeV-scale new physics (and we hope there is),
why doesn’t it manifest itself in flavour changing neutral currents (FCNCs)?
3
No FCNC at tree level in SM
• Charged current interaction is the only flavour changing process in the SM.
• Flavour changing neutral current processes are therefore forbidden at tree level (require a loop process involving a virtual W exchange).
�
qi qjqi qiqi qi qiqi
WZ0 gVij
4
Effective theories• In mesons/baryons there is a clear separation of scale.
!
• We want to study the physics of the mixing/decay at or below a scale Λ, in a theory in which contributions from particles at a scale below and above Λ are present. Replace the full theory with an effective theory valid at Λ,
5
⇤
E
�L
�HmW � mb > ⇤QCD
L(�L,�H) ! L(�L) + Le↵ = L(�L) +X
i
CiOi(�L)
operator product expansion
Fermi’s theory• Example:
➡ In the Fermi model of the weak interaction, the full electroweak lagrangian (which was unknown at the time) is replaced by the low-energy theory (QED) plus a single operator with an effective coupling constant.
6
d u d u
⌫ e ⌫ e
W LEW ! LQED +GFp2(ud)(e⌫̄)
FCNC processes• Two types of FCNC process:
➡ ∆F = 2, meson anti-meson mixing.
➡ ∆F = 1, e.g. Bs → 𝝁+𝝁- . Commonly described as rare decays.
!
• In the SM these processes are suppressed: ➡ Loop processes which are CKM
suppressed and can be highly GIM suppressed.
B0s B0
s
B0
K⇤0
µ+
µ�
µ+
µ�
B0s
7
FCNC processes• Two types of FCNC process:
➡ ∆F = 2, meson anti-meson mixing.
➡ ∆F = 1, e.g. Bs → 𝝁+𝝁- . Commonly described as rare decays.
!
• In the SM these processes are suppressed: ➡ Loop processes which are CKM
suppressed and can be highly GIM suppressed.
B0s B0
s
B0
K⇤0
µ+
µ�
µ+
µ�
B0s
8
Mixing
9
Reminder: GIM mechanism• Take mixing diagram as an
example, have an amplitude
10
Bq Bq
Vtb
V ⇤tq
t
W Wt̄
q̄
q = s, db
b̄V ⇤tq
Vtb
(c, u)
A(B0 ! B0) =X
q,q0
(V ⇤qbVqd)(V
⇤q0bVqd)Aqq0
A(B0 ! B0) =X
q
(V ⇤qbVqd)[V
⇤tbVtd(Atq �Auq) + V ⇤
cbVcd(Acq �Auq)]
summing over the internal up-
type quarks Can then plug-in V ⇤ubVud + V ⇤
cbVcd + Vtb ⇤ Vtd = 0
for the B system the top dominates / mqmq0/m2W
New physics in B mixing?• Introduce a multiplicative factor
11
M12 = M12,SM ·�s,d
consistent with SM (Re ∆ =1, Im ∆ = 0)
New physics in B mixing?• Introducing new physics with at some higher energy scale ΛNP
with coupling 𝜅NP
12
SM contribution from box diagram
NP contribution (at dimension 6), can include tree level FCNC
Le↵ = LSM +X
i
NP
⇤d�4NP
O(d)i
(V ⇤tbVtd)
2 g4m2t
16⇡2m4W
c.f.NP
⇤2NP
Mixing constraints• Everything is consistent with the SM, so instead can set
constraints on NP scale from mixing.
