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What can we learn from hadronic and radiative decaysof light mesons?
Bastian Kubis
Helmholtz-Institut fur Strahlen- und Kernphysik (Theorie)
Bethe Center for Theoretical Physics
Universitat Bonn, Germany
Light Meson Decays Workshop, Jefferson Lab, August 5th 2012
B. Kubis, Hadronic and radiative decays of light mesons – p. 1
Hadronic and radiative decays of light mesons
Chiral perturbation theory and dispersion relations
Final-state interactions of two pions
• Pion vector form factor
• Decays η, η′ → π+π−γ
Final-state interactions of three pions
• 3-particle dynamics for ω/φ → 3π talk by S. Schneider on Wednesday
• η → 3π: quark mass ratios and Dalitz plot parameterstalk by S. Lanz on Tuesday
Meson transition form factors
• η, η′ → γℓ+ℓ− thanks to A. Wirzba
• ω/φ → π0ℓ+ℓ− talk by S. Schneider on Wednesday
Outlook
B. Kubis, Hadronic and radiative decays of light mesons – p. 2
Light mesons without models
Chiral perturbation theory (ChPT) . . . talk by J. Bijnens on Monday
• Effective field theory: simultaneous expansion inquark masses + small momenta
⊲ systematically improvable⊲ well-established link to QCD⊲ so what’s wrong with it?!
B. Kubis, Hadronic and radiative decays of light mesons – p. 3
Light mesons without models
Chiral perturbation theory (ChPT) . . . talk by J. Bijnens on Monday
• Effective field theory: simultaneous expansion inquark masses + small momenta
⊲ systematically improvable⊲ well-established link to QCD⊲ so what’s wrong with it?!
. . . and its limitations
• strong final-state interactions render corrections large
• physics of light pseudoscalars (π, K, η) only⊲ (energy) range limited by resonances
e.g. pion–pion scattering: σ(500), ρ . . .⊲ not applicable to decays of (e.g.) vector mesons at all
−→ marry ChPT and dispersion relations in order to
apply ChPT where it works best!
B. Kubis, Hadronic and radiative decays of light mesons – p. 3
Light mesons without models
Dispersion relations on one page
Re(z)
Im(z)
s
4M2π
analyticity & Cauchy’s theorem:
T (s) =1
2πi
∮
∂Ω
T (z)dz
z − s
B. Kubis, Hadronic and radiative decays of light mesons – p. 4
Light mesons without models
Dispersion relations on one page
Re(z)
Im(z)
s
4M2π
analyticity & Cauchy’s theorem:
T (s) =1
2πi
∮
∂Ω
T (z)dz
z − s
B. Kubis, Hadronic and radiative decays of light mesons – p. 4
Light mesons without models
Dispersion relations on one page
Re(z)
Im(z)
s
4M2π
analyticity & Cauchy’s theorem:
T (s) =1
2πi
∮
∂Ω
T (z)dz
z − s
B. Kubis, Hadronic and radiative decays of light mesons – p. 4
Light mesons without models
Dispersion relations on one page
Re(z)
Im(z)
s
4M2π
analyticity & Cauchy’s theorem:
T (s) =1
2πi
∮
∂Ω
T (z)dz
z − s
B. Kubis, Hadronic and radiative decays of light mesons – p. 4
Light mesons without models
Dispersion relations on one page
Re(z)
Im(z)
s
4M2π
analyticity & Cauchy’s theorem:
T (s) =1
2πi
∮
∂Ω
T (z)dz
z − s
−→ 1
2πi
∫ ∞
4M2π
discT (z)dz
z − s
=1
π
∫ ∞
4M2π
ImT (z)dz
z − s
B. Kubis, Hadronic and radiative decays of light mesons – p. 4
Light mesons without models
Dispersion relations on one page
Re(z)
Im(z)
s
4M2π
analyticity & Cauchy’s theorem:
T (s) =1
2πi
∮
∂Ω
T (z)dz
z − s
−→ 1
2πi
∫ ∞
4M2π
discT (z)dz
z − s
=1
π
∫ ∞
4M2π
ImT (z)dz
z − s
• discT (s) = 2i ImT (s) calculable by “cutting rules”:
T (s) T (s)
e.g. if T (s) is a ππ partial wave −→
discT (s)
2i= ImT (s) =
2qππ√sθ(s−4M2
π)|T (s)|2
B. Kubis, Hadronic and radiative decays of light mesons – p. 4
Light mesons without models
Dispersion relations on one page
Re(z)
Im(z)
s
4M2π
analyticity & Cauchy’s theorem:
T (s) =1
2πi
∮
∂Ω
T (z)dz
z − s
−→ 1
2πi
∫ ∞
4M2π
discT (z)dz
z − s
=1
π
∫ ∞
4M2π
ImT (z)dz
z − s
• discT (s) = 2i ImT (s) calculable by “cutting rules”:
