wir schaffen wissen –heute fÜr morgen andreas crivellinpsi_ch_01.pdf · andreas crivellin...
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WIR SCHAFFEN WISSEN – HEUTE FÜR MORGEN
Explaining the Flavour Anomalieswith New Physics
Andreas CrivellinTheory Group of the Laboratory for Particle Physics
Corfu, 05.09.2017
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• Introduction:
New Physics and Flavour anomalies
− b→sμμ
− b→cτν
− aμ
− Z’ explanations for b→sμμ
• Simultaneous explanations with LQs
• Conclusions
Outline
Page 2Andreas Crivellin
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Dir
ect
se
arc
he
sFlavour observables
Page 3
• At colliders one produces many (up to 1014) heavy quarks
or leptons and measures their decays into light flavours
Finding NP in Flavour Observables
Andreas Crivellin
Flavour observables are sensitive to higher energy scales than collider searches
Experiment
Standard Model
New Physics
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Hints for LFUV
Page 4
Lepton Flavour
Universality Violation
(LFUV)
LFUV
Electron channels:
SM like
b→sµµ5-6σ
R(D(*))
4σ
aµ
3σ
τ→µνν2σ
Andreas Crivellin
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� MSSM
� tan(ß) enhanced slepton loops
� Scalars
� Light scalars with enhanced muon couplings
� Z’
� Very light with τμ couplings (mτ enhancement)
� Leptoquarks
� mt enhaned effects
8
aµ explanations
Chiral enhancement or very light particles
Page 5
e.g. W. Altmannshofer, C. Chen, P.S.B. Dev, A. Soni, arXiv:1607.06832, …
e.g. D. Stockinger, hep-ph/0609168
e.g. A. Djouadi, T. Kohler, M. Spira, J. Tutas, Z.Phys. C46 (1990)
e.g. A. Broggio et at. arXiv:1409.3199 A.C. et al. arXiv:1507.07567
E. Leskow, A.C., G. D'Ambrosio, D. Müller
arXiv:1612.06858
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� Chirally enhanced effects via top-loops
8
Scalar Leptoquarks in aµ
Z→μμ at future colliders
Page 6
E. Leskow, A.C.,
G. D'Ambrosio,
D. Müller
arXiv:1612.06858
,L R
µλ
Left-, right-
handed
muons-top
coupling
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� Charged scalars
� Problems with
q2 distributions
and Bc lifetime
� W’
� Strong constraints
from direct LHC searches
� Leptoquark
� Strong signals in qq→ττ searches
8
R(D) & R(D*)
Large tree-level effect neededExplanation difficult
Page 7
Faroughy et al. arXiv:1609.07138
See talk of Roman
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R(D(*)) and b→sττ (model-independent)
• Large couplings to the second generation needed in
order avoid collider and EW precision bounds
• Cancellation in b→sνν needed: C(1)≈C(3)
Bs→ττ
very strongly
enhanced
LHCb limit
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b→sμμ model-independent analysis
Page 9
• Several 2-3σ deviations in more than 130 observables
− P5’
− R(K)
− R(K*)
− Bs→ϕμμ• 6 NP operators
Modelindependent fit
4-6 σ better than SM
( ) ( )' 5
9 LO s P bµ
µ µγ µγ γ µ=
See talk of Nazila
B. Capdevila, AC, S. Descotes-Genon, J. Matias and J. Virto, arXiv:1704.05340 [hep-ph].
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� Z’
� Leptoquarks
� Loop effects
b→sμμ explanations
Even high scale NP explanations possible
Page 10
U. Haisch et al. 1308.1959, Buras et al. 1311.6729
W. Altmannshofer et al. 1403.1269, AC. et al. 1501.00993, …..
LQ
µ
µb
s
Gudrun Hiller, Martin Schmaltz
arXiv:1411.4773
B. Gripaios, M. Nardecchia, S.A. Renner.
arXiv:1412.1791
D. Bečirević, N. Košnik, O. Sumensari,
R. Zukanovich Funchal, arXiv:1608.07583
L. Calibbi, AC. T. Ota, PRL 2015
…
B. Gripaios, M. Nardecchia, S. Renner, arXiv:1509.05020
See talk of Stephen King
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R(K), R(K*) and µ→eγ with LQs
Page 11
� Three LQs give
a good fit
� Scalar triplet
� Vector singlet
� Vector triplet
� Simultaneous
effect in b→sμμ
and b→see
generate μ→eγ
AC, D. Mueller, A. Signer, Y. Ulrich,
arXiv:1505.xxxx
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New Scalars and Fermions in b→sµµ
� Possible representations
Page 12
2x6x4 possibilitiesPere Arnan, A.C., Lars Hofer and Federico Mescia, arXiv:1608.07832
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Bs mixing
requires
Majorana
Fermions
b→sμμ 3σ
2σ1σ
b→sµµ and Bs mixing
Page 13
Explanation with O(1) couplings
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Implications for New Particles
Page 14
Lepto-quarks
b→sμμR(D(*))
Higgsesaμ
Z’ gauge boson
Extension of the SM is required!