13
Operator Re(⇤) Im(⇤) Re(c) Im(c) Constraint(sL�µdL)(sL�µdL) 9.8⇥ 102 1.6⇥ 104 9.0⇥ 10�7 3.4⇥ 10�9 �mK , "K
(sRdL)(sLdR) 1.8⇥ 104 3.2⇥ 105 6.9⇥ 10�9 2.6⇥ 10�11 �mK , "K(cL�µuL)(cL�µuL) 1.2⇥ 103 2.9⇥ 103 5.6⇥ 10�7 1.0⇥ 10�7 �mD, |q/p|, �D
(cRuL)(cLuR) 6.2⇥ 103 1.5⇥ 104 5.7⇥ 10�8 1.1⇥ 10�8 �mD, |q/p|, �D
(bL�µdL)(bL�µdL) 5.1⇥ 102 9.3⇥ 102 3.3⇥ 10�6 1.0⇥ 10�6 �md, SJ/ K0S
(bRdL)(bLdR) 1.9⇥ 103 3.6⇥ 103 5.6⇥ 10�7 1.7⇥ 10�7 �md, SJ/ K0S
(bL�µsL)(bL�µsL) 1.1⇥ 102 1.3⇥ 102 7.6⇥ 10�6 7.6⇥ 10�6 �ms
(bRsL)(bLsR) 3.7⇥ 102 3.7⇥ 102 1.3⇥ 10�5 1.3⇥ 10�5 �ms
coupling (c = 𝜅) when ΛNP = 1TeV ΛNP in TeV when coupling =1
Small couplings?• New flavour violating sources (if there are any) are highly tuned,
i.e. must come with a small coupling constant or must have a very large mass.
14
NP ⇠ 1 ⇤NP >⇠ 2⇥ 104 TeV
⇠ 1
(4⇡)2⇤NP >⇠ 2⇥ 103 TeV
⇠ (ytV⇤tiVtj)
2 ⇤NP >⇠ 5TeV
⇠(ytV ⇤
tiV⇤tj)
2
(4⇡)2⇤NP >⇠ 0.5TeV
generic tree-level
generic loop-order
tree-level with “alignment”
loop-order with “alignment”
Minimal Flavour Violation• One good way to achieve small couplings is to build models that
have a flavour structure that is aligned to the CKM. ➡ Require that the Yukawa couplings are also the unique source
of flavour breaking beyond the SM.
• This is referred to as minimal flavour violation.
• The couplings to new particles are naturally suppressed by the Hierarchy of the CKM elements.
15
Rare decays
16
Rare b → s decays• Can write a Hamiltonian for the effective theory as
17
He↵ = �4GFp2
VtbV⇤ts
↵e
4⇡
X
i
Ci(µ)Oi(µ) ,
Local operator with different Lorentz structure (vector, axial vector current etc)
Wilson coefficient (integrating out scales above μ)
Rare b → s decays• Can write a Hamiltonian for the effective theory as
!
!
!
!
• Conventional to pull SM loop contributions out the front as constants.
18
He↵ = �4GFp2
VtbV⇤ts
↵e
4⇡
X
i
Ci(µ)Oi(µ) ,
CKM suppressionLoop suppression (1/4π)2
Weak decay (1/mW)2
Beyond the SM• In the same way can introduce new particles that give rise to
corrections
!
!
!
• Once again, the constant, 𝜅, can share some, all or none of the suppression of the SM process.
19
�He↵ =NP
⇤2NP
ONP
NP scale local operator
Operators
20
O7 =mb
es̄�µ⌫PRbFµ⌫ , O0
7 =mb
es̄�µ⌫PLbFµ⌫ ,
O8 = gsmb
e2s̄�µ⌫PRT
abGaµ⌫ , O0
8 = gsmb
e2s̄�µ⌫PLT
abGaµ⌫ ,
O9 = s̄�µPLb ¯̀�µ` , O0
9 = s̄�µPRb ¯̀�µ` ,
O10 = s̄�µPLb ¯̀�µ�5` , O0
10 = s̄�µPRb ¯̀�µ�5` .
right handed currents (suppressed in SM)photon penguin
vector and axial-vector current
Operators (beyond SM)• Scalar and pseudo-scalar operators (e.g. from Higgs penguins)
!
!
!
• Tensor operators
!
!