T (s) T (s)inelastic intermediate states (KK, 4π)suppressed at low energies
−→ will be neglected in the following
B. Kubis, Hadronic and radiative decays of light mesons – p. 4
Pion form factor constrained by analyticity and unitarity
• just two particles in final state: form factor; from unitarity:
=disc
1
2idiscFI(s) = ImFI(s) = FI(s)×θ(s−4M2
π)× sin δI(s) e−iδI(s)
−→ final-state theorem: phase of FI(s) is just δI(s) Watson 1954
B. Kubis, Hadronic and radiative decays of light mesons – p. 5
Pion form factor constrained by analyticity and unitarity
• just two particles in final state: form factor; from unitarity:
=disc
1
2idiscFI(s) = ImFI(s) = FI(s)×θ(s−4M2
π)× sin δI(s) e−iδI(s)
−→ final-state theorem: phase of FI(s) is just δI(s) Watson 1954
• solution to this homogeneous integral equation known:
FI(s) = PI(s)ΩI(s) , ΩI(s) = exp
s
π
∫ ∞
4M2π
ds′δI(s
′)
s′(s′ − s)
PI(s) polynomial, ΩI(s) Omnès function Omnès 1958
• today: high-accuracy ππ (and πK) phase shifts availableAnanthanarayan et al. 2001, García-Martín et al. 2011, Caprini et al. 2012
(Büttiker et al. 2004)
B. Kubis, Hadronic and radiative decays of light mesons – p. 5
Pion vector form factor
• pion vector form factor clearly non-perturbative: ρ resonance
-0,2 0 0,2 0,4 0,6 0,8 1
sππ [GeV2]
1
10
|FV
(sπ
π)|2
ChPT at one loop
data on e+e− → π+π−
Omnès representation
Stollenwerk et al. 2012
−→ Omnès representation vastly extends range of applicability
B. Kubis, Hadronic and radiative decays of light mesons – p. 6
Application: η, η′→ π+π−γ
• η(′) → π+π−γ driven by the chiral anomaly, π+π− in P-wave
−→ final-state interactions the same as for vector form factor
• ansatz: Aη(′)
ππγ = A× P (sππ)× FVπ (sππ), P (sππ) = 1 + α(′)sππ
B. Kubis, Hadronic and radiative decays of light mesons – p. 7
Application: η, η′→ π+π−γ
• η(′) → π+π−γ driven by the chiral anomaly, π+π− in P-wave
−→ final-state interactions the same as for vector form factor
• ansatz: Aη(′)
ππγ = A× P (sππ)× FVπ (sππ), P (sππ) = 1 + α(′)sππ
• spectra with fitted normalisation and slope(s) α(′)
0 0.05 0.1 0.15 0.2
Eγ[GeV]
0
1
2
3
4
5
6
7
8
dΓ/dEγ[arb. units]
0 0.1 0.2 0.3 0.4
Eγ[GeV]
0
5
10
15
20
dΓ/dEγ[arb. units]
Stollenwerk et al. 2012
B. Kubis, Hadronic and radiative decays of light mesons – p. 7
Application: η, η′→ π+π−γ
• η(′) → π+π−γ driven by the chiral anomaly, π+π− in P-wave
−→ final-state interactions the same as for vector form factor
• ansatz: Aη(′)
ππγ = A× P (sππ)× FVπ (sππ), P (sππ) = 1 + α(′)sππ
• divide data by pion form factor −→ P (sππ)
0 0.05 0.1 0.15 0.2 0.25 0.3
sππ [GeV2]
1
1.2
1.4
1.6
P(s π
π)
0 0.2 0.4 0.6 0.8
sππ [GeV2]
1
1.5
2
2.5
3
P(s π
π)
Stollenwerk et al. 2012
−→ exp.: αWASA = (1.89± 0.64)GeV−2, αKLOE = (1.31± 0.08)GeV−2
−→ interpret α(′) by matching to chiral perturbation theory
B. Kubis, Hadronic and radiative decays of light mesons – p. 7
Dispersion relations for three-body decays
Example: ω/φ → 3π
• beyond ChPT: copious efforts to develop EFT for vector mesonsBijnens et al.; Bruns, Meißner; Lutz, Leupold; Gegelia et al.; Kampf et al.. . .
• vector mesons highly important for (virtual) photon processes
B. Kubis, Hadronic and radiative decays of light mesons – p. 8
Dispersion relations for three-body decays
Example: ω/φ → 3π
• beyond ChPT: copious efforts to develop EFT for vector mesonsBijnens et al.; Bruns, Meißner; Lutz, Leupold; Gegelia et al.; Kampf et al.. . .
• vector mesons highly important for (virtual) photon processes
• typically used for 3π decays: improved tree-level models(vector-meson dominance, hidden local symmetry. . . )
+ crossed +ω
ρ
π
π
π
ω
π
π
π
• similarly in experimental analyses φ → 3π: KLOE 2003, CMD-2 2006
sum of 3 Breit–Wigners (ρ+, ρ−, ρ0)+ constant background term
−→ obviously, unitarity relation cannot be fulfilled!