What is the underlying
theory?
Andreas Crivellin
Scalars and
fermions
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Simultaneous Explanation ofR(D), R(D*), aµ
and b→sμμ unsing
Leptoquarks
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Two Scalar Leptoquarks
• scalar leptoquark singlet with Y=-2/3
• scalar leptoquark triplet with Y=-2/3
AC, D. Mueller, T. Ota
arxiv:1703.09226
1Φ
3Φ
Constructive in R(D(*))
Destructive in b→sμμ
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R(D(*)), b→sνν with 2 Scalar LQs
1
3
L L
jk jk
L i j L
jk jkeπ
λ λ
λ λ
≡
=
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R(D(*)), b→sμμ and aμ with 2 scalar LQs
• Scalar leptoquark singlet + triplet with Y=-2/3
• Cancelation in b→sνν imposed
2 out of 3 can be explained
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Vector Leptoquark SU(2) Singelet
• C9=-C10 effect in b→sμμ
• Left handed vector current in R(D) and R(D*)
• No effect in b→sνν
• No proton decay
• Contained within the Pati-Salam model
• Massive vector bosons
− Non-renormalizable without Higgs mechanism
− Pati Salam not possible at the Tev scale
because of KL→μe and K→πμe
Good solution, but difficult UV completion
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Pati-Salam + vector-like fermions
L. Calibbi, AC and T. Li, A model of vector leptoquarks in view of the $B$-physics anomaliesarXiv:1709.00692
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Pati-Salam + vector-like fermions
− 3 light generation (SM fermions)
− 3 heavy generation (vector like)
Only the LQ couples flavour violating
( ) ( )Q Q L L
ij iL ij iL jR ij iL ij iL jRL m q M Q Q M L m L′ ′⊃ − + − + ℓ
, ,R L L
R L L
R L Li i i
Q Q qY Y X
L L
′ = = = ′ ℓ
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R(D(*)) and b→sμμ
Simultaneous explanation possible!Can also account for the AMM of the muon
1
Q
ii
QQ iii Q
ii
Q
ii
m
Ms
m
M
=
+
3 3
1
2
1.5
Q Ls s
M TeV
= =
=
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• P5’ b→dμμ
• R(D) & R(D*) b→sττ
• R(K) & R(K*) μ→eγ
• R(D), R(D*) & aμ τ → μγ
• R(D), R(D*) & b → sμμ b → sτμ
Outlook
Page 23Andreas Crivellin
Intersting experimental prospects
NP
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• Intriguing hints for Lepton Flavour Universality
violating New Physics
•Leptoquarks are prime
candidates for a solution
•Confirming or disproving
the anomalies makes
a model selection
•Predictions for flavor
and LHC observables
Conclusions
Page 24Andreas Crivellin
LHC
Dark Matter
Flavour
Exciting times in particle physics are ahead of us!
NP
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30
� Lμ-Lτ flavour symmetry
� Flavon couples to μ and τ
� is protected
� is not protected
� Effects in
τ µγ→
aµ
h µµ→
W. Altmannshofer, M. Carena, AC, 1604.08221
Lµ-Lτ model for aµ
Page 25
Explanation ofaμ and b→sμμ
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� Avoid vector-like quarks by assigning charges to
baryons as well
� Same mechanism in the quark and lepton sector
� Lμ-Lτ in lepton sector
� Good symmetry for the PMNS matrix
� Effect in but not
� First two quark generations must have the same
charges because the large Cabibbo angle would lead to
huge effect in Kaon mixing
� Anomaly freedom
Solution with horizontal U(1) charges
( ) ( ), ,2Q B a a a= − −Q(L)=(0,1,-1) Q(B)=(a,a,-2a)
9C µµ
9
eeC
Page 26
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∆F=2: Z’ contribution
q
q
q
K
B
B SM
B
K
SM
K
mR
m
Rε
ε
ε
∆=
∆
=
Page 27
Necessarily constructive, but Higgs effects and be destructive.
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Symmetry
breaking
Dynamical explanation of the charges
Page 28
A.C., J. Fuentes-Martin, A. Greljo and G. Isidori arXiv:1611.02703
( ) ( ) ( )3 3 3Q U D
SU SU SU× ×
En
erg
ysc
ale
Quark Sector Lepton Sector
( ) ( ) ( )3 3 3RE
SU SU Oν
× ×ℓ
( ) ( ) ( ) ( )2 2 2 1Q U D q
SU SU SU U× × × ( ) ( )2 1E
SU U×ℓ
( )1q
U ( )1Uℓ
Standard Model
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� 2 Z’ bosons
� Z1 coupling
mainly
to leptons
� Z2 coupling
mainly
to quarks
8
Solution with two Z’s
Different collider signatures
Page 29
Low energy
phenonenology
unchanged