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Axial Form Factors
M. R. Schindler
Institut für KernphysikJohannes Gutenberg-Universität, Mainz
From Parity Violation to Hadronic Structure and more . . .Milos Island
16-20 May, 2006
In collaboration with T. Fuchs, S. Scherer
M. R. Schindler Milos 2006
Outline
Definition and Properties
Axial form factor GA(q2)
Induced pseudoscalar form factor GP(q2)
GA, GP in Lorentz-invariant ChPT
Summary
M. R. Schindler Milos 2006
Definition and Properties
M. R. Schindler Milos 2006
Form factors
Form factors of the nucleonParametrization of nucleon structureElectromagnetic form factors F1(q2), F2(q2)[GE(q2), GM(q2)
]Vector current ∼ γµ
Well known experimentallyImportant test for theories and models
Axial form factors GA(q2), GP(q2), GT (q2)
Axial-vector current ∼ γµγ5Not very well known
M. R. Schindler Milos 2006
Axial-vector current operator
Aµ,a(x) ≡ q(x)γµγ5τa
2q(x), q =
(ud
), a = 1, 2, 3
HermitianA†
µ,i(x) = Aµ,i(x)
Vector under isospin transformations
[Ia, Aµ,b(x)] = iεabcAµ,c(x)
Axial vector under parity
Aµ,i(x)P7→ −Ai
µ(Px)
Charge conjugation
Aµ,i(x)C7→ Aµ,i(x), i = 1, 3
Aµ,i(x)C7→ −Aµ,i(x), i = 2
M. R. Schindler Milos 2006
Definition of axial form factors
Axial-vector current matrix element
〈N(p′)|Aµi (0)|N(p)〉
= u(p′)[GA(q2)γµ +
qµ
2MGP(q2) + i
σµνqν
2MGT (q2)
]γ5
τi
2u(p)
qµ = p′µ − pµ
GA(q2): axial form factorGP(q2): induced pseudoscalar form factorGT (q2): induced pseudotensorial form factor
M. R. Schindler Milos 2006
Properties of axial form factors
Hermiticity for q2 ≤ 0
GA(q2)∗ = GA(q2)
GP(q2)∗ = GP(q2)
GT (q2)∗ = −GT (q2)
For mu = md : invariance under G-conjugation
G = C exp(iπI2)
⇒GT (q2) = 0
M. R. Schindler Milos 2006
Breit-System
~p = −12~q = −~p ′, q0 = 0
〈N (~q2 ) |A0,a(0)|N (−~q
2 )〉 = 0
〈N (~q2 ) |~A
a(0)|N (−~q2 )〉 =
τa
2
[E(−~q
2 )
M(~σ − ~σ · qq)GA(−~q 2) + ~σ · qqD(−~q 2)
]
M. R. Schindler Milos 2006
Axial form factor GA(q2)
M. R. Schindler Milos 2006
Axial form factor GA(q2)
GA(0) = gADetermined from n → p + e− + νeGA(q2 ≈ 0) = gA = 1.2670± 0.0035
GA(q2)
(Quasi)elastic (anti)neutrino scatteringPion electroproductionParametrization
GA(q2) =gA
(1− q2
M2A)2
with MA: axial mass
M. R. Schindler Milos 2006
Neutrino scattering
0.85 0.95 1.05 1.15 1.25MA [GeV]
Average
Argonne (1969)
CERN (1977)
Argonne (1977)
CERN (1979)
BNL (1980)
BNL (1981)
Argonne (1982)
Fermilab (1983)
BNL (1986)
BNL (1987)
BNL (1990)
Argonne (1973)
from V. Bernard, L. Elouadrhiri and U.-G. Meißner,
J. Phys. G 28, R1 (2002)
Global average (new)
MA = (1.001± 0.020) GeV
H. Budd, A. Bodek and J. Arrington,
arXiv:hep-ex/0308005
M. R. Schindler Milos 2006
Pion electroproductionγ∗ + p → n + π+ at threshold
Extract MA from E0+
0.85 0.95 1.05 1.15 1.25MA [GeV]
Frascati (1970)Frascati (1970) GEn=0Frascati (1972)DESY (1973)Daresbury (1975) SPDaresbury (1975) DRDaresbury (1975) FPVDaresbury (1975) BNR
AverageMAMI (1999)Saclay (1993)Olsson (1978)Kharkov (1978)DESY (1976)
Daresbury (1976) SP
Daresbury (1976) BNRDaresbury (1976) DR
from V. Bernard, L. Elouadrhiri and U.-G. Meißner,
J. Phys. G 28, R1 (2002)
Global average
MA = (1.068± 0.017) GeV
M. R. Schindler Milos 2006
Heavy Baryon ChPT: Modification at O(q3)
Notation for amplitude
~M∣∣∣thr
= −4πWmN
i[i(~σ − ~σ · k k)E0+(k2) + i~σ · k kL0+(k2)
]Contribution from pion loops
1 1
2
1 1
2
1
2
M. R. Schindler Milos 2006
Heavy Baryon ChPT: Modification at O(q3)
Modification of the k2 dependence of E (−)0+
E (−)0+ (k2) =
egA
8πFπ[1 +
k2
4m2N
(κV +
12
)+
k2
6r2A︸ ︷︷ ︸
old
+M2
8π2F 2π
f(
k2
M2
)︸ ︷︷ ︸
new
+ · · · ]
Pion electroproduction: MA = (1.068± 0.017) GeV∆MA = 0.056 GeVNeutrino scattering: MA = (1.001± 0.020) GeV
⇒
Agreement
V. Bernard, N. Kaiser, and U.-G. Meißner, Phys. Rev. Lett. 69, 1877 (1992)M. R. Schindler Milos 2006