• particularly simple system: restricted to odd partial waves
−→ P-wave interactions only (neglecting F- and higher)B. Kubis, Hadronic and radiative decays of light mesons – p. 8
From unitarity to integral equation
Decay amplitude can be decomposed into single-variable functions
M(s, t, u) = iǫµναβnµpνπ+pαπ−p
βπ0 F(s, t, u)
F(s, t, u) = F(s) + F(t) + F(u)
Unitarity relation for F(s):
discF(s) = 2iF(s)︸︷︷︸
right-hand cut
+ F(s)︸︷︷︸
left-hand cut
× θ(s− 4M2
π)× sin δ11(s) e−iδ11(s)
B. Kubis, Hadronic and radiative decays of light mesons – p. 9
From unitarity to integral equation
Unitarity relation for F(s):
discF(s) = 2iF(s)︸︷︷︸
right-hand cut
+ F(s)︸︷︷︸
left-hand cut
× θ(s− 4M2
π)× sin δ11(s) e−iδ11(s)
B. Kubis, Hadronic and radiative decays of light mesons – p. 9
From unitarity to integral equation
Unitarity relation for F(s):
discF(s) = 2iF(s)︸︷︷︸
right-hand cut
× θ(s− 4M2
π)× sin δ11(s) e−iδ11(s)
=disc
• right-hand cut only −→ Omnès problem
F(s) = aΩ(s) , Ω(s) = exp
s
π
∫ ∞
4M2π
ds′
s′δ11(s
′)
s′ − s− iǫ
−→ amplitude given in terms of pion vector form factor
++pair0V +0pair+V +0pairVF(s, t, u) =
B. Kubis, Hadronic and radiative decays of light mesons – p. 9
From unitarity to integral equation
Unitarity relation for F(s):
discF(s) = 2iF(s)︸︷︷︸
right-hand cut
+ F(s)︸︷︷︸
left-hand cut
× θ(s− 4M2
π)× sin δ11(s) e−iδ11(s)
• inhomogeneities F(s): angular averages over the F(s)
F(s) = aΩ(s)
1 +s
π
∫ ∞
4M2π
ds′
s′sin δ11(s
′)F(s′)
|Ω(s′)|(s′ − s− iǫ)
F(s) =3
2
∫ 1
−1
dz (1− z2)F(t(s, z)
)Khuri, Treiman 1960
Aitchison 1977
Anisovich, Leutwyler 1998
F(s) = +++ ...
B. Kubis, Hadronic and radiative decays of light mesons – p. 9
From unitarity to integral equation
Unitarity relation for F(s):
discF(s) = 2iF(s)︸︷︷︸
right-hand cut
+ F(s)︸︷︷︸
left-hand cut
× θ(s− 4M2
π)× sin δ11(s) e−iδ11(s)
• inhomogeneities F(s): angular averages over the F(s)
F(s) = aΩ(s)
1 +s
π
∫ ∞
4M2π
ds′
s′sin δ11(s
′)F(s′)
|Ω(s′)|(s′ − s− iǫ)
F(s) =3
2
∫ 1
−1
dz (1− z2)F(t(s, z)
)Khuri, Treiman 1960
Aitchison 1977
Anisovich, Leutwyler 1998
−→ crossed-channel scattering between s-, t-, and u-channel
B. Kubis, Hadronic and radiative decays of light mesons – p. 9
ω/φ → 3π Dalitz plots
• only one subtraction constant a −→ fix to partial width
• normalised Dalitz plot in y = 3(s0−s)2MV (MV −3Mπ)
, x =√3(t−u)
2MV (MV −3Mπ):
ω → 3π : φ → 3π :
• ω Dalitz plot is relatively smooth
• φ Dalitz plot clearly shows ρ resonance bands
B. Kubis, Hadronic and radiative decays of light mesons – p. 10
ω/φ → 3π Dalitz plots
• only one subtraction constant a −→ fix to partial width
• normalised Dalitz plot in y = 3(s0−s)2MV (MV −3Mπ)
, x =√3(t−u)
2MV (MV −3Mπ):
ω → 3π : φ → 3π :
ω → 3π
• ω Dalitz plot is relatively smooth
• φ Dalitz plot clearly shows ρ resonance bands
B. Kubis, Hadronic and radiative decays of light mesons – p. 10
Experimental comparison to φ → 3π
• fit to Dalitz plot: 1.98× 106 events in 1834 bins KLOE 2003
0 100 200 300 400 500 600 700 800 9000
2000
4000
6000
8000
Bin number
#eve
nts
(effi
cien
cyco
rrec
ted)
Omnès χ2 = 1.71 ... 2.06
KLOE (2003)
F(s) = aΩ(s) = exp
[
s
π
∫ ∞
4M2π
ds′
s′δ11(s
′)
s′ − s
]
B. Kubis, Hadronic and radiative decays of light mesons – p. 11
Experimental comparison to φ → 3π
• fit to Dalitz plot: 1.98× 106 events in 1834 bins KLOE 2003
0 100 200 300 400 500 600 700 800 9000
2000
4000
6000
8000
Bin number
#eve
nts
(effi
cien
cyco
rrec
ted)
Omnès χ2 = 1.71 ... 2.06
Disp1 χ2 = 1.17 ... 1.50
KLOE (2003)
F(s) = aΩ(s)
[
1 +s
π
∫ ∞
4M2π
ds′
s′F(s′) sin δ11(s
′)
|Ω(s′)|(s′ − s− iǫ)
]
B. Kubis, Hadronic and radiative decays of light mesons – p. 11
Experimental comparison to φ → 3π
• fit to Dalitz plot: 1.98× 106 events in 1834 bins KLOE 2003
0 100 200 300 400 500 600 700 800 9000
2000
4000
6000
8000
Bin number
#eve
nts
(effi
cien
cyco
rrec
ted)
Omnès χ2 = 1.71 ... 2.06
Disp1 χ2 = 1.17 ... 1.50
Disp2 χ2 = 1.02 ... 1.03
KLOE (2003)
F(s) = aΩ(s)
[
1 + b s+s2
π
∫ ∞
4M2π
ds′
s′2F(s′) sin δ11(s
′)
|Ω(s′)|(s′ − s− iǫ)
]
B. Kubis, Hadronic and radiative decays of light mesons – p. 11
Experimental comparison to φ → 3π
• fit to Dalitz plot: 1.98× 106 events in 1834 bins KLOE 2003
0 100 200 300 400 500 600 700 800 9000
2000
4000
6000
8000
Bin number
#eve
nts
(effi
cien
cyco
rrec
ted)
Omnès χ2 = 1.71 ... 2.06
Disp1 χ2 = 1.17 ... 1.50
Disp2 χ2 = 1.02 ... 1.03
KLOE (2003)
• once-subtracted DR: highly predictive
• twice-subtracted DR: one additional complex parameter fitted
• phenomen. contact term seems to emulate rescattering effects!
