Incoherent φ photo-production from deuteron in SPring-8/LEPS
description
Transcript of Incoherent φ photo-production from deuteron in SPring-8/LEPS
Incoherent φ photo-production from deuteron in SPring-8/LEPS
M. Miyabe for LEPS collaboratorsRCNP Osaka University
Baryons’10
Physics overview Experiment Result and discussion Summary
Contents
2010/12/7Baryons’10
Vector Meson Photo-production
● Vector Meson Dominance
● Pomeron Exchange
● Meson Exchange
N
q_q
_qq =
Decreasing with energy.Dominant at low energies
Slowly increasing with energyAlmost constant around threshold
N
(~ss)
uud
2010/12/7Baryons’10
Titov, Lee, Toki Phys.Rev C59(1999) 2993
Data from: SLAC('73), Bonn(’74),DESY(’78)
Natural parity
exchangeUnnatural parity
exchange
It is important to distinguishthe natural parity exchanges from unnatural ones
P2: 2ndpomeron ~ 0+glueball(Nakano, Toki (1998)
EXPAF97)
=0
deg
ree)
photo-production near threshold
2010/12/7Baryons’10
Polarization observables with linearly polarized
photonDecay Plane // natural parity exchange (-1)J (Pomeron, Scalar mesons)
Polarizationvector of
K+
K+
K-
In meson rest frame
Decay Plane unnatural parity exchange -(-1)J
(Pseudo scalar mesons )
Relative contributions from natural, unnatural parity exchanges
Decay angular distribution of
meson2010/12/7Baryons’10
Decay Angular distribution
Prediction by A. Titov (PRC,2003) -
ρ3=-0.5Pure unnatural
parity exchange
0
P, glueball, , f2’
p
)(2cos~121)( 3
PW
ρ3=0.5 forPure natural
parity exchange
~
~
2010/12/7
Baryons’10
Polarization angle of γ
K decay plane angle
Result from LEPS with proton target
Non monotonic behavior around 2GeV.Natural parity exchange is dominant → 0+ glueball ?Pseudo scalar meson exchange is not negligible.
T. Mibe, et al. PRL95 182001(2005)
ρ3=0.199+/-0.052
ρ3=0.189+/-0.030
E1E1
E2
E2
~
~
2010/12/7Baryons’10
Is the bump structure candidate of the exotic process (2nd Pomeron (glueball))? The model based on Pomeron exchange and pseudo scalar
exchange failed to explain such a non-monotonic behavior. This suggests that unknown natural parity process exist. But natural parity exchange process is comparable to pseudo
scalar exchange process from the value of ρ3.
To extract the natural parity process, detailed study for pseudo scalar π-η exchange is important.
Study of incoherent photo-production from deuteron is unique tool for this purpose.
Explore the exotic process
~
2010/12/7Baryons’10
φ photo-production from Deuteron
1. Coherent production Interact with deuteron itself.
Deuteron is iso-scalar target Iso-vector π exchange is
forbidden. Pure natural parity exchange
except for η-exchange process.
2. Incoherent production Interact with proton or
neutron in deuteron. Estimation the neutron
contribution.2010/12/7 Baryons’10
Due to isospin effect, gπnn = - gπpp → destructive gηnn = gηpp → constructive π-η interference effectDetailed Information for unnatural (π/η)
exchange process
Incoherent production
g(π, η)NN
gφγ (π, η)π,η
φγ
N N2010/12/7Baryons’10
Differential cross section as a function of energy and angle.
Due to πη interference effect, cross section from neutron decrease as low energy and forward angle.2010/12/7Baryons’10
Decay asymmetry as a function of energy and η-exchange strength
Decay asymmetry Σφ=2ρ3
Eγ=2 GeV
if η-exchange contribution is large --> Large difference in decay asymmetry
neutron
protonneutronproton
~
2010/12/7Baryons’10
EXPERIMENT
2010/12/7 Baryons’10
The LEPS beamline
2010/12/7Baryons’10
LEPS spectrometer for charged particles
1m
TOF wall
MWDC 2MWDC 3
MWDC 1
Dipole Magnet (0.7 T) Start
counter
Silicon VertexDetector
AerogelCerenkov(n=1.03)
K-
K+
• Eγ~2.4GeV• Polarization ~95%• > 1 Mcps
2010/12/7Baryons’10
Liq. D2
result
2010/12/7Baryons’10
Invariant mass K+K-
Fit with Gaussian convoluted breit-weigner Resolution~1.5MeV
Cut point for invariant mass is +/-10MeV from peak position
Total Φ event ~ 17k.