• All of these are vanishingly small in SM.
• In principle could also introduce LFV versions of every operator.
21
OS = s̄PRb ¯̀̀ , O0S = s̄PLb ¯̀̀ ,
OP = s̄PRb ¯̀�5` , O0P = s̄PLb ¯̀�5`
OT = s̄�µ⌫b ¯̀�µ⌫` , OT5 = s̄�µ⌫b ¯̀�
µ⌫�5` ,
Generic ∆F = 1 process• In the effective theory, we then have
!
!
!
!
• For inclusive processes can relate sum over exclusive states to calculable quark level decays,
!
• For exclusive processes, need to compute form-factors / decay constants etc.
22
A(B ! f) = V ⇤tbVtq
X
i
Ci(MW )U(µ,MW )hf |Oi(µ)|Bi
Hadronic matrix element
B(B ! Xs�) = B(b ! s�) +O(⇤2QCD/m2
B)
Generic ∆F = 1 process• Inclusive processes are theoretically clean, but
experimentally challenging.
• Exclusive processes are theoretically challenging. ➡ Involve non-perturbative quantities.
• Estimate form-factors using, light-cone-sum-rules and Lattice QCD.
23
Form factors• Unfortunately, we don’t just have free quarks and we need to
compute hadronic matrix elements (form-factors and decay constants). ➡ Non-pertubative QCD, i.e. difficult to estimate.
24
fBFortunately we have tools to help us in different kinematic regimes.
e.g how to deal with this:
Theoretical tools (crib sheet)• Lattice QCD
➡ Non-perturbative approach to QCD using discretised system of points in space and time. As the lattice becomes infinitely large and the points infinitely close together the continuum of QCD is reached.
• Light-Cone-Sum-Rules ➡ Exploit parton-hadron duality to compute form-factors and
decay constants.
• Operator product expansions. ➡ Used to match physics to relevant scales.
25
Theoretical tools (crib sheet)• Heavy quark expansion.
➡ Exploit the heaviness of the b-quark,
• QCD factorisation. ➡ Light quark has large energy in the meson decay frame, e.g.
quarks in π have large energy in B → π decays in the B rest frame.
• Soft Collinear Effective Theory. ➡ Model system as highly energetic quarks interacting with soft
and collinear gluons.
• Chiral perturbation theory.
26
mb � ⇤QCD
Which processes?• Will mainly focus on recent measurements of B decay processes,
b → s transitions are some of the least well tested.
• You can also study FCNC decays of charm and strange mesons.
• The GIM mechanism is more effective in both charm and strange meson decays: ➡ For charm mesons the masses and mass differences, e.g. (mb -
ms), are small. ➡ For strange mesons top contribution is suppressed relative to B
meson decays because Vts ≪ Vtb.
27
Bs → 𝝁+𝝁-
• Golden channel to study FCNC decays.
• Highly suppressed in SM.
1.Loop suppressed.
2.CKM suppressed (at least one off diagonal element)
3.Helicity suppressed (pseudo-scalar B to two spin-1/2 muons)
B0s
µ+
µ�
Z0
t
W
b
s̄
28
neutral current (axial-vector)
also receives contributions from W box diagrams
Bs → 𝝁+𝝁-
• Golden channel to study FCNC decays.
• Highly suppressed in SM.
1.Loop suppressed.
2.CKM suppressed (at least one off diagonal element)
3.Helicity suppressed (pseudo-scalar B to two spin-½ muons)
B0s
µ+
µ�b
s̄
29
Interesting probe of models with new or enhanced scalar operators (no helicity suppression), e.g. SUSY at high tan β.
b
h0
Bs → 𝝁+𝝁- in the SM• Only one operator contributes in SM:
!