B. Kubis, Hadronic and radiative decays of light mesons – p. 11
Predictions for experiment: ω → 3π Dalitz plot parameters
• ω → 3π Dalitz plot smooth −→ polynomial parameterisation
|Fpol(z, φ)|2 = |N |2
1 + 2αz + 2βz3/2 sin 3φ+ 2γz2 + 2δz5/2 sin 3φ+O(z3)
B. Kubis, Hadronic and radiative decays of light mesons – p. 12
Predictions for experiment: ω → 3π Dalitz plot parameters
• ω → 3π Dalitz plot smooth −→ polynomial parameterisation
|Fpol(z, φ)|2 = |N |2
1 + 2αz+2βz3/2 sin 3φ+ 2γz2 + 2δz5/2 sin 3φ
(
|Fpol(z, φ)|2/|F(z, φ)|2 − 1
)
[%]
x [MeV]
y[M
eV]
α× 103 β × 103 γ × 103 δ × 103
84 . . . 96 — — —
74 . . . 84 24 . . . 28 — —
73 . . . 81 24 . . . 28 3 . . . 6 —
74 . . . 83 21 . . . 24 0 . . . 2 7 . . . 8
B. Kubis, Hadronic and radiative decays of light mesons – p. 12
Predictions for experiment: ω → 3π Dalitz plot parameters
• ω → 3π Dalitz plot smooth −→ polynomial parameterisation
|Fpol(z, φ)|2 = |N |2
1 + 2αz + 2βz3/2 sin 3φ+2γz2 + 2δz5/2 sin 3φ
(
|Fpol(z, φ)|2/|F(z, φ)|2 − 1
)
[%]
x [MeV]
y[M
eV]
α× 103 β × 103 γ × 103 δ × 103
84 . . . 96 — — —
74 . . . 84 24 . . . 28 — —
73 . . . 81 24 . . . 28 3 . . . 6 —
74 . . . 83 21 . . . 24 0 . . . 2 7 . . . 8
B. Kubis, Hadronic and radiative decays of light mesons – p. 12
Predictions for experiment: ω → 3π Dalitz plot parameters
• ω → 3π Dalitz plot smooth −→ polynomial parameterisation
|Fpol(z, φ)|2 = |N |2
1 + 2αz + 2βz3/2 sin 3φ+ 2γz2+2δz5/2 sin 3φ
(
|Fpol(z, φ)|2/|F(z, φ)|2 − 1
)
[%]
x [MeV]
y[M
eV]
α× 103 β × 103 γ × 103 δ × 103
84 . . . 96 — — —
74 . . . 84 24 . . . 28 — —
73 . . . 81 24 . . . 28 3 . . . 6 —
74 . . . 83 21 . . . 24 0 . . . 2 7 . . . 8
B. Kubis, Hadronic and radiative decays of light mesons – p. 12
Predictions for experiment: ω → 3π Dalitz plot parameters
• ω → 3π Dalitz plot smooth −→ polynomial parameterisation
|Fpol(z, φ)|2 = |N |2
1 + 2αz + 2βz3/2 sin 3φ+ 2γz2 + 2δz5/2 sin 3φ
(
|Fpol(z, φ)|2/|F(z, φ)|2 − 1
)
[%]
x [MeV]
y[M
eV]
α× 103 β × 103 γ × 103 δ × 103
84 . . . 96 — — —
74 . . . 84 24 . . . 28 — —
73 . . . 81 24 . . . 28 3 . . . 6 —
74 . . . 83 21 . . . 24 0 . . . 2 7 . . . 8
B. Kubis, Hadronic and radiative decays of light mesons – p. 12
Predictions for experiment: ω → 3π Dalitz plot parameters
• ω → 3π Dalitz plot smooth −→ polynomial parameterisation
|Fpol(z, φ)|2 = |N |2
1 + 2αz + 2βz3/2 sin 3φ+ 2γz2 + 2δz5/2 sin 3φ
(
|Fpol(z, φ)|2/|F(z, φ)|2 − 1
)
[%]
x [MeV]
y[M
eV]
α× 103 β × 103 γ × 103 δ × 103
84 . . . 96 — — —
74 . . . 84 24 . . . 28 — —
73 . . . 81 24 . . . 28 3 . . . 6 —
74 . . . 83 21 . . . 24 0 . . . 2 7 . . . 8
−→ 2 Dalitz plot parameters sufficient at 1% accuracy
−→ compare η → 3π0 (same 3-fold symmetry):α = (−31.7± 1.6)× 10−3 PDG average
β ≈ −4× 10−3 γ ≈ +1× 10−3 Schneider, BK, Ditsche 2011
B. Kubis, Hadronic and radiative decays of light mesons – p. 12
Quark masses and η → 3π decays
• η → 3π isospin violating; two sources in the Standard Model:
mu 6= md e2 6= 0
• electromagnetic contribution small Sutherland 1967
Baur, Kambor, Wyler 1996; Ditsche, BK, Meißner 2009
η → π+π−π0 : ALOc (s, t, u) =
B(mu −md)
3√3F 2
π
1 +3(s− s0)
M2η −M2
π
s = (pπ+ + pπ−)2 , 3s0.= M2
η + 3M2π
• ∆I = 1 relation between charged and neutral decay amplitudes:
η → 3π0 : An(s, t, u) = Ac(s, t, u) +Ac(t, u, s) +Ac(u, s, t)
B. Kubis, Hadronic and radiative decays of light mesons – p. 13