2010/12/7Baryons’10
Minimum momentum Pmin spectator approximation
Pmiss
np
φ
np
PCM
γ PKKEKK
PγEγ
PmissEmiss In LAB system, the spectator
momentumbecome minimum when the direction of proton and neutron is anti-parallel to pmiss
In quasi-free event, spectator nucleon has a small momentum such as fermi motion momentum
np
Pmin
= Pmin2010/12/7Baryons’10
Characteristics of Pmin
Quasi-free process makes a peak around zero. coherent process Pmin ~ +0.15 Dominant Pmin ≧0.1 Other inelastic events are
distributed at large negative value.
GeV
GeV
MMD
Pmin2010/12/7 Baryons’10
Deuteron Mass
Differential cross section
Differential cross section at t=tmin About 30% reduction from
free proton Not a simple nuclear
density effect since deuteron is loosely bounded.
Red : incoherent γN→φNBlack: free proton
Lower Histogram Td = (dσ/dt)N/2*(dσ/dt)p
Eγeff (GeV)
dσ/d
t(t=t
min)
(μb)
Tran
spar
ency
ratio
2010/12/7Baryons’10
Differential cross section in KKp mode
Similar degree of reduction such as incoherent process reduction of incoherent
process is not only neutron. π-η interference is small
Red : exclusive KKp eventBlack: free proton
Lower Histogram Td = (dσ/dt)KKp/(dσ/dt)free p
Td
2010/12/7Baryons’10
np
K+ K-
detectNot detect
Spin density matrix element
ρ3N is little bit higher than free proton.
Theoretical prediction of ρ3n is 0.25~0.30. ρ3N is 0.23~0.25 good agreement
Small difference ρ3
p and ρ3n
η-exchange is smallRed : γ+N→φ+NBlack : γ+p→φ+p
Eγeff (GeV)
ρ3 as a function of Eγ~
~
~
~
~ ~
2010/12/7Baryons’10
Non monotonic structure in cross section with Eγ increase at Deuteron target. Differential cross section for incoherent φ photo-production shows a significant
reduction from free proton Some effect other than nuclear density is necessary. Reduction is significant independent with coherent exclusion cut and Eγeff estimation.
From analysis for exclusive KKp event, Reduction is not only neutron but also proton in deuteron. π-η interference is small.
Decay asymmetry ρ3 is similar with free proton one η exchange component is weak.
Bump like structure around Eγ= 2GeV for γ+p→φ+p→Another natural parity process candidate
to cancel out the increasing pseudo-scalar π . More statistic and new data is ready. 2006~7 about 3 times event for proton and deuteron target. 2009 ~10 maximum ~2.9GeV photon beam for proton. detail analysis and extrapolate the energy region.
Summary
~
2010/12/7Baryons’10
Backup
2010/12/7Baryons’10
Differential cross section
Differential cross section at t=tmin About 30% reduction from
free proton Not a simple nuclear
density effect since deuteron is loosely bounded.
Red : incoherent γN→φNBlack: free proton
Lower Histogram Td = (dσ/dt)N/2*(dσ/dt)p
Eγeff (GeV)
dσ/d
t(t=t
min)
(μb
)
Td
2010/12/7Baryons’10
p p
p p
M.A. Pichowsky and T.-S. H. LeePRD 56, 1644 (1997)
Prediction from Pomeron exchange
Prediction from meson exchange
Data from: LAMP2('83), DESY('76), SLAC('73), CERN('82),FNAL('79,'82), ZEUS('95,'96)
Prediction : dominant contribution frompseudo scalar meson exchangenear threshold
Vector Meson Photo-production
2010/12/7Baryons’10
K+
K+
K-
p’
meson rest frame (Gottfried-Jackson(GJ) frame)
K+
K+
K-
pol Productionplanez
Decayplane
z-axis
K+-pol
direction of linear polarization
Decay angular distribution of meson
2010/12/7Baryons’10
Coherent production with deuteron Deuteron is iso-scalar target Iso-vector π exchange is forbidden.
Pure natural parity exchange except for η-exchange process.
2010/12/7 Baryons’10
Result of coherent production off deuterons from LEPS
Differential cross section Decay asymmetry
Differential cross section at t=tmin shows increasing with energy. Dashed line shows theoretical calculations.