• Branching fraction in SM:
30
B(B0d,s ! µ+µ�) ⇡
��V ⇤tbVtq
��2 G2F ↵2
e MBM2µf
2B
16⇡3�H
s
1�4M2
µ
M2B
|C10(mb)|2
CKM factors
Single hadronic matrix element (decay constant)
O10 = (sL�µbL)(µ̄�µ�5µ)
h0|s�µ�5b|Bi = ifBpµ
helicity suppression⇥ M2
µ
M2B
!
Bs → 𝝁+𝝁-• Very rare decay with branching fraction of 10-9:
31
Bs → 𝝁+𝝁- combination• Combining results from CMS
and LHCb experiments from LHC run 1. ➡ Observe Bs signal and
evidence for B0.
32
]2c [MeV/−µ+µm5000 5200 5400 5600 5800
)2 cS/
(S+B
) wei
ghte
d ca
nd. /
(40
MeV
/
0
10
20
30
40
50
60 DataSignal and background
−µ+µ →s0B
−µ+µ →0BCombinatorial bkg.Semileptonic bkg.Peaking bkg.
CMS and LHCb (LHC run I)
]9�[10)�µ+µ⇥0BB(0 0.2 0.4 0.6 0.8
Lln⇤2�
0
2
4
6
8
10SM
]9�[10)�µ+µ⇥s0BB(
0 2 4 6 8
Lln⇤2�
0
10
20
30
40SM
]9�[10)�µ+µ⇥s0BB(
0 1 2 3 4 5 6 7 8 9
]9�[1
0)� µ
+ µ⇥
0B
B(
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
68.27%
95.45%
99.73% 5�10
◊6.3
�1
7�10
◊5.7
�1
9�10
◊2�1
SM
CMS and LHCb (LHC run I)
a
b
c
LHC
b +
CM
S, [a
rXiv
:141
1.44
13]
the end of a long road …
33Year1985 1990 1995 2000 2005 2010 2015
Lim
it (9
0% C
L) o
r BF
mea
sure
men
t
10−10
9−10
8−10
7−10
6−10
5−10
4−10
−µ+µ → 0sSM: B
−µ+µ → 0SM: BD0L3CDFUA1ARGUSCLEO
CMS+LHCbATLASCMSLHCbBaBarBelle
2012 2013 201410−10
9−10
8−10
Testing MFV• Ratio of the rates of the
two decays is a test of MFV which predicts:
34
R0 0.1 0.2 0.3 0.4 0.5
Lln∆2−
0
2
4
6
8
10
SM and MFV
CMS and LHCb (LHC run I)
R(B0/B0s ) /
|Vtd|2
|Vts|2f2B0
f2B0
s
from Lattice
~1/25
Data are consistent with SM/MFV
LHC
b +
CM
S, [a
rXiv
:141
1.44
13]
Photon polarisation• In radiative B decays, angular momentum
conservation allows
!
!
• However, the charged current interaction only couples to left handed quarks. Need to helicity flip the b- or s-quark.
• The right-handed contribution is therefore suppressed by
35
bR(L) sL(R)W−
γL(R)
t
Vtb VtsbL ! sR�R
bR ! sL�L
A(bL ! sR�R)
A(bR ! sL�L)⇠ ms
mb
Inclusive b → s 𝛾• Can perform either a semi-inclusive measurement, summing a
large number of Xs final states (e.g. K+, K*, …) or a fully inclusive measurement where Xs is not reconstructed.
➡ Cuts on M(Xs) or E𝛾 complicate theory calculations.
Result
36
10
* (GeV)γE1.6 1.8 2 2.2 2.4 2.6 2.8 3
Even
ts /
100
MeV
310
410
510
610
* (GeV)γE1.6 1.8 2 2.2 2.4 2.6 2.8 3
Even
ts /
100
MeV
310
410
510
610(a)
* (GeV)γE1.6 1.8 2 2.2 2.4 2.6 2.8 3
Even
ts /
100
MeV
0
2
4
6
8
10
12
310×
* (GeV)γE1.6 1.8 2 2.2 2.4 2.6 2.8 3
Even
ts /
100
MeV
0
2
4
6
8
10
12
310×
Continuum MC MCBB
Signal MC
(b)
FIG. 2: Estimated signal and background yields vs. photon energy in the CM frame based on MC simulation, at two stages ofthe event selection: (a) after requiring an unvetoed high-energy photon (logarithmic scale); (b) after all selection requirements(linear scale). The three contributions are shown cumulatively. The signal distribution is for a KN model withmb = 4.65GeV/c2,while the continuum distribution has been scaled as described in Sec. III.