Quark masses and η → 3π decays
• η → 3π isospin violating; two sources in the Standard Model:
mu 6= md e2 6= 0
• electromagnetic contribution small Sutherland 1967
Baur, Kambor, Wyler 1996; Ditsche, BK, Meißner 2009
η → π+π−π0 : ALOc (s, t, u) =
B(mu −md)
3√3F 2
π
1 +3(s− s0)
M2η −M2
π
s = (pπ+ + pπ−)2 , 3s0.= M2
η + 3M2π
• ∆I = 1 relation between charged and neutral decay amplitudes:
η → 3π0 : An(s, t, u) = Ac(s, t, u) +Ac(t, u, s) +Ac(u, s, t)
• relevance: (potentially) clean access to mu −md
but : large higher-order / final-state interactions
−→ require good theoretical Dalitz-plot description
to extract normalisation
B. Kubis, Hadronic and radiative decays of light mesons – p. 13
η → 3π: final-state interactions
• strong final-state interactions among pions
⊲ tree level: Γ(η → π+π−π0) = 66 eV Cronin 1967
⊲ one-loop: Γ(η → π+π−π0) = 160± 50 eV Gasser, Leutwyler 1985
⊲ experimental: Γ(η → π+π−π0) = 296± 16 eV PDG
• major source: large S-wave final-state rescattering −→use dispersion relations to resum those beyond loop expansion
• similar formalism to ω/φ → 3π, but more partial waves
(S waves I = 0, 2, P wave I = 1)
match subtraction constants to ChPT and/or to datatalk by S. Lanz on Tuesday
B. Kubis, Hadronic and radiative decays of light mesons – p. 14
η → 3π: final-state interactions
• strong final-state interactions among pions
⊲ tree level: Γ(η → π+π−π0) = 66 eV Cronin 1967
⊲ one-loop: Γ(η → π+π−π0) = 160± 50 eV Gasser, Leutwyler 1985
⊲ experimental: Γ(η → π+π−π0) = 296± 16 eV PDG
• major source: large S-wave final-state rescattering −→use dispersion relations to resum those beyond loop expansion
• similar formalism to ω/φ → 3π, but more partial waves
(S waves I = 0, 2, P wave I = 1)
match subtraction constants to ChPT and/or to datatalk by S. Lanz on Tuesday
• on the other hand: consider r =Γ(η → 3π0)
Γ(η → π+π−π0)
ChPT: rtree = 1.54 , r1-loop = 1.46 , r2-loop = 1.47
PDG: r = 1.432± 0.026 (fit) , r = 1.48± 0.05 (average)
−→ agrees rather well Bijnens, Ghorbani 2007
B. Kubis, Hadronic and radiative decays of light mesons – p. 14
η → 3π0 Dalitz plot parameter α
|An(x, y)|2 = |Nn|21 + 2α z + . . .
z ∝ (s− s0)
2 + (t− s0)2 + (u− s0)
2
-0.08 -0.06 -0.04 -0.02 0.00 0.02 0.04 0.06 0.08 0.10
ChPT O(p4)
ChPT O(p6)
Dispersive (KWW)
Crystal Ball@BNL
Crystal Barrel@LEAR
GAMS-2000
KLOE
MAMI-B
MAMI-C
SND
WASA@CELSIUS
WASA@COSY
O(p4) + NREFT (full)
103 × α
+13
+13± 32
−7 . . .− 14
−25± 5
Schneider, BK,Ditsche 2011
PDG average:−31.7± 1.6
B. Kubis, Hadronic and radiative decays of light mesons – p. 15
η → π+π−π0: Dalitz plot parameters
• |Ac(x, y)|2 = |Nc|21 + ay + by2 + dx2 + . . .
x =
√3
2MηQη(u− t )
y = 32MηQη
(s0 − s)
a b d
KLOE −1.09 +−
0.010.02 0.12±0.01 0.057+
−0.0090.017
ChPT O(p6) −1.27 ± 0.08 0.39±0.10 0.055±0.057
ChPT O(p4)+ NREFT −1.21 ± 0.01 0.31±0.02 0.050±0.003
dispersive −1.16 0.24 . . . 0.26 0.09 . . . 0.10
Bijnens, Ghorbani 2007
Schneider, BK, Ditsche 2011
Kambor, Wiesendanger, Wyler 1995
• only one modern precision experiment so far KLOE 2008
−→ WASA-at-COSY coming up soon
• note large discrepancy theory vs. experiment for b !
B. Kubis, Hadronic and radiative decays of light mesons – p. 16
η → 3π Dalitz parameters, charged vs. neutral
• Dalitz plot vs. amplitude expansion: x ∝ t− u , y ∝ s− s0
|Ac|2 = |Nc|21 + ay + by2 + dx2 + . . .
|An|2 = |Nn|2
1 + 2αz + . . .
