Working group e + e - @ Frascati
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Milan 4/11/05 Work group e+e- M. Radici - Time-like form factors 1
Working group e+e- @ FrascatiMilano 4 Nov. 2005
Time - like form factors
Marco Radici
INFN - Pavia
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Outline
1. Why should we measure time-like (TL) form factors (FF) ?
2. What should we learn from TL FF with respect to SL FF ?
3. Which measurements are needed ?
4. Available data and calculations ?
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. Questions in SL region2. Surprise in SL $ TL 3. Few and poor TL data4. Better constrain models
elastic scatteringcross section
Rosenbluth separation
fixed Q2, varyGE slope , GM intercept
large errors in GE
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. Questions in SL region2. Surprise in SL $ TL 3. Few and poor TL data4. Better constrain models
polarizationtransfer
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. Questions in SL region2. Surprise in SL $ TL 3. Few and poor TL data4. Better constrain models
JLab – Hall A Qattan et al. P.R.L. 94 (05) 142301
Blunden et al. nucl-th/0506039
2?
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. Questions in SL region2. Surprise in SL $ TL 3. Few and poor TL data4. Better constrain models
pQCD
JLab polar. transfer data
where is onset of pQCD scaling ?
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GEp
GMp
GEn
GMn
Lomon, P.R. C66 (02) 045501 : VMD
Miller, P.R. C66 (02) 032201(R) : LFCBM
Holzwarth, hep-ph/0201138
Ma, Qing, Schmidt, P.R. C65 (02) 035205 : LF diquark
from H. GaoInt. J. Mod. Phys. E12 (03) 1
erratum E12 (03) 567
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. Questions in SL region2. Surprise in SL $ TL 3. Few and poor TL data4. Better constrain models
SpaceLike TimeLike
analytic continuation by Dispersion Relations (DR)
But
fit to pQCD TimeLike
fit to pQCD SpaceLike
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. Questions in SL region2. Surprise in SL $ TL 3. Few and poor TL data4. Better constrain models
2Q
nMGpQCD + analyticity
But
fit to |GMp|
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. Questions in SL region2. Surprise in SL $ TL 3. Few and poor TL data4. Better constrain models
poor statistic
integrate dover wide
angular range
all data assume
it’s true only at where steep rise is observed
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. Questions in SL region2. Surprise in SL $ TL 3. Few and poor TL data4. Better constrain models
only 1 measurement for neutron (ADONE-1998) again with
scarce angular distributions and with low statistics
no polarization of protons and/or electrons
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. Questions in SL region2. Surprise in SL $ TL 3. Few and poor TL data4. Better constrain models
IJL
CQM
pQCD“improved”
Dispersive approach on BaBar and LearPacetti talk at Nucleon ’05 - Frascati
Brodsky et al. P.R. D69 (04) 054022
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. Form factors are complex2. |FF| from unpol. cross section3. Phases from polarization4. Unphysical region
Dispersion Relation (DR)
F(t) analytic function in t 2 C withcut [t0 = 4m
2, 1)
C
R
Im F(t’) 0 only in [t0=4m2, 1 )
vector-meson poles and multi-hadron continuum
dipole fit to F2 (q2e-i) / F1 (q2 e-i) ! R !
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. Form factors are complex2. |FF| from unpol. cross section3. Phases from polarization4. Unphysical region
unpolarized cross section for
R angular asymmetry
q2<0 Rosenbluth plotchange E, e at fixed q2
) linear plot in
q2>0 measure 2 at fixed q2 ) get Rcos2 typical of Born diagram
measure 3 ) explore 2 mechanisms
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. Form factors are complex2. |FF| from unpol. cross section3. Phases from polarization4. Unphysical region
polarized cross section for
Ax, Az require polarization of the electron beam: Pe 0
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. Form factors are complex2. |FF| from unpol. cross section3. Phases from polarization4. Unphysical region
phases of FF from Final-State Interactions (FSI) of final baryon system : interference of channels with different phases ( Im (GE
*GM) )
pQCD : FSI ! 0 for Q2 ! 1 ) test transition to scaling and Color Transparency (CT)
FSI ! T-odd mechanisms are allowed : generates
not possible in elastic scattering
GE = F1 + F2 = |GE| ei E
GM = F1 + F2 = |GM| ei M
Im (GE*GM) = ( -1) Im F2
*F1
threshold t1=4M2 ! Im( )=0consistent with |GE|=|GM| from GT=1(t1)=0
ambiguity $ - solved by
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. Form factors are complex2. |FF| from unpol. cross section3. Phases from polarization4. Unphysical region
discriminate among models that are close in SL region
IJL
CQM
pQCD“improved”
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. Form factors are complex2. |FF| from unpol. cross section3. Phases from polarization4. Unphysical region
steep rise at threshold
tail of narrow resonance at t ≤ 4M2 (baryonium) ?
should show up as a dip in somehadronic cross section
E687 diffractive photoproduction of 6
Upcoming results from BaBar also
W » 1.9 GeV
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
measure angular dependence of unpol. cross section) angular asymmetry R and test 2 mechanisms
measure Ay / sin (E - M)
measure Ay / Ax / tan (E - M)
utopia : measure Ai j
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
ADONE Q2 = 4.4 GeV (1973)
CERN Q2 ~ 3.6 (1977)
Orsay-DM1 Q2 ~ 3.75-4.56 (1979)
Orsay-DM2 Q2 =4-5 (1983)
LEAR Q2 ~3.5-4.2 (1994)
E760 Q2 ~8.9-13 (1993)
FENICE Q2 ~3.7-6 (1994)
E835 Q2 ~8.8-18.4 (1999) 11.6-18.2 (2003)
CLEO Q2 ~11-12 (2005)
BES Q2 ~4-9 (2005)
BaBar Q2 ~2-20 (2005)
1. data : proton2. models
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. data : proton2. models
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. data : neutron2. models
2Q
nMG
but always assumed
|GEN| = |GM
N| N=p,n
FENICE Q2 ~3.7-6 (1994)
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1. Why TL FF ?2. What do we learn ?3. Which measurements ?4. Available data and models ?
1. data2. models
• Dispersion Relations (DR): analyticity+unitarity+Vector Mesons (VM) (Drechsel, Meissner, Hammer, Hoehler,..) “ “ + input exp. data (Baldini, Pacetti, …)
• VM Dominance (VMD) based models (Iachello, Bijker, Lomon, …)
• Soliton (Holzwarth)
• CQM : Light Front Form (Pace, Salmè, Simula, …) “ “ “ + \pi cloud (Miller, Jennings, .. ) Point Form (Pavia + Graz collaboration) Diquark (Ma, …)
• pQCD “inspired” (Brodsky, Ji, Belitski, Yuan, ..)
• reviews: Brodsky et al. P.R. D69 (04) 054022 Tomasi-Gustafsson et al. E.P.J. A24 (05) 419
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Possible logo ?
(from Pacetti talk at Nucleon’05)