Haberzettl claims: Pion electroproduction data at thresholdcannot be interpreted in terms of GA[H. Haberzettl, Phys. Rev. Lett. 85, 3576 (2000)]
Solution: Minimal coupling does not respect constraintsdue to chiral symmetry[T. Fuchs and S. Scherer, Phys. Rev. C 68, 055501 (2003)]
L(3)eff = const. Ψγµγ5[Dν , f−µν ]Ψ + · · ·
with
f−µν = −2(∂µaν − ∂νaµ) + 2i ([vµ, aν ]− [vν , aµ])
+iF
[~τ · ~π, ∂µvν − ∂νvµ] + · · ·
M. R. Schindler Milos 2006
Induced pseudoscalar form factor GP(q2)
M. R. Schindler Milos 2006
Chiral limit
Axial-vector current divergence-free in chiral limit
M → 0 ⇒ ∂µAµ,a(x) = 0
∂µ〈N(p′)|Aµ,a(x)|N(p)〉 = ∂µ〈N(p′)|eiP·xAµ,a(0)e−iP·x |N(p)〉= iqµeiq·x〈N(p′)|Aµ,a(0)|N(p)〉= 0 ∀ x ,
Dirac equation ⇒
4◦m
2 ◦GA (q2) + q2 ◦
GP (q2) = 0
M. R. Schindler Milos 2006
Chiral limit
Possible solutions◦m= 0 and
◦GP (q2) = 0
◦GP (q2) = −4
◦m
2 ◦GA(q2)q2
GA(0) = gA ≈ 1.26 ⇒◦GP (q2) has pole for q2 → 0
M. R. Schindler Milos 2006
Pion pole contribution
Interpretation in terms of pion pole contribution
Most general pion pole contribution
−2Fπ(q2)gπNN(q2)
q2 −M2 − Σ(q2)uqµγ5
τa
2u
M. R. Schindler Milos 2006
Pion pole contribution: chiral limit
M2 → 0
→ −2F (q2)◦gπNN (q2)
q2−◦Σ (q2)
2◦m u
qµ
2◦m
γ5τa
2u
⇒ Contribution to◦GP
−4◦m F (q2)
◦gπNN (q2)
q2−◦Σ (q2)
with◦Σ (0) = 0
M. R. Schindler Milos 2006
Goldberger-Treiman-Relation
Consider limit
limq2→0
q2 ◦GP,π (q2) = −4
◦m F
◦gπNN
!= −4
◦m
2 ◦GA (0)
Goldberger-Treiman-Relation
◦gA
F=
◦gπNN
◦m
Real world
Satisfied up to ≈ 2%
M. R. Schindler Milos 2006
Experimental data
mµ
2mNGP(q2 = −0.88m2
µ) = gP
Ordinary muon capture (OMC): µ− + p → νµ + n
gP = 8.7± 1.9
Liquid hydrogen target: complications due to formation ofpµp moleculesMuCap experiment at PSI: hydrogen gas
Radiative muon capture (RMC): µ− + p → νµ + n + γ
gP = 12.3± 0.9
q2-dependence: one pion electroproduction experiment
M. R. Schindler Milos 2006
BUT: new measurement of ortho-para transition rate in pµpmolecule
Λnewop = (11.1±1.7±0.9
0.6)×104 s−1 vs. Λoldop = (4.1±1.4)×104 s−1
OMC (Saclay)gP = 0.8± 2.7
RMC (TRIUMF)gP = 10.6± 1.1
average liquid H2gP = 5.6± 4.1
J. H. D. Clark et al., Phys. Rev. Lett. 96, 073401 (2006)
M. R. Schindler Milos 2006
Heavy baryon ChPT
Order O(q3) calculation
GP(q2) =4mNFπgπNN(q2)
M2 − q2 − 23
m2NgA〈r2〉A
gP = 8.23
Allows for systematical corrections
M. R. Schindler Milos 2006
GA, GP in manifestly Lorentz-invariant ChPT
M. R. Schindler Milos 2006
Calculation of GA(q2) and GP(q2) up to and includingO(q4)
Infrared renormalization scheme
GA(q2) = gA +16
gA〈r2〉Aq2 +g3
A4F 2 H(q2)
with H(0) = H ′(0) = 0
gP = 8.09
0.1 0.2 0.3 0.4
Q2@GeV2D
0.2
0.4
0.6
0.8
1
GAHQ2L�GAH0L
-0.1 0 0.1 0.2Q2@GeV2D
-150
-100
-50
0
50
100
150
200
GPHQ2L
M. R. Schindler Milos 2006
Electromagnetic form factors
Compare to situation for e.m. form factors
Inclusion of vector mesons (ρ, ω, Φ)
M. R. Schindler, J. Gegelia and S. Scherer, Eur. Phys. J. A 26, 1 (2005)M. R. Schindler Milos 2006
Inclusion of axial-vector meson a1
Reformulated infrared renormalization → inclusion ofaxial-vector mesons as explicit degrees of freedom
L(3)πA = fA〈AµνFµν
− 〉
L(0)AN = GANΨAµγµγ5Ψ
GAVMA (q2) = −8fAGAN
q2
q2 −M2a1
GAVMP (q2) = 32m2
N fAGAN1
q2 −M2a1
effectively only one additional coupling constant fAGAN
M. R. Schindler Milos 2006
Summary
M. R. Schindler Milos 2006
Summary
Axial form factors parameterize axial structure of nucleonGA(q2)
(Anti)neutrino scatteringPion electroproductionDiscrepancy explained in HBChPT
GP(q2)
Ordinary muon capture (OMC)Radiative muon capture (RMC)Results for gP do not agreeTheory agrees with OMC
Infrared renormalizationInclusion of a1 mesonOnly one additional low energy constant
M. R. Schindler Milos 2006