Ac = Nc
1 + ay + by2 + dx2 + . . .
An = Nn
1 + αz + . . .
a = 2Re a , b = |a|2 + 2Re b , d = 2Re d , α = Re α
B. Kubis, Hadronic and radiative decays of light mesons – p. 17
η → 3π Dalitz parameters, charged vs. neutral
• Dalitz plot vs. amplitude expansion: x ∝ t− u , y ∝ s− s0
|Ac|2 = |Nc|21 + ay + by2 + dx2 + . . .
|An|2 = |Nn|2
1 + 2αz + . . .
Ac = Nc
1 + ay + by2 + dx2 + . . .
An = Nn
1 + αz + . . .
a = 2Re a , b = |a|2 + 2Re b , d = 2Re d , α = Re α
• isospin relation between neutral and charged parameters:
α =1
2
(b+ d
)−→ α =
1
4
(
b+ d− a2
4− (Im a)2
)
<1
4
(
b+ d− a2
4
)
Bijnens, Ghorbani 2007
B. Kubis, Hadronic and radiative decays of light mesons – p. 17
η → 3π Dalitz parameters, charged vs. neutral
• Dalitz plot vs. amplitude expansion: x ∝ t− u , y ∝ s− s0
|Ac|2 = |Nc|21 + ay + by2 + dx2 + . . .
|An|2 = |Nn|2
1 + 2αz + . . .
Ac = Nc
1 + ay + by2 + dx2 + . . .
An = Nn
1 + αz + . . .
a = 2Re a , b = |a|2 + 2Re b , d = 2Re d , α = Re α
• isospin relation between neutral and charged parameters:
α =1
4
(
b+ d− a2
4
)
− ζ1(1 + ζ2a)2 , ζ1 = 0.050± 0.005 , ζ2 = 0.225± 0.003
ζ1/2 determined by ππ phases Schneider, BK, Ditsche 2011
B. Kubis, Hadronic and radiative decays of light mesons – p. 17
η → 3π Dalitz parameters, charged vs. neutral
• Dalitz plot vs. amplitude expansion: x ∝ t− u , y ∝ s− s0
|Ac|2 = |Nc|21 + ay + by2 + dx2 + . . .
|An|2 = |Nn|2
1 + 2αz + . . .
Ac = Nc
1 + ay + by2 + dx2 + . . .
An = Nn
1 + αz + . . .
a = 2Re a , b = |a|2 + 2Re b , d = 2Re d , α = Re α
• isospin relation between neutral and charged parameters:
α =1
4
(
b+ d− a2
4
)
− ζ1(1 + ζ2a)2 , ζ1 = 0.050± 0.005 , ζ2 = 0.225± 0.003
ζ1/2 determined by ππ phases Schneider, BK, Ditsche 2011
• use precise KLOE data on a, b, d as input KLOE 2008
αtheoKLOE = −0.062± 0.003stat
+0.004−0.006syst ± 0.003ππ
αexpKLOE = −0.030± 0.004stat
+0.002−0.004syst
significanttension!
B. Kubis, Hadronic and radiative decays of light mesons – p. 17
η → 3π Dalitz parameters, charged vs. neutral
• Dalitz plot vs. amplitude expansion: x ∝ t− u , y ∝ s− s0
|Ac|2 = |Nc|21 + ay + by2 + dx2 + . . .
|An|2 = |Nn|2
1 + 2αz + . . .
Ac = Nc
1 + ay + by2 + dx2 + . . .
An = Nn
1 + αz + . . .
a = 2Re a , b = |a|2 + 2Re b , d = 2Re d , α = Re α
• isospin relation between neutral and charged parameters:
α =1
4
(
b+ d− a2
4
)
− ζ1(1 + ζ2a)2 , ζ1 = 0.050± 0.005 , ζ2 = 0.225± 0.003
ζ1/2 determined by ππ phases
• displayed as constraint in a− b plane:
-1.40 -1.35 -1.30 -1.25 -1.20 -1.15 -1.10 -1.05 -1.00a
0.05
0.10
0.15
0.20
0.25
0.30
0.35
0.40
0.45
b
O(p4) + NREFT
KLOE
NREFT imaginary part
NO imaginary part
B. Kubis, Hadronic and radiative decays of light mesons – p. 17
Hadronic decays of the η′
• large final-state interactions expected in η′ → ηππ and η′ → 3π
−→ unitarised U(3) ChPT e.g. Borasoy, Nißler 2005
• only includes two-particle unitarity:
−→ dispersive study in progress Schneider, BK
B. Kubis, Hadronic and radiative decays of light mesons – p. 18
Hadronic decays of the η′
• large final-state interactions expected in η′ → ηππ and η′ → 3π
−→ unitarised U(3) ChPT e.g. Borasoy, Nißler 2005
• only includes two-particle unitarity:
−→ dispersive study in progress Schneider, BK
• claim: Gross, Treiman, Wilczek 1979
Γ(η′ → π0π+π−)
Γ(η′ → ηπ+π−)∝
(md −mu
ms
)2
assumptions: (a) A(η′ → π0π+π−) = ǫπ0η ×A(η′ → ηπ+π−)
(b) amplitudes "essentially flat" in phase space
• refuted in unitarised U(3) ChPT: assumptions too simplisticBorasoy, Meißner, Nißler 2006
B. Kubis, Hadronic and radiative decays of light mesons – p. 18
(g − 2)µ, light-by-light, and transition form factors
Czerwinski et al., arXiv:1207.6556 [hep-ph]
• leading and next-to-leading hadronic effects in (g − 2)µ:
had
had
−→ hadronic light-by-light soon dominant uncertainty
B. Kubis, Hadronic and radiative decays of light mesons – p. 19
(g − 2)µ, light-by-light, and transition form factors
Czerwinski et al., arXiv:1207.6556 [hep-ph]
• leading and next-to-leading hadronic effects in (g − 2)µ:
had
had
−→ hadronic light-by-light soon dominant uncertainty
• important contribution: pseudoscalar pole terms
singly / doubly virtual form factors
FPγγ∗(M2P , q
2, 0) and FPγ∗γ∗(M2P , q
21 , q
22)
π0, η, η′
B. Kubis, Hadronic and radiative decays of light mesons – p. 19
(g − 2)µ, light-by-light, and transition form factors
Czerwinski et al., arXiv:1207.6556 [hep-ph]
• leading and next-to-leading hadronic effects in (g − 2)µ:
had
had
−→ hadronic light-by-light soon dominant uncertainty
• important contribution: pseudoscalar pole terms
singly / doubly virtual form factors
FPγγ∗(M2P , q
2, 0) and FPγ∗γ∗(M2P , q
21 , q
22)
• for specific virtualities: linked tovector-meson conversion decays
π0, η, η′
−→ e.g. Fπ0γ∗γ∗(M2π0 , q21,M
2ω) measurable in ω → π0ℓ+ℓ− etc.