Decay asymmetry showsnatural parity exchange is dominant
W. Chang et al., Physics Letter B 658, 209 (2008).
2010/12/7Baryons’10
Differential cross section Increase with energy Model prediction including Pomeron and η-exchange is
under estimate. No bump structure. Decay asymmetry Pure natural-parity exchange η-exchange is weak?
Additional natural parity process is required!
Summary of results of coherent production
2010/12/7Baryons’10
Linearly polarized Photon
• Backward Compton scattering by using UV laser light• Intensity (typ.) : 2.5 * 106 cps• Tagging Region : 1.5 GeV< E < 2.4 GeV• Linear Polarization : 95 % at 2.4 GeV
E (Tagger) (GeV) E (GeV)
Cou
nts
Line
ar p
olar
izat
ion
2010/12/7Baryons’10
Check for coherent exclusion
Without pmin cut. Reduction is
significant Eγ< 2.0 GeV,
coherent contamination is small.
2010/12/7Baryons’10
Exclusive KKp event in LH2
Eγ
dσ/dt t=tmin (μb)
2010/12/7Baryons’10
|dσ/dt|N and |dσ/dt|KKP
|dσ/dt|N /|dσ/dt|KKP
|dσ/dt|N -|dσ/dt|KKP
Eγeff (GeV)
|dσ/dt|KKP
2010/12/7Baryons’10
Spin density matrix elements
)(2cos~121)( 3
PW
2
12
1 cos~sin~121
23)(cosW
22 cos~21
21)( W
)(2cos~121)( 4
PW
2cos~121)( 5 PW
1-dimensional projections
100
1115
211
1114
211
1113
0112
0001
2~Im2/1~Im2/1~
~
~
Relations to standard definition
2010/12/7Baryons’10
Alvin Kiswandhi Phys. Lett. B(2010)2010/12/7Baryons’10
Comparison with proton
2010/12/7Baryons’10
Measure the Incoherent φ photo-production from deuteron target γ+N→φ+N. Differential cross section(bump structure) (π 、 η)-interference Decay asymmetry η-exchange process magnitude
Extract quasi-free γ+N→φ+N events clearly.
Explore in the bump structure observed in φ photo-production from free protons.
The objectives of this thesis
2010/12/7Baryons’10
Nuclear transparency ratio TA=σA/(A*σN ) (=Pout) Mass number
dependence is larger than theoretical calculation. Large σφN in nuclear
medium. How about deuteron
case?
T. Ishikawa et al, Phys. Lett. B 608, 215 (2005) 2010/12/7Baryons’10
Summary of data taking● Trigger condition : TAG*UpVeto*STA*AC*TOF● Run period (150mm-long LH2) 2002,May - 2002.July (150mm-long LD2) 2002,July – 2003 Feb, Apr-
Jun● Total number of trigger
2.26*108 trigger 4.64*108 trigger
2010/12/7Baryons’10
Number of reconstructed track ≧2 Particle identification of K+ and K- particles(PID) Decay in flight cut (DIF) Vertex cut to select events produced at the deuteron
target. Tagger cut to select reconstructed track at Tagger Invariant Mass K+K- to select phi events Missing Mass cut to select γ + N → φ X events.
φ Event selection
2010/12/7Baryons’10
Particle identification and decay in flight cut
Consistency of TOF hit position Difference of y-position of
TOF ≦80mm Difference TOF slat
number ≦ 1 Number of outlier Noutl ≦ 6 χ2 probability Prob(χ2)≧0.02
Kaon identification is 4σ
Decay in flight cut
2010/12/7Baryons’10
Vertex cut
-1120. < Vertex z < 880. -30< Vertex(x,y) < 30 2010/12/7Baryons’10
Missing Mass cut
Missing mass distribution for
γ + p → φ X (MMp)
Smearing due to the fermi motion effect. Cut region for MMp
with LD2 is 80 MeV.
2010/12/7Baryons’10
Summary of φ selection
2010/12/7Baryons’10
LEPS spectrometer has designed for forward φ→K+K- event Exclusive γ+n→φ+n event can’t be accepted.Precise analysis forCoherent processFinal State Interaction(FSI)Fermi motion effectFortunately, we have acceptance of exclusive
γ+p→φ+p →K+K-p too.