CM Electron Momentum (GeV/c)0 0.5 1 1.5 2 2.5 30
200
400
600
800
1000
1200
Signal MC
MCBBContinuum MC
(a)
)γ* (e,θcos -1 -0.8 -0.6 -0.4 -0.2 0 0.2 0.4 0.6 0.8 10
200
400
600
8001000
1200
1400
1600
1800 (b)
CM Muon Momentum (GeV/c)0 0.5 1 1.5 2 2.5 30
100
200
300
400
500
600 (c)
)γ,µ* (θcos -1 -0.8 -0.6 -0.4 -0.2 0 0.2 0.4 0.6 0.8 10
200
400
600
800
1000
1200
1400
1600 (d)
FIG. 3: Lepton distributions from MC simulation, after the photon selection requirements but before applying lepton tag andNN criteria. Plots (a) and (b) are for electron tags, plots (c) and (d) for muon tags. Plots (a) and (c) show the CM-framemomentum distributions, with vertical lines indicating the minimum selection requirements. Plots (b) and (d) show the cosineof the CM angle between the lepton and the high-energy photon, after applying the momentum criteria; the vertical lines showthe minimum requirement on this quantity. The signal (black dots) is from a KN model with mb = 4.65GeV/c2. The BBbackground (solid blue histogram) and continuum background (dashed red) are from the MC simulations. Each distribution isseparately normalized to best illustrate its behavior.
shapes in MC
background subtracted data
BaBar, Phys. Rev. D. 86. 112008 (2012)
B(B ! Xs�)E�>1.6 GeV = (343± 21± 7)⇥ 10�6
BF consistent with SM expectation (impressive prediction of the SM)
b → s 𝛾 constraints
37
time dependent CP violation in B ! [K0
S⇡0]�
inclusive branching fraction.
angular distribution of B ! K⇤e+e�
• Constraints on right-handed currents in b → s 𝛾 decays:
Results are consistent with LH polarisation expected in SM
decays
38
!"#$%&$%$"'$(
J/�(1S)
�(2S)C(�)7
C(�)7 C(�)
9C(�)
9 C (�)10
4 [m(µ)]2 q2
d�dq2
)"*(
+,"-(*!.#)"'$(
',"#%!/01,".(&%,2(
)/,3$(,4$"('5)%2(
#5%$.5,6*((
cc̄
b ! cc̄stree levelphoton
penguin
b ! s`+`�
decay rates
39
b ! s`+`�
]4c/2 [GeV2q0 5 10 15 20
]-2
GeV
4 c × -7
[10
2 q/d
Bd
0
0.5
1
1.5
Theory BinnedLHCb CMS
]4c/2 [GeV2q0 5 10 15 20
]2/G
eV4 c ×
-8 [1
02 q
/dBd 0
1
2
3
4
5
LCSR Lattice Data
LHCb−µ+µ+ K→+B B0 ! K⇤0 µ+µ�
• 7 form-factors
• Enhancement at low q2 from virtual photon
• 3 form-factors
• No enhancement at low q2 from virtual photon (angular momentum conservation).