B. Kubis, Hadronic and radiative decays of light mesons – p. 19
Transition form factors in η → γℓ+ℓ−
• 2-pion contribution to Fηγ∗γ(s, 0) intimately linked to Aηππγ :
η π+
π−
γ∗
γ
discFηγ∗γ(s, 0) ∝ Aηππγ(s, 0)× FV ∗
π (s) = A× P (s)× |FVπ (s)|2
F(I=1)ηγ∗γ (s, 0) = 1 +
B(η→π+π−γ)︷︸︸︷
Aηππγ
Aηγγ
︸︷︷︸
B(η→γγ)
e s
12π2
∫ ∞
4M2π
ds′q3ππ(s
′)
s′3/2P (s′)︸ ︷︷ ︸
1+α s′
|FVπ (s′)|2s′ − s
• corrections from isoscalar contributions −→ here small
• in particular: form factor slope bη function of α(η → π+π−γ)
−→ indications for significant deviation from VMD pictureHanhart, Stollenwerk, Wirzba, work in progress
B. Kubis, Hadronic and radiative decays of light mesons – p. 20
Transition form factors in ω, φ → π0ℓ+ℓ−
• long-standing puzzle: transition form factor ω → π0ℓ+ℓ− far fromvector-meson-dominance picture see e.g. Terschlüsen, Leupold 2010
disc
ω
π0
π0
ωπ
+
π−
=
fωπ0(s) = fωπ0(0) +s
12π2
∫ ∞
4M2π
ds′q3ππ(s
′)FV ∗π (s′)f1(s
′)
s′3/2(s′ − s)Köpp 1974
• f1(s) = fω→3π1 (s) = F(s) + F(s) P-wave projection of F(s, t, u)
• subtracting dispersion relation once yields
⊲ better convergence for ω → π0γ∗ transition form factor
⊲ sum rule for ω → π0γ −→ saturated at 90–95%
fωπ0(0) =1
12π2
∫ ∞
4M2π
ds′q3ππ(s
′)
s′3/2FV ∗π (s′)f1(s
′) , Γω→π0γ ∝ |fV π0(0)|2
Schneider, BK, Niecknig 2012
B. Kubis, Hadronic and radiative decays of light mesons – p. 21
Numerical results: ω → π0γ∗
0 0.1 0.2 0.3 0.4 0.5 0.6
1
10
100
√s [GeV]
|Fωπ0(s)|2
NA60 ’09NA60 ’11Lepton-GVMDTerschlüsen et al.f1(s) = aΩ(s)full dispersive
0.2 0.3 0.4 0.5 0.6 0.70
1
2
3
4
5
6
7
8
9
√s [GeV]
dΓω→
π0µ+µ−/d
s[10−
6G
eV−1]
0 0.1 0.2 0.3 0.4 0.5 0.610-8
10-7
10-6
10-5
10-4
10-3
10-2
10-1
100
0.2 0.3 0.4 0.5 0.6 0.70
3
6
9
10em
6√s [GeV]
dΓω→
π0e+e−/d
s[G
eV−1]
• clear enhancement vs. pure VMD
• unable to account for steep rise (similar in φ → ηℓ+ℓ−?)
B. Kubis, Hadronic and radiative decays of light mesons – p. 22
Numerical results: φ → π0γ∗
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8
1
10
100
√s [GeV]
|Fφπ0(s)|2
VMDf1(s) = aΩ(s)once subtracted f1(s)
twice subtracted f1(s)
0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.90
1
2
3
4
5
6
7
√s [GeV]
dΓφ→
π0µ+µ−/d
s[10−
8G
eV−1]
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.910-10
10-9
10-8
10-7
10-6
10-5
10-4
10-3
10-2
0.2 0.3 0.4 0.5 0.6 0.7 0.801
2
34
5
6
7
10em
8
√s [GeV]
dΓφ→
π0e+e−/d
s[G
eV−1]
• measurement would be extremely helpful: ρ in physical region!