Procedure analysis for quasi-free like Incoherent γ+N→φ+N production
2010/12/7Baryons’10
Energy Definitions
For cross section100MeV step
For decay asymmetry 200MeV step
2010/12/7Baryons’10
Minimum momentum spectator approximation
Pmiss
np
np
φ
np
PCM
np
γ PKKEKK
PγEγ
PmissEmiss
In lab system, the missing momentumbecome minimum when the direction of proton and neutron is anti-parallel to pmiss
The momentum of pn system as
In quasi-free event, spectator nucleon has a small momentum such as fermi motion momentum
2010/12/7Baryons’10
Coherent production
Pcm ~ 0 Pmin ~ γβMpn ~ 0.5 Pmiss Positive momentum
around > 0.1 GeV/c
2010/12/7 Baryons’10
Pmin by Monte-Carlo simulation
Peak due to the quasi-free process is symmetric around zero. σ ~44 MeV Coherent process Dominant at Pmin
> 0.1GeV
cut point is Pmin ~ 0.1GeV.
Pmin distribution in MC
GeV
2010/12/7 Baryons’10
Effective photon energy
Due to Fermi-motion, total energy of KKN system was smeared. Pmin strongly correlated to z-
component of fermi momentum inside deuteron. Pmin could be used for
estimating Fermi momenta of target nucleons. Total center of mass energy
s of KKN system
Pmin vs. Fermi momentum z
GeV
GeV
Pmin
Fermi momentum
2010/12/7Baryons’10
Conversion Eγeff from Eγ
Effective photon energy Eγeff as
s is the center of mass total energy of KKN system.
Resolution for Eγ is improved. (~50%) Eγ resolution GeV
2010/12/7Baryons’10
Contamination of coherent process into incoherent process
Real data(black) MC(blue/red)Contamination ratio of coherent to incoherent
Contamination of coherent process is large at High energy region. less than 10% at Pmin≦0.09
Pmin cut
Pmin
2010/12/7Baryons’10
Validity check of Pmin cut-point for incoherent process
slope Differential cross section
Distributions are flat at |Pmin|=<0.09 except for E1 and E2. about 10% fluctuation from the tighter cut.
Pmin cutPmin cut
E9E9 E8 E7
E6 E5 E4
E3 E2
E1
E2E1
E3
E4E5 E6
E7E8
2010/12/7Baryons’10
Conversion to effective photon flux
Photon flux ωγ for each Eγ as ωγ(Eγ)=Frac(Eγ) * Ntag Frac(Eγ) : photon fraction for EγNtag : corrected tagger scalar count
In nucleon at rest frame,
At one specific Eγeff, it depends on some Eγ which spread over because of fermi motion.Conversion ratio from each Eγ bin is calculated using Monte-Carlo.
Eγeff
Eγeff (GeV)
Pmin<0.09Pmin : all
ωγ
2010/12/7Baryons’10
Conversion ratio
At one specific Eγeff
Conversion ratio from each Eγ bin 10 MeV bining for each
Eγeff and Eγ Eγ resolution ~
10MeV
2010/12/7 Baryons’10
Estimate the Final state interaction
Momentum of outgoing nucleon is small, and FSI effect is enhanced near threshold .
Strength of FSI is enhanced in small relative momentum p and n. (similar kinematics in coherent)
np
n
φγ
p
FSI enhancement factor
pn relative momentum kk = |pn – pp|/2 2010/12/7Baryons’10
Monte Carlo simulation
Real data are fitted by distributions of coherent, inciherent and FSI processes produced by MC. FSI contribution is
very weak at all energy bin.
<< 1%
Missing Mass distribution MMD
Black :real, red coherent green: incoherent, blue: FSI
GeV2010/12/7Baryons’10
P-N relative momentum fitData were fitted by results FSI and coherent prodeced by MC.
χ2/ndf distributionas a function of FSI strength
χ2 is better with smaller FSI effect. weak
FSI effect is negligible small
GeV
2010/12/7Baryons’10
Background from non-resonant KK events Backgrounds under the KK
invariant mass spectrum are mainly from non-resonant KK events. Estimate the background
contamination into phi events by using the side band region
Non-resonant K+K- invariant massGeV
2010/12/7Baryons’10
Differential cross section t dependence.