Large theory uncertainties (from QCD)
K+
⇡�K⇤0 ✓K
µ+
µ�
B0
✓`
(a) ✓K and ✓` definitions for the B0decay
µ�
µ+
K+
⇡�B0
K⇤0�
K+ ⇡�
n̂K⇡
�p̂K⇡
µ�
µ+
n̂µ+µ�
(b) � definition for the B0decay
⇡+
K�K⇤0
µ�
µ+
B0
�
K� ⇡+
n̂K⇡
� p̂K⇡
µ�
µ+
n̂µ�µ+
(c) � definition for the B0decay
B →K*0 µ+µ-
• Four-body final state. ➡ Angular distribution provides
many observables that are sensitive to NP.
e.g. at low q2 the angle between the decay planes is sensitive to the photon polarisation.
• System described by three angles and q2.
40
B →K*0 µ+µ-
41
1
d(�+
¯
�)/dq2d
3(�+
¯
�)
d
~⌦
����P
=
9
32⇡
h34 (1� FL) sin
2 ✓K + FL cos2 ✓K +
+
14 (1� FL) sin
2 ✓K cos 2✓l
�FL cos2 ✓K cos 2✓l + S3 sin
2 ✓K sin
2 ✓l cos 2�
+S4 sin 2✓K sin 2✓l cos�+ S5 sin 2✓K sin ✓l cos�
+
43AFB sin
2 ✓K cos ✓l + S7 sin 2✓K sin ✓l sin�
+S8 sin 2✓K sin 2✓l sin�+ S9 sin2 ✓K sin
2 ✓l sin 2�i
Angular distribution:
fraction of longitudinal polarisation of the K*
forward-backward asymmetry of the dilepton system
The observables depend on form-factors for the B → K* transition plus the Wilson coefficients.
Latest LHCb result, shown at Moriond 2015, LHCb-CONF-2015-002
42
Form-factor “free” observables
• Can construct ratios of observables which in QCD factorisation/SCET are independent of form-factors.
43
local tension with SM predictions (vector like NP contribution or unexpected large QCD effect?)
P 05 = S5/
pFL(1� FL)
Late
st L
HC
b re
sult,
sho
wn
at M
orio
nd 2
015,
LH
Cb-
CO
NF-
2015
-002
global fits to b → s data• Global fits to the b → s data favour
a new vector like contribution.
➡ Could be sign of new physics (heavier partner of the Z) or a sign that we don’t understand something about QCD, loop contributions will also look vector-like.
44
cc
branching fractions angular observables
combination
Interpretation of global fits
45
Optimist’s view point Pessimist’s view point
Vector-like contribution could come from new tree level contribution from a Z’ with mass of few TeV (the Z’ will also contribute to mixing, a challenge for model builders)
Vector-like contribution could point to a problem with our understanding of QCD, e.g. are we correctly estimating the contribution for charm loops that produce dimuon pairs via a virtual photon.
More work needed from experiment/theory to disentangle the two
(charged) lepton flavour violation
46
Charged LFV• Essentially forbidden in SM by
smallness of the neutrino mass. Powerful null test of the SM.
• Any visible signal would be an indication of NP.
47
x ⌫µ� e�
�
B(µ ! e�) / m4⌫
m4W
⇠ 10�54
µ LFV• Three different signatures
1. at rest (MEG at PSI).
2. (SINDRUM at PSI).
3. µ conversion in field of nucleus.
48
SINDRUM 1983–1986 @SIN(PSI) B(μ→eee) <1.0×10-12
25 year’s ago
SINDRUM II 1989–1993 @PSI R(μAu→eAu)<7.0×10-13
MEG 2008–2013@PSI B(μ→eγ) <5.7×10-13
µ ! e�
µ ! 3e
𝜏 LFV
• Expect improvement from Belle 2 and for 𝜏 → 3µ from LHCb.
49
large number of experimental signatures
A look into the future
50
New Physics? • As we saw in the last lecture, measurements of the CKM matrix
and the properties (closure) of the Unitarity triangle are consistent with the Standard Model picture of flavour physics. ➡ Nobel prize for Kobayahsi and Maskawa in 2008.