• partial-wave amplitude backed up by experiment
B. Kubis, Hadronic and radiative decays of light mesons – p. 23
Summary
Dispersion relations for meson decays
• based on fundamental principles ofunitarity, analyticity, crossing symmetry
• rigorous treatment of two- and three-hadron final states
• extends range of applicability (at least) to full elastic regime
• matching to ChPT where it works best:
(sub)threshold, normalisation, slopes. . .
• relates hadronic to radiative decays / transition form factors
B. Kubis, Hadronic and radiative decays of light mesons – p. 24
Summary
Dispersion relations for meson decays
• based on fundamental principles ofunitarity, analyticity, crossing symmetry
• rigorous treatment of two- and three-hadron final states
• extends range of applicability (at least) to full elastic regime
• matching to ChPT where it works best:
(sub)threshold, normalisation, slopes. . .
• relates hadronic to radiative decays / transition form factors
Omissions
• not-extremely-rare decays not yet seen experimentally: η′ → 4πGuo, BK, Wirzba 2011
• impact of transition form factors on rare leptonic decays
π0 → e+e−, η → ℓ+ℓ− KTeV 2007
B. Kubis, Hadronic and radiative decays of light mesons – p. 24
Spares
B. Kubis, Hadronic and radiative decays of light mesons – p. 25
ππ scattering constrained by analyticity and unitarity
Roy equations = coupled system of partial-wave dispersion relations+ crossing symmetry + unitarity
• twice-subtracted fixed-t dispersion relation:
T (s, t) = c(t) +1
π
∫ ∞
4M2π
ds′
s2
s′2(s′ − s)+
u2
s′2(s′ − u)
ImT (s′, t)
• subtraction function c(t) determined from crossing symmetry
B. Kubis, Hadronic and radiative decays of light mesons – p. 26
ππ scattering constrained by analyticity and unitarity
Roy equations = coupled system of partial-wave dispersion relations+ crossing symmetry + unitarity
• twice-subtracted fixed-t dispersion relation:
T (s, t) = c(t) +1
π
∫ ∞
4M2π
ds′
s2
s′2(s′ − s)+
u2
s′2(s′ − u)
ImT (s′, t)
• subtraction function c(t) determined from crossing symmetry
• project onto partial waves tIJ(s) (angular momentum J , isospin I)−→ coupled system of partial-wave integral equations
tIJ(s) = kIJ(s) +
2∑
I′=0
∞∑
J′=0
∫ ∞
4M2π
ds′KII′
JJ′(s, s′)ImtI′
J′(s′)
Roy 1971
• subtraction polynomial kIJ(s): ππ scattering lengthscan be matched to chiral perturbation theory Colangelo et al. 2001
• kernel functions KII′
JJ′(s, s′) known analytically
B. Kubis, Hadronic and radiative decays of light mesons – p. 26
ππ scattering constrained by analyticity and unitarity
• elastic unitarity −→ coupled integral equations for phase shifts
• modern precision analyses:⊲ ππ scattering Ananthanarayan et al. 2001, García-Martín et al. 2011
⊲ πK scattering Büttiker et al. 2004
• example: ππ I = 0 S-wave phase shift & inelasticity
400 600 800 1000 1200 1400
s1/2
(MeV)
0
50
100
150
200
250
300
CFDOld K decay dataNa48/2K->2 π decayKaminski et al.Grayer et al. Sol.BGrayer et al. Sol. CGrayer et al. Sol. DHyams et al. 73
δ0
(0)
1000 1100 1200 1300 1400
s1/2
(MeV)
0
0.5
1
η00(s)
Cohen et al.Etkin et al.Wetzel et al.Hyams et al. 75Kaminski et al.Hyams et al. 73Protopopescu et al.CFD .
ππ KK
ππ ππ
García-Martín et al. 2011
• strong constraints on data from analyticity and unitarity!
B. Kubis, Hadronic and radiative decays of light mesons – p. 27
Pion vector form factor and ahvpµ
• more refined representation: taken from talk by G. Colangelo 2008
F πV (s) = Ω1(s)×Gω(s)× Ωinel(s)
Gω(s): ρ− ω mixingΩinel(s): inelastic for
√s & (Mπ +Mω), parametrized using
conformal mapping techniques Trocóniz, Ynduráin 2002Comparison CMD2(04)–KLOE
0.6 0.65 0.7 0.75 0.8 0.85 0.9 0.95 1
E (GeV)
0
10
20
30
40
50
|Fπ|2
CMD2 dataKLOE dataFit to both sets
• achieve amazing precisionfor hadronic contribution toaµ below 1 GeV:
ahvpµ (√s ≤ 2MK)
= (493.7± 1.0)× 10−10
Colangelo et al. (preliminary)
• check of data compatibilitywith analyticity / unitarity
• also extension to higher energies Hanhart 2012
B. Kubis, Hadronic and radiative decays of light mesons – p. 28
Transition form factor beyond the πω threshold
0 0.2 0.4 0.6 0.8 1 1.2 1.40.1
1
10
100
√s [GeV]
|Fφπ0(s)|2
NA60 ’09NA60 ’11Lepton-G
VMDCMD-2
Terschlüsen et al.f1(s) = aΩ(s)
once subtracted f1(s)
• full solution above naive VMD, but still too low
• higher intermediate states (4π / πω) more important?
B. Kubis, Hadronic and radiative decays of light mesons – p. 29