Fitting function : dσ/dt = C*exp(-b*t) (red curve)
Slope parameter b as a function of Eγeff
nonmonotonic behavior of slope,Slope b = 3.74 +/- 0.12 (free proton b=3.38+/-0.23)
GeVEγefft (GeV2)
dσ/dt (μb)
2010/12/7Baryons’10
Energy dependence of differential cross section at t=tmin
Cross section does not simply increase with energy
at Eγ ~ 2.2 GeV
dσ/dt at (t=tmin) with Constant slope b=3.742010/12/7 Baryons’10
Differential cross section with tighter Pmin cut
nonmonotonic behavior of slope,Slope b = 3.45 +/- 0.13 (free proton b=3.38+/-0.23)
dσ/dt at (t=tmin) with b=3.45 t dependence Pmin ≦50
Cross section decreases at E1~E3
Eγeff (GeV)Eγeff (GeV)
dσ/dt(t=tmin) (μb)
Black histogram : 90MeV, Red : 50MeV2010/12/7Baryons’10
3-particle KKp mode All particles (KKp) in the
final state were detected to select the exclusive proton events. The statistics is very limited
but, the bump-like structure is seen as well as the results from free-proton target.
dσ/dt at (t=tmin) with Constant slope b=3.38
dσ/dt(t=tmin) (μb)
2010/12/7Baryons’10
Decay angular distribution
ρ1~5 as a function of EγDecay angular distribution 2010/12/7Baryons’10
Differential cross section at Eγ In the original Eγ, similar
reduction appeared Eγ ~ 1.9GeV Photon flux is similar for
both Eγ and Eγeff .
2010/12/7Baryons’10
Eγeff at KKp mode
Eγeff(KK) : calculated with K+K- Eγeff(KKp) :calculated with K+K- p Estimation of Eγeff works well.
Eγeff(KK) Eγeff(KKp)
2010/12/7Baryons’10
Tighter Pmin cutDifferential cross section at t=tmin
Red : incoherent γN→φNBlack: free proton
Red : γ+N→φ+NBlack : γ+p→φ+p
ρ3 as a function of Eγ
Decrease in Highest energy region
Eγeff (GeV) Eγeff (GeV)
ρ3
Td
dσ/dt(t=tmin) (μb)
2010/12/7Baryons’10
Backup figures
2010/12/7Baryons’10
Nuclear transparency ratio
2010/12/7Baryons’10
Eγ vs. Eγ(n)
Eγ
Eγ(n)
2010/12/7Baryons’10
Spin density matrix
Horz Vert
2010/12/7Baryons’10
Spin density matrix
2010/12/7Baryons’10
ρ
Horz, Vert Horz+Vert
2010/12/7Baryons’10
Spin density matrix element
2010/12/7Baryons’10
Spin density matrix element
Vert
Horz
2010/12/7Baryons’10
Pmin dependence
slope Differential cross section
2010/12/7Baryons’10
Photon flux
2010/12/7Baryons’10
Photon flux
2010/12/7Baryons’10
Comparison to LEPS result
2010/12/7Baryons’10
Pmin<50MeV
2010/12/7Baryons’10
Tagger cut
2010/12/7Baryons’10
Coherent contamination
2010/12/7Baryons’10
Lambda(1520)
2010/12/7Baryons’10
Non-resonant BG
2010/12/7Baryons’10
2010/12/7Baryons’10
Experiment at Spring-8
•8GeV electron storage ring Harima Hyogo
2010/12/7Baryons’10
Liquid hydrogen target150mm
2010/12/7Baryons’10
Drift Chamber calibration
Depth of the multi hit TDC ~3 (before 8) High Voltage value of
sense wire is large. Threshold for discri-
amp is low. Noisy level is high
2010/12/7Baryons’10
t0 calibration
Large fluctuation in TDC offset value t0 . Every 10 run
calibration.
DC-t0 run dependencerun
tdc
2010/12/7Baryons’10
xt-calibration Xdrift = c1t+c2t2+c3t3+c4
Correct the origin-point Calcurate parameters
when resolution and efficiency are down
2010/12/7Baryons’10
Result of calibration
Number of outlier Χ^2 probability
LH2(short)
LH2(long)
LH2(long)2010/12/7Baryons’10
2010/12/7Baryons’10
Decay angular distribution
● W0,W1,W2 are parameterized by the 9 spin density matrix elements.
Re() Im() andIm()
),(),,( 0 WW
),()2sin(),()2cos( 21 WPWP Unpolarized part
Polarized part
K.Schilling et al. Nucl. Phys. B15(1970) 408
2010/12/7Baryons’10
Final state interaction
2010/12/7Baryons’10