• However, there are some interesting “hints” of new physics: ➡ Tension in Vub (and Vcb).
➡ Enhancement of D(*)𝜏ν.
➡ P5’ anomaly in B →K*0 µ+µ-.
➡ Muon g-2.
• There’s still plenty of room for discoveries …
51
all at ~3𝜎
LHCb running conditions• LHCb is currently running at a luminosity of 4x1032 cm-2s-1 .
• Displacing LHC beams to run at a lower luminosity that ATLAS and CMS.
!
!
• How do we interpret this number?
!
!
• Higher luminosity means more B mesons produced per year and in turn better statistical precision.
52
�(pp ! bb) = (75.3± 5.4± 13.0)µb
⇠ 30 k bb pairs per second
running at a levelled luminosity
in LHCb acceptance
LHCb upgrade• Aim to run at 2x1033.
• Main limitation with the current detector is the 1 MHz readout rate.
• Need to cut much harder maintain the 1MHz rate with higher luminosity (end up removing as much signal and background).
• Ambitious plan to read out the full detector at 40 MHz to a software farm.
• Also plans to replace vertex and tracking detectors to cope with higher luminosity.
• Upgrade planned for LS2 (2018).
53
current trigger scheme
54Peter Križan, Ljubljana
e- 2.6 A
e+ 3.6 A
To obtain x40 higher luminosity
Colliding bunches
Damping ring
Low emittance gun
Positron source
New beam pipe& bellows
Belle II
New IR
TiN-coated beam pipe with antechambers
Redesign the lattices of HER & LER to squeeze the emittance
Add / modify RF systems for higher beam current
New positron target / capture section
New superconducting /permanent final focusing quads near the IP
Low emittance electrons to inject
Low emittance positrons to inject
Replace short dipoles with longer ones (LER)
KEKB to SuperKEKB
Rare kaon decays• Two rare kaon decay experiments are just starting:
➡ KOTO at J-PARC, searching for ➡ NA62 at CERN, searching for
• The main advantage of final states with neutrinos is that there is no contribution from quark loops involving light quarks (which can annihilate to produce charged leptons).
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K+ ! ⇡+⌫⌫̄
K0L ! ⇡0⌫⌫̄
KOTO NA62
also CP
Charged LFV • Upgrade to MEG underway,
aiming for O(10-14). Expected to start data taking soon.
• New µ →3e experiment (Mu3e) at PSI.
• Two new conversion experiments, one at PSI (Mu2e) and one at J-PARC (COMET).
• Expect improvements for LFV 𝜏 decays from Belle 2.
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50 μm thick silicon wafer
Interesting challenges, e.g. very thin detectors
for µ→3e.
Recap• In today’s lecture we discussed:
➡ Flavour changing neutral current processes and constraints on new particles.
➡ Minimal flavour violation. ➡ Charged lepton flavour violation. ➡ Future flavour experiments.
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Further reading• There are a number of good sets of lecture notes on flavour physics
available on arXiv that give a more detailed overview of this field.
➡ A. J. Buras, “Weak Hamiltonian, CP violation and rare decays,” [arXiv:hep-ph/9806471].
➡ A. J. Buras, “Flavor physics and CP violation,” [arXiv:hep-ph/0505175].
➡ G. Isidori, “Flavor physics and CP violation,” [arXiv:1302.0661].
➡ Y. Grossman, “Introduction to flavor physics,” [arXiv:1006.3534].
➡ Y. Nir, “Flavour physics and CP violation,” [arXiv:1010.2666].
➡ M. Neubert, “Effective field theory and heavy quark physics,” [arXiv:hep-ph/0512222].
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Further reading• Most introductory particle physics text books include a basic
introduction to flavour physics.
• There are also more specialist books available, e.g. ➡ I. I. Bigi and A. I. Sanda. “CP violation” ➡ CP violation, G.C.Branco, L.Lavoura & J.P.Silva
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Fin
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